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NAME:
ABSCAL
PURPOSE:
Apply the FITS BZERO and BSCALE keyword values to a data array
CALLING SEQUENCE:
RESULT = ABSCAL( Value, Header, /DEBUG)
INPUTS:
VALUE - Any scalar, vector, or array (usually an integer type giving a
relative intensity).
HEADER - A FITS header array containing the absolute calibration
keyword BSCALE, and optionally BZERO and BUNIT.
OUTPUT:
RESULT = BSCALE*VALUE + BZERO, where the BSCALE and BZERO scalars
are taken from the FITS header.
If the absolute calibration keywords do not exist, then
RESULT = VALUE, and !ERR = -1.
OPTIONAL INPUT KEYWORD:
/DEBUG - If DEBUG is set, then ABSCAL will print the
calibration units given by the BUNIT keyword.
REVISION HISTORY:
Written W. Landsman, STX Corporation January 1987
Use DEBUG keyword instead of !DEBUG September 1995
Converted to IDL V5.0 W. Landsman September 1997
CALLS:
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Name: ace_files
Purpose: return ace data file names for desired time range & type
Input Parameters:
t0,t1 - desired time range
Output:
function returns file list
CALLS: ***
BOX_MESSAGE, BREAK_FILE [1], BREAK_FILE [2], BREAK_FILE [3], CONCAT_DIR [1]
CONCAT_DIR [2], CONCAT_DIR [3], FILE2TIME, TIME2FILE, break_file [4]
concat_dir [4], data_chk [1], data_chk [2], file_list [1], file_list [2]
get_logenv [1], get_logenv [2], ssw_strsplit, ut_time [1], ut_time [2]
CALLED BY:
get_acedata
History:
5-Sep-2001 - S.L.Freeland
6-Sep-2001 - S.L.Freeland - handle "current" daily file (fixed name)
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NAME: ACGAUNT
PURPOSE: Calculate continuum gaunt factor using approximations
of R. Mewe (18-JUN-85) to full calculations of
paper VI (Arnaut and Rothenflug for ion balances).
CATEGORY:
CALLING SEQUENCE: cgauntf = acgaunt( wave, te_6)
cgauntf = acgaunt( wave, te_6, G1=gff, G2=gfb, G3=g2p)
INPUTS: wave = Wavelength in Angstrom (1-d vector or scalar)
te_6 = Temperature in 10^6 K (1-d vector or scalar)
OPTIONAL INPUTS: none.
OUTPUTS: Function result
= cgauntf(n_elements(te_6), n_elements(wave))
= array of approximate continuum gaunt factors.
OPTIONAL OUTPUTS:
G1 = Free-free Gaunt factor
G2 = Free-bound Gaunt factor
G3 = 2-photon Gaunt factor
CALLS: ***
INDD [1], INDD [2], MKDARR [1], MKDARR [2]
CALLED BY:
BREM_49, CONFLX [1], CONFLX [2]
COMMON BLOCKS: none
SIDE EFFECTS: none
RESTRICTIONS: none
PROCEDURE: see a paper of R. Mewe et al. (A & Ap)
MODIFICATIONS: written by N.Nitta from a Fortran version, March 1991.
31-jul-93, JRL, Added a check on the exponent to prevent floating underflow message
23-Jun-94, DMZ, made Gaunt factors double precision
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NAME:
AD2XY
PURPOSE:
Compute X and Y from native coordinates and a FITS astrometry structure
EXPLANATION:
If a WCS projection (Calabretta & Greisen 2002, A&A, 395, 1077) is
present, then the procedure WCSXY2SPH is used to compute native
coordinates. If distortion is present then this is corrected.
In all cases, the inverse of the CD matrix is applied and offset
from the reference pixel to obtain X and Y.
AD2XY is generally meant to be used internal to other procedures. For
interactive purposes, use ADXY.
CALLING SEQUENCE:
AD2XY, a ,d, astr, x, y
INPUTS:
A - R.A. or longitude in DEGREES, scalar or vector
D - Dec. or longitude in DEGREES, scalar or vector
ASTR - astrometry structure, output from EXTAST procedure containing:
.CD - 2 x 2 array containing the astrometry parameters CD1_1 CD1_2
in DEGREES/PIXEL CD2_1 CD2_2
.CDELT - 2 element vector giving increment at reference point in
DEGREES/PIXEL
.CRPIX - 2 element vector giving X and Y coordinates of reference pixel
(def = NAXIS/2) in FITS convention (first pixel is 1,1)
.CRVAL - 2 element vector giving coordinates of the reference pixel
in DEGREES
.CTYPE - 2 element vector giving projection types
.LONGPOLE - scalar longitude of north pole (default = 180)
.PV2 - Vector of additional parameter (e.g. PV2_1, PV2_2) needed in
some projections
.DISTORT - Optional substructure specifying distortion parameters
OUTPUTS:
X - row position in pixels, scalar or vector
Y - column position in pixels, scalar or vector
X,Y will be in the standard IDL convention (first pixel is 0), and
*not* the FITS convention (first pixel is 1)
NOTES:
AD2XY tests for presence of WCS coordinates by the presence of a dash
in the 5th character position in the value of CTYPE (e.g 'DEC--SIN').
PROCEDURES USED:
TAG_EXIST(), WCSSPH2XY
REVISION HISTORY:
Converted to IDL by B. Boothman, SASC Tech, 4/21/86
Use astrometry structure, W. Landsman Jan. 1994
Do computation correctly in degrees W. Landsman Dec. 1994
Only pass 2 CRVAL values to WCSSPH2XY W. Landsman June 1995
Don't subscript CTYPE W. Landsman August 1995
Converted to IDL V5.0 W. Landsman September 1997
Understand reversed X,Y (X-Dec, Y-RA) axes, W. Landsman October 1998
Consistent conversion between CROTA and CD matrix W. Landsman October 2000
No special case for tangent projection W. Landsman June 2003
Work for non-WCS coordinate transformations W. Landsman Oct 2004
CALLS:
CALLED BY
ADXY, ARCBAR, ATV, CONS_DEC, CONS_RA, HASTROM, IMDBASE, POINTING3, STARFIELD, XYXY
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PURPOSE: Add two 2-d arrays, where the dimensions do not need to
be equal. Allow the second array to be rotated
(not yet implemented) and translated with respect
to the first array. If (because of size difference or
translation) the second array is not added
completely into the first array, either clip (the default)
the part of the second array that 'hangs outside' of the
dimensions of the first, or expand the output array
to hold both arrays completely via the no_clip keyword.
PARAMETERS:
REQ: arr1 - First array to be added to.
REQ: arr2 - Array to be added to arr1
OPTIONAL KEYWORDS:
x_tr - x-translation of arr2 prior to addition to arr_1
y_tr - y-translation of arr2 prior to addition to arr_1
rot_d - degrees to rotate arr1 prior to addition to arr_1
NOT CURRENTLY IMPLEMENTED
no_clip - Return the array that is the union of the two
arrays, with elements in neither set to zero.
min_thr1 - Minimum scalar threshold below which array values
from arr1 should not be added to the new composite array.
max_thr1 - Maximum scalar Threshold above which array values
from arr1 should not be added to the new composite array.
min_thr2 - Minimum scalar threshold below which array values
from arr2should not be added to the new composite array.
max_thr2 - Maximum scalar Threshold above which array values
from arr2 should not be added to the new composite array.
max_dim - Maximum dimensions of output array.
NOT CURRENTLY IMPLEMENTED
no_out - If not no_clip, return array 1 if arrays have no
overlap. Default is to return an error.
NOT CURRENTLY IMPLEMENTED
arr_av - Averages the result of array addition by pixel.
(divides each pixel by 1. or 2.); THIS WILL BE
EXPANDED.
OPTIONAL OUTPUT:
arr_tally - Array with same dimensions as output array, whose
integer entries count how many times each pixel
had a value added to it. (This array can be used
to keep a running tally when this function is
called iteratively.) Must be the same dimensions
as 'arr1'. NOT YET IMLEMENTED WITH NO_CLIP OPTION.
HISTORY: Jan-20-2000, Phil Shirts
May-26-2000, (PGS) allowed each array to have a max and min
threshold with, min_thr1, min_thr2, max_thr1,
max_thr2 INSTEAD of min_thr, max_thr.
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Name: add_kw2hdr
Category: UTIL
Purpose: Add keywords set in _EXTRA to a FITS header. The mapping of _extra
keywords to header keywords is controlled via the keywords kw_list and
hdr_list
Calling sequence: new_hdr = add_kw2hdr( header, KW_LIST=kws, HDT_LIST=hdrs )
Input:
hdr - FITS header for modification.
Output:
Modified FITS header.
Input keywords:
KW_LIST - list of keywords to search for in _extra
HDR_LIST - names keyword parameters will be given in FITS header.
HDR_COMMENTS - string array containing comments for added parameters.
Output keywords:
ERR_MSG - string containing error message. Null if no errors occurred during
execution.
ERR_CODE - 0/1 if no error/ an error occurred during execution.
Calls: ***
FXADDPAR [1], FXADDPAR [2], FXPAR [1], FXPAR [2], wc_where [1], wc_where [2]
CALLED BY
mk_rmf_hdr, wrt_ebounds_ext
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Project : HESSI
Name : ADD_METHOD
Purpose : Dynamically add a method to a class (and it's objects)
Category : utility objects
Explanation : Based on method name (e.g. CLONE), looks for a class
definition file (e.g. CLONE__DEFINE.PRO). It then makes a
temporary copy of this file, and replaces all instances
of CLASS::METHOD with OBJ::METHOD where OBJ is the
class name that you want to add METHOD to. It then
compiles this temporary file.
Syntax : IDL> add_method,method,object
CALLED BY:
CHAN_DEFINE, HTTP__DEFINE, MAP__DEFINE, PLOT_MAP_DEFINE, XYPLOT__DEFINE, plotman
Examples : IDL> add_method,'clone',map_object
or
IDL> add_method,'gen::getprop',map_object
Inputs : METHOD = string method name
: OBJECT = object reference (or class name)
Outputs : None
Keywords : ERR = error string
VERBOSE = set for output messages
Restrictions: METHOD must have a METHOD__DEFINE.PRO in !path
If user enters method such as, for example, GEN::GETPROP
the method name is the part after the ::
If :: is not present, then the input is assumed to be a
class and all it's methods are added.
Added method(s) will only apply during current IDL session
CALLS: ***
APPEND_ARR, ARR2STR [1], Arr2Str [2], BREAK_FILE [1], BREAK_FILE [2]
BREAK_FILE [3], EXIST, GET_TEMP_DIR, HAVE_PROC, IS_METHOD_ADDED, MK_TEMP_FILE
OBJ_COMPILE, PR_SYNTAX, RD_ASCII [1], RD_ASCII [2], TRIM, VALID_CLASS
break_file [4], file_append [1], file_append [2], get_uniq, str_replace [1]
str_replace [2]
Side Effects: New method will override existing method of target object
History : Written: 9 July 2000, D. Zarro (EIT/GSFC)
Modified: 24 August 2000, Zarro (EIT/GSFC) - vectorized
Modified: 3 Sept 2001, Zarro (EITI/GSFC) - added option
to add specific method via: class::method_name
Modified: 4 May 2002, Zarro (EER/GSFC) - switched to
using CD instead of adding temporary path when using
RESOLVE_ROUTINE. IDL 6.0 has a problem with this.
Contact : dzarro@solar.stanford.edu
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PROJECT:
SOHO - CDS
NAME:
ADD_PATH
PURPOSE:
Add directory (and optionally all its subdirs) into IDL path
CALLING SEQUENCE:
ADD_PATH, path_name [,/append] [,index=index]
INPUTS:
path_name -- A string scalar of a valid directory name.
OPTIONAL INPUTS:
INDEX -- Position in the !path where the directory name is inserted;
ignored if the keyword APPEND is set.
OUTPUTS:
None, but !path is changed.
OPTIONAL OUTPUTS:
None.
KEYWORD PARAMETERS:
APPEND -- By default, the given directory name is added in the
beginning of !path. Set this keyword will add the directory
name in the end of !path.
EXPAND -- Set this keyword if the PATH_NAME needs to be expanded.
SORT_PATH -- sort added path alphabetically
CATEGORY:
Utilities, OS
PREVIOUS HISTORY:
Written October 8, 1994, by Liyun Wang, GSFC/ARC
CALLS: ***
ARR2STR [1], Arr2Str [2], CHK_DIR [1], CHK_DIR [2], CONCAT_DIR [1], CONCAT_DIR [2]
CONCAT_DIR [3], DATATYPE [1], DATATYPE [2], DATATYPE [3], STR_SEP, concat_dir [4]
CALLED BY:
DO_EIT_SCALING, EIT__DEFINE, GET_GEV, GET_NAR, HSI_LIGHTCURVE_TEST, HXRS__DEFINE
ITOOL_RD_FITS, LOAD_EIT_COLOR, LOAD_PATH, READ_EIT_FILE, SPECPLOT__DEFINE
hessi_version
MODIFICATION HISTORY:
Version 2, Liyun Wang, GSFC/ARC, October 17, 1994
Added EXPAND keyword
Version 3, William Thompson, GSFC, 29 August 1995
Modified to use OS_FAMILY
Version 4, Zarro (EITI/GSFC), 20 Jan 2002, added /QUIET
25-May-2002, Zarro (EITI/GSFC) - added /SORT_PATH and cleaned up
18-Feb-2004, Zarro (L-3Com/GSFC) - added calls to LOCAL_NAME and
GET_PATH_DELIM
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Project : SOHO-CDS
Name : ADD_PROP
Purpose : Add a property to a map object
Category : imaging
Explanation :
Syntax : add_prop,map,property=value
CALLED BY:
DIFF_MAP, DROT_RASTER, HESSI IMAGE STRATEGY CLASS DEFINITION, HSI_FITS2MAP [1]
INDEX2MAP, MK_EIT_MAP, hsi_image__getaxis [2]
Examples : add_prop,map,units='arcsecs'
Inputs : MAP = map structure
PROPERTY = property name
VALUE = property value
REPLACE = set to replace with new value if property exists
Opt. Inputs : None
Outputs : MAP = new map with property added
Opt. Outputs:
Keywords : See inputs
CALLS: ***
DATATYPE [1], DATATYPE [2], DATATYPE [3], JOIN_STRUCT [1], JOIN_STRUCT [2]
PR_SYNTAX, REP_PROP, VALID_MAP
Common : None
Restrictions: Cannot have two properties with same name
Side effects: None
History : Written 18 March 1998, D. Zarro, SAC/GSFC
Contact : dzarro@solar.stanford.edu
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Project : SOHO - CDS
Name : ADD_PSYS
Purpose : Add plotting system variables
Category : utility
Syntax : IDL> add_sys
Inputs : None
Outputs : None
CALLS: ***
DEVICELIB [1], DEVICELIB [2], IMAGELIB, UITDBLIB [1], UITDBLIB [2]
CALLED BY:
EIS_IMAGE_TOOL [1], EIS_IMAGE_TOOL [2], IMAGE_TOOL
Side Effects: !device, !image, etc defined
History : 6-May-2004, D. Zarro (L-3Con/GSFC). Written
Contact : DZARRO@SOLAR.STANFORD.EDU
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Project : SDAC
Name : ADD_TAG
Purpose : add a tag to a structure
Use : NEW_STRUCT=ADD_TAG(STRUCT,TAG,TAG_NAME)
Inputs : STRUCT = input structure (array or scalar)
: TAG_VALUE = tag variable to add
: TAG_NAME = tag name
Outputs : NEW_STRUCT = new structure
Keywords : NAME = new name for structure
INDEX = index or tag name where to append new tag [def = last]
ERR = error message [blank if ok]
DUPLICATE = set to allow duplicate tag names
TOP_LEVEL = If set, then only the top level is searched to
determine if the tag already exists.
NO_COPY = do not make copy of input TAG variable
(it will be destroyed after input)
NO_PAIR = if adding an array to a structure array, then
add_tag will pair each array element with the
corresponding structure array element. Setting
/NO_PAIR disables this behavior and will add the
entire array to each structure array element.
CALLS: ***
ADD_TAG2, ADD_TAG_ERR, ERR_STATE, EXIST, HAVE_PROC, IDL_RELEASE, IS_STRING, LAST_ITEM
PR_SYNTAX, REPLICATE2, SINCE_VERSION [1], SINCE_VERSION [2], STRUP, TAG_EXIST [1]
TAG_EXIST [2], is_struct
CALLED BY:
BBSO__DEFINE, BOOST_TAG, CH_READ_FITS, CIV_SUBTRACT, COORD_ADDINDEX, CWF_STATUS
DEF_CDS_DETAIL, DEF_CDS_STUDY, DROT_MAP, DROT_MAP_FAST, EIS_RASTER_BROWSER [1]
EIT__DEFINE, FITS WRITER CLASS FOR ANY RHESSI DATA TYPES
FITSFILE__DEFINE [2], FIT_CDS_MAP, GEN__DEFINE, GET_CDS_STUDY, GET_NAR
GET_UDP_HEAD, GOES__DEFINE, HEAD2STC, HESSI BINNED EVENTLIST CLASS DEFINITION
HESSI IMAGE RAW CLASS DEFINITION [2]
HESSI IMAGE STRATEGY CLASS DEFINITION
HESSI IMAGING ALGORITHM ABSTRACT CLASS DEFINITION
HESSI PARAMETER SELECTION TOOL [1], HSI_EVENTLIST_TO_SPECTROGRAM [1]
HSI_SPECTROGRAMACCBIN [5], HSI_SPECTROGRAMCHAN_OVERLAP_FIX
HSI_SPECTROGRAM_DECIM_CORRECT, HSI_SPECTROGRAM_DECIM_TABLE
HSI_SPECTRUM__DEFINE, KPNO__DEFINE, Load_Main [1], Load_Main [2]
MAKE_CHIANTI_SPEC, MAP2WCS, MAP__DEFINE, MDI__DEFINE, MK_CDS_STUDY, MK_HELP_STC
MK_NEW_MAP, MK_OLD_MAP, MK_POINT_STC, NANCAY__DEFINE, NIS_ROTATE, NORH_FIXINDEX
PLOT_MAP, PLOT_MAP2 WARNINGTEMPORARY FIX ONLY FOR 16 bit ZBuffer support
RD_GOES, RD_RESOURCE, READ_NRH, REP_TAG_NAME, REP_TAG_VALUE, ROT_MAP, SHOW_RES_STC
SHOW_SYNOP__DEFINE, SPECTROGRAM CLASS DEFINITION, SPECTRUM CLASS DEFINITION
SPEX_DATA_OUT [1], SPEX_DATA_OUT [2], SPEX_GEN__DEFINE, SPEX__DEFINE, SPLIT_TAGS
ST_SUMER, TR_DARK_SUB, UPDATE_CAMPAIGN, UPDATE_KAP, WCS_DECOMP_ANGLE
WCS_FIND_PIXEL_LIST, WCS_FIND_POSITION, WCS_FIND_SPECTRUM, WCS_FIND_TABLE
WCS_FIND_TIME, WCS_RECTIFY, WCS_SIMPLE, XYPLOT__DEFINE, XZOOM_PLAN, ZHOVER, ch_ss
eis_raster_browser [2], fit_comp_kw, fitshead2struct, get_gevloc_data
hsi_clean_options, hsi_flarelistdata_ext__define, hsi_image__getaxis [2]
hsi_image_fitsread, hsi_params_2_top_struct, hsi_select_by_coincidence
hsi_show_flags [2], hsi_spectrogramACCBIN [2], hsi_spectrogram__define [1]
hsi_spectrogram__define [2], hsi_spectrogram__define [3]
hsi_spectrogram__get_obs [1], hsi_spectrogram__livetime [1], hsi_ui_img
hsi_ui_spec, make_grid_sphere, make_mirror, mdi_write_genxcat, mk_sxh, plotman, ptim
read_trace, setssw_windows, spectrogram__define, spex_bk__define
spex_bksub__define, spex_convert_results [1], spex_convert_results [2]
spex_data__define, ssw_kyoto2dst, str_key, str_sub2top, str_top2sub
sxt_cba2os1 [1], sxt_cba2os1 [2], sxt_mornint, trace_last_movie [1]
trace_last_movie [3], trace_scale, trace_special_movie [1]
trace_special_movie [2], trace_special_movie [3], trace_special_movie2
wrt_fits_bin_exten [2], wrt_rate_ext, xpickfile, xpickfile2
Restrictions: Cannot add more than one tag at a time
Category : Structure handling
Written : Dominic Zarro (ARC)
Version : Version 1, 7 November 1994 -- written
Version 2, 16 June 1996 -- cleaned up
Version 3, 11-Aug-1997, William Thompson, GSFC
Added keyword TOP_LEVEL
Version 4, 8-Oct-1998, Zarro (SMA/GSFC) - converted to using
CREATE_STRUCT
Version 5, 24-Dec-2004, Zarro (L-3Com/GSFC) - vectorized
01-Feb-05, Csillaghy (Univ. Applied Sciences NW Switzerland)
- changed n_elements( struct ) to size(struct /dim ), see at the end.
02-Nov-2005, Kim Tolbert - Previously only handled 1-D structure in
the pairing mode. Now if structure is > 1-D, and last
dimension matches last dimension of tag_value, then add_tag will
place each tag_value in the corresponding structure element, unless
no_pair is set.
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Project : SDAC
Name : ADD_TAG
Purpose : add a tag to a structure
Use : NEW_STRUCT=ADD_TAG(STRUCT,TAG,TAG_NAME)
Inputs : STRUCT = input structure (array or scalar)
: TAG_VALUE = tag variable to add
: TAG_NAME = tag name
Outputs : NEW_STRUCT = new structure
Opt. Outputs: None.
Keywords : NAME = new name for structure
INDEX = index or tag name where to append new tag [def = last]
ERR = error message [blank if ok]
DUPLICATE = set to allow duplicate tag names
TOP_LEVEL = If set, then only the top level is searched to
determine if the tag already exists.
NO_COPY = do not make copy of input TAG variable
(it will be destroyed after input)
CALLS: ***
ADD_TAG2, ADD_TAG_ERR, DATATYPE [1], DATATYPE [2], DATATYPE [3], DELVARX [1]
DELVARX [2], DELVARX [3], DELVARX [4], EXIST, IDL_RELEASE, MERGE_STRUCT
SPLIT_STRUCT, TAG_EXIST [1], TAG_EXIST [2], TRIM, delvarx [5]
CALLED BY:
BBSO__DEFINE, BOOST_TAG, CH_READ_FITS, CIV_SUBTRACT, COORD_ADDINDEX, CWF_STATUS
DEF_CDS_DETAIL, DEF_CDS_STUDY, DROT_MAP, DROT_MAP_FAST, EIS_RASTER_BROWSER [1]
EIT__DEFINE, FITS WRITER CLASS FOR ANY RHESSI DATA TYPES
FITSFILE__DEFINE [2], FIT_CDS_MAP, GEN__DEFINE, GET_CDS_STUDY, GET_NAR
GET_UDP_HEAD, GOES__DEFINE, HEAD2STC, HESSI BINNED EVENTLIST CLASS DEFINITION
HESSI IMAGE RAW CLASS DEFINITION [2]
HESSI IMAGE STRATEGY CLASS DEFINITION
HESSI IMAGING ALGORITHM ABSTRACT CLASS DEFINITION
HESSI PARAMETER SELECTION TOOL [1], HSI_EVENTLIST_TO_SPECTROGRAM [1]
HSI_SPECTROGRAMACCBIN [5], HSI_SPECTROGRAMCHAN_OVERLAP_FIX
HSI_SPECTROGRAM_DECIM_CORRECT, HSI_SPECTROGRAM_DECIM_TABLE
HSI_SPECTRUM__DEFINE, KPNO__DEFINE, Load_Main [1], Load_Main [2]
MAKE_CHIANTI_SPEC, MAP2WCS, MAP__DEFINE, MDI__DEFINE, MK_CDS_STUDY, MK_HELP_STC
MK_NEW_MAP, MK_OLD_MAP, MK_POINT_STC, NANCAY__DEFINE, NIS_ROTATE, NORH_FIXINDEX
PLOT_MAP, PLOT_MAP2 WARNINGTEMPORARY FIX ONLY FOR 16 bit ZBuffer support
RD_GOES, RD_RESOURCE, READ_NRH, REP_TAG_NAME, REP_TAG_VALUE, ROT_MAP, SHOW_RES_STC
SHOW_SYNOP__DEFINE, SPECTROGRAM CLASS DEFINITION, SPECTRUM CLASS DEFINITION
SPEX_DATA_OUT [1], SPEX_DATA_OUT [2], SPEX_GEN__DEFINE, SPEX__DEFINE, SPLIT_TAGS
ST_SUMER, TR_DARK_SUB, UPDATE_CAMPAIGN, UPDATE_KAP, WCS_DECOMP_ANGLE
WCS_FIND_PIXEL_LIST, WCS_FIND_POSITION, WCS_FIND_SPECTRUM, WCS_FIND_TABLE
WCS_FIND_TIME, WCS_RECTIFY, WCS_SIMPLE, XYPLOT__DEFINE, XZOOM_PLAN, ZHOVER, ch_ss
eis_raster_browser [2], fit_comp_kw, fitshead2struct, get_gevloc_data
hsi_clean_options, hsi_flarelistdata_ext__define, hsi_image__getaxis [2]
hsi_image_fitsread, hsi_params_2_top_struct, hsi_select_by_coincidence
hsi_show_flags [2], hsi_spectrogramACCBIN [2], hsi_spectrogram__define [1]
hsi_spectrogram__define [2], hsi_spectrogram__define [3]
hsi_spectrogram__get_obs [1], hsi_spectrogram__livetime [1], hsi_ui_img
hsi_ui_spec, make_grid_sphere, make_mirror, mdi_write_genxcat, mk_sxh, plotman, ptim
read_trace, setssw_windows, spectrogram__define, spex_bk__define
spex_bksub__define, spex_convert_results [1], spex_convert_results [2]
spex_data__define, ssw_kyoto2dst, str_key, str_sub2top, str_top2sub
sxt_cba2os1 [1], sxt_cba2os1 [2], sxt_mornint, trace_last_movie [1]
trace_last_movie [3], trace_scale, trace_special_movie [1]
trace_special_movie [2], trace_special_movie [3], trace_special_movie2
wrt_fits_bin_exten [2], wrt_rate_ext, xpickfile, xpickfile2
Restrictions: Cannot add more than one tag at a time
Category : Structure handling
Written : Dominic Zarro (ARC)
Version : Version 1.0, 7 November 1994 -- written
Version 2.0, 16 June 1996 -- cleaned up
Version 3, 11-Aug-1997, William Thompson, GSFC
Added keyword TOP_LEVEL
Version 4 8-Oct-1998, Zarro (SMA/GSFC) - converted to using
CREATE_STRUCT
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Name:
ADDTIME
Purpose:
If optional keyword delta_min is supplied, then add a offset in
decimal minutes to an external time (H,M,S,MS,D,M,Y).
If optional keyword difference is supplied, return the difference
as Value = [A] - [B], where Value will be minutes (floating).
Inputs:
A = Base time, any format.
Calling Sequence:
Result = addtime(A,delta_min=delta_min) ; Result is [h,m,s,ms,d,m,y]
Result = addtime(A,difference=B) ; Result is minutes (float)
Result = addtime(A,difference=B,/sec) ; Result is seconds (float)
Outputs:
Function returns New time time, if delta_min keyword is provided.
Function returns difference of A-B, if B keyword is provied.
OPTIONAL INPUT KEYWORDS:
delta_min Decimal minutes (positive or negative) to add to A.
If /secs is set, this should be in secs.
B 2nd time to subtract from A in any format.
secs If set, return the result in seconds with diff=keyword
If set, the input delta should be specified in secs
CALLS: ***
Ex2Int [1], Ex2Int [2], Int2Ex [1], Int2Ex [2], anytim2ex [1], anytim2ex [2]
CALLED BY:
ACOPY [1], ANAL_BCS_PHA, ANAL_STIMS, BCS_SPMOVIE [1], BCS_SPMOVIE [2]
COVER_PAGE [1], COVER_PAGE [2], DR, DSN_DMP_FINDER, DSN_FINAL, FIND_CAL [1]
FIND_CAL [2], GET_TRANGE, MK_HXI_MAP, MK_ORB_WEEK, OBS_EVENT, OBS_PLOT
OP_ADD_SPECIAL, PLOT_HXT, SXT_POWL, Sxt_goes_teem, TRACE_SSWHERE [1]
UPDATE_SXT_CO_INDEX, WOBS_PLOT, XMOVIE_SFM, any_decay_time, any_fsp, anyrts
auto_bck_find, bck_interp, choose_interval, contact_sum, contacts [1]
contacts [2], copy_visible, diskbench, dsn_input, fidrange [1], fidrange [2]
fmt_pass, fmt_rasm, get_dn_rate [1], get_dn_rate [2], getm1ans
go_lasdisk golaserdisk, go_lasdisk2 golaserdisk, go_nvs5, goes_plot [1]
goes_plot [2], goes_plot [3], goes_plot [4], goes_plot [5], hxt_images2ps
hxt_utplot, interp_arr [1], interp_arr [2], interp_arr [3], last_lc, launch [1]
launch [2], make_32 [1], make_32 [2], mk_orbit_files, mk_orbit_sum, mult_th_fsp
op_bdr_opt, op_edit [1], op_edit [2], op_get_event [1], op_get_event [2]
op_pass_sheets [1], op_pass_sheets [2], op_saa_med [1], op_saa_med [2]
op_same_time [1], op_same_time [2], op_term_score, op_terminator [1]
op_terminator [2], op_time_sort, op_times, pass_sheets, plot_ar_pfi, plot_fov [1]
plot_nar [1], plot_nar [2], plot_ssw_fov, pr_maxmin_hk, rdtbl, run_dsnfil
save_event [1], save_event [2], sft_files, sgt_time, sxt_anycomp, sxt_dn_int
sxt_mwave, sxt_resp_inp, sxt_t6_resp0, tim2tfss, tim_bin, time_interp
trace_sswhere [2], trace_sswhere [3], trace_sswhere [4], valid_pass, valid_pass2
valid_pass3, valid_pass4 [1], valid_pass4 [2], ycopy, ydump
Procedure:
Calls ex2int and int2ex to do the calculations.
MODIFICATION HISTORY:
15-oct-91, Written, JRL
26-oct-91, Update, JRL - To handle hrs > 24 case
22-jun-92, Update, JRL - eliminate the 24:00 hour case
11-sep-92, Update, JRL - Call anytim2ex to convert input to external.
27-jul-94, JRL - Return the result in secs (with massive help from JMM!)
6-Mar-95, JRL - Improved logic so delta=<large numbers> doesn't overflow
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Project : SOHO - CDS
Name :
ADJUST()
Purpose :
Adjust the range of an image.
Explanation :
Adjusts the range of an image. Basically equivalent to using the
">" and "<" operators, except that pixels equal to MISSING are ignored
and not changed by this procedure.
Use :
Result = ADJUST( ARRAY, <keywords> )
Inputs :
ARRAY = Array to be scaled.
Opt. Inputs :
None.
Outputs :
Result of function is scaled image.
Opt. Outputs:
None.
Keywords :
MINIMUM = Lower limit to scale image into. If not passed, then
MIN(ARRAY) is assumed.
MAXIMUM = Upper limit to scale image into. If not passed, then
MAX(ARRAY) is assumed.
MISSING = Value flagging missing pixels.
Calls : ***
GET_IM_KEYWORD, GOOD_PIXELS
Common :
None.
Restrictions:
In general, the SERTS image display routines use several non-standard
system variables. These system variables are defined in the procedure
IMAGELIB. It is suggested that the command IMAGELIB be placed in the
user's IDL_STARTUP file.
Some routines also require the SERTS graphics devices software,
generally found in a parallel directory at the site where this software
was obtained. Those routines have their own special system variables.
Side effects:
None.
Category :
Utilities, Image_display.
Prev. Hist. :
William Thompson, March 1991.
William Thompson, August 1992, renamed BADPIXEL to MISSING.
Written :
William Thompson, GSFC, March 1991.
Modified :
Version 1, William Thompson, GSFC, 14 May 1993.
Incorporated into CDS library.
Version 2, 11-May-2005, William Thompson, GSFC
Handle NaN values
Version :
Version 2, 11-May-2005
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Project : SOHO - CDS
Name :
ADJUST_COLOR
Purpose :
Adjust the color table with the cursor.
Explanation :
Use the graphics cursor to control the lower limit and range of the
color tables.
Cursor is repeatedly sampled. X position is the lower limit (e.g.
cutoff). Y position controls range of color table. Initially, the
cutoff is set to 0 and the range is 255 with the cursor at the upper
left corner. When any key is struck the lower limit and range are
printed and the procedure is exited.
Use :
ADJUST_COLOR [, R,G,B ]
Inputs :
None required.
Opt. Inputs :
R = Red color gun vector, 256 elements, 0 to 255.
(usually read from device)
G = Green color gun vector.
B = Blue color gun vector.
Outputs :
None.
Opt. Outputs:
None.
Keywords :
DISABLE = If passed, then TVSELECT is not used.
NOCURSOR = If passed, then TVCRS is not called. TVCRS is not called
for Tektronix terminals in any case.
Calls : ***
TVSELECT, TVUNSELECT
Common :
If the parameters are omitted, the color vectors are read using
TVLCT,/GET. Regardless of the number of parameters, the colors in
common are not changed.
Restrictions:
In general, the SERTS image display routines use several non-standard
system variables. These system variables are defined in the procedure
IMAGELIB. It is suggested that the command IMAGELIB be placed in the
user's IDL_STARTUP file.
Some routines also require the SERTS graphics devices software,
generally found in a parallel directory at the site where this software
was obtained. Those routines have their own special system variables.
Side effects:
None.
Category :
Utilities, Image_display.
Prev. Hist. :
DMS, JULY, 1982. Written.
WTT, AUGUST, 1990. Ported to version 2 for non-windowed devices.
William Thompson, April 1992, changed to use TVLCT,/GET instead of
common block.
Written :
David M. Stern, RSI, July 1982.
Modified :
Version 1, William Thompson, GSFC, 14 May 1993.
Incorporated into CDS library.
Version 2, William Thompson, GSFC, 8 April 1998
Changed !D.N_COLORS to !D.TABLE_SIZE for 24-bit displays
Version :
Version 2, 8 April 1998
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Name: adjust_times
Purpose: check input times and adjust if required
Input Parameters:
t0 - start time - any Yohkoh format
t1 - stop time
Output Parameters:
t0 - start time (adjusted) ; output is always Yohkoh string format
t1 - stop time (adjusted)
Keyword Parameters
maxdays - if set, maximum number of days allowed (t1-t0)
timerange - 2 element vector; force times to fall in this range
earliest - same as timerange(0)
latest - same as timerange(1)
status (output) - true (1) if no problems, false (0) if problems/adjust.
deltat (output) - delta Time (seconds between final output times)
CALLS: ***
anytim2ints [1], anytim2ints [2], fmt_tim [1], fmt_tim [2], int2secarr [1]
int2secarr [2], timegrid, ut_time [1], ut_time [2]
History:
28-sep-1995 (S.L.Freeland) to simplify checking WWW form times
Warning - input times may be clobbered (I mean adjusted)
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NAME:
ADSTRING
PURPOSE:
Return RA and Dec as character string(s) in sexigesimal format.
EXPLANATION:
RA and Dec may be entered as either a 2 element vector or as
two separate vectors (or scalars). One can also specify the precision
of the declination in digits after the decimal point.
CALLING SEQUENCE
result = ADSTRING( ra_dec, precision, /TRUNCATE )
or
result = ADSTRING( ra,dec,[ precision, /TRUNCATE ] )
INPUTS:
RA_DEC - 2 element vector giving the Right Ascension and declination
in decimal degrees.
or
RA - Right ascension in decimal degrees, numeric scalar or vector
DEC - Declination in decimal degrees, numeric scalar or vector
OPTIONAL INPUT:
PRECISION - Integer scalar (0-4) giving the number of digits after the
decimal of DEClination. The RA is automatically 1 digit more.
This parameter may either be the third parameter after RA,DEC
or the second parameter after [RA,DEC]. It is not available
for just DEC. If no PRECISION parameter is passed, a
precision of 1 for both RA and DEC is returned to maintain
compatibility with past ADSTRING functions. Values of
precision larger than 4 will be truncated to 4. If
PRECISION is 3 or 4, then RA and Dec should be input as
double precision.
OPTIONAL INPUT KEYWORD:
/TRUNCATE - if set, then the last displayed digit in the output is
truncated in precision rather than rounded. This option is
useful if ADSTRING() is used to form an official IAU name
(see http://vizier.u-strasbg.fr/Dic/iau-spec.htx )with
coordinate specification. The IAU name will typically be
be created by applying STRCOMPRESS/REMOVE) after the ADSTRING()
call, e.g.
strcompress( adstring(ra,dec,0,/truncate), /remove) ;IAU format
OUTPUT:
RESULT - Character string(s) containing HR,MIN,SEC,DEC,MIN,SEC formatted
as ( 2I3,F5.(p+1),2I3,F4.p ) where p is the PRECISION
parameter. If only a single scalar is supplied it is
converted to a sexigesimal string (2I3,F5.1).
CALLS: ***
RADEC, SIXTY
CALLED BY:
ADXY, ASTDISP, ASTRO, CURVAL, EQ2HOR, HOR2EQ, IMCONTOUR, PRECESS, TVLASER
EXAMPLE:
(1) Display CRVAL coordinates in a FITS header, H
IDL> crval = sxpar(h,'CRVAL*') ;Extract 2 element CRVAL vector (degs)
IDL> print, adstring(crval) ;Print CRVAL vector sexigesimal format
(2) print,adstring(30.42,-1.23,1) ==> ' 02 01 40.80 -01 13 48.0'
print,adstring(30.42,+0.23) ==> ' 02 01 40.8 +00 13 48.0'
print,adstring(+0.23) ==> '+00 13 48.0'
(3) The first two calls in (2) can be combined in a single call using
vector input
print,adstring([30.42,30.42],[-1.23,0.23], 1)
PROCEDURES CALLED:
RADEC, SIXTY()
REVISION HISTORY:
Written W. Landsman June 1988
Addition of variable precision and DEC seconds precision fix.
ver. Aug. 1990 [E. Deutsch]
Output formatting spiffed up October 1991 [W. Landsman]
Remove ZPARCHECK call, accept 1 element vector April 1992 [W. Landsman]
Call ROUND() instead of NINT() February 1996 [W. Landsman]
Check roundoff past 60s October 1997 [W. Landsman]
Work for Precision =4 November 1997 [W. Landsman]
Converted to IDL V5.0 W. Landsman 24-Nov-1997
Major rewrite to allow vector inputs W. Landsman February 2000
Fix possible error in seconds display when Precision=0
P. Broos/W. Landsman April 2002
Added /TRUNCATE keyword, put leading zeros in seconds display
P. Broos/W. Landsman September 2002
Fix declination zero values under vector processing W.Landsman Feb 2004
Fix possible problem in leading zero display W. Landsman June 2004
Assume since V5.4, omit fstring() call W. Landsman April 2006
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NAME:
ADXY
PURPOSE:
Use a FITS header to convert astronomical to pixel coordinates
EXPLANATION:
Use an image header to compute X and Y positions, given the
RA and Dec (or longitude, latitude) in decimal degrees.
CALLING SEQUENCE:
ADXY, HDR ;Prompt for Ra and DEC
ADXY, hdr, a, d, x, y, [ /PRINT, ALT= ]
INPUTS:
HDR - FITS Image header containing astrometry parameters
OPTIONAL INPUTS:
A - Right ascension in decimal DEGREES, scalar or vector
D - Declination in decimal DEGREES, scalar or vector
If A and D are not supplied, user will be prompted to supply
them in either decimal degrees or HR,MIN,SEC,DEG,MN,SC format.
OPTIONAL OUTPUT:
X - row position in pixels, same number of elements as A and D
Y - column position in pixels
X and Y will be in standard IDL convention (first pixel is 0) and not
the FITS convention (first pixel is 1). As in FITS an integral
value corresponds to the center of a pixel.
CALLS: ***
AD2XY, ADSTRING, EXTAST, GETOPT, GSSSADXY, REPCHR [1], REPCHR [2], REPCHR [3], SXPAR [1]
SXPAR [2], SXPAR [3], TEN
OPTIONAL KEYWORD INPUT:
/PRINT - If this keyword is set and non-zero, then results are displayed
at the terminal.
ALT - single character 'A' through 'Z' or ' ' specifying an alternate
astrometry system present in the FITS header. The default is
to use the primary astrometry or ALT = ' '. If /ALT is set,
then this is equivalent to ALT = 'A'. See Section 3.3 of
Greisen & Calabretta (2002, A&A, 395, 1061) for information about
alternate astrometry keywords.
OPERATIONAL NOTES:
If less than 5 parameters are supplied, or if the /PRINT keyword is
set, then the X and Y positions are displayed at the terminal.
If the procedure is to be used repeatedly with the same header,
then it would be faster to use AD2XY.
PROCEDURES CALLED:
AD2XY, ADSTRING(), EXTAST, GETOPT(), TEN()
REVISION HISTORY:
W. Landsman HSTX January, 1988
Use astrometry structure W. Landsman January, 1994
Changed default ADSTRING format W. Landsman September, 1995
Converted to IDL V5.0 W. Landsman September 1997
Check if latitude/longitude reversed in CTYPE keyword W. L. Feb. 2004
Added ALT keyword W. Landsman September 2004
Work for non-spherical coordinate transformation W. Landsman May 2005
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NAME:
AFFINE
PURPOSE:
Apply the affine transformation given by the input parameters
to IMAGE.
CATEGORY:
Z3 - Image processing, geometric transforms, image registration.
CALLING SEQUENCE:
transformed_image = AFFINE(image,mx,my,sx,theta,xc,yc)
INPUTS:
IMAGE: The image to be transformed. Must be 2-D.
MX, MY: Magnification factors in x and y directions.
SX: Horizontal shear term.
THETA: Rotation angle in DEGREES. THETA > 0 => counterclockwise rotation.
XC, YC: Center of rotation.
KEYWORDS:
INTERP: Set this keyword for bilinear interpolation. If this keyword
is set to 0 or omitted, nearest neighbor sampling is used.
Note that setting this keyword is the same as using the
ROT_INT User Library function. This change (and others)
essentially makes ROT_INT obsolete.
CUBIC: If specified and non-zero, "Cubic convolution"
interpolation is used. This is a more
accurate, but more time-consuming, form of interpolation.
CUBIC has no effect when used with 3 dimensional arrays.
If this parameter is negative and non-zero, it specifies the
value of the cubic interpolation parameter as described
in the INTERPOLATE function. Valid ranges are -1 <= Cubic < 0.
Positive non-zero values of CUBIC (e.g. specifying /CUBIC)
produce the default value of the interpolation parameter
which is -1.0.
MISSING: The data value to substitute for pixels in the output image
that map outside the input image.
OUTPUTS:
NONE
RETURNS:
TIMAGE: the affine transformation of input image IMAGE.
COMMON BLOCKS:
None.
SIDE EFFECTS:
None.
RESTRICTIONS:
None.
PROCEDURE:
Uses POLY_2D to warp the input image according to the
given parameters.
See: Image Processing for Scientific Applications
Bernd J\"ahne
CRC Press, 1997, Chapter 8.
Same as ROT.PRO but includes shear term and /PIVOT is assumed.
MODIFICATION HISTORY:
T. Berger, LMATC, 26-February-1998.
S.L.Freeland, LMSAL, 10-March-1998 - backward compatible IDV V < 5
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NAME:
AFFINE_SOLVE
PURPOSE:
Calculate the parameters of a general affine image
transformation given a set of points from two images:
one of the images is assumed to be the reference image,
the other is assumed to be an image translated, rotated,
scaled, and possibly sheared relative to the reference image.
The form of the general transformation is affine:
X = tranformed coordinates = [T+ M S R T-] X'
where, in homogeneous coordinates,
X = TRANSPOSE[x, y, 1]: test image vector
T+ = [[1,0,x0],[0,1,y0],[0,0,1]]: translatation of (0,0) back to (x0,y0)
M = [[mx,0,0],[0,my,0],[0,0,1]]:scale
S = [[1,sx,0],[0,1,0],[0,0,1]]: horizontal shear
R = [[cos(t),-sin(t),0],[sin(t),cos(t),0],[0,0,1]]:
rotate clockwise by angle t about origin.
T- = [[1,0,-x0],[0,1,-y0],[0,0,1]]:center of rotation to (0,0)
X' = TRANSPOSE[x',y',1]: reference image vector
CATEGORY:
Z3 - Image processing, geometric transforms, image registration.
CALLING SEQUENCE:
AFFINE_SOLVE, xin,xrefin,sx,sy,s,theta,x0,y0
INPUTS:
XIN: 2xN dimensional array of points taken from image1
which correspond to the same points in the reference image.
Xi = XIN(0,*)
Yi = XIN(1,*)
N is the number of points.
XPIN: 2xN dimensional array of points from the "reference image"
which correspond to points in the image.
KEYWORDS:
VERBOSE: If set, print the transformation elements to the screen.
OUTPUTS:
MX, MY: Magnification factors in x and y axes, respectively.
SX: Horizontal shearing factor.
THETA: Rotation angle in degrees.
XC,YC: Center of rotation vector elements OR translation
vector elements.
CALLED BY:
IMAGE_REGISTER
COMMON BLOCKS:
None.
SIDE EFFECTS:
None.
RESTRICTIONS:
N, the number of matched points in the transformed and reference
images should be large (greater than 20), should be taken from
widely spaced locations in the image field-of-view, and should
be measured to within 1-pixel for greatest accuracy.
Off-center rotation and translation require a two-stage approach
for image registration. i.e. in the first stage, apply the parameters
given by this routine to the test image. A second set of points
is then selected from the image and the reference image, and
a second run of this program should output a final translation
to be applied to the test image to bring it in registration with
the reference image. This is tested for and the user is alerted.
PROCEDURE:
Using least squares estimation, determine the elements
of the general affine transformation (rotation and/or scaling
and/or translation and/or shearing) of an image onto a reference
image.
See: Image Processing for Scientific Applications
Bernd J\"ahne
CRC Press, 1997, Chapter 8.
Use AFFINE.PRO (or ROT.PRO if no shear is found) to apply the
transformation to the test image after computing them with this routine.
MODIFICATION HISTORY:
Written: T. Berger, LMATC, 24-Feb-1998.
Added no rotation/translation test. TEB, 2-March-98.
10-March-1998 - S.L.Freeland - Backward compatible for IDL V<5
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NAME:
AIRTOVAC
PURPOSE:
Convert air wavelengths to vacuum wavelengths
EXPLANATION:
Wavelengths are corrected for the index of refraction of air under
standard conditions. Wavelength values below 2000 A will not be
altered. Uses the IAU standard for conversion given in Morton
(1991 Ap.J. Suppl. 77, 119)
CALLING SEQUENCE:
AIRTOVAC, WAVE
INPUT/OUTPUT:
WAVE - Wavelength in Angstroms, scalar or vector
WAVE should be input as air wavelength(s), it will be
returned as vacuum wavelength(s). WAVE is always converted to
double precision upon return.
EXAMPLE:
If the air wavelength is W = 6056.125 (a Krypton line), then
AIRTOVAC, W yields an vacuum wavelength of W = 6057.8019
METHOD:
See Morton (Ap. J. Suppl. 77, 119) for the formula used
REVISION HISTORY
Written W. Landsman November 1991
Converted to IDL V5.0 W. Landsman September 1997
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NAME:
AITOFF
PURPOSE:
Convert longitude, latitude to X,Y using an AITOFF projection.
EXPLANATION:
This procedure can be used to create an all-sky map in Galactic
coordinates with an equal-area Aitoff projection. Output map
coordinates are zero longitude centered.
CALLING SEQUENCE:
AITOFF, L, B, X, Y
INPUTS:
L - longitude - scalar or vector, in degrees
B - latitude - same number of elements as L, in degrees
OUTPUTS:
X - X coordinate, same number of elements as L. X is normalized to
be between -180 and 180
Y - Y coordinate, same number of elements as L. Y is normalized to
be between -90 and 90.
NOTES:
See AIPS memo No. 46, page 4, for details of the algorithm. This
version of AITOFF assumes the projection is centered at b=0 degrees.
REVISION HISTORY:
Written W.B. Landsman STX December 1989
Modified for Unix:
J. Bloch LANL SST-9 5/16/91 1.1
Converted to IDL V5.0 W. Landsman September 1997
CALLED BY
AITOFF_GRID, MASK_OFF, PE_GRID
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NAME:
AITOFF_GRID
PURPOSE:
Produce an overlay of latitude and longitude lines over a plot or image
EXPLANATION:
The grid is plotted on the current graphics device. AITOFF_GRID
assumes that the ouput plot coordinates span the x-range of
-180 to 180 and the y-range goes from -90 to 90.
CALLING SEQUENCE:
AITOFF_GRID [,DLONG,DLAT, LABEL=, /NEW, CHARTHICK=, CHARSIZE=,
FONT=, _EXTRA=]
OPTIONAL INPUTS:
DLONG = Optional input longitude line spacing in degrees. If left
out, defaults to 30.
DLAT = Optional input latitude line spacing in degrees. If left
out, defaults to 30.
OPTIONAL INPUT KEYWORDS:
LABEL = Optional keyword specifying that the latitude and
longitude lines on the prime meridian and the
equator should be labeled in degrees. If LABELS is
given a value of 2, i.e. LABELS=2, then the longitude
labels will be in hours instead of degrees.
CHARSIZE = If /LABEL is set, then CHARSIZE specifies the size
of the label characters (passed to XYOUTS)
CHARTHICK = If /LABEL is set, then CHARTHICK specifies the
thickness of the label characters (passed to XYOUTS)
FONT = scalar font graphics keyword (-1,0 or 1) for text
/NEW = If this keyword is set, then AITOFF_GRID will create
a new plot grid, rather than overlay an existing plot.
Any valid keyword to OPLOT such as COLOR, LINESTYLE, THICK can be
passed to AITOFF_GRID (though the _EXTRA facility) to to specify the
color, style, or thickness of the grid lines.
OUTPUTS:
Draws grid lines on current graphics device.
CALLS: ***
AITOFF
CALLED BY:
PE_GRID
EXAMPLE:
Create a labeled Aitoff grid of the Galaxy, and overlay stars at
specified Galactic longitudes, glong and latitudes, glat
IDL> aitoff_grid,/label,/new ;Create labeled grid
IDL> aitoff, glong, glat, x,y ;Convert to X,Y coordinates
IDL> plots,x,y,psym=2 ;Overlay "star" positions
PROCEDURES USED:
AITOFF
NOTES:
If labeling in hours (LABEL=2) then the longitude spacing should be
a multiple of 15 degrees
AUTHOR AND MODIFICATIONS:
J. Bloch 1.2 6/2/91
Converted to IDL V5.0 W. Landsman September 1997
Create default plotting coords, if needed W. Landsman August 2000
Added _EXTRA, CHARTHICK, CHARSIZE keywords W. Landsman March 2001
Several tweaks, plot only hours not minutes W. Landsman January 2002
Allow FONT keyword to be passed to XYOUTS. T. Robishaw Apr. 2006
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Name: align_cube_correl
Purpose: align a data cube via cross correlation; update coordinates
Input Parameters:
index - the header structures ; SSW standards w/pointing fields
data - the data cube
offsets - the derived offesets fltarr(2,nimage)
Calling Sequence:
align_cube_correl, index, incube, outindex, outcube ; header & cube
-OR- align_cube_correl, incube, outcube ; just cube?
-OR- align_cube_correl, inoutcube ; just cube?
History:
15-October-1998 - S.L.Freeland
Distillation based on review of SSW correlation/alignment SW by:
G.L.Slater (SXT..) get_off, cube-align, translate
J.P.Wuelser (SXT/MEES) korrel, poly_movie
T.Tarbell (TRACE) tr_get_disp
5-Feb-2003 - S.L.Freeland - assure all calling modes permitted
Proto type - When called with 'index' structures, will
adjust the 'pointing' standard tags to reflect alignement and
return in 'outindex'
CALLS: ***
BOX_MESSAGE, IMAGE_TRANSLATE, data_chk [1], data_chk [2], get_correl_offsets
Side Effects:
Called with one paramater, (input cube), the input is overwritten
by the aligned version (memory conservation, for example)
Method:
call get_correl_offsets to get the cross correlation offsets for cube
call image_translate to align the cube (via poly2d method)
Category:
2D , 3D, Image, Alignment, Cross Correlation
Restrictions:
update of coordinates not yet implemented
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Name: align_label
Purpose: meta-label (via xyouts) an image via relative positions/align
Input Parameters:
label - the text label
Output Parameters:
ddevx, devy - derived x and y position in device coord
sizex, sizey - width and heighth of LABEL in device coord
Keyword Parameters:
ur/ul/uc - upper right, upper left, upper center
lr/ll/lc - lower right, lower left, lower center
cr/cl/cc - center right, center left, center center
charsize / size (synonums) - desired label SIZE (per xyouts) def=1.0
pixpad / pad (synonyms) - number of pixels to 'pad'
info_only - if set, do not issue xyouts (return devx, devy...)
_extra - pass unknown keywords to xyouts via inherit.
Calling Examples:
IDL> align_label,'Label Text', /ur ; label upper right
IDL> align_label,'Label Text', /uc,pad=10 ; top center, 10 pix pad
IDL> align_label,'TEXT',/lr,color=100,size=2 ; lower right
; keywords->xyouts
CALLED BY:
ssw_find_transit
History:
17-Nov-1999 S.L.Freeland - integrate a couple of existing functions
size determination from xyouts/
CALLS: ***
BOX_MESSAGE, STR2ARR [1], STR2ARR [2], WDEF [1], WDEF [2], data_chk [1]
data_chk [2], str_subset
See Also:
Knight et al), label_image.pro (W.Thompson), legend.pro (Astronomy Lib
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NAME:
ALL_VALS
PURPOSE:
Find and sort unique values in an array
CATEGORY:
CALLING SEQUENCE:
out = all_vals(in)
INPUTS:
in any array
OPTIONAL INPUT PARAMETERS:
KEYWORD PARAMETERS:
OUTPUTS:
out sorted array of unique values
OPTIONAL OUTPUT PARAMETERS:
CALLS: ***
UNIQ [1], UNIQ [2], UNIQ [3]
CALLED BY:
ANAL_BCS_PHA, ANAL_STIMS, BCS_SPMOVIE [1], BCS_SPMOVIE [2], FIND_CAL [1]
FIND_CAL [2], GOOD_MAX [1], GOOD_MAX [2], MEMCHK_TIMES, OBS_PLOT, SUMM_CALS
SXT_TVEC, TRACE_SSWHERE [1], WBS_TVEC, ext_bcschan [1], ext_bcschan [2]
plot_fov [1], plot_goesp, plot_ssw_fov, plotbft [1], pr_plan_area [1]
pr_plan_area [2], read_trace, ssw_fs_cat2db, ssw_install [2], ssw_swmap_uniqinfo
trace_sswhere [2], trace_sswhere [3], trace_sswhere [4]
COMMON BLOCKS:
SIDE EFFECTS:
RESTRICTIONS:
PROCEDURE:
MODIFICATION HISTORY:
RDB Sep-98 Written, modelled on old library routine
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Project : HESSI
Name : ALLOW_FONT
Purpose : platform/OS independent check if current system
supports given font
Category : system utility
Syntax : IDL> a=allow_font()
Outputs : 1/0 if yes/no
CALLS: ***
ALLOW_WINDOWS, EXIST, IS_STRING, IS_WOPEN, OS_FAMILY, STRUP, WDEL
History : 14 May 2003, Zarro (EER/GSFC)
Contact : dzarro@solar.stanford.edu
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Project : HESSI
Name : ALLOW_GIF
Purpose : platform/OS independent check if current system
supports writing GIF files
Category : system utility
Syntax : IDL> a=allow_gif()
Outputs : 1/0 if yes/no
CALLS: ***
CLOSE_LUN, EXIST, GET_TEMP_DIR, MK_TEMP_FILE, WRITE_GIF, is_open
CALLED BY:
SSW_WRITE_GIF, WR_MOVIE, sxi_latest
History : 7 Apr 2003, Zarro (EER/GSFC)
Contact : dzarro@solar.stanford.edu
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Project : HESSI
Name : ALLOW_SOCKETS
Purpose : check if sockets are supported
Category : system utility sockets
Syntax : IDL> a=allow_sockets()
Outputs : 1/0 if yes/no
CALLS: ***
OS_FAMILY, XACK
CALLED BY:
GET_SOHO_ROLL, GOES__DEFINE, HSI_FIND_FILE, HTTP__DEFINE, SOCK_OPEN, SYNOP_DEFINE
History : 28 Mar 2002, Zarro (L-3Com/GSFC)
Contact : dzarro@solar.stanford.edu
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Project : HESSI
Name : ALLOW_WINDOWS
Purpose : platform/OS independent check if current device
allows windows
Category : system utility
Syntax : IDL> a=allow_windows()
Outputs : 1/0 if yes/no
CALLS: ***
HAVE_WIDGETS [1], HAVE_WIDGETS [2], HAVE_WINDOWS [1], HAVE_WINDOWS [2]
SINCE_VERSION [1], SINCE_VERSION [2]
CALLED BY:
ALLOW_FONT, CHAN_DEFINE, COLORSET, GET_XWIN [1], IS_WOPEN, OVSA_LTC_DEFINE
RDWRT_BUFF, SMART_WINDOW, SPECPLOT__DEFINE, XACK, XTEXT, get_xwin [2]
History : Version 1, 4-Nov-1999, Zarro (SM&A/GSFC)
13 Dec 2001, Zarro (EITI/GSFC) - added DEVICE call
22 Oct 2002, Zarro (EER/GSFC) - added FSTAT check
Contact : dzarro@solar.stanford.edu
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PROJECT:
SDAC
NAME:
ALPHA_PAGE
PURPOSE:
This procedure switches to alpha from graphics page under Tektronix.
CATEGORY:
GRAPHICS
CALLING SEQUENCE:
ALPHA_PAGE
INPUTS:
None
OUTPUTS:
None
CALLED BY:
CAL_SHER, FLDISPLAY, FSOC, FS_ARCHIVE_DRAW, FS_AUTO_LOG, FS_GRAPH, GET_TRIG
Intervals [1], Intervals [2], LOG_MENU, PAGE_PRINT, QLDISPLAY, RATESDUMPOC
RAWDUMPOC, SPEX_BACKGROUND [1], SPEX_BACKGROUND [2], SPEX_COMMONS [2]
SPEX_COMMONS [4], SPEX_PROC [1], SPEX_PROC [2], TYPE_FLARE, batse_menu
drm_4_spex [1], drm_4_spex [2], spec_plot [1], spec_plot [2], spec_plot [3]
spec_plot [4], spex_intervals [1], spex_intervals [2], spex_spec_plot [1]
spex_spec_plot [2], spex_spec_plot [3], spex_spec_plot [4]
SIDE EFFECTS:
Issues a carriage return if called.
RESTRICTIONS:
PROCEDURE:
A command string (string(24b)) is issued through print to switch the terminal
COMMON BLOCKS:
None.
MODIFICATION HISTORY:
Written by: AKT
Version 2: RAS, 23-Mar-1995, only called for Tektronix
Version 3, richard.schwartz@gsfc.nasa.gov, 7-sep-1997, more documentation
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Name: alphagen
Purpose: return array ['A', 'B', 'C'...] (sindgen with alpha)
Calling Sequence:
alpha=alphagen(10 [,/lower])
CALLED BY
where_title [1], where_title [2]
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NAME:
ALTAZ2HADEC
PURPOSE:
Convert Horizon (Alt-Az) coordinates to Hour Angle and Declination.
EXPLANATION::
Can deal with the NCP singularity. Intended mainly to be used by
program hor2eq.pro
CALLING SEQUENCE:
ALTAZ2HADEC, alt, az, lat, ha, dec
INPUTS
alt - the local apparent altitude, in DEGREES, scalar or vector
az - the local apparent azimuth, in DEGREES, scalar or vector,
measured EAST of NORTH!!! If you have measured azimuth west-of-south
(like the book MEEUS does), convert it to east of north via:
az = (az + 180) mod 360
lat - the local geodetic latitude, in DEGREES, scalar or vector.
OUTPUTS
ha - the local apparent hour angle, in DEGREES. The hour angle is the
time that right ascension of 0 hours crosses the local meridian.
It is unambiguously defined.
dec - the local apparent declination, in DEGREES.
CALLED BY:
HOR2EQ
EXAMPLE:
Arcturus is observed at an apparent altitude of 59d,05m,10s and an
azimuth (measured east of north) of 133d,18m,29s while at the
latitude of +43.07833 degrees.
What are the local hour angle and declination of this object?
IDL> altaz2hadec, ten(59,05,10), ten(133,18,29), 43.07833, ha, dec
===> Hour angle ha = 336.683 degrees
Declination, dec = 19.1824 degrees
The widely available XEPHEM code gets:
Hour Angle = 336.683
Declination = 19.1824
REVISION HISTORY:
Written Chris O'Dell Univ. of Wisconsin-Madison May 2002
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NAME:
AMEDIAN
PURPOSE:
Works the same as MEDIAN, but the effect tapers off at the edges.
CALLING SEQUENCE:
Result = AMEDIAN( ARRAY, WIDTH )
INPUT PARAMETERS:
ARRAY = One or two-dimensional array to be median filtered.
WIDTH = Width of the median filter box.
OPTIONAL KEYWORD PARAMETERS:
None.
CALLS: ***
REVERSE
CALLED BY:
GUESS_FIT_PAR
COMMON BLOCKS:
None.
SIDE EFFECTS:
None.
RESTRICTIONS:
ARRAY must be one or two-dimensional.
PROCEDURE:
A larger array is constructed with the border filled with the reflected
edges of the original array. Then MEDIAN is applied to this larger
array, and the area corresponding to the original array is returned as
the result of the function.
MODIFICATION HISTORY:
William Thompson, February 1993.
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Project : SOHO - CDS
Name : AMOEBA_C
Purpose : Reiteratively fits an arbitrary function
Explanation : Fits an arbitrary function to a series of data points via a
least-squares reiterative technique.
The procedure used is taken from Numerical Recipes.
Use : AMOEBA_C, X, Y, FNAME, PARAM
Inputs : X = Positions.
Y = Data values.
FNAME = Name of function to be fitted (string variable).
PARAM = Parameters of fit. Passed as first guess. Returned
as fitted values.
Opt. Inputs : None.
Outputs : PARAM = Parameters of fit. See note above.
Opt. Outputs: None.
Keywords :
ACCURACY = Accuracy to cut off at. Defaults to 1E-5.
MAX_ITER = Maximum number of reiterations. Defaults to 20.
POISSON = If set, then a Poisson error distribution is assumed, and
the weights are set accordingly to 1/Y.
ERROR = Array of errors. The weights are set accordingly to
1/ERROR^2 (normal distribution). Overrides POISSON.
LAMBDA = Initial step sizes for PARAM, or if scalar then fraction of
PARAM. Defaults to 1E-2. When passed as an array, this
parameter can be used to hold parameters constant by setting
LAMBDA(I)=0 for those parameters.
NOPRINT = If set, then no printout is generated.
CHISQR = Returned value of chi-squared. Only relevant if ERROR
passed explicitly.
N_ITER = Number of iterations used.
ABSOLUTE = If set, then the sum of the absolute differences is
minimized instead of the sum of the squares. This is
equivalent to assuming a double-sided exponential
distribution.
LORENTZ = If set, then a Lorentz distribution is used instead of a
normal distribution. Not truely meaningful unless ERROR is
passed.
PRANGE = Range of acceptable parameter values. Must have the
dimensions (NPAR,2), where PRANGE(*,0) are the minimum
values and PRANGE(*,1) are the maximum values. Only those
ranges where PRANGE(*,1) are larger than PRANGE(*,0) are
implemented--all other parameters are considered to be
unbounded.
Calls : ***
FORM_CHISQR, FORM_SIGMAS
CALLED BY:
CDS_LINEFIT_WRAP, DSPEXP, WCS_FIT_GRISM, hrts_w [1]
Common : None
Restrictions: The user defined function is passed by name as a character
string in the variable FNAME. The function must have the form.
Y = F(X,PARAM)
where X is the independent variable, and PARAM is the vector
containing the parameters of the fit.
Unless LAMBDA is passed as an array, if the initial guess for
PARAM contains any zeroes, then those parameters will be kept
constant at zero.
Side effects: The statistical interpretation of CHISQR is unclear if either
ABSOLUTE or LORENTZ is set.
Category : Utilities, Curve_Fitting
Prev. Hist. :
William Thompson, August, 1989.
William Thompson, June 1991, modified to use keywords.
William Thompson, December 1992, modified to use other fitting
strategies besides minimizing the root-mean-square. Also
removed keyword WEIGHTS as this was incompatible with this
strategy.
Written : William Thompson, GSFC, August 1989
Modified : Version 1, William Thompson, GSFC, 9 January 1995
Incorporated into CDS library
Version 2, William Thompson, GSFC, 6 October 1995
Fixed typo.
Version 3, William Thompson, GSFC, 10 December 1997
Renamed to AMOEBA_C to avoid conflict with IDL/v5
routine of the same name.
Version 4, William Thompson, GSFC, 05-Jun-1998
Fixed bug where LAMBDA was not being properly accepted
if a vector.
Version 5, William Thompson, GSFC, 27-Apr-1999
Added keyword PRANGE.
Version 6, William Thompson, GSFC, 04-May-1999
Allow for case where either PARAM or LAMBDA is set to
zero to keep a parameter constant.
Version 7, William Thompson, GSFC, 23-Dec-2005
Use CALL_FUNCTION instead of EXECUTE
Version : Version 7, 23-Dec-2005
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Project : SOHO - CDS
Name : AMOEBA_F
Purpose : Reiteratively minimizes an arbitrary function
Explanation : Minimizes an arbitrary function via a least-squares reiterative
technique.
The procedure used is taken from Numerical Recipes.
Use : AMOEBA_F, FNAME, PARAM
Inputs : FNAME = Name of function to be minimized (string variable).
PARAM = Parameters of fit. Passed as first guess. Returned
as fitted values.
Opt. Inputs : None.
Outputs : PARAM = Parameters of fit. See note above.
Opt. Outputs: None.
Keywords : ACCURACY = Accuracy to cut off at. Defaults to 1E-5.
MAX_ITER = Maximum number of reiterations. Defaults to 20.
LAMBDA = Initial step sizes for PARAM, or if scalar then
fraction of PARAM. Defaults to 1E-2.
NOPRINT = If set, then no printout is generated.
CHISQR = Returned value of chi-squared. Only relevant if
ERROR passed explicitly.
N_ITER = Number of iterations used.
Calls : None.
Common : None
Restrictions: The user defined function is passed by name as a character
string in the variable FNAME. The function must have the form.
Y = F(PARAM)
where PARAM is the vector containing the parameters of the fit.
Unless LAMBDA is passed as an array, the initial guess for
PARAM must not contain any zeroes.
Side effects: None.
Category : Utilities, Curve_Fitting
Prev. Hist. : William Thompson, August, 1989.
William Thompson, June 1991, modified to use keywords.
Written : William Thompson, GSFC, August 1989
Modified : Version 1, William Thompson, GSFC, 9 January 1995
Incorporated into CDS library
Version 2, William Thompson, GSFC, 6 October 1995
Fixed typo.
Version 3, William Thompson, GSFC, 05-Jun-1998
Fixed bug where LAMBDA was not being properly accepted
if a vector.
Version 4, William Thompson, GSFC, 23-Dec-2005
Use CALL_FUNCTION instead of EXECUTE
Version : Version 4, 23-Dec-2005
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NAME:
AMOEBAX
PURPOSE:
Multidimensional minimization of a function FUNC(X), where
X is an N-dimensional vector, using the downhill simplex
method of Nelder and Mead, 1965, Computer Journal, Vol 7, pp 308-313.
This routine is based on the AMOEBA routine, Numerical
Recipes in C: The Art of Scientific Computing (Second Edition), Page
411, and is used by permission.
Amoebax adds to the built in amoeba with a convergence
criterion on the location of the minimum in addition to the
value of the minimum.
CATEGORY:
Function minimization/maximization. Simplex method.
CALLING SEQUENCE:
Result = AMOEBAX(Ftol, Xtol, ....)
INPUTS:
FTOL: the fractional tolerance to be achieved in the function
value. e.g. the fractional decrease in the function value in the
terminating step. This should never be less than the
machine's single or double precision. Set ftol LE 0.0 to turn
this criterion off
XTOL: the tolerance in the function variables to be achieved,
i.e. the convergence criterion on the *location* of the minimum.
Set xtol LE 0.0 to turn this criterion off. If xtol LE 0,
amoebax behaves just like the built in amoeba. Do not set
both ftol and xtol LE 0.0 or the routine will exit
immediately without finding the minimum.
KEYWORD PARAMETERS:
FUNCTION_NAME: a string containing the name of the function to
be minimized. If omitted, the function FUNC is minimized.
This function must accept an Ndim vector as its only parameter and
return a scalar single or double precision floating point value as its
result.
FUNCTION_VALUE: (output) on exit, an Ndim+1 element vector
containing the function values at the simplex points. The first
element contains the function minimum.
NCALLS: (output) the of times the function was evaluated.
NMAX: the maximum number of function evaluations allowed
before terminating. Default = 5000.
P0: Initial starting point, an Ndim element vector. The starting
point must be specified using either the keyword SIMPLEX, or P0 and
SCALE. P0 may be either single or double precision floating.
For example, in a 3-dimensional problem, if the initial guess
is the point [0,0,0], and it is known that the function's
minimum value occurs in the interval: -10 <
X(0) < 10, -100 < X(1) < 100, -200 < X(2) < 200, specify: P0=[0,0,0],
SCALE=[10, 100, 200].
SCALE: a scalar or Ndim element vector contaiing the problem's
characteristic length scale for each dimension.
SCALE is used with P0 to form an initial (Ndim+1) point simplex.
If all dimensions have the same scale, specify a scalar.
SIMPLEX: (output and/or optional input) On input, if P0 and SCALE
are not set, SIMPLEX contains the Ndim+1 vertices, each of
Ndim elements, of starting simplex, in either single or double
precision floating point, in an (Ndim, Ndim+1) array. On output,
SIMPLEX contains the simplex, of dimensions (Ndim, Ndim+1), enclosing
the function minimum. The first point, Simplex(*,0), corresponds to
the function's minimum.
OUTPUTS:
Result: If the minimum is found, an Ndim vector, corresponding to
the Function's minimum value is returned. If a function minimum
within the given tolerance, is NOT found in the given number of
evaluations, a scalar value of -1 is returned.
CALLS: ***
AMOTRY
CALLED BY:
AUTO_ALIGN_IMAGES, STOKESFIT
COMMON BLOCKS:
None.
SIDE EFFECTS:
None.
PROCEDURE:
This procedure implements the Simplex method, described in
Numerical Recipes, Section 10.4. See also the POWELL procedure.
Advantages: requires only function evaluations, not
derivatives, may be more reliable than the POWELL method.
Disadvantages: not as efficient as Powell's method, and usually
requires more function evaluations.
Results are performed in the mode (single or double precision)
returned by the user-supplied function. The mode of the inputs P0,
SCALE, or SIMPLEX, should match that returned by the function. The
mode of the input vector supplied to the user-written function, is
determined by P0, SCALE, or SIMPLEX.
EXAMPLE:
Use Amoeba to find the slope and intercept of a straight line fitting
a given set of points minimizing the maximum error:
The function to be minimized returns the maximum error,
given p(0) = intercept, and p(1) = slope:
FUNCTION FUNC, p
COMMON FUNC_XY, x, y
RETURN, MAX(ABS(y - (p(0) + p(1) * x)))
END
Put the data points into a common block so they are accessible to the
function:
COMMON FUNC_XY, x, y
Define the data points:
x = findgen(17)*5
y = [ 12.0, 24.3, 39.6, 51.0, 66.5, 78.4, 92.7, 107.8, 120.0, $
135.5, 147.5, 161.0, 175.4, 187.4, 202.5, 215.4, 229.9]
Call the function. Fractional tolerance = 1 part in 10^5,
Initial guess = [0,0], and the minimum should be found within
a distance of 100 of that point:
r = AMOEBAX(1.0e-5, 1.e-4, SCALE=1.0e2, P0 = [0, 0], FUNCTION_VALUE=fval)
Check for convergence:
if n_elements(r) eq 1 then message,'AMOEBA failed to converge'
Print results.
print, 'Intercept, Slope:', r, 'Function value (max error): ', fval(0)
Intercept, Slope: 11.4100 2.72800
Function value: 1.33000
MODIFICATION HISTORY:
DMS, May, 1996. Written.
T. Metcalf 2005-03-30 Added check on convergence of the
minimum location in addition to the
minimum value (xtol).
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Name: anahead2struct
Purpose: convert an ana header (per lapalma) -> SSW structure
CALLS:
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Name: anydata2paper
Purpose: analyze your data and submit to selected Journal
Input Parameters:
index, data - any SSW standards
Keyword Parameters:
filling_factor - if not supplied, will derive a number between
10e-4 and 1 which best suppports your theory
buzzwords - buzzwords to include - if supplied as a switch, will
default to buzzword-du-jour
bypass_peer_review - obvious (may make this the default...)
journal - (default='Apj')
landmark - if set, make this a landmark paper
error_analysis - if set, include detailed error analysis
(by popular demand, default denies any and all sources of error)
fast - if set, run an order of magnitude faster
Calling Example:
IDL> anydata2paper,index,data,journal='Nature',title='How CMEs Work',$
filling_factor='best_fudge', equations='NONE', $
buzzwords=['sigmoids','helicity','exploding sheared core fields',$
'magnetic carpet','dimming'], /bypass_peer_review, /fast
Side Effects
Generated paper will be written to selected journal data base for
publication in next available issue.
CALLS: ***
BOX_MESSAGE
History:
Circa 1990 - S.L.Freeland - Written
15-Feb-2000 - Pons and Fleischman - add /BYPASS_PEER_REVIEW
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CALLS: ***
ATIME [1], ATIME [2], CHECKVAR [1], DATATYPE [1], DATATYPE [2], DATATYPE [3]
Int2Ex [1], Int2Ex [2], UTIME [1], UTIME [2], Utime2str [1], Utime2str [2]
anytim2ints [1], anytim2ints [2], checkvar [2], gt_day [1], gt_day [2]
gt_time [1], gt_time [2], int2sec [1], int2sec [2], timstr2ex [1], timstr2ex [2]
CALLED BY:
ALIGN1BIGGRAM, ANYTIM_REPORT, BATSE_FLARES_WEEK, BATSE_ON, BATSE_SPEC_GAIN_FDB
BATSE_TIME_INPUT, BCS, Build_Schedule, CALC_LOI_ROLL, CALIBRATE [1], CARR2DATE
CARR2EX, CH2KVT, CH2KVT_GAIN, CHECK_FOR_30S, CHECK_OVERFLOW, CHECK_SFC_PNT, CHKPOINT
CLEAN_GOES, CONT_EDGES, CONT_READ, CP_CATREAD, CP_CATRESET, CP_CATTIME
CREATE_GIF_HTML, CREATE_HTML, CRYSTAL_RES, Create_update_tar, DATETIME OBJECT
DATPLOT, DISCSP_BANDS, DISCSP_EDGES, DISCSP_READ, DISPLOI_MON5K, DO_EVENTLISTS
DO_QLARCHIVE, DROT_NAR, ECI2GEOGRAPHIC, ECL_FRAC, EIT_COPY, EUTPLOT, FDBREAD
FILT_EVENTS, FIND_DBFILE, FIND_GOOD_OCCS, FIND_PACKET
FITS WRITER CLASS FOR ANY RHESSI DATA TYPES, FITS_TIME, FLIST, FLISTOC
FORMAT_INTERVALS, FSOC, FSPLOT, FS_ACC_CONT, FS_ACC_DISCSP, FS_GEN_ARR, FS_GRAPH
FS_OPEN [1], FS_READ_DD, Fits_spectra [1], Fits_spectra [2], GAP_FILE, GAP_FINDER
GEOGRAPHIC2ECI, GETGPSaVG [1], GETGPSaVG [2], GETSATaVG, GET_BATSE_POINTING
GET_DISCSP511, GET_DROT_DUR, GET_FITS_TIME, GET_LAD_GAIN, GET_NAR, GET_OCCS
GET_OCC_ONDAY, GET_SLLD, GET_SPEC_CAL, GET_SPEC_GAIN, GFITS_R, GFITS_W
GOES_CHIANTI_TEM, GOES_FITS_FILES, GOES_MEWE_TEM, GOES_TEM, GOES_TF, GOES_TF_COEFF
GOES_TRANSFER, GOES__DEFINE, GRS_EXTRACT, GRWCH_ST, HESSI
HESSI CALIBRATED EVENTLIST CLASS DEFINITION [3]
HESSI FASTRATE CLASS DEFINITION, HESSI IMAGE FILE CLASS DEFINITION [1]
HESSI IMAGE RAW CLASS DEFINITION [2]
HESSI IMAGE STRATEGY CLASS DEFINITION
HESSI MONITOR RATE CLASS DEFINITION
HESSI MULTI IMAGE CLASS DEFINITION [2]
HESSI MULTI IMAGE CLASS DEFINITION [3], HESSI PACKET FILE ABSTRACT CLASS
HESSI ROLL_DB CLASS DEFINITION, HESSI SIMULATION CLASS DEFINITION
HESSI SOHDATA CLASS DEFINITION, HESSI Search Lookup Table Index
HESSI_REF_TIME, HSI_ANY2SCTIME, HSI_ANY_SOHDATA, HSI_ASPECT_SIM
HSI_BUILD_OBS_TIME, HSI_CLKDELTAFILETIME_2_UT, HSI_CLK_DELTA_WRITE
HSI_CLOCK_DRIFT, HSI_DO_QLOOK_PLOTS, HSI_EVENTLIST_TEST, HSI_FITS2MAP [1]
HSI_GET_CLOCK_SYNCH, HSI_GET_TIMEBIN, HSI_IMAGE_TEST [2]
HSI_IMAGE_TEST__define, HSI_LOCATE_FLARE [2], HSI_LOCATE_FLARE [4]
HSI_MAP_EVALUATOR [1], HSI_MODEL_TO_SCORE, HSI_NOSAAN, HSI_NPAK_HISTOGRAM
HSI_ORBFILETIME_2_UT, HSI_PACKET2FITS, HSI_PAK2FILETIMES, HSI_QLOOK_ASPECT
HSI_QLOOK_SUMMARY_PAGE__DEFINE, HSI_RD_FITS_SPECTRUM, HSI_REF_TIME
HSI_SCORE2FILE, HSI_SCTIME2ANY, HSI_SEQ_CNT_CHECK, HSI_SET_FILE_TIME
HSI_SMEXHDR_RCVD_TIME, HSI_SPECTROGRAMCHAN_OVERLAP_FIX
HSI_SPECTROGRAM_DECIM_CORRECT, HSI_SPECTROGRAM_DECIM_TABLE
HSI_SPECTRUM__DEFINE, HSI_SRM__DEFINE, HSI_SSR_FILL_PER_ORBIT [2]
HSI_TIME_N_ORBITS, HSI_TOHBAN_FLARE_COUNTER, HSI_UT_2_CLKDELTAFILETIME
HSI_VCFILE_PACKET_RATE, HSI_VCFILE_TIMES, HSI_WRITE_LEVEL0, HSI_tplot2any
HXARCHIVE, HXFITS, HXR2FILE, HXRBS, HXRBS_ESC, HXRFITS_ARCHIVE, HXRFITS_HEAD
HXRS__DEFINE, HXT_CAL_FIX [1], HXT_CAL_FIX [2], Hessi_obs_summary
Hsi_contact2fits [1], Hsi_contact2fits [2], Hsi_daily_catalog [1]
Hsi_daily_catalog [2], Hsi_monitor_rate_read, LAY1GKM, LONLAT2XY, Load_sher
MAKE_SOLCALTRAJ, MDI__DEFINE, MERGE_DISCSP_HKG_OCC, MJD2ANY, MK_MER_CONT
NAR2COORD, NEAREST_GEV, NEAR_CONJ, NORH_F2EVF [1], NORH_F2EVF [2], NORH_FIXINDEX
NORH_IMG2IDX [1], NORH_IMG2IDX [2], NORH_JST2UT [1], NORH_JST2UT [2], NORH_MKSZ
NORH_PR_EVX [1], NORH_PR_EVX [2], NORH_PR_INFO [1], NORH_PR_INFO [2]
NORH_RD_TCX [1], NORH_RD_TCX [2], NORH_RD_TSX [1], NORH_RD_TSX [2]
NORH_SEL_DIFF [1], NORH_SEL_DIFF [2], NORH_SYNTH_BYF [1], NORH_SYNTH_BYF [2]
NORH_TCX2IDX [1], NORH_TCX2IDX [2], NORH_TIM2F [1], NORH_TIM2F [2]
NORH_TRANS_BYF [1], NORH_TRANS_BYF [2], NORH_UT2JST [1], NORH_UT2JST [2]
NORP_CLB_INTEG, NORP_CLB_SN, NORP_GT_NDATA, NORP_NCLB_TIME, NORP_RDT2DATA_17G
NORP_RDT2DATA_1G, NORP_RDT2DATA_2G, NORP_RDT2DATA_35G, NORP_RDT2DATA_4G
NORP_RDT2DATA_80G, NORP_RDT2DATA_9G, NORP_RDT2TIMEJ [1], NORP_RDT2TIMEJ [2]
NORP_RD_AVG [1], NORP_RD_AVG [2], NORP_RD_DAILY [1], NORP_RD_DAILY [2]
NORP_RD_DAT, NORP_RD_RDT, OCC_DBASE, ORBIT_DN, ORBIT_INPUT_TIME, PARSE_ATIME [1]
PARSE_GROSSC_ATTITUDE, PLOTBATSE, PLOTBATSE_QL, PLOT_HSI, PLOT_MAP, PLOT_OCCS
PLOT_OCC_ONDAY, PROFILES2, PR_PATROLS, PURGE_KAPS, Pointing_Change, QL_DAY_PLOT
QL_ORBIT_PLOT, QL_PLOTTER, QL_READBDB, RD_GOES, RD_GOES_SDAC, RD_NEAR_PIN [1]
RD_NEAR_PIN [2], READCOL [3], READQUAL, READ_CONT, READ_DISCLA, READ_HXRS_FITS [1]
READ_HXRS_FITS [2], READ_HXRS_FITS [3], READ_MINICAT, READ_MONTH_CAT
READ_OCC_DISCSP, RESTORE_QLOOK, ROLL_PLOT, Radio Spectrogram FITS File reader
Radiospectrogram FITS File reader [1]
Radiospectrogram FITS File reader [2], SET_UTAXIS, SITE__DEFINE
SOLB_PLOT_POINTING [1], SOLB_PLOT_POINTING [2], SOLB_READ_REPOINT [1]
SOLB_READ_REPOINT [2], SOLB_SPACECRAFT_POINTING [1]
SOLB_SPACECRAFT_POINTING [2], SOLEPHUT, SPARTAN_PLANNER, SPECPLOT__DEFINE
SPECTRA2FITS, SPECTROGRAM CLASS DEFINITION, SPECTRUM CLASS DEFINITION
SPEX_COMMONS [2], SPEX_COMMONS [4], SPEX_DATA_GENX [1], SPEX_DATA_GENX [2]
SPEX_DRM__DEFINE, SPEX_FITINT__DEFINE, SPEX_GEN__DEFINE, SPEX_PROC [1]
SPEX_PROC [2], SPEX_SAVE [1], SPEX_SAVE [2], SPEX__DEFINE, STEREO_SIMUL
SXT_BAKEOUT_IN, SXT_COVERAGE, SXT_ECLIPSE, SXT_EXPOSURE_MAP, Shers_load [1]
TEMP_BCK_TIME_INTV, TEST_CAL, TIM2CARR, TIMESTAMP, TIME_AXIS__DEFINE, TIME_F_NAME
TJD2YMD, TOK_RD_DAILY, TRACE_ALIGN_CUBE, TRACE_COPY, TRACE_CUBE_POINTING
TRACE_GBO, TRACE_MDI_ALIGN, TRACE_SSWHERE [1], TV_SYNOP, TWIDGET, TYKW_RDT2TIMEJ
TYKW_RD_DAILY, TYKW_RD_DAT, UNFORMAT_INTERVALS, UPDATE_HTML, UTIME [1], UTIME [2]
UTPLOT_IMAGE, UTPLOT__DEFINE, UT_2_YYDOY [1], VIEW_TRACE_MOSAIC, WRITE_MONTH_CAT
XSM_VALID, XYPLOT__DEFINE, YMD2TJD, YOHKOH_TERM_PREDICT, ZDEROTATE, ZHDRUNIT
accum_counts [1], accum_counts [2], anahead2struct, anytim2weekinfo
auto_bck_find0, avsig_1 [1], avsig_1 [4], avsig_1 [6], avsig_temp
batse_create_html, batse_sea_html, check_cals, cp_catwidget, cw_ut_range
data2files, days_til_next_solar_max, db_gbo, decode_gev, default_rate_header
difference_movie, disp_sci160k [1], disp_sci160k [2], doytim2ints
drm_4_spex [1], drm_4_spex [2], eit_fulldisk, eit_proton_summary, evt_grid
find_uvexp, fix_decon_pits, fixinate_trace, flare_hist, get_acedata
get_epoch_sfcs [1], get_epoch_sfcs [2], get_gevloc_data, get_goes_defsat [1]
get_goes_defsat [2], get_infox, get_solar_indices, get_utevent [1]
get_utevent [2], get_utrange, go_sxt_sss2secondary, go_yo_prod_batch
goes_plot [1], goes_plot [2], goes_plot [3], goes_plot [4], goes_plot [5]
grid_data [1], grid_data [2], gtab_summary, gtt_orbit, has_overlap [1]
has_overlap [2], hsi_1orbit_allpak, hsi_anytim_2_filename, hsi_as_sim
hsi_as_sim_packet, hsi_aspect [1], hsi_aspect [2], hsi_ast_seesource_time
hsi_ast_sourceangle, hsi_atten_state, hsi_bad_pak, hsi_badpak_test
hsi_bproj2size, hsi_chk_obj, hsi_cld_sav_init, hsi_clk_delta_calc
hsi_clock_drift_dxdt, hsi_clock_drift_redo, hsi_clock_drift_soc
hsi_create_filedb, hsi_cw_ut_range, hsi_data_recovery_fraction
hsi_decimation_anomaly, hsi_default_resolutions, hsi_default_tailfracs
hsi_demodulator [1], hsi_do_qlook_image [1], hsi_do_qlook_image [2]
hsi_earthangle, hsi_endfileinfo_fill, hsi_ephemeris__define
hsi_ephemeris_concat, hsi_ephemeris_fill, hsi_filedb__define [1]
hsi_filedb__define [2], hsi_filedb_filename, hsi_filedb_read [1]
hsi_filedb_read [2], hsi_filedb_write, hsi_filedb_write_ascii
hsi_filename_2_anytim, hsi_fits_header, hsi_flare2time, hsi_flare_flag
hsi_flare_id_assign, hsi_flare_id_check, hsi_flare_in_int, hsi_flare_list2ar
hsi_flare_list2goes [1], hsi_flare_list2goes [2], hsi_flare_list__define [1]
hsi_flare_list__define [2], hsi_flare_list_fill [1], hsi_flare_list_fill [2]
hsi_flare_position_image [1], hsi_flare_position_image [2], hsi_format_flare
hsi_full_sun_image [1], hsi_full_sun_image [2], hsi_gbo, hsi_get_e_edges [1]
hsi_get_orbit_info, hsi_get_total_time, hsi_getflare, hsi_image__getaxis [2]
hsi_image_plot, hsi_image_raw__define, hsi_imagefile_2_plotman
hsi_lambda_vs_t, hsi_last_id_write filename last_id, hsi_locate_flare [1]
hsi_locate_flare [3], hsi_mod_variance__define, hsi_mod_variance_concat
hsi_monthly_filename, hsi_mult_filedb_otp, hsi_mult_flare_list_inp
hsi_mult_qspec, hsi_new_spec_bck, hsi_night_bck, hsi_obs_flag
hsi_obs_summ_allrates [1], hsi_obs_summ_concat, hsi_obs_summ_fill [1]
hsi_obs_summ_fill [2], hsi_obs_summ_flag__define, hsi_obs_summ_flag_concat
hsi_obs_summ_otp, hsi_obs_summ_rate__define, hsi_obs_summ_rate_concat
hsi_obs_summ_soc__define, hsi_obs_summ_soc_concat, hsi_obs_summ_timarr
hsi_obs_summ_write, hsi_obs_summary__define [1], hsi_obs_summary__define [2]
hsi_obs_summary_adapter__define, hsi_obs_summary_concat, hsi_obs_times
hsi_ok_intv [1], hsi_ok_intv [2], hsi_onedatagap__define, hsi_orbpar4bck
hsi_params2script, hsi_particle_rate__define, hsi_particle_rate_concat
hsi_plot_flux, hsi_pmtras_lookup, hsi_print_decimation_state
hsi_qlook__define, hsi_qlook_call_ospex [1], hsi_qlook_call_ospex [2]
hsi_qlook_concat, hsi_qlook_image, hsi_qlook_monitor_rate__define
hsi_qlook_packet_rate__define, hsi_qlook_pointing__define
hsi_qlook_rate_per_det__define, hsi_qlook_roll_angle__define
hsi_qlook_roll_period__define, hsi_qlook_spectrum
hsi_qlook_spin_axis__define, hsi_qspec [1], hsi_qspec [2], hsi_rd_ephfile
hsi_rd_orbit_files, hsi_rdstatevectorfile, hsi_read_all_flare_list
hsi_read_vcfiletimes, hsi_replace_flare_list, hsi_select_flare
hsi_show_flags [2], hsi_show_flare_on_image, hsi_sim_pflux_2_cflux
hsi_spectrogramACCBIN [2], hsi_spectrogram__define [1]
hsi_spectrogram__define [2], hsi_spectrogram__define [3]
hsi_spectrogram__get_obs [1], hsi_spectrogram__livetime [1]
hsi_spectrum__filewrite, hsi_spectrum__fitswrite, hsi_ssr_fill_per_orbit [1]
hsi_state_vectors, hsi_test_files, hsi_test_packet_rate, hsi_test_qlook
hsi_time_widget, hsi_ui_flarecat, hsi_ui_img, hsi_ui_img_doimage [1]
hsi_ui_img_doimage [2], hsi_ui_lc, hsi_ui_obs, hsi_ui_qlimage, hsi_ui_spec
hsi_vcfile_gaps, hsi_vis_fwdfit, hsi_whichflare, hsi_whole_flare_list
hsi_write_all_flare_list, hsi_write_decimation_settings
hsi_write_txt_flare_list, hsi_xy_test [1], hsi_xy_test [2], hsi_xy_test_new
hxrbs_response, hxrs_drm2fits [1], hxrs_drm2fits [2], hxrs_drm2fits [3]
image2movie, imspec [10], imspec [11], imspec [12], imspec [13], imspec [14]
imspec [15], imspec [16], imspec [17], imspec [18], imspec [19], imspec [1]
imspec [20], imspec [21], imspec [22], imspec [23], imspec [24], imspec [25]
imspec [26], imspec [27], imspec [28], imspec [29], imspec [2], imspec [30]
imspec [31], imspec [32], imspec [33], imspec [34], imspec [35], imspec [36]
imspec [3], imspec [4], imspec [5], imspec [6], imspec [7], imspec [8], imspec [9]
index2fov, kluge_att, lasco_time2file, lasco_time2nrlwww, lastgki, later, lcur_image
les_archive_info, make_goes_chianti_response [1]
make_goes_chianti_response [2], make_goes_chianti_response [3]
make_goes_chianti_response [4], make_grid_sphere, map2index, mark_intervals
may_eclipse, mdi_time2file, mees_log_read, mees_name_format, mk_mdi_fits
mk_sff_pair [1], mk_sff_pair [2], mk_ssc [1], mk_ssc [2], mk_ssc_batch [1]
mk_ssc_batch [2], mk_sumer_dbase_ff, mk_synsfc_coeff [1], mk_synsfc_coeff [2]
mksort, mon_sci5k, mrdfits_spectra, norh_alpha, norh_t2azel, op_term_score
option_changer [1], option_changer [2], parse_atime [2], pctime2ssw
phoenix_filedb_get, phoenix_spg_get, plot_ace, plot_fov [1], plot_goes_ospex
plotman, plotman_draw_event, plotman_setaxes, plotman_zoom, pmtras_analysis
pr_his_index [1], pr_his_index [2], pr_his_index [3], ptim, rapp_get_spectrogram
rd_goesp_ascii, rd_goesx_ascii, rd_mdi [1], rd_mdi [2], rd_sxs_pha [1]
rd_sxs_pha [2], rd_therm_rs232, rd_wbs_pha [1], rd_wbs_pha [2], rdbda_smm
read_eit, read_genxcat, read_hessi_4_ospex, read_hessi_4_spex [1]
read_hessi_4_spex [2], read_hessi_fits_4_spex [1]
read_hessi_fits_4_spex [2], read_lapalma, read_mdi, read_soxs_4_ospex
read_trace, read_xsm_4_ospex, read_yohkoh_4_spex [1], read_yohkoh_4_spex [2]
redo_disploi, redo_mon_sci5k, rhessi_get_spin_axis_position, save_idl_routines
sec_name_format, soxs_readfile, special_movie, spectro_plot2
spectrogram__define, spex_bk__define, spex_bkint__define, spex_bksub__define
spex_data__define, spex_evnt [1], spex_evnt [2], spex_hessi_image__define
spex_image__define, ssc_files [1], ssc_files [2], ssc_files [3], ssw_build_trace
ssw_composite, ssw_deltat, ssw_expand_times, ssw_flare_locator, ssw_fov_context
ssw_fs_cat2db, ssw_getcme_cactus, ssw_getcme_cdaw, ssw_getdst
ssw_gxd_remove_flares, ssw_javamovie, ssw_nar2armurl, ssw_pos2zenith
ssw_sec_aktxt2struct, ssw_time2filelist, ssw_time2paths, ssw_timestat
ssw_track_fov, sswdb_files, sswstruct_fill [1], stt_plot, sxi_files, sxt_files
sxt_his2dbase, sxt_is_synsfc, sxt_mk3 mk3 index data [1]
sxt_mk3 mk3 index data [2], sxt_orhis, sxt_prep [1], sxt_prep [2], sxt_prep [3]
sxt_ssn2fits [1], sxt_uvf_info [1], sxt_uvf_info [3], t_utplot [1], t_utplot [2]
time_at_meridian, time_window, timegrid, tr_lut_conv, tr_rd_index
tr_wrt_fits_i1 [2], trace_cosmic2hist_accum, trace_files, trace_get_vignette
trace_goodobs, trace_movie_index [1], trace_movie_index [2]
trace_recent_movie_summary, trace_sswhere [2], trace_sswhere [3]
trace_sswhere [4], trace_wave2point, ut_2_yydoy [2], ut_label, valid_time_range
wbs_response [1], wbs_response [2], week_loop [1], week_loop [2], week_loop [3]
weeks_in_year [1], weeks_in_year [2], where_are [1], where_are [2]
which_hessi_version, write_genxcat, xy2lonlat, xzchange, yo_index2path
yoh_orb_interp [1], yoh_orb_interp [2], yohkoh_files, yohkoh_legacy_files [1]
yohkoh_legacy_files [2], zcheck_hdr, zmovify, ztrack
Procedure: TAI2_SEC1979
Purpose: This function converts an array of seconds with ref to 1-jan-1958
including leap seconds to an array referenced to 1-jan-1979
History;
11-jan-2006, richard.schwartz@gsfc.nasa.gov
[Previous]
[Next]
CALLS: ***
ATIME [1], ATIME [2], CHECKVAR [1], DATATYPE [1], DATATYPE [2], DATATYPE [3]
Int2Ex [1], Int2Ex [2], UTIME [1], UTIME [2], Utime2str [1], Utime2str [2]
anytim2ints [1], anytim2ints [2], checkvar [2], gt_day [1], gt_day [2]
gt_time [1], gt_time [2], int2sec [1], int2sec [2], timstr2ex [1], timstr2ex [2]
CALLED BY:
ALIGN1BIGGRAM, ANYTIM_REPORT, BATSE_FLARES_WEEK, BATSE_ON, BATSE_SPEC_GAIN_FDB
BATSE_TIME_INPUT, BCS, Build_Schedule, CALC_LOI_ROLL, CALIBRATE [1], CARR2DATE
CARR2EX, CH2KVT, CH2KVT_GAIN, CHECK_FOR_30S, CHECK_OVERFLOW, CHECK_SFC_PNT, CHKPOINT
CLEAN_GOES, CONT_EDGES, CONT_READ, CP_CATREAD, CP_CATRESET, CP_CATTIME
CREATE_GIF_HTML, CREATE_HTML, CRYSTAL_RES, Create_update_tar, DATETIME OBJECT
DATPLOT, DISCSP_BANDS, DISCSP_EDGES, DISCSP_READ, DISPLOI_MON5K, DO_EVENTLISTS
DO_QLARCHIVE, DROT_NAR, ECI2GEOGRAPHIC, ECL_FRAC, EIT_COPY, EUTPLOT, FDBREAD
FILT_EVENTS, FIND_DBFILE, FIND_GOOD_OCCS, FIND_PACKET
FITS WRITER CLASS FOR ANY RHESSI DATA TYPES, FITS_TIME, FLIST, FLISTOC
FORMAT_INTERVALS, FSOC, FSPLOT, FS_ACC_CONT, FS_ACC_DISCSP, FS_GEN_ARR, FS_GRAPH
FS_OPEN [1], FS_READ_DD, Fits_spectra [1], Fits_spectra [2], GAP_FILE, GAP_FINDER
GEOGRAPHIC2ECI, GETGPSaVG [1], GETGPSaVG [2], GETSATaVG, GET_BATSE_POINTING
GET_DISCSP511, GET_DROT_DUR, GET_FITS_TIME, GET_LAD_GAIN, GET_NAR, GET_OCCS
GET_OCC_ONDAY, GET_SLLD, GET_SPEC_CAL, GET_SPEC_GAIN, GFITS_R, GFITS_W
GOES_CHIANTI_TEM, GOES_FITS_FILES, GOES_MEWE_TEM, GOES_TEM, GOES_TF, GOES_TF_COEFF
GOES_TRANSFER, GOES__DEFINE, GRS_EXTRACT, GRWCH_ST, HESSI
HESSI CALIBRATED EVENTLIST CLASS DEFINITION [3]
HESSI FASTRATE CLASS DEFINITION, HESSI IMAGE FILE CLASS DEFINITION [1]
HESSI IMAGE RAW CLASS DEFINITION [2]
HESSI IMAGE STRATEGY CLASS DEFINITION
HESSI MONITOR RATE CLASS DEFINITION
HESSI MULTI IMAGE CLASS DEFINITION [2]
HESSI MULTI IMAGE CLASS DEFINITION [3], HESSI PACKET FILE ABSTRACT CLASS
HESSI ROLL_DB CLASS DEFINITION, HESSI SIMULATION CLASS DEFINITION
HESSI SOHDATA CLASS DEFINITION, HESSI Search Lookup Table Index
HESSI_REF_TIME, HSI_ANY2SCTIME, HSI_ANY_SOHDATA, HSI_ASPECT_SIM
HSI_BUILD_OBS_TIME, HSI_CLKDELTAFILETIME_2_UT, HSI_CLK_DELTA_WRITE
HSI_CLOCK_DRIFT, HSI_DO_QLOOK_PLOTS, HSI_EVENTLIST_TEST, HSI_FITS2MAP [1]
HSI_GET_CLOCK_SYNCH, HSI_GET_TIMEBIN, HSI_IMAGE_TEST [2]
HSI_IMAGE_TEST__define, HSI_LOCATE_FLARE [2], HSI_LOCATE_FLARE [4]
HSI_MAP_EVALUATOR [1], HSI_MODEL_TO_SCORE, HSI_NOSAAN, HSI_NPAK_HISTOGRAM
HSI_ORBFILETIME_2_UT, HSI_PACKET2FITS, HSI_PAK2FILETIMES, HSI_QLOOK_ASPECT
HSI_QLOOK_SUMMARY_PAGE__DEFINE, HSI_RD_FITS_SPECTRUM, HSI_REF_TIME
HSI_SCORE2FILE, HSI_SCTIME2ANY, HSI_SEQ_CNT_CHECK, HSI_SET_FILE_TIME
HSI_SMEXHDR_RCVD_TIME, HSI_SPECTROGRAMCHAN_OVERLAP_FIX
HSI_SPECTROGRAM_DECIM_CORRECT, HSI_SPECTROGRAM_DECIM_TABLE
HSI_SPECTRUM__DEFINE, HSI_SRM__DEFINE, HSI_SSR_FILL_PER_ORBIT [2]
HSI_TIME_N_ORBITS, HSI_TOHBAN_FLARE_COUNTER, HSI_UT_2_CLKDELTAFILETIME
HSI_VCFILE_PACKET_RATE, HSI_VCFILE_TIMES, HSI_WRITE_LEVEL0, HSI_tplot2any
HXARCHIVE, HXFITS, HXR2FILE, HXRBS, HXRBS_ESC, HXRFITS_ARCHIVE, HXRFITS_HEAD
HXRS__DEFINE, HXT_CAL_FIX [1], HXT_CAL_FIX [2], Hessi_obs_summary
Hsi_contact2fits [1], Hsi_contact2fits [2], Hsi_daily_catalog [1]
Hsi_daily_catalog [2], Hsi_monitor_rate_read, LAY1GKM, LONLAT2XY, Load_sher
MAKE_SOLCALTRAJ, MDI__DEFINE, MERGE_DISCSP_HKG_OCC, MJD2ANY, MK_MER_CONT
NAR2COORD, NEAREST_GEV, NEAR_CONJ, NORH_F2EVF [1], NORH_F2EVF [2], NORH_FIXINDEX
NORH_IMG2IDX [1], NORH_IMG2IDX [2], NORH_JST2UT [1], NORH_JST2UT [2], NORH_MKSZ
NORH_PR_EVX [1], NORH_PR_EVX [2], NORH_PR_INFO [1], NORH_PR_INFO [2]
NORH_RD_TCX [1], NORH_RD_TCX [2], NORH_RD_TSX [1], NORH_RD_TSX [2]
NORH_SEL_DIFF [1], NORH_SEL_DIFF [2], NORH_SYNTH_BYF [1], NORH_SYNTH_BYF [2]
NORH_TCX2IDX [1], NORH_TCX2IDX [2], NORH_TIM2F [1], NORH_TIM2F [2]
NORH_TRANS_BYF [1], NORH_TRANS_BYF [2], NORH_UT2JST [1], NORH_UT2JST [2]
NORP_CLB_INTEG, NORP_CLB_SN, NORP_GT_NDATA, NORP_NCLB_TIME, NORP_RDT2DATA_17G
NORP_RDT2DATA_1G, NORP_RDT2DATA_2G, NORP_RDT2DATA_35G, NORP_RDT2DATA_4G
NORP_RDT2DATA_80G, NORP_RDT2DATA_9G, NORP_RDT2TIMEJ [1], NORP_RDT2TIMEJ [2]
NORP_RD_AVG [1], NORP_RD_AVG [2], NORP_RD_DAILY [1], NORP_RD_DAILY [2]
NORP_RD_DAT, NORP_RD_RDT, OCC_DBASE, ORBIT_DN, ORBIT_INPUT_TIME, PARSE_ATIME [1]
PARSE_GROSSC_ATTITUDE, PLOTBATSE, PLOTBATSE_QL, PLOT_HSI, PLOT_MAP, PLOT_OCCS
PLOT_OCC_ONDAY, PROFILES2, PR_PATROLS, PURGE_KAPS, Pointing_Change, QL_DAY_PLOT
QL_ORBIT_PLOT, QL_PLOTTER, QL_READBDB, RD_GOES, RD_GOES_SDAC, RD_NEAR_PIN [1]
RD_NEAR_PIN [2], READCOL [3], READQUAL, READ_CONT, READ_DISCLA, READ_HXRS_FITS [1]
READ_HXRS_FITS [2], READ_HXRS_FITS [3], READ_MINICAT, READ_MONTH_CAT
READ_OCC_DISCSP, RESTORE_QLOOK, ROLL_PLOT, Radio Spectrogram FITS File reader
Radiospectrogram FITS File reader [1]
Radiospectrogram FITS File reader [2], SET_UTAXIS, SITE__DEFINE
SOLB_PLOT_POINTING [1], SOLB_PLOT_POINTING [2], SOLB_READ_REPOINT [1]
SOLB_READ_REPOINT [2], SOLB_SPACECRAFT_POINTING [1]
SOLB_SPACECRAFT_POINTING [2], SOLEPHUT, SPARTAN_PLANNER, SPECPLOT__DEFINE
SPECTRA2FITS, SPECTROGRAM CLASS DEFINITION, SPECTRUM CLASS DEFINITION
SPEX_COMMONS [2], SPEX_COMMONS [4], SPEX_DATA_GENX [1], SPEX_DATA_GENX [2]
SPEX_DRM__DEFINE, SPEX_FITINT__DEFINE, SPEX_GEN__DEFINE, SPEX_PROC [1]
SPEX_PROC [2], SPEX_SAVE [1], SPEX_SAVE [2], SPEX__DEFINE, STEREO_SIMUL
SXT_BAKEOUT_IN, SXT_COVERAGE, SXT_ECLIPSE, SXT_EXPOSURE_MAP, Shers_load [1]
TEMP_BCK_TIME_INTV, TEST_CAL, TIM2CARR, TIMESTAMP, TIME_AXIS__DEFINE, TIME_F_NAME
TJD2YMD, TOK_RD_DAILY, TRACE_ALIGN_CUBE, TRACE_COPY, TRACE_CUBE_POINTING
TRACE_GBO, TRACE_MDI_ALIGN, TRACE_SSWHERE [1], TV_SYNOP, TWIDGET, TYKW_RDT2TIMEJ
TYKW_RD_DAILY, TYKW_RD_DAT, UNFORMAT_INTERVALS, UPDATE_HTML, UTIME [1], UTIME [2]
UTPLOT_IMAGE, UTPLOT__DEFINE, UT_2_YYDOY [1], VIEW_TRACE_MOSAIC, WRITE_MONTH_CAT
XSM_VALID, XYPLOT__DEFINE, YMD2TJD, YOHKOH_TERM_PREDICT, ZDEROTATE, ZHDRUNIT
accum_counts [1], accum_counts [2], anahead2struct, anytim2weekinfo
auto_bck_find0, avsig_1 [1], avsig_1 [4], avsig_1 [6], avsig_temp
batse_create_html, batse_sea_html, check_cals, cp_catwidget, cw_ut_range
data2files, days_til_next_solar_max, db_gbo, decode_gev, default_rate_header
difference_movie, disp_sci160k [1], disp_sci160k [2], doytim2ints
drm_4_spex [1], drm_4_spex [2], eit_fulldisk, eit_proton_summary, evt_grid
find_uvexp, fix_decon_pits, fixinate_trace, flare_hist, get_acedata
get_epoch_sfcs [1], get_epoch_sfcs [2], get_gevloc_data, get_goes_defsat [1]
get_goes_defsat [2], get_infox, get_solar_indices, get_utevent [1]
get_utevent [2], get_utrange, go_sxt_sss2secondary, go_yo_prod_batch
goes_plot [1], goes_plot [2], goes_plot [3], goes_plot [4], goes_plot [5]
grid_data [1], grid_data [2], gtab_summary, gtt_orbit, has_overlap [1]
has_overlap [2], hsi_1orbit_allpak, hsi_anytim_2_filename, hsi_as_sim
hsi_as_sim_packet, hsi_aspect [1], hsi_aspect [2], hsi_ast_seesource_time
hsi_ast_sourceangle, hsi_atten_state, hsi_bad_pak, hsi_badpak_test
hsi_bproj2size, hsi_chk_obj, hsi_cld_sav_init, hsi_clk_delta_calc
hsi_clock_drift_dxdt, hsi_clock_drift_redo, hsi_clock_drift_soc
hsi_create_filedb, hsi_cw_ut_range, hsi_data_recovery_fraction
hsi_decimation_anomaly, hsi_default_resolutions, hsi_default_tailfracs
hsi_demodulator [1], hsi_do_qlook_image [1], hsi_do_qlook_image [2]
hsi_earthangle, hsi_endfileinfo_fill, hsi_ephemeris__define
hsi_ephemeris_concat, hsi_ephemeris_fill, hsi_filedb__define [1]
hsi_filedb__define [2], hsi_filedb_filename, hsi_filedb_read [1]
hsi_filedb_read [2], hsi_filedb_write, hsi_filedb_write_ascii
hsi_filename_2_anytim, hsi_fits_header, hsi_flare2time, hsi_flare_flag
hsi_flare_id_assign, hsi_flare_id_check, hsi_flare_in_int, hsi_flare_list2ar
hsi_flare_list2goes [1], hsi_flare_list2goes [2], hsi_flare_list__define [1]
hsi_flare_list__define [2], hsi_flare_list_fill [1], hsi_flare_list_fill [2]
hsi_flare_position_image [1], hsi_flare_position_image [2], hsi_format_flare
hsi_full_sun_image [1], hsi_full_sun_image [2], hsi_gbo, hsi_get_e_edges [1]
hsi_get_orbit_info, hsi_get_total_time, hsi_getflare, hsi_image__getaxis [2]
hsi_image_plot, hsi_image_raw__define, hsi_imagefile_2_plotman
hsi_lambda_vs_t, hsi_last_id_write filename last_id, hsi_locate_flare [1]
hsi_locate_flare [3], hsi_mod_variance__define, hsi_mod_variance_concat
hsi_monthly_filename, hsi_mult_filedb_otp, hsi_mult_flare_list_inp
hsi_mult_qspec, hsi_new_spec_bck, hsi_night_bck, hsi_obs_flag
hsi_obs_summ_allrates [1], hsi_obs_summ_concat, hsi_obs_summ_fill [1]
hsi_obs_summ_fill [2], hsi_obs_summ_flag__define, hsi_obs_summ_flag_concat
hsi_obs_summ_otp, hsi_obs_summ_rate__define, hsi_obs_summ_rate_concat
hsi_obs_summ_soc__define, hsi_obs_summ_soc_concat, hsi_obs_summ_timarr
hsi_obs_summ_write, hsi_obs_summary__define [1], hsi_obs_summary__define [2]
hsi_obs_summary_adapter__define, hsi_obs_summary_concat, hsi_obs_times
hsi_ok_intv [1], hsi_ok_intv [2], hsi_onedatagap__define, hsi_orbpar4bck
hsi_params2script, hsi_particle_rate__define, hsi_particle_rate_concat
hsi_plot_flux, hsi_pmtras_lookup, hsi_print_decimation_state
hsi_qlook__define, hsi_qlook_call_ospex [1], hsi_qlook_call_ospex [2]
hsi_qlook_concat, hsi_qlook_image, hsi_qlook_monitor_rate__define
hsi_qlook_packet_rate__define, hsi_qlook_pointing__define
hsi_qlook_rate_per_det__define, hsi_qlook_roll_angle__define
hsi_qlook_roll_period__define, hsi_qlook_spectrum
hsi_qlook_spin_axis__define, hsi_qspec [1], hsi_qspec [2], hsi_rd_ephfile
hsi_rd_orbit_files, hsi_rdstatevectorfile, hsi_read_all_flare_list
hsi_read_vcfiletimes, hsi_replace_flare_list, hsi_select_flare
hsi_show_flags [2], hsi_show_flare_on_image, hsi_sim_pflux_2_cflux
hsi_spectrogramACCBIN [2], hsi_spectrogram__define [1]
hsi_spectrogram__define [2], hsi_spectrogram__define [3]
hsi_spectrogram__get_obs [1], hsi_spectrogram__livetime [1]
hsi_spectrum__filewrite, hsi_spectrum__fitswrite, hsi_ssr_fill_per_orbit [1]
hsi_state_vectors, hsi_test_files, hsi_test_packet_rate, hsi_test_qlook
hsi_time_widget, hsi_ui_flarecat, hsi_ui_img, hsi_ui_img_doimage [1]
hsi_ui_img_doimage [2], hsi_ui_lc, hsi_ui_obs, hsi_ui_qlimage, hsi_ui_spec
hsi_vcfile_gaps, hsi_vis_fwdfit, hsi_whichflare, hsi_whole_flare_list
hsi_write_all_flare_list, hsi_write_decimation_settings
hsi_write_txt_flare_list, hsi_xy_test [1], hsi_xy_test [2], hsi_xy_test_new
hxrbs_response, hxrs_drm2fits [1], hxrs_drm2fits [2], hxrs_drm2fits [3]
image2movie, imspec [10], imspec [11], imspec [12], imspec [13], imspec [14]
imspec [15], imspec [16], imspec [17], imspec [18], imspec [19], imspec [1]
imspec [20], imspec [21], imspec [22], imspec [23], imspec [24], imspec [25]
imspec [26], imspec [27], imspec [28], imspec [29], imspec [2], imspec [30]
imspec [31], imspec [32], imspec [33], imspec [34], imspec [35], imspec [36]
imspec [3], imspec [4], imspec [5], imspec [6], imspec [7], imspec [8], imspec [9]
index2fov, kluge_att, lasco_time2file, lasco_time2nrlwww, lastgki, later, lcur_image
les_archive_info, make_goes_chianti_response [1]
make_goes_chianti_response [2], make_goes_chianti_response [3]
make_goes_chianti_response [4], make_grid_sphere, map2index, mark_intervals
may_eclipse, mdi_time2file, mees_log_read, mees_name_format, mk_mdi_fits
mk_sff_pair [1], mk_sff_pair [2], mk_ssc [1], mk_ssc [2], mk_ssc_batch [1]
mk_ssc_batch [2], mk_sumer_dbase_ff, mk_synsfc_coeff [1], mk_synsfc_coeff [2]
mksort, mon_sci5k, mrdfits_spectra, norh_alpha, norh_t2azel, op_term_score
option_changer [1], option_changer [2], parse_atime [2], pctime2ssw
phoenix_filedb_get, phoenix_spg_get, plot_ace, plot_fov [1], plot_goes_ospex
plotman, plotman_draw_event, plotman_setaxes, plotman_zoom, pmtras_analysis
pr_his_index [1], pr_his_index [2], pr_his_index [3], ptim, rapp_get_spectrogram
rd_goesp_ascii, rd_goesx_ascii, rd_mdi [1], rd_mdi [2], rd_sxs_pha [1]
rd_sxs_pha [2], rd_therm_rs232, rd_wbs_pha [1], rd_wbs_pha [2], rdbda_smm
read_eit, read_genxcat, read_hessi_4_ospex, read_hessi_4_spex [1]
read_hessi_4_spex [2], read_hessi_fits_4_spex [1]
read_hessi_fits_4_spex [2], read_lapalma, read_mdi, read_soxs_4_ospex
read_trace, read_xsm_4_ospex, read_yohkoh_4_spex [1], read_yohkoh_4_spex [2]
redo_disploi, redo_mon_sci5k, rhessi_get_spin_axis_position, save_idl_routines
sec_name_format, soxs_readfile, special_movie, spectro_plot2
spectrogram__define, spex_bk__define, spex_bkint__define, spex_bksub__define
spex_data__define, spex_evnt [1], spex_evnt [2], spex_hessi_image__define
spex_image__define, ssc_files [1], ssc_files [2], ssc_files [3], ssw_build_trace
ssw_composite, ssw_deltat, ssw_expand_times, ssw_flare_locator, ssw_fov_context
ssw_fs_cat2db, ssw_getcme_cactus, ssw_getcme_cdaw, ssw_getdst
ssw_gxd_remove_flares, ssw_javamovie, ssw_nar2armurl, ssw_pos2zenith
ssw_sec_aktxt2struct, ssw_time2filelist, ssw_time2paths, ssw_timestat
ssw_track_fov, sswdb_files, sswstruct_fill [1], stt_plot, sxi_files, sxt_files
sxt_his2dbase, sxt_is_synsfc, sxt_mk3 mk3 index data [1]
sxt_mk3 mk3 index data [2], sxt_orhis, sxt_prep [1], sxt_prep [2], sxt_prep [3]
sxt_ssn2fits [1], sxt_uvf_info [1], sxt_uvf_info [3], t_utplot [1], t_utplot [2]
time_at_meridian, time_window, timegrid, tr_lut_conv, tr_rd_index
tr_wrt_fits_i1 [2], trace_cosmic2hist_accum, trace_files, trace_get_vignette
trace_goodobs, trace_movie_index [1], trace_movie_index [2]
trace_recent_movie_summary, trace_sswhere [2], trace_sswhere [3]
trace_sswhere [4], trace_wave2point, ut_2_yydoy [2], ut_label, valid_time_range
wbs_response [1], wbs_response [2], week_loop [1], week_loop [2], week_loop [3]
weeks_in_year [1], weeks_in_year [2], where_are [1], where_are [2]
which_hessi_version, write_genxcat, xy2lonlat, xzchange, yo_index2path
yoh_orb_interp [1], yoh_orb_interp [2], yohkoh_files, yohkoh_legacy_files [1]
yohkoh_legacy_files [2], zcheck_hdr, zmovify, ztrack
Procedure: SEC1979_2TAI
Purpose: This function converts an array of seconds with ref to 1-jan-1979
to an array referenced to 1-jan-1958 plus leap seconds
History;
11-jan-2006, richard.schwartz@gsfc.nasa.gov
[Previous]
[Next]
CALLS: ***
ATIME [1], ATIME [2], CHECKVAR [1], DATATYPE [1], DATATYPE [2], DATATYPE [3]
Int2Ex [1], Int2Ex [2], UTIME [1], UTIME [2], Utime2str [1], Utime2str [2]
anytim2ints [1], anytim2ints [2], checkvar [2], gt_day [1], gt_day [2]
gt_time [1], gt_time [2], int2sec [1], int2sec [2], timstr2ex [1], timstr2ex [2]
CALLED BY:
ALIGN1BIGGRAM, ANYTIM_REPORT, BATSE_FLARES_WEEK, BATSE_ON, BATSE_SPEC_GAIN_FDB
BATSE_TIME_INPUT, BCS, Build_Schedule, CALC_LOI_ROLL, CALIBRATE [1], CARR2DATE
CARR2EX, CH2KVT, CH2KVT_GAIN, CHECK_FOR_30S, CHECK_OVERFLOW, CHECK_SFC_PNT, CHKPOINT
CLEAN_GOES, CONT_EDGES, CONT_READ, CP_CATREAD, CP_CATRESET, CP_CATTIME
CREATE_GIF_HTML, CREATE_HTML, CRYSTAL_RES, Create_update_tar, DATETIME OBJECT
DATPLOT, DISCSP_BANDS, DISCSP_EDGES, DISCSP_READ, DISPLOI_MON5K, DO_EVENTLISTS
DO_QLARCHIVE, DROT_NAR, ECI2GEOGRAPHIC, ECL_FRAC, EIT_COPY, EUTPLOT, FDBREAD
FILT_EVENTS, FIND_DBFILE, FIND_GOOD_OCCS, FIND_PACKET
FITS WRITER CLASS FOR ANY RHESSI DATA TYPES, FITS_TIME, FLIST, FLISTOC
FORMAT_INTERVALS, FSOC, FSPLOT, FS_ACC_CONT, FS_ACC_DISCSP, FS_GEN_ARR, FS_GRAPH
FS_OPEN [1], FS_READ_DD, Fits_spectra [1], Fits_spectra [2], GAP_FILE, GAP_FINDER
GEOGRAPHIC2ECI, GETGPSaVG [1], GETGPSaVG [2], GETSATaVG, GET_BATSE_POINTING
GET_DISCSP511, GET_DROT_DUR, GET_FITS_TIME, GET_LAD_GAIN, GET_NAR, GET_OCCS
GET_OCC_ONDAY, GET_SLLD, GET_SPEC_CAL, GET_SPEC_GAIN, GFITS_R, GFITS_W
GOES_CHIANTI_TEM, GOES_FITS_FILES, GOES_MEWE_TEM, GOES_TEM, GOES_TF, GOES_TF_COEFF
GOES_TRANSFER, GOES__DEFINE, GRS_EXTRACT, GRWCH_ST, HESSI
HESSI CALIBRATED EVENTLIST CLASS DEFINITION [3]
HESSI FASTRATE CLASS DEFINITION, HESSI IMAGE FILE CLASS DEFINITION [1]
HESSI IMAGE RAW CLASS DEFINITION [2]
HESSI IMAGE STRATEGY CLASS DEFINITION
HESSI MONITOR RATE CLASS DEFINITION
HESSI MULTI IMAGE CLASS DEFINITION [2]
HESSI MULTI IMAGE CLASS DEFINITION [3], HESSI PACKET FILE ABSTRACT CLASS
HESSI ROLL_DB CLASS DEFINITION, HESSI SIMULATION CLASS DEFINITION
HESSI SOHDATA CLASS DEFINITION, HESSI Search Lookup Table Index
HESSI_REF_TIME, HSI_ANY2SCTIME, HSI_ANY_SOHDATA, HSI_ASPECT_SIM
HSI_BUILD_OBS_TIME, HSI_CLKDELTAFILETIME_2_UT, HSI_CLK_DELTA_WRITE
HSI_CLOCK_DRIFT, HSI_DO_QLOOK_PLOTS, HSI_EVENTLIST_TEST, HSI_FITS2MAP [1]
HSI_GET_CLOCK_SYNCH, HSI_GET_TIMEBIN, HSI_IMAGE_TEST [2]
HSI_IMAGE_TEST__define, HSI_LOCATE_FLARE [2], HSI_LOCATE_FLARE [4]
HSI_MAP_EVALUATOR [1], HSI_MODEL_TO_SCORE, HSI_NOSAAN, HSI_NPAK_HISTOGRAM
HSI_ORBFILETIME_2_UT, HSI_PACKET2FITS, HSI_PAK2FILETIMES, HSI_QLOOK_ASPECT
HSI_QLOOK_SUMMARY_PAGE__DEFINE, HSI_RD_FITS_SPECTRUM, HSI_REF_TIME
HSI_SCORE2FILE, HSI_SCTIME2ANY, HSI_SEQ_CNT_CHECK, HSI_SET_FILE_TIME
HSI_SMEXHDR_RCVD_TIME, HSI_SPECTROGRAMCHAN_OVERLAP_FIX
HSI_SPECTROGRAM_DECIM_CORRECT, HSI_SPECTROGRAM_DECIM_TABLE
HSI_SPECTRUM__DEFINE, HSI_SRM__DEFINE, HSI_SSR_FILL_PER_ORBIT [2]
HSI_TIME_N_ORBITS, HSI_TOHBAN_FLARE_COUNTER, HSI_UT_2_CLKDELTAFILETIME
HSI_VCFILE_PACKET_RATE, HSI_VCFILE_TIMES, HSI_WRITE_LEVEL0, HSI_tplot2any
HXARCHIVE, HXFITS, HXR2FILE, HXRBS, HXRBS_ESC, HXRFITS_ARCHIVE, HXRFITS_HEAD
HXRS__DEFINE, HXT_CAL_FIX [1], HXT_CAL_FIX [2], Hessi_obs_summary
Hsi_contact2fits [1], Hsi_contact2fits [2], Hsi_daily_catalog [1]
Hsi_daily_catalog [2], Hsi_monitor_rate_read, LAY1GKM, LONLAT2XY, Load_sher
MAKE_SOLCALTRAJ, MDI__DEFINE, MERGE_DISCSP_HKG_OCC, MJD2ANY, MK_MER_CONT
NAR2COORD, NEAREST_GEV, NEAR_CONJ, NORH_F2EVF [1], NORH_F2EVF [2], NORH_FIXINDEX
NORH_IMG2IDX [1], NORH_IMG2IDX [2], NORH_JST2UT [1], NORH_JST2UT [2], NORH_MKSZ
NORH_PR_EVX [1], NORH_PR_EVX [2], NORH_PR_INFO [1], NORH_PR_INFO [2]
NORH_RD_TCX [1], NORH_RD_TCX [2], NORH_RD_TSX [1], NORH_RD_TSX [2]
NORH_SEL_DIFF [1], NORH_SEL_DIFF [2], NORH_SYNTH_BYF [1], NORH_SYNTH_BYF [2]
NORH_TCX2IDX [1], NORH_TCX2IDX [2], NORH_TIM2F [1], NORH_TIM2F [2]
NORH_TRANS_BYF [1], NORH_TRANS_BYF [2], NORH_UT2JST [1], NORH_UT2JST [2]
NORP_CLB_INTEG, NORP_CLB_SN, NORP_GT_NDATA, NORP_NCLB_TIME, NORP_RDT2DATA_17G
NORP_RDT2DATA_1G, NORP_RDT2DATA_2G, NORP_RDT2DATA_35G, NORP_RDT2DATA_4G
NORP_RDT2DATA_80G, NORP_RDT2DATA_9G, NORP_RDT2TIMEJ [1], NORP_RDT2TIMEJ [2]
NORP_RD_AVG [1], NORP_RD_AVG [2], NORP_RD_DAILY [1], NORP_RD_DAILY [2]
NORP_RD_DAT, NORP_RD_RDT, OCC_DBASE, ORBIT_DN, ORBIT_INPUT_TIME, PARSE_ATIME [1]
PARSE_GROSSC_ATTITUDE, PLOTBATSE, PLOTBATSE_QL, PLOT_HSI, PLOT_MAP, PLOT_OCCS
PLOT_OCC_ONDAY, PROFILES2, PR_PATROLS, PURGE_KAPS, Pointing_Change, QL_DAY_PLOT
QL_ORBIT_PLOT, QL_PLOTTER, QL_READBDB, RD_GOES, RD_GOES_SDAC, RD_NEAR_PIN [1]
RD_NEAR_PIN [2], READCOL [3], READQUAL, READ_CONT, READ_DISCLA, READ_HXRS_FITS [1]
READ_HXRS_FITS [2], READ_HXRS_FITS [3], READ_MINICAT, READ_MONTH_CAT
READ_OCC_DISCSP, RESTORE_QLOOK, ROLL_PLOT, Radio Spectrogram FITS File reader
Radiospectrogram FITS File reader [1]
Radiospectrogram FITS File reader [2], SET_UTAXIS, SITE__DEFINE
SOLB_PLOT_POINTING [1], SOLB_PLOT_POINTING [2], SOLB_READ_REPOINT [1]
SOLB_READ_REPOINT [2], SOLB_SPACECRAFT_POINTING [1]
SOLB_SPACECRAFT_POINTING [2], SOLEPHUT, SPARTAN_PLANNER, SPECPLOT__DEFINE
SPECTRA2FITS, SPECTROGRAM CLASS DEFINITION, SPECTRUM CLASS DEFINITION
SPEX_COMMONS [2], SPEX_COMMONS [4], SPEX_DATA_GENX [1], SPEX_DATA_GENX [2]
SPEX_DRM__DEFINE, SPEX_FITINT__DEFINE, SPEX_GEN__DEFINE, SPEX_PROC [1]
SPEX_PROC [2], SPEX_SAVE [1], SPEX_SAVE [2], SPEX__DEFINE, STEREO_SIMUL
SXT_BAKEOUT_IN, SXT_COVERAGE, SXT_ECLIPSE, SXT_EXPOSURE_MAP, Shers_load [1]
TEMP_BCK_TIME_INTV, TEST_CAL, TIM2CARR, TIMESTAMP, TIME_AXIS__DEFINE, TIME_F_NAME
TJD2YMD, TOK_RD_DAILY, TRACE_ALIGN_CUBE, TRACE_COPY, TRACE_CUBE_POINTING
TRACE_GBO, TRACE_MDI_ALIGN, TRACE_SSWHERE [1], TV_SYNOP, TWIDGET, TYKW_RDT2TIMEJ
TYKW_RD_DAILY, TYKW_RD_DAT, UNFORMAT_INTERVALS, UPDATE_HTML, UTIME [1], UTIME [2]
UTPLOT_IMAGE, UTPLOT__DEFINE, UT_2_YYDOY [1], VIEW_TRACE_MOSAIC, WRITE_MONTH_CAT
XSM_VALID, XYPLOT__DEFINE, YMD2TJD, YOHKOH_TERM_PREDICT, ZDEROTATE, ZHDRUNIT
accum_counts [1], accum_counts [2], anahead2struct, anytim2weekinfo
auto_bck_find0, avsig_1 [1], avsig_1 [4], avsig_1 [6], avsig_temp
batse_create_html, batse_sea_html, check_cals, cp_catwidget, cw_ut_range
data2files, days_til_next_solar_max, db_gbo, decode_gev, default_rate_header
difference_movie, disp_sci160k [1], disp_sci160k [2], doytim2ints
drm_4_spex [1], drm_4_spex [2], eit_fulldisk, eit_proton_summary, evt_grid
find_uvexp, fix_decon_pits, fixinate_trace, flare_hist, get_acedata
get_epoch_sfcs [1], get_epoch_sfcs [2], get_gevloc_data, get_goes_defsat [1]
get_goes_defsat [2], get_infox, get_solar_indices, get_utevent [1]
get_utevent [2], get_utrange, go_sxt_sss2secondary, go_yo_prod_batch
goes_plot [1], goes_plot [2], goes_plot [3], goes_plot [4], goes_plot [5]
grid_data [1], grid_data [2], gtab_summary, gtt_orbit, has_overlap [1]
has_overlap [2], hsi_1orbit_allpak, hsi_anytim_2_filename, hsi_as_sim
hsi_as_sim_packet, hsi_aspect [1], hsi_aspect [2], hsi_ast_seesource_time
hsi_ast_sourceangle, hsi_atten_state, hsi_bad_pak, hsi_badpak_test
hsi_bproj2size, hsi_chk_obj, hsi_cld_sav_init, hsi_clk_delta_calc
hsi_clock_drift_dxdt, hsi_clock_drift_redo, hsi_clock_drift_soc
hsi_create_filedb, hsi_cw_ut_range, hsi_data_recovery_fraction
hsi_decimation_anomaly, hsi_default_resolutions, hsi_default_tailfracs
hsi_demodulator [1], hsi_do_qlook_image [1], hsi_do_qlook_image [2]
hsi_earthangle, hsi_endfileinfo_fill, hsi_ephemeris__define
hsi_ephemeris_concat, hsi_ephemeris_fill, hsi_filedb__define [1]
hsi_filedb__define [2], hsi_filedb_filename, hsi_filedb_read [1]
hsi_filedb_read [2], hsi_filedb_write, hsi_filedb_write_ascii
hsi_filename_2_anytim, hsi_fits_header, hsi_flare2time, hsi_flare_flag
hsi_flare_id_assign, hsi_flare_id_check, hsi_flare_in_int, hsi_flare_list2ar
hsi_flare_list2goes [1], hsi_flare_list2goes [2], hsi_flare_list__define [1]
hsi_flare_list__define [2], hsi_flare_list_fill [1], hsi_flare_list_fill [2]
hsi_flare_position_image [1], hsi_flare_position_image [2], hsi_format_flare
hsi_full_sun_image [1], hsi_full_sun_image [2], hsi_gbo, hsi_get_e_edges [1]
hsi_get_orbit_info, hsi_get_total_time, hsi_getflare, hsi_image__getaxis [2]
hsi_image_plot, hsi_image_raw__define, hsi_imagefile_2_plotman
hsi_lambda_vs_t, hsi_last_id_write filename last_id, hsi_locate_flare [1]
hsi_locate_flare [3], hsi_mod_variance__define, hsi_mod_variance_concat
hsi_monthly_filename, hsi_mult_filedb_otp, hsi_mult_flare_list_inp
hsi_mult_qspec, hsi_new_spec_bck, hsi_night_bck, hsi_obs_flag
hsi_obs_summ_allrates [1], hsi_obs_summ_concat, hsi_obs_summ_fill [1]
hsi_obs_summ_fill [2], hsi_obs_summ_flag__define, hsi_obs_summ_flag_concat
hsi_obs_summ_otp, hsi_obs_summ_rate__define, hsi_obs_summ_rate_concat
hsi_obs_summ_soc__define, hsi_obs_summ_soc_concat, hsi_obs_summ_timarr
hsi_obs_summ_write, hsi_obs_summary__define [1], hsi_obs_summary__define [2]
hsi_obs_summary_adapter__define, hsi_obs_summary_concat, hsi_obs_times
hsi_ok_intv [1], hsi_ok_intv [2], hsi_onedatagap__define, hsi_orbpar4bck
hsi_params2script, hsi_particle_rate__define, hsi_particle_rate_concat
hsi_plot_flux, hsi_pmtras_lookup, hsi_print_decimation_state
hsi_qlook__define, hsi_qlook_call_ospex [1], hsi_qlook_call_ospex [2]
hsi_qlook_concat, hsi_qlook_image, hsi_qlook_monitor_rate__define
hsi_qlook_packet_rate__define, hsi_qlook_pointing__define
hsi_qlook_rate_per_det__define, hsi_qlook_roll_angle__define
hsi_qlook_roll_period__define, hsi_qlook_spectrum
hsi_qlook_spin_axis__define, hsi_qspec [1], hsi_qspec [2], hsi_rd_ephfile
hsi_rd_orbit_files, hsi_rdstatevectorfile, hsi_read_all_flare_list
hsi_read_vcfiletimes, hsi_replace_flare_list, hsi_select_flare
hsi_show_flags [2], hsi_show_flare_on_image, hsi_sim_pflux_2_cflux
hsi_spectrogramACCBIN [2], hsi_spectrogram__define [1]
hsi_spectrogram__define [2], hsi_spectrogram__define [3]
hsi_spectrogram__get_obs [1], hsi_spectrogram__livetime [1]
hsi_spectrum__filewrite, hsi_spectrum__fitswrite, hsi_ssr_fill_per_orbit [1]
hsi_state_vectors, hsi_test_files, hsi_test_packet_rate, hsi_test_qlook
hsi_time_widget, hsi_ui_flarecat, hsi_ui_img, hsi_ui_img_doimage [1]
hsi_ui_img_doimage [2], hsi_ui_lc, hsi_ui_obs, hsi_ui_qlimage, hsi_ui_spec
hsi_vcfile_gaps, hsi_vis_fwdfit, hsi_whichflare, hsi_whole_flare_list
hsi_write_all_flare_list, hsi_write_decimation_settings
hsi_write_txt_flare_list, hsi_xy_test [1], hsi_xy_test [2], hsi_xy_test_new
hxrbs_response, hxrs_drm2fits [1], hxrs_drm2fits [2], hxrs_drm2fits [3]
image2movie, imspec [10], imspec [11], imspec [12], imspec [13], imspec [14]
imspec [15], imspec [16], imspec [17], imspec [18], imspec [19], imspec [1]
imspec [20], imspec [21], imspec [22], imspec [23], imspec [24], imspec [25]
imspec [26], imspec [27], imspec [28], imspec [29], imspec [2], imspec [30]
imspec [31], imspec [32], imspec [33], imspec [34], imspec [35], imspec [36]
imspec [3], imspec [4], imspec [5], imspec [6], imspec [7], imspec [8], imspec [9]
index2fov, kluge_att, lasco_time2file, lasco_time2nrlwww, lastgki, later, lcur_image
les_archive_info, make_goes_chianti_response [1]
make_goes_chianti_response [2], make_goes_chianti_response [3]
make_goes_chianti_response [4], make_grid_sphere, map2index, mark_intervals
may_eclipse, mdi_time2file, mees_log_read, mees_name_format, mk_mdi_fits
mk_sff_pair [1], mk_sff_pair [2], mk_ssc [1], mk_ssc [2], mk_ssc_batch [1]
mk_ssc_batch [2], mk_sumer_dbase_ff, mk_synsfc_coeff [1], mk_synsfc_coeff [2]
mksort, mon_sci5k, mrdfits_spectra, norh_alpha, norh_t2azel, op_term_score
option_changer [1], option_changer [2], parse_atime [2], pctime2ssw
phoenix_filedb_get, phoenix_spg_get, plot_ace, plot_fov [1], plot_goes_ospex
plotman, plotman_draw_event, plotman_setaxes, plotman_zoom, pmtras_analysis
pr_his_index [1], pr_his_index [2], pr_his_index [3], ptim, rapp_get_spectrogram
rd_goesp_ascii, rd_goesx_ascii, rd_mdi [1], rd_mdi [2], rd_sxs_pha [1]
rd_sxs_pha [2], rd_therm_rs232, rd_wbs_pha [1], rd_wbs_pha [2], rdbda_smm
read_eit, read_genxcat, read_hessi_4_ospex, read_hessi_4_spex [1]
read_hessi_4_spex [2], read_hessi_fits_4_spex [1]
read_hessi_fits_4_spex [2], read_lapalma, read_mdi, read_soxs_4_ospex
read_trace, read_xsm_4_ospex, read_yohkoh_4_spex [1], read_yohkoh_4_spex [2]
redo_disploi, redo_mon_sci5k, rhessi_get_spin_axis_position, save_idl_routines
sec_name_format, soxs_readfile, special_movie, spectro_plot2
spectrogram__define, spex_bk__define, spex_bkint__define, spex_bksub__define
spex_data__define, spex_evnt [1], spex_evnt [2], spex_hessi_image__define
spex_image__define, ssc_files [1], ssc_files [2], ssc_files [3], ssw_build_trace
ssw_composite, ssw_deltat, ssw_expand_times, ssw_flare_locator, ssw_fov_context
ssw_fs_cat2db, ssw_getcme_cactus, ssw_getcme_cdaw, ssw_getdst
ssw_gxd_remove_flares, ssw_javamovie, ssw_nar2armurl, ssw_pos2zenith
ssw_sec_aktxt2struct, ssw_time2filelist, ssw_time2paths, ssw_timestat
ssw_track_fov, sswdb_files, sswstruct_fill [1], stt_plot, sxi_files, sxt_files
sxt_his2dbase, sxt_is_synsfc, sxt_mk3 mk3 index data [1]
sxt_mk3 mk3 index data [2], sxt_orhis, sxt_prep [1], sxt_prep [2], sxt_prep [3]
sxt_ssn2fits [1], sxt_uvf_info [1], sxt_uvf_info [3], t_utplot [1], t_utplot [2]
time_at_meridian, time_window, timegrid, tr_lut_conv, tr_rd_index
tr_wrt_fits_i1 [2], trace_cosmic2hist_accum, trace_files, trace_get_vignette
trace_goodobs, trace_movie_index [1], trace_movie_index [2]
trace_recent_movie_summary, trace_sswhere [2], trace_sswhere [3]
trace_sswhere [4], trace_wave2point, ut_2_yydoy [2], ut_label, valid_time_range
wbs_response [1], wbs_response [2], week_loop [1], week_loop [2], week_loop [3]
weeks_in_year [1], weeks_in_year [2], where_are [1], where_are [2]
which_hessi_version, write_genxcat, xy2lonlat, xzchange, yo_index2path
yoh_orb_interp [1], yoh_orb_interp [2], yohkoh_files, yohkoh_legacy_files [1]
yohkoh_legacy_files [2], zcheck_hdr, zmovify, ztrack
Procedure: ANYTIM_SEC_TEST
Purpose: This function returns 1 if it detects an anytim seconds format.
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NAME:
anytim
PURPOSE:
This function converts one of several recognized time formats into the selected
output format.
CALLING SEQUENCE:
xx = anytim(roadmap, out_styl='ints')
or
xx = anytim(roadmap, /INTS)
xx = anytim('12:33 5-Nov-91', out_sty='ex')
or
xx = anytim('12:33 5-Nov-91', /EX)
xx = anytim('12:33 91/11/5',/EX)
xx = anytim([0, 4000], out_style= 'sec')
or
xx = anytim([0, 4000], /SEC)
CATEGORY:
Time, Utplot, time conversions
INPUT:
item - The input time
Form can be
(1) structure with a .time and .day
tags, those tags may also appear in a .gen tag
which is the first tag of the top structure,
if one element in structure, will return scalar output
for 1-d datatypes, or
(2) the standard 7-element longword external (EX) representation [hh,mm,ss,msec,dd,mm,(yy)yy],
or (3) a string of the format "hh:mm dd-mmm-yy" or "yy/mm/dd",
or (4) a 2xN array where the two dimensions hold (MSOD, DS79),
.i.e. (MilliSecondsOfDay, DaySince 1-jan-1979), so called Internal Structure (INTS),
1-jan-1979 is {anytim2ints_full, time:0L, day:1L}
or (5) a double or float array of seconds from 1-jan-79.
1-d, single time element inputs, the EX or array form of INTS, i.e.
size(item) is [ 1, 7, 2, 7] or [1, 2, 3, 2] return scalar results for
/sec output.
N.B. Within other SSW procedures, notably those of CDS and probably others, the epoch
for double(single) precision seconds is NOT 00:00:00.00 1 January 1979. This
function DOES NOT work properly with times relative to other epochs. To work with
times with other epochs, there is normally a conversion routine to put the
time in unversal format, such as the UTC_INT or UTC_EXT format. Please see
the aaareadme.txt file in $SSW/gen/idl/time/aaareadme.txt
You'll find many useful time handling routines in
$SSW/gen/idl/time, $SSW/gen/idl/genutil, $SSW/gen/idl/utplot,
$SSW/gen/idl_libs/astron/...
!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!
N.B. 2 digit year representations in EX or String formats are interpreted between
years 1950 and 2049.
!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!
The UTC procedures, utc2int, str2utc, and int2utc are included using
CALL_FUNCTION so anytim will compile and work without these routines
and their subsequent calls to procedures in the utc directory.
Allowed formats include those supported under UTC code, see STR2UTC.PRO:
= A character string containing the date and time. The
target format is the CCSDS ASCII Calendar Segmented
Time Code format (ISO 8601), e.g.
"1988-01-18T17:20:43.123Z"
The "Z" is optional. The month and day can be
replaced with the day-of-year, e.g.
"1988-018T17:20:43.123Z"
Other variations include
"1988-01-18T17:20:43.12345"
"1988-01-18T17:20:43"
"1988-01-18"
"17:20:43.123"
Also, the "T" can be replaced by a blank, and the
dashes "-" can be replaced by a slash "/". This is
the format used by the SOHO ECS.
In addition this routine can parse dates where only
two digits of the year is given--the year is assumed
to be between 1950 and 2049.
Character string months, e.g. "JAN" or "January", can
be used instead of the number. In that case, it
assumes that the date is either in day-month-year or
month-day-year format, e.g. "18-JAN-1988" or
"Jan-18-1988". However, if the first parameter is
four digits, then year-month-day is assumed, e.g.
"1988-Jan-18".
Dates in a different order than year-month-day are
supported, but unless the month is given as a
character string, then these are only supported
through the /MDY and /DMY keywords.
End UTC documentation
CALLS: ***
ATIME [1], ATIME [2], CHECKVAR [1], DATATYPE [1], DATATYPE [2], DATATYPE [3]
Int2Ex [1], Int2Ex [2], UTIME [1], UTIME [2], Utime2str [1], Utime2str [2]
anytim2ints [1], anytim2ints [2], checkvar [2], gt_day [1], gt_day [2]
gt_time [1], gt_time [2], int2sec [1], int2sec [2], timstr2ex [1], timstr2ex [2]
CALLED BY:
ALIGN1BIGGRAM, ANYTIM_REPORT, BATSE_FLARES_WEEK, BATSE_ON, BATSE_SPEC_GAIN_FDB
BATSE_TIME_INPUT, BCS, Build_Schedule, CALC_LOI_ROLL, CALIBRATE [1], CARR2DATE
CARR2EX, CH2KVT, CH2KVT_GAIN, CHECK_FOR_30S, CHECK_OVERFLOW, CHECK_SFC_PNT, CHKPOINT
CLEAN_GOES, CONT_EDGES, CONT_READ, CP_CATREAD, CP_CATRESET, CP_CATTIME
CREATE_GIF_HTML, CREATE_HTML, CRYSTAL_RES, Create_update_tar, DATETIME OBJECT
DATPLOT, DISCSP_BANDS, DISCSP_EDGES, DISCSP_READ, DISPLOI_MON5K, DO_EVENTLISTS
DO_QLARCHIVE, DROT_NAR, ECI2GEOGRAPHIC, ECL_FRAC, EIT_COPY, EUTPLOT, FDBREAD
FILT_EVENTS, FIND_DBFILE, FIND_GOOD_OCCS, FIND_PACKET
FITS WRITER CLASS FOR ANY RHESSI DATA TYPES, FITS_TIME, FLIST, FLISTOC
FORMAT_INTERVALS, FSOC, FSPLOT, FS_ACC_CONT, FS_ACC_DISCSP, FS_GEN_ARR, FS_GRAPH
FS_OPEN [1], FS_READ_DD, Fits_spectra [1], Fits_spectra [2], GAP_FILE, GAP_FINDER
GEOGRAPHIC2ECI, GETGPSaVG [1], GETGPSaVG [2], GETSATaVG, GET_BATSE_POINTING
GET_DISCSP511, GET_DROT_DUR, GET_FITS_TIME, GET_LAD_GAIN, GET_NAR, GET_OCCS
GET_OCC_ONDAY, GET_SLLD, GET_SPEC_CAL, GET_SPEC_GAIN, GFITS_R, GFITS_W
GOES_CHIANTI_TEM, GOES_FITS_FILES, GOES_MEWE_TEM, GOES_TEM, GOES_TF, GOES_TF_COEFF
GOES_TRANSFER, GOES__DEFINE, GRS_EXTRACT, GRWCH_ST, HESSI
HESSI CALIBRATED EVENTLIST CLASS DEFINITION [3]
HESSI FASTRATE CLASS DEFINITION, HESSI IMAGE FILE CLASS DEFINITION [1]
HESSI IMAGE RAW CLASS DEFINITION [2]
HESSI IMAGE STRATEGY CLASS DEFINITION
HESSI MONITOR RATE CLASS DEFINITION
HESSI MULTI IMAGE CLASS DEFINITION [2]
HESSI MULTI IMAGE CLASS DEFINITION [3], HESSI PACKET FILE ABSTRACT CLASS
HESSI ROLL_DB CLASS DEFINITION, HESSI SIMULATION CLASS DEFINITION
HESSI SOHDATA CLASS DEFINITION, HESSI Search Lookup Table Index
HESSI_REF_TIME, HSI_ANY2SCTIME, HSI_ANY_SOHDATA, HSI_ASPECT_SIM
HSI_BUILD_OBS_TIME, HSI_CLKDELTAFILETIME_2_UT, HSI_CLK_DELTA_WRITE
HSI_CLOCK_DRIFT, HSI_DO_QLOOK_PLOTS, HSI_EVENTLIST_TEST, HSI_FITS2MAP [1]
HSI_GET_CLOCK_SYNCH, HSI_GET_TIMEBIN, HSI_IMAGE_TEST [2]
HSI_IMAGE_TEST__define, HSI_LOCATE_FLARE [2], HSI_LOCATE_FLARE [4]
HSI_MAP_EVALUATOR [1], HSI_MODEL_TO_SCORE, HSI_NOSAAN, HSI_NPAK_HISTOGRAM
HSI_ORBFILETIME_2_UT, HSI_PACKET2FITS, HSI_PAK2FILETIMES, HSI_QLOOK_ASPECT
HSI_QLOOK_SUMMARY_PAGE__DEFINE, HSI_RD_FITS_SPECTRUM, HSI_REF_TIME
HSI_SCORE2FILE, HSI_SCTIME2ANY, HSI_SEQ_CNT_CHECK, HSI_SET_FILE_TIME
HSI_SMEXHDR_RCVD_TIME, HSI_SPECTROGRAMCHAN_OVERLAP_FIX
HSI_SPECTROGRAM_DECIM_CORRECT, HSI_SPECTROGRAM_DECIM_TABLE
HSI_SPECTRUM__DEFINE, HSI_SRM__DEFINE, HSI_SSR_FILL_PER_ORBIT [2]
HSI_TIME_N_ORBITS, HSI_TOHBAN_FLARE_COUNTER, HSI_UT_2_CLKDELTAFILETIME
HSI_VCFILE_PACKET_RATE, HSI_VCFILE_TIMES, HSI_WRITE_LEVEL0, HSI_tplot2any
HXARCHIVE, HXFITS, HXR2FILE, HXRBS, HXRBS_ESC, HXRFITS_ARCHIVE, HXRFITS_HEAD
HXRS__DEFINE, HXT_CAL_FIX [1], HXT_CAL_FIX [2], Hessi_obs_summary
Hsi_contact2fits [1], Hsi_contact2fits [2], Hsi_daily_catalog [1]
Hsi_daily_catalog [2], Hsi_monitor_rate_read, LAY1GKM, LONLAT2XY, Load_sher
MAKE_SOLCALTRAJ, MDI__DEFINE, MERGE_DISCSP_HKG_OCC, MJD2ANY, MK_MER_CONT
NAR2COORD, NEAREST_GEV, NEAR_CONJ, NORH_F2EVF [1], NORH_F2EVF [2], NORH_FIXINDEX
NORH_IMG2IDX [1], NORH_IMG2IDX [2], NORH_JST2UT [1], NORH_JST2UT [2], NORH_MKSZ
NORH_PR_EVX [1], NORH_PR_EVX [2], NORH_PR_INFO [1], NORH_PR_INFO [2]
NORH_RD_TCX [1], NORH_RD_TCX [2], NORH_RD_TSX [1], NORH_RD_TSX [2]
NORH_SEL_DIFF [1], NORH_SEL_DIFF [2], NORH_SYNTH_BYF [1], NORH_SYNTH_BYF [2]
NORH_TCX2IDX [1], NORH_TCX2IDX [2], NORH_TIM2F [1], NORH_TIM2F [2]
NORH_TRANS_BYF [1], NORH_TRANS_BYF [2], NORH_UT2JST [1], NORH_UT2JST [2]
NORP_CLB_INTEG, NORP_CLB_SN, NORP_GT_NDATA, NORP_NCLB_TIME, NORP_RDT2DATA_17G
NORP_RDT2DATA_1G, NORP_RDT2DATA_2G, NORP_RDT2DATA_35G, NORP_RDT2DATA_4G
NORP_RDT2DATA_80G, NORP_RDT2DATA_9G, NORP_RDT2TIMEJ [1], NORP_RDT2TIMEJ [2]
NORP_RD_AVG [1], NORP_RD_AVG [2], NORP_RD_DAILY [1], NORP_RD_DAILY [2]
NORP_RD_DAT, NORP_RD_RDT, OCC_DBASE, ORBIT_DN, ORBIT_INPUT_TIME, PARSE_ATIME [1]
PARSE_GROSSC_ATTITUDE, PLOTBATSE, PLOTBATSE_QL, PLOT_HSI, PLOT_MAP, PLOT_OCCS
PLOT_OCC_ONDAY, PROFILES2, PR_PATROLS, PURGE_KAPS, Pointing_Change, QL_DAY_PLOT
QL_ORBIT_PLOT, QL_PLOTTER, QL_READBDB, RD_GOES, RD_GOES_SDAC, RD_NEAR_PIN [1]
RD_NEAR_PIN [2], READCOL [3], READQUAL, READ_CONT, READ_DISCLA, READ_HXRS_FITS [1]
READ_HXRS_FITS [2], READ_HXRS_FITS [3], READ_MINICAT, READ_MONTH_CAT
READ_OCC_DISCSP, RESTORE_QLOOK, ROLL_PLOT, Radio Spectrogram FITS File reader
Radiospectrogram FITS File reader [1]
Radiospectrogram FITS File reader [2], SET_UTAXIS, SITE__DEFINE
SOLB_PLOT_POINTING [1], SOLB_PLOT_POINTING [2], SOLB_READ_REPOINT [1]
SOLB_READ_REPOINT [2], SOLB_SPACECRAFT_POINTING [1]
SOLB_SPACECRAFT_POINTING [2], SOLEPHUT, SPARTAN_PLANNER, SPECPLOT__DEFINE
SPECTRA2FITS, SPECTROGRAM CLASS DEFINITION, SPECTRUM CLASS DEFINITION
SPEX_COMMONS [2], SPEX_COMMONS [4], SPEX_DATA_GENX [1], SPEX_DATA_GENX [2]
SPEX_DRM__DEFINE, SPEX_FITINT__DEFINE, SPEX_GEN__DEFINE, SPEX_PROC [1]
SPEX_PROC [2], SPEX_SAVE [1], SPEX_SAVE [2], SPEX__DEFINE, STEREO_SIMUL
SXT_BAKEOUT_IN, SXT_COVERAGE, SXT_ECLIPSE, SXT_EXPOSURE_MAP, Shers_load [1]
TEMP_BCK_TIME_INTV, TEST_CAL, TIM2CARR, TIMESTAMP, TIME_AXIS__DEFINE, TIME_F_NAME
TJD2YMD, TOK_RD_DAILY, TRACE_ALIGN_CUBE, TRACE_COPY, TRACE_CUBE_POINTING
TRACE_GBO, TRACE_MDI_ALIGN, TRACE_SSWHERE [1], TV_SYNOP, TWIDGET, TYKW_RDT2TIMEJ
TYKW_RD_DAILY, TYKW_RD_DAT, UNFORMAT_INTERVALS, UPDATE_HTML, UTIME [1], UTIME [2]
UTPLOT_IMAGE, UTPLOT__DEFINE, UT_2_YYDOY [1], VIEW_TRACE_MOSAIC, WRITE_MONTH_CAT
XSM_VALID, XYPLOT__DEFINE, YMD2TJD, YOHKOH_TERM_PREDICT, ZDEROTATE, ZHDRUNIT
accum_counts [1], accum_counts [2], anahead2struct, anytim2weekinfo
auto_bck_find0, avsig_1 [1], avsig_1 [4], avsig_1 [6], avsig_temp
batse_create_html, batse_sea_html, check_cals, cp_catwidget, cw_ut_range
data2files, days_til_next_solar_max, db_gbo, decode_gev, default_rate_header
difference_movie, disp_sci160k [1], disp_sci160k [2], doytim2ints
drm_4_spex [1], drm_4_spex [2], eit_fulldisk, eit_proton_summary, evt_grid
find_uvexp, fix_decon_pits, fixinate_trace, flare_hist, get_acedata
get_epoch_sfcs [1], get_epoch_sfcs [2], get_gevloc_data, get_goes_defsat [1]
get_goes_defsat [2], get_infox, get_solar_indices, get_utevent [1]
get_utevent [2], get_utrange, go_sxt_sss2secondary, go_yo_prod_batch
goes_plot [1], goes_plot [2], goes_plot [3], goes_plot [4], goes_plot [5]
grid_data [1], grid_data [2], gtab_summary, gtt_orbit, has_overlap [1]
has_overlap [2], hsi_1orbit_allpak, hsi_anytim_2_filename, hsi_as_sim
hsi_as_sim_packet, hsi_aspect [1], hsi_aspect [2], hsi_ast_seesource_time
hsi_ast_sourceangle, hsi_atten_state, hsi_bad_pak, hsi_badpak_test
hsi_bproj2size, hsi_chk_obj, hsi_cld_sav_init, hsi_clk_delta_calc
hsi_clock_drift_dxdt, hsi_clock_drift_redo, hsi_clock_drift_soc
hsi_create_filedb, hsi_cw_ut_range, hsi_data_recovery_fraction
hsi_decimation_anomaly, hsi_default_resolutions, hsi_default_tailfracs
hsi_demodulator [1], hsi_do_qlook_image [1], hsi_do_qlook_image [2]
hsi_earthangle, hsi_endfileinfo_fill, hsi_ephemeris__define
hsi_ephemeris_concat, hsi_ephemeris_fill, hsi_filedb__define [1]
hsi_filedb__define [2], hsi_filedb_filename, hsi_filedb_read [1]
hsi_filedb_read [2], hsi_filedb_write, hsi_filedb_write_ascii
hsi_filename_2_anytim, hsi_fits_header, hsi_flare2time, hsi_flare_flag
hsi_flare_id_assign, hsi_flare_id_check, hsi_flare_in_int, hsi_flare_list2ar
hsi_flare_list2goes [1], hsi_flare_list2goes [2], hsi_flare_list__define [1]
hsi_flare_list__define [2], hsi_flare_list_fill [1], hsi_flare_list_fill [2]
hsi_flare_position_image [1], hsi_flare_position_image [2], hsi_format_flare
hsi_full_sun_image [1], hsi_full_sun_image [2], hsi_gbo, hsi_get_e_edges [1]
hsi_get_orbit_info, hsi_get_total_time, hsi_getflare, hsi_image__getaxis [2]
hsi_image_plot, hsi_image_raw__define, hsi_imagefile_2_plotman
hsi_lambda_vs_t, hsi_last_id_write filename last_id, hsi_locate_flare [1]
hsi_locate_flare [3], hsi_mod_variance__define, hsi_mod_variance_concat
hsi_monthly_filename, hsi_mult_filedb_otp, hsi_mult_flare_list_inp
hsi_mult_qspec, hsi_new_spec_bck, hsi_night_bck, hsi_obs_flag
hsi_obs_summ_allrates [1], hsi_obs_summ_concat, hsi_obs_summ_fill [1]
hsi_obs_summ_fill [2], hsi_obs_summ_flag__define, hsi_obs_summ_flag_concat
hsi_obs_summ_otp, hsi_obs_summ_rate__define, hsi_obs_summ_rate_concat
hsi_obs_summ_soc__define, hsi_obs_summ_soc_concat, hsi_obs_summ_timarr
hsi_obs_summ_write, hsi_obs_summary__define [1], hsi_obs_summary__define [2]
hsi_obs_summary_adapter__define, hsi_obs_summary_concat, hsi_obs_times
hsi_ok_intv [1], hsi_ok_intv [2], hsi_onedatagap__define, hsi_orbpar4bck
hsi_params2script, hsi_particle_rate__define, hsi_particle_rate_concat
hsi_plot_flux, hsi_pmtras_lookup, hsi_print_decimation_state
hsi_qlook__define, hsi_qlook_call_ospex [1], hsi_qlook_call_ospex [2]
hsi_qlook_concat, hsi_qlook_image, hsi_qlook_monitor_rate__define
hsi_qlook_packet_rate__define, hsi_qlook_pointing__define
hsi_qlook_rate_per_det__define, hsi_qlook_roll_angle__define
hsi_qlook_roll_period__define, hsi_qlook_spectrum
hsi_qlook_spin_axis__define, hsi_qspec [1], hsi_qspec [2], hsi_rd_ephfile
hsi_rd_orbit_files, hsi_rdstatevectorfile, hsi_read_all_flare_list
hsi_read_vcfiletimes, hsi_replace_flare_list, hsi_select_flare
hsi_show_flags [2], hsi_show_flare_on_image, hsi_sim_pflux_2_cflux
hsi_spectrogramACCBIN [2], hsi_spectrogram__define [1]
hsi_spectrogram__define [2], hsi_spectrogram__define [3]
hsi_spectrogram__get_obs [1], hsi_spectrogram__livetime [1]
hsi_spectrum__filewrite, hsi_spectrum__fitswrite, hsi_ssr_fill_per_orbit [1]
hsi_state_vectors, hsi_test_files, hsi_test_packet_rate, hsi_test_qlook
hsi_time_widget, hsi_ui_flarecat, hsi_ui_img, hsi_ui_img_doimage [1]
hsi_ui_img_doimage [2], hsi_ui_lc, hsi_ui_obs, hsi_ui_qlimage, hsi_ui_spec
hsi_vcfile_gaps, hsi_vis_fwdfit, hsi_whichflare, hsi_whole_flare_list
hsi_write_all_flare_list, hsi_write_decimation_settings
hsi_write_txt_flare_list, hsi_xy_test [1], hsi_xy_test [2], hsi_xy_test_new
hxrbs_response, hxrs_drm2fits [1], hxrs_drm2fits [2], hxrs_drm2fits [3]
image2movie, imspec [10], imspec [11], imspec [12], imspec [13], imspec [14]
imspec [15], imspec [16], imspec [17], imspec [18], imspec [19], imspec [1]
imspec [20], imspec [21], imspec [22], imspec [23], imspec [24], imspec [25]
imspec [26], imspec [27], imspec [28], imspec [29], imspec [2], imspec [30]
imspec [31], imspec [32], imspec [33], imspec [34], imspec [35], imspec [36]
imspec [3], imspec [4], imspec [5], imspec [6], imspec [7], imspec [8], imspec [9]
index2fov, kluge_att, lasco_time2file, lasco_time2nrlwww, lastgki, later, lcur_image
les_archive_info, make_goes_chianti_response [1]
make_goes_chianti_response [2], make_goes_chianti_response [3]
make_goes_chianti_response [4], make_grid_sphere, map2index, mark_intervals
may_eclipse, mdi_time2file, mees_log_read, mees_name_format, mk_mdi_fits
mk_sff_pair [1], mk_sff_pair [2], mk_ssc [1], mk_ssc [2], mk_ssc_batch [1]
mk_ssc_batch [2], mk_sumer_dbase_ff, mk_synsfc_coeff [1], mk_synsfc_coeff [2]
mksort, mon_sci5k, mrdfits_spectra, norh_alpha, norh_t2azel, op_term_score
option_changer [1], option_changer [2], parse_atime [2], pctime2ssw
phoenix_filedb_get, phoenix_spg_get, plot_ace, plot_fov [1], plot_goes_ospex
plotman, plotman_draw_event, plotman_setaxes, plotman_zoom, pmtras_analysis
pr_his_index [1], pr_his_index [2], pr_his_index [3], ptim, rapp_get_spectrogram
rd_goesp_ascii, rd_goesx_ascii, rd_mdi [1], rd_mdi [2], rd_sxs_pha [1]
rd_sxs_pha [2], rd_therm_rs232, rd_wbs_pha [1], rd_wbs_pha [2], rdbda_smm
read_eit, read_genxcat, read_hessi_4_ospex, read_hessi_4_spex [1]
read_hessi_4_spex [2], read_hessi_fits_4_spex [1]
read_hessi_fits_4_spex [2], read_lapalma, read_mdi, read_soxs_4_ospex
read_trace, read_xsm_4_ospex, read_yohkoh_4_spex [1], read_yohkoh_4_spex [2]
redo_disploi, redo_mon_sci5k, rhessi_get_spin_axis_position, save_idl_routines
sec_name_format, soxs_readfile, special_movie, spectro_plot2
spectrogram__define, spex_bk__define, spex_bkint__define, spex_bksub__define
spex_data__define, spex_evnt [1], spex_evnt [2], spex_hessi_image__define
spex_image__define, ssc_files [1], ssc_files [2], ssc_files [3], ssw_build_trace
ssw_composite, ssw_deltat, ssw_expand_times, ssw_flare_locator, ssw_fov_context
ssw_fs_cat2db, ssw_getcme_cactus, ssw_getcme_cdaw, ssw_getdst
ssw_gxd_remove_flares, ssw_javamovie, ssw_nar2armurl, ssw_pos2zenith
ssw_sec_aktxt2struct, ssw_time2filelist, ssw_time2paths, ssw_timestat
ssw_track_fov, sswdb_files, sswstruct_fill [1], stt_plot, sxi_files, sxt_files
sxt_his2dbase, sxt_is_synsfc, sxt_mk3 mk3 index data [1]
sxt_mk3 mk3 index data [2], sxt_orhis, sxt_prep [1], sxt_prep [2], sxt_prep [3]
sxt_ssn2fits [1], sxt_uvf_info [1], sxt_uvf_info [3], t_utplot [1], t_utplot [2]
time_at_meridian, time_window, timegrid, tr_lut_conv, tr_rd_index
tr_wrt_fits_i1 [2], trace_cosmic2hist_accum, trace_files, trace_get_vignette
trace_goodobs, trace_movie_index [1], trace_movie_index [2]
trace_recent_movie_summary, trace_sswhere [2], trace_sswhere [3]
trace_sswhere [4], trace_wave2point, ut_2_yydoy [2], ut_label, valid_time_range
wbs_response [1], wbs_response [2], week_loop [1], week_loop [2], week_loop [3]
weeks_in_year [1], weeks_in_year [2], where_are [1], where_are [2]
which_hessi_version, write_genxcat, xy2lonlat, xzchange, yo_index2path
yoh_orb_interp [1], yoh_orb_interp [2], yohkoh_files, yohkoh_legacy_files [1]
yohkoh_legacy_files [2], zcheck_hdr, zmovify, ztrack
OPTIONAL KEYWORD INPUT:
out_style - Output representation, specified by a string:.r ../anytim
INTS - structure with [msod, ds79] - day 0 N.B. 31-dec-1978
IDL> help,/st,anytim('1-jan-1979',/ints)
** Structure ANYTIM2INTS_FULL, 2 tags, length=8, data length=8:
TIME LONG 0
DAY LONG 1
STC - same as INTS
2XN - longword array [msod,ds79] X N
EX - 7 element external representation (hh,mm,ss,msec,dd,mm,yyyy)
UTIME - Utime format, Real*8 seconds since 1-jan-79, DEFAULT!!!!
SEC - same as Utime format
SECONDS - same as Utime format
TAI - standard seconds from 1-jan-1958. Includes leap seconds unlike "SECONDS" output.
NB- The TAI format cannot be used as an input to ANYTIM because it will be interpreted as
number of days (in seconds) from 1-jan-1979.
ATIME - Variable Atime format, Yohkoh
Yohkoh style - 'dd-mon-yy hh:mm:ss.xxx' or
HXRBS pub style - 'yy/mm/dd, hh:mm:ss.xxx'
depending on atime_format set by
hxrbs_format or yohkoh_format
YOHKOH - yohkoh style string
HXRBS - HXRBS Atime format /pub, 'yy/mm/dd, hh:mm:ss.xxx'
YY/MM/DD- same as HXRBS
MJD - UTC-type structure
= The UTC date/time as a data structure with the
elements:
MJD = The Modified Julian Day number
TIME = The time of day, in milliseconds
since the start of the day.
Both are long integers.
UTC_INT - Same as MJD
UTC_EXT - UTC external format, a structure
containing the elements, YEAR, MONTH, DAY, HOUR, MINUTE,
SECOND, and MILLISECOND as shortword integers.
CCSDS - A string variable containing the calendar date in the
format recommended by the Consultative Committee for
Space Data Systems (ISO 8601), e.g.
"1988-01-18T17:20:43.123Z"
ECS - A variation on the CCSDS format used by the EOF Core
System. The "T" and "Z" separators are eliminated, and
slashes are used instead of dashes in the date, e.g.
"1988/01/18 17:20:43.123"
VMS - Similar to that used by the VMS operating system, this
format uses a three-character abbreviation for the
month, and rearranges the day and the year, e.g.
"18-JAN-1988 17:20:43.123"
STIME - Based on !STIME in IDL, this format is the same as the
second accuracy, e.g.
VMS format, except that the time is only given to 0.01
second accuracy, e.g.
"18-JAN-1988 17:20:43.12"
SYSTEM - Based on IDL's system time, seconds from 1-jan-1970
TAI - another seconds from time specification. This time from
1-jan-1958 including leap seconds
or by keywords
/ints -
/stc
/_2xn
/external
/utime
/seconds
/atimes
/yohkoh
/hxrbs
/yymmdd
/mjd
/utc_int
/utc_ext
/ccsds
/ecs
/vms
/stime
/TAI
mdy - If set, use the MM/DD/YY order for converting the string date
date_only - return only the calendar date portion,
e.g. anytim('93/6/1, 20:00:00',/date_only,/hxrbs) ==> '93/06/01'
time_only - return only the time of day portion
e.g. anytim('93/6/1, 20:00:00',/time_only,/hxrbs) ==> '20:00:00.000'
truncate - truncate the msec portion of the time displayed in strings.
FIDUCIAL - string input
If the string contains 'tai' or 'sys' then the fiducial used to interpret
seconds input and output is changed from the default one of 1-jan-1979 to
1-jan-1970 or 1-jan-1958 respectively. Otherwise the 1-jan-1979 epoch is
used to reference double precision floating point values.
ORDINATE - the number of elements in this variable is compared to the number of elements
in item if item is an integer format. If the ratio of number of elements is 2 or 7 then
the routine will interpret item as being in the 2xN or 7xN formats
keyword output:
error - set if an error, dummy for now, ras 18-Nov-93
restrictions:
one dimensional or scalar longwords will be interpreted as
double precision seconds unless they have either two or seven
elements
Should not be used to interpret an array of mixed string formats.
If the formats are mixed then the array should be processed element by element.
HISTORY:
Written 31-Oct-93 ras
modified 4-jan-94 ras, made argument recognition more robust
also made output dimensions similar for /yohkoh and /hxrbs
modified 25-jan-94 ras, made SEC or SECONDS work
ras 30-jan-94, fixed string outputs for /date and /time
ras 9-feb-94, fixed typo
ras 15-jun-1995, integrated Bill Thompson's UTC formats, for input and output
start adjusting to 4 digit years
ras, 20-jun-1995, put calls to utc functions inside call_function to reduce need
to include utc directories, default structure is Yohkoh as before,
utc structures are tested for explicitly
ras, 23-jun-1995, stopped searching for 'T' to identify CCSDS format, now 'Z'
made sear for 4 digit year more exacting
ras, 28-jul-95, restored item using item_old if necessary
Version 11, ras, 27-mar-1997, added truncate keyword
Version 12, ras, 16-jul-1997, fixed truncation problem with date strings
using atime, yohkoh, hxrbs, or yymmdd keywords.
Version 13, richard.schwartz@gsfc.nasa.gov
1. Supports input and output of 4 digit years.
2. Longword support on all integer day structures.
3. No modulo reduction of ex year format.
4. Simplify structure checking for input.
Version 14, richard.schwartz@gsfc.nasa.gov, 24-oct-1997, cleared bug in checking tags
in structure inhibiting finding of yohkoh gen tag. Bug put in on mod 13.
Version 15, richard.schwartz@gsfc.nasa.gov, 28-oct-1997, DATE and TRUNCATE
keywords can be used together with vms, ecs, and stime output format
without producing null strings, same effect as using only DATE keyword.
Version 16, richard.schwartz@gsfc.nasa.gov, 30-oct-1997, change
time and date keywords to time_only and date_only for consistency
with SSW/gen/idl/time routines by W. Thompson.
Version 17, richard.schwartz@gsfc.nasa.gov, 16-Mar-1998, scalar output for EX format
in only 1-D array.
Version 18, richard.schwartz@gsfc.nasa.gov, 20-Apr-1998, added TAI output and supports
'hh:mm:ss.xxx yy/mm/dd' now.
Version 19, richard.schwartz@gsfc.nasa.gov, 13-aug-1998, route 4+ month strings to STR2UTC.
Version 20, richard.schwartz@gsfc.nasa.gov, 9-sep-1998, converts 2 digit years in EXternal format to
4 digit years using 1950-2049 window.
Version 21, richard.schwartz@gsfc.nasa.gov, 24-oct-1998, passes double and single precision seconds through
unchanged except float converted to double.
Version 22, richard.schwartz@gsfc.nasa.gov, 12-nov-1999, uses error code in str2utc to trap errors for that
function.
Version 23, richard.schwartz@gsfc.nasa.gov, 15-dec-1999, handle strings like dd/mon/yy with STR2UTC.
Version 23, richard.schwartz@gsfc.nasa.gov, 20-jun-2000. Fixed problem with non 1d structures. Now
it can handle them and return the same dimensions.
Version 24, richard.schwartz@gsfc.nasa.gov, 16-feb-2001. Made compatible with new timstr2ex.
Version 25, richard.schwartz@gsfc.nasa.gov, 2-apr-2001. Use input dimensions for output as default
when possible, that is for all input/output formats except 2xN and 7xN int and longword. Also, treat
single element string arrays as scalars for output.
Version 26, richard.schwartz@gsfc.nasa.gov, 14-jun-2001. unsigned and double long integers
are now supported identically to normal integers within anytim.
1-jul-2001, richard.schwartz@gsfc.nasa.gov, replace [0] with (0)
2-jul-2002, richard.schwartz@gsfc.nasa.gov, changed documentation re fiducial for
INTS (STC) output and input formats.
8-sep-2005, richard.schwartz@gsfc.nasa.gov, fix longword input for seconds roundoff
problem.
21-dec-2005, richard.schwartz@gsfc.nasa.gov, added FIDUCIAL to allow switching
time bases from idl system of 1-jan-1970, to hxrbs standard 1-jan-1979, or tai system
starting 1-jan-1958 but including leap seconds
6-jan-2006, added test routine for determining seconds input format. Assumes that floats and
doubles are seconds as before, organizes the acceptance of integer formats better. Integers
are accepted as long as they aren't blocked 2xN or 7xN which are assumed to be special
integer formats EXTERNAL and _2xn, added keyword ordinate which can be used
with item to eliminate ambiguity of the integer formats.
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Project : SOHO - CDS
Name : ANYTIM2CAL()
Purpose : Converts (almost) any time format to calendar format.
Explanation : Tests the type of input and tries to use the appropriate
conversion routine to create the date/time in a user
selectable calendar format for, for example, printing in
documents, tables etc.
Use : IDL> utc = anytim2cal(any_format, form=xx)
Inputs : any_format - date/time in any of the acceptable CDS
time formats -- for acceptable formats see file
aaareadme.txt.
Opt. Inputs : None
Outputs : Function returns string array in format requested.
Opt. Outputs: None
Keywords :
FORM = n where...
n output format
0 dd/mmm/yy hh:mm:ss [default]
1 dd-mmm-yy hh:mm:ss
2 dd/mm/yy hh:mm:ss
3 dd-mm-yy hh:mm:ss
4 mm/dd/yy hh:mm:ss
5 mm-dd-yy hh:mm:ss
6 yy/mm/dd hh:mm:ss
7 yy-mm-dd hh:mm:ss
8 yyyymmddhhmmss
9 dd-mmm-yyyy hh:mm:ss.sss (VMS-like)
10 dd-mmm-yyyy hh:mm:ss.ss (!stime-like)
11 yyyy/mm/dd hh:mm:ss.sss (cpt use)
etc TBD
DATE - Output only the date in format above.
TIME - Output only the time in format above.
MSEC - Include milliseconds in the "ss" fields above (="ss.sss").
ERRMSG - If defined and passed, then any error messages will be returned
to the user in this parameter rather than being printed to
the screen. If no errors are encountered, then a null string
is returned. In order to use this feature, the string ERRMSG
must be defined first, e.g.,
ERRMSG = ''
ANYTIM2CAL, DT, ERRMSG=ERRMSG, ...
IF ERRMSG NE '' THEN ...
Calls : ***
ANYTIM2UTC [1], ANYTIM2UTC [2], CHECK_EXT_TIME, PRINT_STR, SAFE_STRING, TRIM
UTC2STR
CALLED BY:
ANYTIM2UTC [1], ANYTIM2UTC [2], CAT_FITS, CDS_VEL_SLICE [1], CHIANTI_NE
CHIANTI_TE, CH_LINE_LIST, DROT_COORD, DROT_RASTER, EIS_CPT_COMMAND_STORE_ADD [1]
EIS_CPT_COMMAND_STORE_ADD [2], EIS_CPT_DAISY_CHAIN [1]
EIS_CPT_DAISY_CHAIN [2], EIS_CPT_DATARATE_OUTPUT [1]
EIS_CPT_DATARATE_OUTPUT [2], EIS_CPT_DATA_RATE_PROCESS [1]
EIS_CPT_DATA_RATE_PROCESS [2], EIS_CPT_NOW [1], EIS_CPT_NOW [2]
EIS_CPT_OBSTBL [1], EIS_CPT_OBSTBL [2], EIS_CPT_TIMEFORMAT [1]
EIS_CPT_TIMEFORMAT [2], EIS_CPT_TIMELINE_ITEM_OUTPUT [1]
EIS_CPT_TIMELINE_ITEM_OUTPUT [2], EIT_DAILY, EIT_PREP, EXPORT_PLAN
GET_CDS_TEMPS, GET_ORBIT [1], GET_ORBIT [2], GET_ORBIT_CDF, GET_ORBIT_CDF2
GET_ORBIT_FITS, GET_SC_ATT [1], GET_SC_ATT [2], LIST_FITS, MK_SYNOPTIC
ORBIT_FILE_TYPE, PLOT_HKLZ, QCALIB, QWAVECAL, READ_FULL_ATT, READ_SC_ATT, SHOW_CDHS
SHOW_PLAN, SHOW_SYNOPTIC, TP_WRT_IEF, WPLOT_NONOP, WPLOT_SUBHTR [2], ch_ss
eis_cpt_gui [1], eis_cpt_gui [2], eis_dr_obj__DEFINE [1]
eis_dr_obj__DEFINE [2], eis_ti2utc [1], eis_ti2utc [2], sgt_raster_time
Common : None
Restrictions: None
Side effects: If no parameters are passed, ERRMSG is returned as a string
array. If any other error occurs and ERRMSG is set, ERRMSG
is returned as a string of '-1'.
Category : Util, time
Prev. Hist. : None
Written : C D Pike, RAL, 24-May-94
Modified : Version 1, C.D. Pike, RAL, 24 May 1994
Version 2, Donald G. Luttermoser, GSFC/ARC, 20 December 1994
Added the keyword ERRMSG. Added forms 4 and 5.
Version 3, CDP, make work with vector input and
added formats 6 & 7. 5-Jan-95
Version 4, CDP, fix round off giving 60 in seconds field.
23-Jan-95
Version 5, William Thompson, GSFC, 25 January 1995
Changed to call intrinsic ROUND instead of NINT. The
version of NINT in the Astronomy User's Library doesn't
automatically select between short and long integers as
the CDS version does.
Version 6, Donald G. Luttermoser, GSFC/ARC, 30 January 1995
Added ERRMSG keyword to internally called procedures.
Version 7, Donald G. Luttermoser, GSFC/ARC, 8 February 1995
Added form 8. Allowed for input to be either scalar
or vector.
Version 8, Donald G. Luttermoser, GSFC/ARC, 13 February 1995
Added the /MSEC keyword. Streamlined code to get
rid of redundancies.
Version 9, William Thompson, GSFC/ARC, 16 February 1995
Rewrote to call CHECK_EXT_TIME. This is used instead
of the logic introduced in version 4 for checking the
validity of the time returned.
Version 10 Fixed array input bug in /msec code. CDP, 20-Feb-95
Version 11 Add VMS and !stime-like formats 9/10. CDP, 15/3/95
Version 12 Add type 11 format. CDP, 15-DEc-95
Version 13, 18-Mar-1998, William Thompson, GSFC
Use SAFE_STRING instead of STRING
Version 14, 27-Apr-2005, William Thompson, GSFC
Fix problem with FORM=11 and /DATE or /TIME
Version : Version 13, 18-Mar-1998
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Project : STEREO - SSC
Name : ANYTIM2CDF()
Purpose : Convert CDS time values to CDF epoch values
Explanation : This procedure calls ANYTIM2UTC and CDF_EPOCH to convert CDS
time values to the "CDF_EPOCH" datatype used within Common Data
Format files.
Use : EPOCH = ANYTIM2CDF(DATE)
Inputs : DATE = Array of epoch values from a CDF file.
Opt. Inputs : None
Outputs : Function returns the dates converted into CDF_EPOCH format.
The CDF documentation describes this as the number of
milliseconds since 1-Jan-0000. (Experiment shows that this
value omits leap seconds.)
Opt. Outputs: None
Keywords : ERRMSG = If defined and passed, then any error messages
will be returned to the user in this parameter
rather than being handled by the IDL MESSAGE
utility. If no errors are encountered, then a null
string is returned. In order to use this feature,
the string ERRMSG must be defined first, e.g.,
ERRMSG = ''
RESULT = ANYTIM2CDF( DATE, ERRMSG=ERRMSG )
IF ERRMSG NE '' THEN ...
Also accepts any keywords for ANYTIM2UTC
Calls : ***
ANYTIM2UTC [1], ANYTIM2UTC [2], UTC2TAI
Common : None
Restrictions: None
Side effects: If an error condition is encountered, and the ERRMSG keyword is
used, then the single value -1 is returned.
Leap seconds, e.g. "2005-12-31T23:59:60", are treated as the
same as the first second of the next day. The previous
behavior was to treat them as a repeat of 23:59:59.
Category : CDF, Time
Prev. Hist. : None
History : Version 1, 11-Jan-2006, William Thompson, GSFC
Version 2, 17-Feb-2006, William Thompson, GSFC
Speed up by using CDF_EPOCH only for a single date, and
then using UTC2TAI with /NOCORRECT for more
processing. Note that this changes the behavior of
leap seconds.
Contact : WTHOMPSON
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Name:
anytim2dd79
Purpose:
Convert time in any standard format to decimal d79,
Input:
TIME_ARR - The usual suspects
Output:
N vector of dd79's
CALLS: ***
Ex2Int [1], Ex2Int [2], anytim2ex [1], anytim2ex [2]
CALLED BY:
GET_SUMER_FLAT, mk_sumer_dbase_ff, sumer_ffdb
History:
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NAME:
anytim2doy
PURPOSE:
Given a time in the form of a (1) structure, (2) 7-element time
representation, or (3) a string representation,
return the day of the year for that day
CALLING SEQUENCE:
xx = anytim2doy(roadmap)
xx = anytim2doy('12:33 5-Nov-91')
INPUT:
tim_in - The input time
Form can be (1) structure with a .time and .day
field, (2) the standard 7-element external representation
or (3) a string of the format "hh:mm dd-mmm-yy"
CALLS: ***
anytim2ex [1], anytim2ex [2], anytim2ints [1], anytim2ints [2]
CALLED BY:
auto_toban, mees_name_format, mk_bad_pix_map_load, mk_daily_ints, mk_nar [1]
mk_nar [2], sec_name_format, timeline, topsdb [1], topsdb [2], web_seq
OPTIONAL KEYWORD INPUT:
string - If set, return the output in the form YYDDD (ie: 98020)
OPTIONAL KEYWORD OUTPUT:
year - The year for the time(s) passed in
HISTORY:
Written 7-Jun-92 by M.Morrison
11-Jan-94 (MDM) - Updated the header information
18-Feb-98 (MDM) - Added /STRING option
5-Mar-98 (MDM) - Changed from STRING to FSTRING
- Changed logic to do '1-Jan-YY' conversion
once per year rather than the full array
(speeds it up considerably for
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NAME:
anytim2ex
PURPOSE:
Given a time in the form of a (1) structure, (2) 7-element time
representation, or (3) a string representation, or (4) an array
2xN where the first dimension holds (MSOD, DS79)
convert to the 7-element time representation (hh,mm,ss,msec,dd,mm,yy)
CALLING SEQUENCE:
xx = anytim2ex(roadmap)
xx = anytim2ex('12:33 5-Nov-91')
xx = anytim2ex([0, 4000])
INPUT:
tim_in - The input time
Form can be (1) structure with a .time and .day
field, (2) the standard 7-element external representation
or (3) a string of the format "hh:mm dd-mmm-yy"
CALLS: ***
Int2Ex [1], Int2Ex [2], gt_day [1], gt_day [2], gt_time [1], gt_time [2]
timstr2ex [1], timstr2ex [2]
CALLED BY:
ACOPY [1], ADDTIME [1], ADDTIME [2], ALIGN_AR, ANAL_BCS_PHA, BCS_ADDGOES
BCS_BROWSE24, BCS_LOAD_CAT, BCS_SPMOVIE [1], BCS_SPMOVIE [2], BUILD_SSX, CARR2EX
CV_BSC2BSD, DISK_SUMMARY, DISPLOI_MON5K, DR, DSN_DMP_FINDER, DSN_FINAL, EUTPLOT
GBO_HEL, GET_FRAME_TIME, GET_SID, GET_SUBARR2, GET_TRACUBE, GET_TRANGE
GO_DSN_FINAL [1], GO_DSN_FINAL [2], G_H, HXTPIXON, HXT_QLOOK, JD2EX, MK_BSC [1]
MK_BSC [2], MK_ORB_WEEK, OBS_PLOT, OP_ADD_SPECIAL, OUTPLOT [1], OUTPLOT [2]
OUTPLOT [3], OUT_GRSPHL1, OUT_GRSPHL2, OUT_HXSPH, PRINT_OP, RD_AR, READ_SPFDGRS
READ_SPFDHXS, SEL_AR, TIM2JD [1], TIM2JD [2], TV_SSX, UPDATE_SXT_CO_INDEX
UPDATE_TERM, UTPLOT [1], UTPLOT [2], UTPLOT [3], UTPLOT [4], UTPLOT [5], WBDA [1]
WBDA [2], WBS_DB2, WOBS_PLOT, any_decay_time, any_fsp, anyrts, anytim2dd79
anytim2doy [1], anytim2doy [2], anytim2weekid [1], anytim2weekid [2]
anytim2weeks [1], anytim2weeks [2], ar_prep, auto_bck_find, auto_toban
bbso_copy [1], bbso_copy [2], bbso_name_fix, cam_run_sum, cancel_dsn_fil
cfl_summary [1], cfl_summary [2], check_compile [1], check_compile [2]
check_dumps [1], check_sci5k_trunc, chk_flares [1], chk_flares [2], contacts [1]
contacts [2], daily_forecast [2], days_2_xmas, disp_sci5k, disp_therm_rs232
do_reg_backup, doy2ex [1], doy2ex [2], dsn_input, event_movie [1], event_movie [2]
file_info2 [1], file_info2 [2], fits2time [1], fits2time [2], fits2time [3]
fits_disp_month [1], fits_disp_month [2], gbo_pfi, get1hk_info [1]
get1hk_info [2], get_gbo_pfi, get_hk_info [1], get_hk_info [2], get_mk3 [1]
get_mk3 [2], get_sfm, get_sirius_yr, get_sunset, getm1ans, go_lasdisk golaserdisk
go_lasdisk2 golaserdisk, go_nvs5, goes3sec_copy, goes_teem, goesem_eqn [1]
goest_eqn [1], grs32_fsp, grsl_fsp, gtab_file, hxi_interp, hxs_fsp, hxsgrs_fsp
hxt_fsp, hxt_fsp1, hxt_sources, hxtimg_accum, interp_arr [1], interp_arr [2]
interp_arr [3], interp_img, ip_que_dmpver, jitter_gif_xyimg, kp_name_fix
ksc_commands, last_lc, laststat [1], laststat [2], launch [1], launch [2], mk_aoslos
mk_bad_pix_map_load, mk_daily_ints, mk_gbl, mk_gev [1], mk_gev [2], mk_gsn_obs
mk_gsn_obs_s1, mk_gx, mk_hst_summary, mk_imgsum_html, mk_lasteit_movie
mk_mdi_fits, mk_mdi_iap, mk_op_file, mk_orbit_files, mk_pnt, mk_ptv_title, mk_sd2
mk_sdc [2], mk_sdc [3], mk_sdc [4], mk_sdl, mk_sfc [1], mk_sfc [2], mk_sl [1]
mk_sl [2], mk_sot, mk_ssl, mk_trace_i1, mk_week_file [1], mk_week_file [2]
monthly_summary, mplot_nar, mult_th_fsp, mwlt_select, new_disp_sci5k [1]
new_disp_sci5k [2], nob_img_copy, nob_name_fix, norik_name_fix, op_facom_ftp
op_get_special, plot_ar_pfi, plot_nar [1], plot_nar [2], plot_ref, plot_trav [1]
plot_trav [2], plot_trav [3], pr_evn [2], pr_nar, pr_trav_summ, pref_super
print_ogsel, rd_gbl_raw [1], rd_gbl_raw [2], rd_goes_fits, rd_lonlat, rd_sci5k
rd_so_at_ftr, rd_therm_rs232, rd_week_file [1], rd_week_file [2]
rd_week_file [3], rd_week_file [4], redo_disploi, redo_mon_sci5k, reslot, sda2fits
selsis_copy [1], selsis_copy [2], seq_run_sum [1], seq_run_sum [2], sft2sfc
soon2fits, sxt2file, sxt2mpeg, sxt_interp [1], sxt_interp [2], sxthxt_fsp, sxtth_hxt
syst2ex [1], syst2ex [2], syst2ex [3], term_times, time_2_fileid, timeline
topsdb [1], topsdb [2], tr_reformat, unixtime2ex, ut_time [1], ut_time [2], web_seq
week2ex [1], week2ex [2], weekid [2], weekid2ex [1], weekid2ex [2], weekid2ex [3]
wfile, xdisp_fits, xdisp_trace [1], xdisp_trace2, xdisp_trace3, xhkplot, xread_hist
xset_chain [1], xset_chain [2], xwrite_hist, ycopy, ydb_exist [2], ydump
OPTIONAL KEYWORD INPUT:
mdy - If set, use the MM/DD/YY order for converting the string date
HISTORY:
Written 15-Nov-91 by M.Morrison
5-Jan-93 (MDM) - Added /MDY option for TIMSTR2EX
11-Jan-93 (MDM) - Updated document header
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NAME:
anytim2ints
PURPOSE:
Given a time in the form of a (1) structure, (2) 7-element time
representation, or (3) a string representation, or (4) an array
2xN where the first dimension holds (MSOD, DS79)
convert to the a simple structure with .TIME and .DAY
CALLING SEQUENCE:
xx = anytim2ints(roadmap)
xx = anytim2ints('1-sep-91', off=findgen(1000)*86400)
xx = anytim2ints('12:33 5-Nov-91')
xx = anytim2ints([0, 4000])
INPUT:
tim_in - The input time
Form can be (1) structure with a .time and .day
field, (2) the standard 7-element external representation
or (3) a string of the format "hh:mm dd-mmm-yy"
CALLS: ***
CHECK_TIME, Ex2Int [1], Ex2Int [2], gt_day [1], gt_day [2], gt_time [1], gt_time [2]
timstr2ex [1], timstr2ex [2]
CALLED BY:
ANAL_BCS_PHA, ANAL_STIMS, ANYTIM2MSV, Alt_tim_sel, BCS_24HR_PLOT [1]
BCS_24HR_PLOT [3], BCS_CONT [1], BCS_CONT [2], BCS_SPMOVIE [1], BCS_SPMOVIE [2]
BCS_TVEC, BSC_TIM2DSET, BUILD_SSX, CARR2EX, CCCA, CONV_A2H [1], CONV_A2H [2]
CONV_H2A [1], CONV_H2A [2], CONV_LP2INDEX, CV_BSC2BSD, DISPLOI_MON5K, DO_TEEM
DSN_DMP_FINDER, FE25_BSC_TEMP, FIRST_LIGHT [1], FIRST_LIGHT [2], FITIM2INTS
FITS_TIME, GET_FRAME_TIME, GET_LATLON, GET_SUBARR2, GET_SUNCENTER [1]
GET_SUNCENTER [2], GET_TIME_LAPSE, GET_TRACUBE, GOES2DPE, GOES_TEK [1]
GOES_TEK [2], GOES_TODAY, GT_BSC_TIME, Goes_bck0, HELIOCENTRIC, HXASCAN2HXAXY
HXTIMG2INTS, HXTPIXON, HXT_FLARE_POS, HXT_IMAGE_TIME, HXT_LCURVE, HXT_QLOOK
HXT_TIME2FRAME, IRUHXA2SXT, IRUHXASCAN2SXT [1], IRUHXASCAN2SXT [2], JD2EX
MAKE_VTRANGE, MK_ORB_WEEK, MSV2INTS, NORH_IMG2IDX [1], NORH_IMG2IDX [2]
NORH_JST2UT [1], NORH_JST2UT [2], NORH_PR_EVX [1], NORH_PR_EVX [2]
NORH_TCX2IDX [1], NORH_TCX2IDX [2], NORH_TSX2IDX [1], NORH_TSX2IDX [2]
NORH_UT2JST [1], NORH_UT2JST [2], NORP_RDT2DATA_17G, NORP_RDT2DATA_1G
NORP_RDT2DATA_2G, NORP_RDT2DATA_35G, NORP_RDT2DATA_4G, NORP_RDT2DATA_9G
NORP_RD_DAT, OBS_PLOT, OVER_THE_LIMB, PLOT_BSC_AS2, PLOT_CLON, PP_MWLT2SXT
PP_SXT2VLA, QUICKATT [1], QUICKATT [2], QUICKDARK [2], RD_HXT_DBOOK, SSDA
SXT_OBSRPT, Sxt_goes_teem, TIM2JD [1], TIM2JD [2], TIM2UPOS, TRACE_MDI_ALIGN
TRACE_SSWHERE [1], TV_SSX, TV_SYNOP, TYKW_RD_DAT, ULYSSES_FEM, VIEW_TRACE_MOSAIC
WBS_DB2, WOBS_PLOT, XMOVIE_SFM, adjust_times, ads_into_att, ads_into_pnt
adsdirs [1], adsdirs [2], align_hxi, align_prep [1], align_prep [2]
align_prep [3], any_decay_time, anystr2tim [1], anystr2tim [2], anytim [1]
anytim [2], anytim [3], anytim [4], anytim [5], anytim2doy [1], anytim2doy [2]
anytim2weekid [1], anytim2weekid [2], anytim2weeks [1], anytim2weeks [2]
ars2_plan, atr2hxa_dbase, auto_bck_find, auto_toban, bbso_copy [1], bbso_copy [2]
bck_interval, bcs_clock_fix, bcs_trange, box_sxtth_hxt, build_timarr [1]
build_timarr [2], cam_run_sum, ccd_hdr_info, cfl_summary [1], cfl_summary [2]
check_oldprocess [1], check_oldprocess [2], check_oldprocess [3]
check_oldprocess [4], check_sci5k_trunc, choose_interval, cnvt [2]
cont2time [1], cont2time [2], contact_num [1], contact_num [2], contacts [1]
contacts [2], conv_a2ap, conv_a2p [1], conv_a2p [2], conv_p2a [1], conv_p2a [2]
copy_visible, dat2bsc, days_2_xmas, deciyr2ints, decode_gev, def_yssysv [1]
def_yssysv [2], delete_week [1], delete_week [2], disp_sci5k, disp_therm_rs232
do_ads, do_tr_reformat, doy2ex [1], doy2ex [2], doytim2ints, dps_fname2time
ea_view_angle [2], edac_summary, emi_plot [1], event_movie [1], event_movie [2]
evt_grid, ex2week [1], ex2week [2], fem_grid [1], fem_grid [2], file_info2 [1]
file_info2 [2], fits_disp_month [1], fits_disp_month [2], fix_hxtindex
fl_mktext, fort2hxi [1], fort2hxi [2], gbo_pfi, get1gbo, get1hk_info [1]
get1hk_info [2], get_ar, get_atr, get_att, get_del_pnt, get_hk_info [1]
get_hk_info [2], get_hxt_pos, get_ksc_holiday, get_mk3 [1], get_mk3 [2]
get_mwlt_roll, get_orb_epoch, get_pnt, get_rb0p [1], get_rb0p [2], get_roll
get_selsis, get_seq_tab, get_sfm, get_sirius [1], get_sirius [2], get_suncenter2
get_sunset, get_sxa, get_utevent [1], get_utevent [2], go_teem [1], go_teem [2]
go_teem_nn, go_teem_t, goes2str, goes3sec_copy, goes_gaps, goes_log, goes_plot [1]
goes_plot [2], goes_plot [3], goes_plot [4], goes_plot [5], goes_summary
goes_teem, goesem_eqn [1], goest_eqn [1], grs32_fsp, grsl_fsp, gt_day [1]
gt_day [2], gt_time [1], gt_time [2], gtab_summary, gtt_info, gtt_orbit, hkplot_info
hxi_interp, hxs_chsums, hxs_fsp, hxsgrs_fsp, hxt_chsums, hxt_fsp, hxt_fsp1, hxt_utplot
hxtaccumulate, hxtimg_accum, image2movie, in_fov, int2secarr [1], int2secarr [2]
interpol_yoh, ip_que_dmpver, iperr_sea, jitter_gif_xyimg, jst, killold [1]
killold [2], ksc_commands, last_lc, list_nrt_times, list_tfi, mk_att [1], mk_att [2]
mk_daily_ints, mk_evn [1], mk_evn [2], mk_fem [1], mk_fem [2], mk_gbl, mk_gsn_obs
mk_gsn_obs_s1, mk_gx, mk_hst_summary, mk_mdi_fits, mk_mdi_iap, mk_mo_log, mk_obs_str
mk_orbit [1], mk_orbit [2], mk_pnt, mk_sdm, mk_sdmi, mk_sfc [1], mk_sfc [2]
mk_sun_mosaic, mk_timarr [1], mk_timarr [2], mk_trace_i1, mk_week_file [1]
mk_week_file [2], mk_ydbtab, mon_health [1], mon_health [2], mon_sci5k
monthly_summary, mwlt_select, mwlt_tape2jpeg, new_disp_sci5k [1]
new_disp_sci5k [2], new_edac_summary, new_mon_health [1], new_mon_health [2]
nn_rd3_sxt_noaa, nob_img_copy, obs_summary, op_times, oplot_nts, pfi_dominant
pfi_loc, pl_dt_genx, pl_monitor_center, plot_door_open, plot_evn, plot_fem
plot_fov [1], plot_gbl [1], plot_gbl [2], plot_gsn, plot_loi_mmad
plot_loi_summary [1], plot_loi_summary [2], plot_pzt_corr, plot_shutter_perf
plot_ssw_fov, plot_therm_rs232a, plot_therm_rs232c, plot_trav [1], plot_trav [2]
plot_trav [3], plott_bda, plott_hda, plott_wda, ploty [1], ploty [2], pr_evn [2]
pr_fem, pr_gbe, pr_gev, pr_gsn [1], pr_gsn [2], pr_his_index [1], pr_his_index [2]
pr_his_index [3], pr_nar, pr_nel, pr_seq_frame_info, pr_sxtobs, pr_tim2week [1]
pr_tim2week [2]
pro interpretfemfemfemtimefemflgfemstrfemstrverboseverbose
pro loadopfemfiletimeOGfemverboseverbose
pro loadoptextfiletimeOGverboseverbose
pro plotogonalgdogtimeogfemtimefemflgstarttimestarttimeendtimeendtimepsps
pro showaoslosgdfemtimefemflg, quick_hkplot [1], quick_hkplot [2]
quick_plottrav, rd_gbl_raw [1], rd_gbl_raw [2], rd_goes3sec [1], rd_goes3sec [2]
rd_goes_fits, rd_gxd [1], rd_gxd [2], rd_gxd [3], rd_old_obs, rd_pnt_hist, rd_rasm
rd_raw_station_plan, rd_rdb [1], rd_rdb [2], rd_so_at_ftr, rd_sol, rd_soup
rd_srspas, rd_station_plan, rd_therm_rs232, rd_week_file [1], rd_week_file [2]
rd_week_file [3], rd_week_file [4], read_eit, read_mdi, read_spartan, redo_disploi
redo_mon_sci5k, ref_term [2], reget_dc_image, res_freq, reslot
return a solar disk mask using SSW standard keywords, sda2fits, search_obs
sel_dc_image [1], sel_dc_image [2], sel_dc_image [3], sel_filetimes [1]
sel_filetimes [2], sel_timrange [1], sel_timrange [2], selsis_copy [1]
selsis_copy [2], seq_run_sum [1], seq_run_sum [2], show_contacts, show_hxafid
soon_cadence, soon_search [1], soon_search [3], soon_table, ssw_check_contrib
sswstruct_fill [1], sxl2radiance, sxt_anycomp, sxt_eff_area, sxt_fl_analxpro
sxt_flux [1], sxt_flux [2], sxt_flux [3], sxt_interp [1], sxt_interp [2]
sxt_mwave, sxt_t6_resp0, sxtbox_teem, sxthxt_fsp, sxtth_hxt, telem_sum, term_obs
term_times, tfr_summary, tfr_summary2, tim2dset [1], tim2dset [2], tim2match [1]
tim2match [2], tim2match [3], tim2orbit [1], tim2orbit [2], tim_bin, time_interp
time_smooth, timegrid, timeline, timeline2html, topsdb [1], topsdb [2]
tr_decode_head [1], tr_decode_head [2], tr_inventory_telem, tr_rd_index
tr_rd_inventory, tr_reformat, tr_wrt_fits_i1 [1], trace_sswhere [2]
trace_sswhere [3], trace_sswhere [4], track_h2a [1], track_h2a [2]
track_h2a [3], ut_time [1], ut_time [2], utcursor [1], utcursor [2], v_orbital
wdefroi [3], wdefroi [4], web_seq, week2ex [1], week2ex [2], weekid [2]
weekid2ex [1], weekid2ex [2], weekid2ex [3], wrt_fits_bin_exten [2], xanal_emi
xdate [1], xdate [2], xdisp_sci5k, xdisp_trace2, xfem_grid, xhkplot, xread_hist
xset_chain [1], xset_chain [2], xso_search, xspr [1], xspr [2], ydb_exist [2]
yopos [1], yopos [2], yoyo_man2
OPTIONAL KEYWORD INPUT:
offset - The input time can be offset by a scalar or vector number of
seconds. If "offset" is an array, it should be the same
length at tim_in
HISTORY:
Written 30-May-92 by M.Morrison
5-Jan-93 (MDM) - Added /MDY option for TIMSTR2EX
12-May-93 (MDM) - Modified to allow TIM_IN to be a single time, and
OFFSET to be an array
11-Jan-94 (MDM) - Updated document header
15-jan-00 (PGS) - Added 'def_for' to pass to timstr2ex.pro for rd_srspas.pro, y2k fix
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Project : SOHO - CDS
Name : anytim2jd()
Purpose : Converts any input time format to full Julian day.
Explanation : Converts any time format to the equivalent Julian
day value. Returns result in a structure with the
tags int (long) and frac (double).
Use : IDL> jd = anytim2jd(any_format)
Inputs : any_format - date/time in any of the acceptable CDS
time formats -- for acceptable formats see file
aaareadme.txt.
Opt. Inputs : None
Outputs : Function returns JD in a structure {int:0L,frac:0.0d0}.
Opt. Outputs: None
Keywords : ERRMSG = If defined and passed, then any error messages will
be returned to the user in this parameter rather
than being printed to the screen. If no errors are
encountered, then a null string is returned. In
order to use this feature, the string ERRMSG must
be defined first, e.g.,
ERRMSG = ''
JD = anytim2jd ( DT, ERRMSG=ERRMSG, ...)
IF ERRMSG NE '' THEN ...
Calls : ***
ANYTIM2UTC [1], ANYTIM2UTC [2], INT2UTC, JULDAY
CALLED BY:
PB0R, SXIG12_PREP
Common : None
Restrictions: None
Side effects: None
Category : Util, time
Prev. Hist. : None
Written : C D Pike, RAL, 16-May-94
Modified : Version 1, C D Pike, RAL, 16-May-94
Version 2, William Thompson, GSFC, 14 November 1994
Changed .DAY to .MJD
Version 3, Donald G. Luttermoser, GSFC/ARC, 20 December 1994
Added the keyword ERRMSG. Included ON_ERROR flag.
Version 4, Donald G. Luttermoser, GSFC/ARC, 30 January 1995
Added ERRMSG keyword to internally called procedured.
Made error handling routine more robust.
Version 5, Donald G. Luttermoser, GSFC/ARC, 13 February 1995
Allowed for input to be either scalar or vector.
Version 6, William Thompson, GSFC, 28 January 1997
Allow for long input arrays.
Version 7, Zarro, GSFC, 4 Feb 1997
Changed name from ANYTIM2JD
Version : Version 7
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Project : SOHO - CDS
Name : ANYTIM2TAI()
Purpose : Converts any standard CDS time format to TAI.
Explanation : Tests the type of input and tries to use the appropriate
conversion routine to create the date/time in CDS TAI
time format.
Use : IDL> tai = anytim2tai(any_format)
Inputs : any_format - date/time in any of the acceptable CDS
time formats -- for acceptable formats see file
aaareadme.txt.
Opt. Inputs : None
Outputs : Function returns CDS TAI double precision time value.
Opt. Outputs: None
Keywords : ERRMSG = If defined and passed, then any error messages
will be returned to the user in this parameter
rather than being printed to the screen. If no
errors are encountered, then a null string is
returned. In order to use this feature, the
string ERRMSG must be defined first, e.g.,
ERRMSG = ''
TAI = ANYTIM2TAI ( DT, ERRMSG=ERRMSG, ...)
IF ERRMSG NE '' THEN ...
Calls : ***
ANYTIM2UTC [1], ANYTIM2UTC [2], DATATYPE [1], DATATYPE [2], DATATYPE [3], UTC2TAI
CALLED BY:
ADD_CDS_POINT, ADD_EFFICIENCY, ADD_EFF_AREA, ADD_MIRSHIFT, ADD_TILTCAL
ADD_WAVECAL, ADD_WAVE_EFF, BBSO__DEFINE, CACHE_LIST, CDS_SLIT6_BURNIN, CHECK_LOCK
CHKSCPCKTIME, CRONTAB, DISPLAY_CDS_BURNIN, DROT_COORD, DROT_RASTER, DROT_XY
DSP_POINT, EIS_CPT_CHECK_TIME_PERIOD [1], EIS_CPT_CHECK_TIME_PERIOD [2]
EIS_CPT_NOW [1], EIS_CPT_NOW [2], EIS_CPT_OBSTBL_MAP_PARSE [1]
EIS_CPT_OBSTBL_MAP_PARSE [2], EIS_CPT_TEST [1], EIS_CPT_TEST [2]
EIS_CPT_test_parameters [1], EIS_CPT_test_parameters [2], EIS_DROT_FOV [1]
EIS_DROT_FOV [2], EIS_IMAGE_TOOL [1], EIS_IMAGE_TOOL [2], EIS_ITOOL_STC [1]
EIS_ITOOL_STC [2], EIS_LIST_EXPER [1], EIS_LIST_EXPER [2], EIS_LIST_MAIN [1]
EIS_LIST_MAIN [2], EIT_COPY, EIT_GBO, EIT__DEFINE, EXPORT_PLAN, FID2TIME
FID__DEFINE, FILE_CONTENT, FILE_SINCE, FIND_CAMPAIGN, FIND_CAT, FIND_PROC
GET_CDS_OH, GET_CDS_PLAN, GET_CDS_PNTCAL, GET_CDS_STATE, GET_CDS_TEMPS
GET_DROT_DUR, GET_EFFICIENCY, GET_EFF_AREA, GET_FID, GET_FITS_TIME, GET_LATEST_KAP
GET_MAP_TIME, GET_MIRSHIFT, GET_NIMCP, GET_RECENT_EIT, GET_SID, GET_SOHO_ROLL
GET_SUMER_FILES, GET_TILTCAL, GET_WAVE_EFF, GET_WIDTH_CORR, GIS_CALIB_FF_LTGD
GIS_ERROR, GOES__DEFINE, GT_DURATION, HC_SINCE, HFITS__DEFINE, HSI_SOCK_LIST
IMAGE_TOOL, ITOOL_DIFF_ROT, ITOOL_GETFILE, ITOOL_PICKFILE, LABEL_TAI, LATEST_IMAGE
LIST_CACHE__DEFINE, LVIEW_XY, MAP2WCS, MDI_GBO, MEAN_MAP, MK_HXI_MAP, MK_IVM_MAP
MK_PLAN_CAMP, MK_PLAN_PLOT, MK_PLAN_WHERE, MK_POINT_STC, MK_SUMMARY, MK_SXT_MAP
MK_WAVECAL, MOVIE_MAP, NEAREST_GEV, NEAR_TIME, PARSE_TIME, PICK_TIMES
PLAN_XCAT_SUMM, PLOT_MAP, PLOT_SPLAN, PRED_PROG_NUM, RD_CDS_POINT, RD_PLAN
RD_RESOURCE, RD_RSTN, READ_KAP, REDUCE_LEVEL_1, ROT_XY, ROUND_TIME, RSTN__DEFINE
SHOW_SYNOP__DEFINE, SITE__DEFINE, SUM_ANA_TEMP, SXI_GBO, SYNOP_DEFINE, SYNOP_PATH
SYSTIM, TRACE_COPY, TRACE_GBO, UPDATE_CAMPAIGN, UPDATE_KAP, UTPLOT__DEFINE, WCS2MAP
WHERE_MAP, WHERE_TIMES, XCAMP, XCAT, XCPT, XCRON, XIAP, XREPORT, XVALIDATE, Y2KFIX, YMD2DATE
db_gbo, eis_datetime_gui [1], eis_datetime_gui [2], eis_dr_obj__DEFINE [1]
eis_dr_obj__DEFINE [2], eis_get_current_time [1], eis_get_current_time [2]
eis_mk_plan_gui [1], eis_mk_plan_gui [2]
eis_timeline_graphics_axes_default [1]
eis_timeline_graphics_axes_default [2], get_def_times, hsi_gbo, ihy_db
mk_sumer_map [1], mk_sumer_map [2], mk_sumer_map [3], sgt_raster_time
trace_build_mosaic3
Common : None
Restrictions: None
Side effects: None
Category : Util, time
Prev. Hist. : Based on ANYTIM2UTC by C. D. Pike.
Written : William Thompson, GSFC, 20 May 1996
Modified : Version 1, William Thompson, GSFC, 20 May 1996
Version 2, 05-Oct-1999, William Thompson, GSFC
Add support for Yohkoh 7-element external time.
Version 3, 31-Jul-2001, William Thompson, GSFC
Changed MESSAGE to MESSAGE, /CONTINUE
Version 4, 16-Feb-2004, CDP. Added /quiet keyword because it was
already required in the code.
Version 5, 08-Sep-2004, William Thompson, GSFC
Added keyword NOCORRECT
Version 6, 07-Dec-2005, William Thompson, GSFC
Moved handling of Yohkoh formats to ANYTIM2UTC
Version : Version 6, 07-Dec-2005
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Project : SOHO - CDS
Name : ANYTIM2UTC()
Purpose : Converts (almost) any time format to CDS UTC format.
Explanation : Tests the type of input and tries to use the appropriate
conversion routine to create the date/time in CDS UTC
format (either internal (default), external or string)
CDS time format.
Use : IDL> utc = anytim2utc(any_format)
Inputs : any_format - date/time in any of the acceptable CDS
time formats -- for acceptable formats see file
aaareadme.txt.
Opt. Inputs : None
Outputs : Function returns CDS UTC time structure.
Opt. Outputs: None
Keywords : EXTERNAL = Create output in external format
CCSDS = Create string output in CCSDS format
ECS = Create string output in ECS format
VMS = Create string output in VMS format
STIME = Create string output in STIME format
Only one of the above keywords can be set. If none of them are
set, then the output is in internal format. The following
keywords are only valid if a string format was selected.
DMY = Normally the date is in the order year-month-day.
However, if DMY is set then the order is
day-month-year. Note that if the month is given as
a character string, then the default is
day-month-year.
MDY = If set, then the date is in the order
month-day-year.
YMD = If set, then the date is in the order
year-month-day.
TRUNCATE = If set, then the time will be truncated to 1 second
accuracy. Note that this is not the same thing as
rounding off to the nearest second, but is a
rounding down.
DATE_ONLY = If set, then only the date part of the string is
returned.
TIME_ONLY = If set, then only the time part of the string is
returned.
UPPERCASE = If set, then the month field in either the VMS or
STIME format is returned as uppercase.
NOZ = When set, the "Z" delimiter (which denotes UTC
time) is left off the end of the CCSDS/ISO-8601
string format. It was decided by the FITS
committee to not append the "Z" in standard FITS
keywords.
The following keywords are always valid.
QUIET = If set, then no informational messages are printed.
ERRMSG = If defined and passed, then any error messages
will be returned to the user in this parameter
rather than being printed to the screen. If no
errors are encountered, then a null string is
returned. In order to use this feature, the
string ERRMSG must be defined first, e.g.,
ERRMSG = ''
UTC = ANYTIM2UTC ( DT, ERRMSG=ERRMSG, ...)
IF ERRMSG NE '' THEN ...
Other keywords to the underlying routines can also be passed,
via the _EXTRA mechanism.
Calls : ***
ANYTIM2CAL, DATATYPE [1], DATATYPE [2], DATATYPE [3], GET_UTC, INT2UTC, STR2UTC [1]
STR2UTC [2], STR2UTC [3], STR_SEP, TAG_EXIST [1], TAG_EXIST [2], TAI2UTC
UTC2INT [1], UTC2INT [2], UTC2INT [3]
CALLED BY:
ADJUST_HDR_TCR, ANYTIM2CAL, ANYTIM2CDF, ANYTIM2TAI, ANYTIM2WEEK, ARCMIN2HEL2
BBSO__DEFINE, CAT_DIRECTORY, CAT_DURATION, CAT_FITS, CAT_OPEN [1], CAT_TO_TEXT
CDS2JD, CDSPICKFILE, CDS_ASRUN_POINT, CDS_FILES, CDS_PLAN_BRIEF, CDS_PLAN_POINT
CDS_SNAPSHOT, CFITSLIST, CF_GIS1A, CF_GIS1B, CF_GIS1C, CF_GIS2A [1], CF_GIS4A
CF_GIS4B, CF_GIS4C, CHECK_KAP, CHKSCPCKTIME, DATE_CODE, DISPLAY_CDS_BURNIN
DISPLAY_NIMCP, DMOVIE [1], DMOVIE [2], DROT_MAP, DROT_MAP_FAST, DROT_NAR, DSP_WAV
DTSELECT, EIS_CAT [1], EIS_CAT [2], EIS_CPT_NOW [1], EIS_CPT_NOW [2]
EIS_CPT_OBSTBL_MAP_TEXT [1], EIS_CPT_OBSTBL_MAP_TEXT [2]
EIS_CPT_TIMEFORMAT [1], EIS_CPT_TIMEFORMAT [2]
EIS_CPT_TIME_PERIOD_DEFAULT [1], EIS_CPT_TIME_PERIOD_DEFAULT [2]
EIS_DROT_FOV [1], EIS_DROT_FOV [2], EIS_IMAGE_TOOL [1], EIS_IMAGE_TOOL [2]
EIS_IMAGE_TOOL_EVENT [1], EIS_IMAGE_TOOL_EVENT [2], EIS_LOAD_IMAGE [1]
EIS_LOAD_IMAGE [2], EIS_PLAN_STC [1], EIS_PLAN_STC [2], EIS_PLOT_OBEV [1]
EIS_PLOT_OBEV [2], EIS_PLOT_OPEV, EIS_PLOT_STEV [1], EIS_PLOT_STEV [2]
EIT_CATRD [1], EIT_COPY, EIT_DAILY, EIT_DISPLAY, EIT_FXPAR, EIT_GBO, EIT_IMAGE
EIT_MKMOVIE, EIT_PA, EIT_PA_PROCESS, EIT_PA_ev, EIT_POSTAGE, EIT_PREP, EIT_SUBFIELD
EIT_SUB_DRAW, EIT_SUB_MAN_INPUT, EIT_SUB_ROTATE, EIT_SUB_UTIL_HELIO
EIT_TIME_CORRECTION, EIT__DEFINE, ETHZ__DEFINE, EXPORT_PLAN, FILE_CONTENT
FILE_DATE_MOD, FILT_EVENTS, FIND_CAMPAIGN, FIND_FID, FIND_KAP_FILE, FLUSH_CATALOG
FTP_BBSO, FTP_KISF, FTP_MLSO_IMAGES, FTP_MWSO, FTP_NOBE, FTP_SYNOP, GDSPSPEC
GET_CDS_OH, GET_CDS_PNTCAL, GET_DETAIL, GET_EFFICIENCY, GET_EFF_AREA, GET_FID
GET_FITS_CDELT, GET_FITS_CEN, GET_FITS_TIME, GET_GEV, GET_LATEST_IAP
GET_LATEST_KAP, GET_LIST, GET_MAP_TIME, GET_MIRSHIFT, GET_NAR, GET_NOAA
GET_ORBIT [1], GET_ORBIT [2], GET_ORBIT_CDF, GET_ORBIT_CDF2, GET_ORBIT_FITS
GET_PLAN, GET_PLAN_TIME, GET_PLAN_TT, GET_RECENT_EIT, GET_ROLL_OR_XY
GET_SC_ATT [1], GET_SC_ATT [2], GET_SC_POINT, GET_SOHO_ROLL, GET_SOLAR_RADIUS
GET_SUMER_FILES, GET_SYNOPTIC, GET_TILTCAL, GET_VDS_SLITPOS, GET_VDS_STATE
GET_WAVECAL, GET_WAVE_EFF, GET_WIDTH_CORR, GISPLOT, GIS_UTPLOT, GOES__DEFINE
GT_BIMAGE, GT_CDS_TIME, GT_LAMBDA, GT_MIMAGE, GT_VALID, GT_WLIMITS, HEL2ARCMIN [1]
HFITS__DEFINE, HTML_SPLAN, HTTP__DEFINE, IMAGE_TOOL, IMAGE_TOOL_EVENT, ITOOL2MAP
ITOOL_BUTTON_REFRESH, ITOOL_DIFF_ROT, ITOOL_DISP_ROT, ITOOL_EIT_DEGRID
ITOOL_GETFILE, ITOOL_LOAD_IMAGE, ITOOL_PICKFILE, ITOOL_RD_GIF, ITOOL_SET_CSI
LABEL_TAI, LAST_KAP_VERS, LAT2Y, LATEST_IMAGE, LIST_ANOMALY, LIST_CACHE__DEFINE
LIST_CDROM, LIST_DETAIL, LIST_EXP_COMM, LIST_FITS, LIST_PLAN, LIST_RESOURCE
LIST_SUPPORT, MAKE_MAP, MAP2WCS, MAP__DEFINE, MDI_GBO, MKDI_C1, MKQUERY, MK_CDS_PLAN
MK_GISPLOT_LBL, MK_GIS_PLT, MK_IVM_MAP, MK_PLAN_CHANGE, MK_PLAN_CLONE
MK_PLAN_CUSTOM, MK_PLAN_FORM, MK_PLAN_HTML, MK_PLAN_PLOT, MK_PLAN_PRIV
MK_PLAN_RECAL, MK_SOHO, MK_SOHO_CUSTOM, MK_SOHO_EDP, MK_SOHO_TARGET, MK_TIMETICK
MK_WAVECAL, MONO_SPEC, MOVIE_MAKER, NDSPSPEC, NIS_BIAS_DEMO, NRL2EIT, OPLOT_SPLAN
OSRA__DEFINE, OVSA_LTC_DEFINE, PARSE_TIME, PB0R, PLOT_HELIO [1], PLOT_HELIO [2]
PLOT_MAP, PLOT_MAP2 WARNINGTEMPORARY FIX ONLY FOR 16 bit ZBuffer support
PLOT_RESOURCE, PLOT_VDS_BIAS, POINTING3, POLY_SPEC, PRG_DETAIL, PRG_PLAN, QTILT
QUERY_ANOMALY, RD_CDS_POINT, RD_GOES, RD_PLAN, RD_RESOURCE, RD_RSTN, READCDSFITS
READ_FULL_ATT, READ_KAP, READ_MERGED_DSN, READ_SC_ATT, REDUCE_LEVEL_1
ROT_SUBIMAGE, ROT_XY, ROUND_TIME, RSTN__DEFINE, RTMOVIE, SELECTD, SET_KAP_VERS
SHOW_PLAN, SHOW_SYNOP__DEFINE, SID__DEFINE, SITE__DEFINE, SOHOFILE2TIME
SOHO_CAMPAIGN, SOHO_ITEMS_HTML, SOHO_XY, STARFIELD, SUBFIELD_EV, SUM_ANA_TEMP
SUN_EPHEM, SURVANAL, SXI_GBO, S_HK0_SYSCONFIG, TEXT_ANOMALY, TIME2FID, TIME_AVERAGE
TIME_CHECK, TIME_CORRECTION, TPANALYZE, TRACE_COPY, TRACE_GBO, TRACE_MOSAIC_IMAGE
UPDATE_CAMPAIGN, UPDATE_CDS_TARGETS, UPDATE_IAP, UPDATE_KAP, UPDATE_MM
UPDATE_SOHO_TARGETS, UTC2DIFF, UTPLOT__DEFINE, V4DIFF_ROT, VALID_TIME, VDS_CALIB
VDS_READ_FLAT, VSO__DEFINE, WCS2MAP, WCS_FIND_TIME, WEEK2UTC, WHERE_OFF_LIMB
WRITE_ANOMALY, WRITE_CAP, WRITE_CIF, WRITE_IAP, XCALENDAR, XCAMP, XCAT, XCLONE_PLAN
XCPT, XGET_SYNOPTIC, XGET_UTC, XIAP, XREPORT, XREPORT_EDIT, XVALIDATE, XZOOM_PLAN
Y2KFIX, YMD2DATE, anytim2jd, closest_time, datify, datify_fname, db_gbo, dsp_menu
ef2time, eis_cpt_gui [1], eis_cpt_gui [2], eis_ct_summary_gui [1]
eis_ct_summary_gui [2], eis_datetime_gui [1], eis_datetime_gui [2]
eis_dr_obj__DEFINE [1], eis_dr_obj__DEFINE [2], eis_get_events_filename [2]
eis_get_events_filename [4], eis_import_linelist [1]
eis_import_linelist [2], eis_mk_plan_gui [1], eis_mk_plan_gui [2]
eis_read_linelist_block [1], eis_read_linelist_block [2]
eis_read_raster_block [1], eis_read_raster_block [2]
eis_read_study_block [1], eis_read_study_block [2]
eis_timeline_plot_gui [1], eis_timeline_plot_gui [2], eit_dark, eit_degrid
eit_degrid_fft, eit_dump, eit_file2path, eit_find_last_cal, eit_findcalgroup
eit_flat, eit_getcal, eit_getlimb, eit_norm_response [1], eit_point
fitshead2struct, get_def_times, get_eit_data, hsi_gbo, hsi_plot_flux, ihy_db
mk_atlas, mk_mdi_fits, mk_sumer_map [1], mk_sumer_map [2], mk_sumer_map [3]
smk_atlas, soho_fac, vso_format, write_ovsa_fits, zdiff_rot
Common : None
Restrictions: None
Side effects: None
Category : Util, time
Prev. Hist. : None
Written : C D Pike, RAL, 16-May-94
Modified : Version 1, C D Pike, RAL, 16-May-94
Version 2, William Thompson, GSFC, 14 November 1994
Changed .DAY to .MJD
Version 3, Donald G. Luttermoser, GSFC/ARC, 20 December 1994
Added the keyword ERRMSG. Included ON_ERROR flag.
Version 4, Donald G. Luttermoser, GSFC/ARC, 30 January 1995
Added ERRMSG keyword to internally called procedures.
Made error handling routine more robust.
Version 5, Donald G. Luttermoser, GSFC/ARC, 8 February 1995
Allowed for input to be either scalar or vector.
Version 6, William Thompson, GSFC, 14 March 1995
Added keywords VDS, STIME, TRUNCATE, DATE_ONLY,
TIME_ONLY, UPPERCASE
Version 7, William Thompson, GSFC, 5 May 1995
Fixed bug with use of ERRMSG keyword.
Made so that TAI times are supported.
Version 8, William Thompson, GSFC, 8 May 1995
Fixed bug introduced in version 7
Version 9 C D Pike, RAL, 17-May-95
Handle time only (no date) string input.
Version 10, William Thompson, GSFC, 20 December 1995
Fixed bug with use of ERRMSG keyword when string
contained no "-" characters.
Version 11, William Thompson, GSFC, 23 October 1996
Added keywords DMY, MDY, YMD.
Removed attempt at automatic recognition of DMY
option--no longer needed with version 11 of STR2UTC.
Version 12, William Thompson, GSFC, 28 January 1997
Allow for long input arrays.
Version 13, William Thompson, GSFC, 17 September 1997
Added keyword NOZ.
Version 14, 05-Oct-1999, William Thompson, GSFC
Add support for Yohkoh 7-element external time.
Version 15, 11-Aug-2003, William Thompson, GSFC
Implement many keywords through _EXTRA.
Version 16, 31-Mar-2004, Zarro (L-3Com/GSFC)
Fixed error message bug
Version 17, 25-Oct-2005, William Thompson, GSFC
Handle structures through UTC2INT - interprets any
structure with MJD and TIME as CDS internal time
Version 18, 07-Dec-2005, William Thompson, GSFC
Add support for Yohkoh {DAY:, TIME:} structures.
Version 19, 20-Jun-2006, William Thompson, GSFC
Preserve dimensionality
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Project : SOHO / STEREO
Name : ANYTIM2WEEK
Purpose : Returns the ISO-8601 week number for a given date
Category : Time
Explanation : Returns the ISO-8601 week number associated with a given
calendar date. ISO-8601 defines week 1 as the week containing
the first Thursday of the year. In the Gregorian calendar,
this is equivalent to the week which includes January 4th.
Syntax : WEEK = ANYTIM2WEEK( DATE [, YEAR_OUT ] )
Examples : WEEK = ANYTIM2WEEK( '1-Jan-2006', YEAR_OUT )
PRINT, WEEK, YEAR_OUT
52 2005
Inputs : DATE = The date, in any format supported by ANYTIM2UTC
Opt. Inputs : None.
Outputs : The result of the function is the week number.
Opt. Outputs: YEAR_OUT = The year that this week is associated with, which
might be the previous or next year, depending on the
date. See the above example.
Keywords : None.
Calls : ***
ANYTIM2UTC [1], ANYTIM2UTC [2], WEEK2UTC
Common : None.
Restrictions: None.
Side effects: None.
Prev. Hist. : Unrecorded.
History : Version 1, 24-Jan-2006, S.V. Haugan, ESA
Contact : SVHAUGAN
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Purpose: return week-requested information for input time vector
Input Parameters:
times - time vector in any SSW format
Output Parameters:
years - integer year for input times
weeks - integer week for input times
Output:
Function output if /FIRST set, output is YYYYMMDD or YYMMDD (first DOW)
Function output if /WID set, output is YYYY_WW or YY_WW (weekid)
DEFAULT
Keyword Parameters:
wid - (switch) if set, return 'YYYY_WW' (weekid) DEFAULT
first - (switch) if set, return 'YYYYMMDD' correponding to 1st DOW
year2digit (switch) if set, return year as 2 digit (YYMMDD or YY_WW)
CALLS: ***
FSTRING, TIME2FILE, anytim [1], anytim [2], anytim [3], anytim [4], anytim [5]
ex2week [1], ex2week [2], week2ex [1], week2ex [2]
CALLED BY:
cdrom_files [2], do_tr_inventory, ssw_time2paths, sxt_files, sxt_his2dbase
sxt_patch_att, tr_reformat, trace_cat2data, trace_file2path, trace_files
trace_get1www_image, trace_make_tma, trace_make_tmr [1], trace_make_tmr [2]
write_genxcat, yohkoh_files
History:
29-Jan-1998 - S.L.Freeland - package some common TRACE/YOHKOH/SSW
time->week conversions
Routines Called:
anytim, anytim2ints, ex2week
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NAME:
anytim2weeks
PURPOSE:
Given a starting and ending time, return a vector
of week numbers and year numbers where the times fall
INPUT:
sttim - the start time in "any" format
OPTIONAL INPUT:
entim - if not defined, just return the week/year for
the start time
OUTPUT:
weeks - the week number
years - the year numbers
CALLS: ***
anytim2ex [1], anytim2ex [2], anytim2ints [1], anytim2ints [2], ex2dow [1]
ex2dow [2], ex2week [1], ex2week [2]
CALLED BY:
OBS_PLOT, do_reg_backup, dsn_input, get1gbo, goes_summary, rd_old_obs
rd_week_file [1], rd_week_file [2], rd_week_file [3], rd_week_file [4]
show_obs3, show_obs4, tim2weekid, weekid [2], ydb_exist [2], ydb_install [1]
ydb_install [2]
OPTIONAL KEYWORD INPUT:
nobackup - If set, then do not back up a week if the start
time is within 90 minutes of the first day of the week.
string - If set, then return the answer in string format (WIDs)
HISTORY:
Written Feb-92 by M.Morrison
8-Feb-92 (MDM) - Added code to back up a week if the start time
is within 90 minutes of the first day of a week
29-Aug-94 (MDM) - Added /NOBACKUP option to NOT back up a week
when start time is within 90 minutes of the first
day of the week.
20-Sep-94 (MDM) - Added /STRING option
10-Dec-99 (JRL) - Applied the y2k fixes
02-Jan-01 (PGS) - Modified Y2K fix, as ex2week now returns a 4-digit
year element, rather than 2-digit. Check for 54 'week'
year (e.g., 2000)
02-mar-01 (PGS) - widened legacy format filter: accepts strictly 2-digit
years now, as well as integers starting at 0: e.g., 101 = 2001
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PROJECT:
SSW
NAME:
ANYTIM_REPORT
PURPOSE:
This routine checks the performance of anytim for all of its inputs and outputs.
CATEGORY:
UTPLOT
CALLING SEQUENCE:
CALLS: ***
FCHECK, anytim [1], anytim [2], anytim [3], anytim [4], anytim [5]
INPUTS:
Input - a time array to use for validation.
OPTIONAL INPUTS:
none
KEYWORD OUTPUTS:
MAXDIFF - maximum difference for Input for format i vs format j.
OUT - Text report.
OPTIONAL OUTPUTS:
none
KEYWORDS:
none
COMMON BLOCKS:
none
SIDE EFFECTS:
none
RESTRICTIONS:
none
PROCEDURE:
The input array is first converted to the ith output format, converted to seconds,
and the absolute value is taken vs the same for the jth format.
MODIFICATION HISTORY:
2 april 2001, richard.schwartz@gsfc.nasa.gov
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NAME:
APER
PURPOSE:
Compute concentric aperture photometry (adapted from DAOPHOT)
EXPLANATION:
APER can compute photometry in several user-specified aperture radii.
A separate sky value is computed for each source using specified inner
and outer sky radii.
CALLING SEQUENCE:
APER, image, xc, yc, [ mags, errap, sky, skyerr, phpadu, apr, skyrad,
badpix, /NAN, /EXACT, /FLUX, PRINT = , /SILENT,
/MEANBACK, SETSKYVAL = ]
INPUTS:
IMAGE - input image array
XC - vector of x coordinates.
YC - vector of y coordinates
OPTIONAL INPUTS:
PHPADU - Photons per Analog Digital Units, numeric scalar. Converts
the data numbers in IMAGE to photon units. (APER assumes
Poisson statistics.)
APR - Vector of up to 12 REAL photometry aperture radii.
SKYRAD - Two element vector giving the inner and outer radii
to be used for the sky annulus. Ignored if the SETSKYVAL
keyword is set.
BADPIX - Two element vector giving the minimum and maximum value
of a good pixel. If badpix is not supplied or if BADPIX[0] is
equal to BADPIX[1] then it is assumed that there are no bad
pixels. Note that fluxes will not be computed for any star
with a bad pixel within the aperture area, but that bad pixels
will be simply ignored for the sky computation. The BADPIX
parameter is ignored if the /NAN keyword is set.
OPTIONAL KEYWORD INPUTS:
CLIPSIG - if /MEANBACK is set, then this is the number of sigma at which
to clip the background. Default=3
CONVERGE_NUM: if /MEANBACK is set then if the proportion of
rejected pixels is less than this fraction, the iterations stop.
Default=0.02, i.e., iteration stops if fewer than 2% of pixels
excluded.
/EXACT - By default, APER counts subpixels, but uses a polygon
approximation for the intersection of a circular aperture with
a square pixel (and normalize the total area of the sum of the
pixels to exactly match the circular area). If the /EXACT
keyword, then the intersection of the circular aperture with a
square pixel is computed exactly. The /EXACT keyword is much
slower and is only needed when small (~2 pixels) apertures are
used with very undersampled data.
/FLUX - By default, APER uses a magnitude system where a magnitude of
25 corresponds to 1 flux unit. If set, then APER will keep
results in flux units instead of magnitudes.
MAXITER if /MEANBACK is set then this is the ceiling on number of
clipping iterations of the background. Default=5
/MEANBACK - if set, then the background is computed using the 3 sigma
clipped mean (using meanclip.pro) rather than using the mode
computed with mmm.pro. This keyword is useful for the Poisson
count regime or where contamination is known to be minimal.
/NAN - If set then APER will check for NAN values in the image. /NAN
takes precedence over the BADPIX parameter. Note that fluxes
will not be computed for any star with a NAN pixel within the
aperture area, but that NAN pixels will be simply ignored for
the sky computation.
PRINT - if set and non-zero then APER will also write its results to
a file aper.prt. One can specify the output file name by
setting PRINT = 'filename'.
READNOISE - Scalar giving the read noise (or minimum noise for any
pixel. This value is passed to the procedure mmm.pro when
computing the sky, and is only need for images where
the noise is low, and pixel values are quantized.
/SILENT - If supplied and non-zero then no output is displayed to the
terminal.
SETSKYVAL - Use this keyword to force the sky to a specified value
rather than have APER compute a sky value. SETSKYVAL
can either be a scalar specifying the sky value to use for
all sources, or a 3 element vector specifying the sky value,
the sigma of the sky value, and the number of elements used
to compute a sky value. The 3 element form of SETSKYVAL
is needed for accurate error budgeting.
OUTPUTS:
MAGS - NAPER by NSTAR array giving the magnitude for each star in
each aperture. (NAPER is the number of apertures, and NSTAR
is the number of stars). If the /FLUX keyword is not set, then
a flux of 1 digital unit is assigned a zero point magnitude of
25.
ERRAP - NAPER by NSTAR array giving error for each star. If a
magnitude could not be determined then ERRAP = 9.99 (if in
magnitudes) or ERRAP = !VALUES.F_NAN (if /FLUX is set).
SKY - NSTAR element vector giving sky value for each star in
flux units
SKYERR - NSTAR element vector giving error in sky values
CALLS: ***
GETOPT, MEANCLIP, MMM, PIXWT, STRN [1], STRN [2], STRN [3], STRNUMBER [1], STRNUMBER [2]
STRNUMBER [3], STRNUMBER [4]
CALLED BY:
ATV, T_APER
EXAMPLE:
Determine the flux and error for photometry radii of 3 and 5 pixels
surrounding the position 234.2,344.3 on an image array, im. Compute
the partial pixel area exactly. Assume that the flux units are in
Poisson counts, so that PHPADU = 1, and the sky value is already known
to be 1.3, and that the range [-32767,80000] for bad low and bad high
pixels
IDL> aper, im, 234.2, 344.3, flux, eflux, sky,skyerr, 1, [3,5], -1, $
[-32767,80000],/exact, /flux, setsky = 1.3
PROCEDURES USED:
GETOPT, MMM, PIXWT(), STRN(), STRNUMBER()
NOTES:
Reasons that a valid magnitude cannot be computed include the following:
(1) Star position is too close (within 0.5 pixels) to edge of the frame
(2) Less than 20 valid pixels available for computing sky
(3) Modal value of sky could not be computed by the procedure MMM
(4) *Any* pixel within the aperture radius is a "bad" pixel
(5) The total computed flux is negative
APER was modified in June 2000 in two ways: (1) the /EXACT keyword was
added (2) the approximation of the intersection of a circular aperture
with square pixels was improved (i.e. when /EXACT is not used)
REVISON HISTORY:
Adapted to IDL from DAOPHOT June, 1989 B. Pfarr, STX
FLUX keyword added J. E. Hollis, February, 1996
SETSKYVAL keyword, increase maxsky W. Landsman, May 1997
Work for more than 32767 stars W. Landsman, August 1997
Don't abort for insufficient sky pixels W. Landsman May 2000
Added /EXACT keyword W. Landsman June 2000
Allow SETSKYVAL = 0 W. Landsman December 2000
Set BADPIX[0] = BADPIX[1] to ignore bad pixels W. L. January 2001
Fix chk_badpixel problem introduced Jan 01 C. Ishida/W.L. February 2001
Set bad fluxes and error to NAN if /FLUX is set W. Landsman Oct. 2001
Remove restrictions on maximum sky radius W. Landsman July 2003
Added /NAN keyword W. Landsman November 2004
Set badflux=0 if neither /NAN nor badpix is set M. Perrin December 2004
Added READNOISE keyword W. Landsman January 2005
Added MEANBACK keyword W. Landsman October 2005
Correct typo when /EXACT and multiple apertures used. W.L. Dec 2005
Remove VMS-specific code W.L. Sep 2006
Add additional keywords if /MEANBACK is set W.L Nov 2006
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Project : SOHO - CDS
Name : APPEND_ARR
Category : Utility
Purpose : Manageable method for concatanating arrays
Syntax : IDL> result=append_arr(input,append)
Inputs : INPUT = array (or scalar) that requires appending
APPEND = array (or scalar) to append
Outputs : concatanated arrays
Keywords : NO_COPY = set to not create internal copy of
INPUT & APPEND (it will be destroyed)
CALLS: ***
ERR_STATE, EXIST
CALLED BY:
ADD_METHOD, Compound widget for packet control parameter selection, EIT_COPY
FILE2FID, FIND_CAT, FIND_FID, FIND_PROC, FITS WRITER CLASS FOR RHESSI IMAGES
FRAME ABSTRACT CLASS DEFINITION, FTP_BBSO, FTP_KISF, FTP_MLSO_IMAGES, FTP_MWSO
FTP_NOBE, FTP__DEFINE, GET_FID, GET_FITS_CEN, GET_METHODS, GET_SUMER_FILES
GOES__DEFINE, HAVE_FILES, HAVE_TAG, HESSI CLEAN ALGORITHM CLASS DEFINITION
HESSI ROLL_DB CLASS DEFINITION, HSI_FIND_FILE, HSI_SOCK_FIND, HSI_SOCK_LIST
HTTP__DEFINE, JOIN_STRUCT [2], JSMOVIE, JSMOVIE2, LOC_FILE [2], MDI_COPY, MDI_LATEST
MK_LINK, MK_SUMER_DBASE, OBJ_DISSECT, OBJ_PARENTS, PAIR_STRUCT, PLOT_MAP, RD_RSTN
REBIN_FID, SHOW_SYNOP__DEFINE, SITE__DEFINE, SPEX_FIT__DEFINE, STRIP_ARG
STRUCTURE TO VOTABLE, STR_CHUNK, STR_EXPAND, SYNOP_DEFINE, TRACE_COPY, WRAP_TXT
XALIVE, XDIFF, XYPLOT__DEFINE, axis_get_expanded_range, axis_get_limits, db_gbo
fit_comp_kw, fit_model_components, gzip, hsi_format_flare, hsi_params_write_pro
hsi_plot_flux, hsi_select_flare, hsi_show_flags [2], ihy_db, list_sp_files
mark_poly, ospex_params_write_pro, plotman, read_hessi_4_ospex_params
spex_bk__define, spex_bkint__define, spex_hessi_image__define, str_sub2top
str_top2sub
to return information about a function which can consist of multiple
uncompress, wc_where_arr
History : Written: 1-Oct-1998, Zarro (SM&A/GSFC)
Modified: 26-March-2000, Zarro - sped up with SIZE and CATCH
Modified: 25-Feb-2003, Zarro - improved error checking
Contact : DZARRO@SOLAR.STANFORD.EDU
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Project : SOHO - CDS
Name : APPEND_SDB
Purpose : append 'sdb' directories to ZDBASE
Category : Planning
Syntax : IDL> append_sdb
CALLS: ***
CHKLOG [1], CHKLOG [2], EXP_ZDBASE, GET_PATH_DELIM, IS_BLANK, IS_DIR, IS_STRING
LOCAL_NAME, MKLOG
Side effects: Environment/logical ZDBASE is reset
History : 15-Feb-2004, Zarro (L-3Com/GSFC), Written
Contact : DZARRO@SOLAR.STANFORD.EDU
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Project : SOHO - CDS
Name : APPLY_LOCK
Purpose : create a LOCK file
Category : Planning
Explanation : creates a LOCK file with the creation date saved in file.
Syntax : IDL> apply_lock,lock_file
Inputs : LOCK_FILE = lock file name (with path)
Keywords : ERR - message string
QUIET - turn off printing
EXPIRE - seconds after which LOCK file expires
CALLS: ***
CHKLOG [1], CHKLOG [2], DATATYPE [1], DATATYPE [2], DATATYPE [3], ESPAWN, EXIST
GET_PID, GET_USER_ID, IS_BLANK, TRIM
CALLED BY:
LOCK_ZDBASE, db_gbo, ihy_db
History : Version 1, 17-July-1996, D M Zarro. Written
Contact : DZARRO@SOLAR.STANFORD.EDU
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NAME:
ARCBAR
PURPOSE:
Draw an arc bar on an image showing the astronomical plate scale
CALLING SEQUENCE:
ARCBAR, hdr, arclen,[ COLOR= , /DATA, LABEL= , /NORMAL, POSITION =,
/SECONDS, SIZE=, THICK=, FONT= ]
INPUTS:
hdr - image FITS header with astrometry, string array
arclen - numeric scalar giving length of bar in arcminutes (default)
or arcseconds (if /SECONDS is set)
OPTIONAL KEYWORD INPUTS:
COLOR - integer scalar specifying the color to draw the arcbar (using
PLOTS), default = !P.COLOR
/DATA - if set and non-zero, then the POSITION keyword is given in data
units
LABEL - string giving user defined label for bar. Default label is size
of bar in arcminutes
/NORMAL - if this keyword is set and non-zero, then POSITION is given in
normalized units
POSITION - 2 element vector giving the (X,Y) position in device units
(or normalized units if /NORMAL is set, or data units if /DATA
is set) at which to place the scale bar. If not supplied,
then the user will be prompted to place the cursor at the
desired position
/SECONDS - if set, then arlen is specified in arcseconds rather than
arcminutes
SIZE - scalar specifying character size of label, default = 1.0
THICK - Character thickness of the label, default = !P.THICK
FONT - scalar font graphics keyword (-1,0 or 1) for text
EXAMPLE:
Place a 3' arc minute scale bar, at position 300,200 of the current
image window, (which is associated with a FITS header, HDR)
IDL> arcbar, HDR, 3, pos = [300,200]
CALLS: ***
AD2XY, EXTAST, GSSSADXY, SXPAR [1], SXPAR [2], SXPAR [3], TVCURSOR
RESTRICTIONS:
When using using a device with scalable pixels (e.g. postscript)
the data coordinate system must be established before calling ARCBAR.
If data coordinates are not set, then ARCBAR assumes that the displayed
image size is given by the NAXIS1 keyword in the FITS header.
PROCEDURE CALLS:
AD2XY, EXTAST, GSSSADXY, SXPAR()
REVISON HISTORY:
written by L. Taylor (STX) from ARCBOX (Boothman)
modified for Version 2 IDL, B. Pfarr, STX, 4/91
New ASTROMETRY structures W.Landsman, HSTX, Jan 94
Recognize a GSSS header W. Landsman June 94
Added /NORMAL keyword W. Landsman Feb. 96
Use NAXIS1 for postscript if data coords not set, W. Landsman Aug 96
Fixed typo for postscript W. Landsman Oct. 96
Account for zeropoint offset in postscript W. Landsman Apr 97
Converted to IDL V5.0 W. Landsman September 1997
Added /DATA, /SECONDS keywords W. Landsman July 1998
Use device-independent label offset W. Landsman August 2001
Allow font keyword to be passed. T. Robishaw Apr. 2006
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Project : SOHO - CDS
Name : ARCMIN2HEL2()
Purpose : Convert arcmin from sun centre to heliographic coords,
using the correct (perspective) transformation.
Derived from arcmin2hel (which uses an orthographic
transformation); meant as a drop-in replacement.
Explanation : Converts an (x,y) position given in arcmins relative to the
solar disk centre to heliographic coordinates for the date
supplied (default date = today). The formula used is
valid for any viewpoint -- though results can be "funny"
from viewpoints inside the Sun.
Use : IDL> helio = arcmin2hel(xx,yy,date=date)
Inputs : xx - E/W coordinate in arc minutes relative to sun center
(West is positive); can be a vector
yy - S/N coordinate in arc minutes relative to sun center
(North is positive); can be a vector
Opt. Inputs : None
Outputs : Function returns a 2xN element vector: [lat, long] in
degrees, where N is number of elements in XX and YY
Opt. Outputs: None
Keywords : date - date/time in any CDS format
soho - if set uses the SOHO view point rather than
the Earth. Note this functionality is
duplicated by the system variable SC_VIEW,
which in turn is set by the procedures
USE_EARTH_VIEW or USE_SOHO_VIEW.
off_limb - flag which is true if the coordinates are beyond
the solar limb.
error - Output keyword containing error message;
a null string is returned if no error occurs
radius - solar radius value [output in arcmin units]
no_copy - input xx and yy arrays are destroyed
p - If specified, override pb0r for p angle
b0 - If specified, override pb0r for b angle
r0 - If specified, override pb0r for solar apparent
dia: r0 is the observer's distance from the
Sun, in solar radii (one may use "zunits" to
convert fron solar radii to, say, kilometers).
l0 - If specified, this is the longitude (relative
to Earth- or SOHO- central meridian) of the
sub-observer meridian. Useful for reprojections
and locations far from Earth.
sphere - If set, return longitude over the whole sphere
rather than mirror reflecting around the
lon=90 meridian. (Useful for nonzero B angle)
backside - If set, return the farthest, rather than nearest,
matching point.
Calls : ***
ANYTIM2UTC [1], ANYTIM2UTC [2], ARCMIN2HEL, DELVARX [1], DELVARX [2], DELVARX [3]
DELVARX [4], GET_UTC, PB0R, TRIM, delvarx [5], is_number [1], is_number [2]
Restrictions: If the supplied coordinates are outside the solar disk, the
region is projected onto the limb.
Prev. Hist. : Original by J P Wuelser.
Written : CDS version by C D Pike, RAL, 6 Sept 93
Modified : Converted to use CDS time and pb0r routines, CDP, 17-May-94
Version 3, William Thompson, GSFC, 14 November 1994
Modified .DAY to .MJD
Version 4, July 31, 1995, Liyun Wang, GSFC/ARC
Vectorized the input parameters (i.e., the two
input parameters can be vectors)
Added ERROR keyword
Version 5, 26-Feb-96, CDP
Added SOHO keyword.
Version 6, March 11, 1996, Liyun Wang, GSFC/ARC
Modified such that point of view can be changed to
SOHO if the env variable SC_VIEW is set to 1
Version 7, March 13, 1996, Liyun Wang, GSFC/ARC
Allow scalar and vector input.
Version 8, August 2, 1996, Liyun Wang, NASA/GSFC
Error from calling PB0R is ignored
Version 9, June 10, 1997, Liyun Wang, NASA/GSFC
Fixed a bug that occurs when trying to avoid off-limb points
Version 10, Sept 10, 1997, Zarro SAC/GSFC
Added RADIUS output keyword
Version 11, Oct 7, 1997, Zarro SAC/GSFC
Added some calls to TEMPORARY
Version 12, November 4, 1997 Giulio Del Zanna, UCLAN, UK
corrected the fact that the DATE format was changed
inside the routine (e.g. string to a structure)
Version 13, February 20, 1998, Zarro (SAC/GSC)
- Added more error checking and improved memory management
- Added /NO_COPY (use with care)
Version 14, Dec 17, 1998, DeForest (Stanford/GSFC)
- Added PB0R overrides on a keyword-by-keyword basis
Version 15, 6-Jan-1999, DeForest (Stanford/GSFC)
- Added keyword override to remove mirror-image behavior
around the azimuthal meridian.
Version 16, 7-Jan-99, Zarro (SMA/GSFC)
- Made use of SOHO keyword more logical
Version 17, 8-Apr-99, DeForest (Stanford/GSFC)
- Added L0 keyword; renamed R -> R0 to avoid conflict with
"radius" keyword (FDWIM).
Version 17.5, 8-Apr-99, DeForest (Stanford/GSFC)
- Modified interpretation of R0 keyword to agree with
hel2arcmin: observer distance from Sun.
Version 17.6, 9-Apr-99, Andretta (CUA/GSFC)
- Corrected a bug in the distance-radius conversion
Version 18, 23-Feb-2000, DeForest (SWRI)
- Changed to the correct (non-orthographic)
transformation.
Version 19, 22-Aug-2001, Zarro (EITI/GSFC)
Added ANGLES keyword
Version 20, 29-Nov-2001, William Thompson, GSFC
Corrected bug with (0,0) as input
Version 21, 15-Mar-2002, Zarro/Andretta.
Correct bugs in use of ANGLES and SOHO keywords
Version 22, 12-July-2004, Zarro (L-3Com/GSFC)
Added check for negative square roots
Version 23, 10-Jan-2005, Zarro (L-3Com/GSFC)
Added /DEBUG and converted () to []
14-March-05, Zarro (L-3Com/GSFC) - added more
calls to TEMPORARY
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NAME:
ARCTAN
PURPOSE:
Generalized arctan function that resolves the 180-degree ambiguity
which is not resolved with the standard atan function.
INPUTS:
x =cos(angle), can be arrays
y =sin(angle), can be arrays
OUTPUTS:
a =angle [0<a<2*pi] in radian
a_deg =angle [0<a<360] in degrees
CALLED BY:
COORD_CART_HELIO [1], C_TO_S, FWD_MODELMAP, STEREO_LOOP
EXAMPLE:
a0 =225.*(!pi/180.)
x =cos(a0)
y =sin(a0)
arctan,x,y,a,a_deg
print,a_deg --> 225. ;180-degree ambiguity is resolved
print,atan(y/x)*(180./!pi) --> 45. ;180-degree ambiguity is not resolved
MODIFICATION HISTORY:
1990, written, aschwand@lmsal.com
1999 Dec 1, contributed to SSW
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Project : SOHO-CDS
Name : ARR2GIF
Purpose : Write images to a series of GIF files
Category : imaging
Explanation :
Syntax : IDL> arr2gif,images,file
CALLS: ***
CONCAT_DIR [1], CONCAT_DIR [2], CONCAT_DIR [3], CONGRID [1], CONGRID [2]
CONGRID [3], DATATYPE [1], DATATYPE [2], DATATYPE [3], EXIST, EXPAND_TILDE [1]
EXPAND_TILDE [2], SSW_WRITE_GIF, TEST_OPEN, TRIM, concat_dir [4]
Examples :
Inputs : IMAGES = times series of 2-d images (x,y,t)
Opt. Inputs : None
Outputs : FILE = filename with listing of individual GIF filenames
Opt. Outputs: None
Keywords : XSIZE,YSIZE = new sizes to CONGRID images
FILE = filename with listing of individual GIF filenames
OUT_DIR = output directory for GIF files (def=curr or home)
INTERP= smooth images
History : Written 22 March 1997, D. Zarro, ARC/GSFC
Version 2, 13-Aug-2003, William Thompson
Use SSW_WRITE_GIF instead of WRITE_GIF
Contact : dzarro@solar.stanford.edu
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Project : SSW
Name : ARR2STR()
Purpose : Convert an array to a delimited string.
Explanation :
Use : IDL> s = arr2str(array,'-')
s = arr2str(array,delim='-')
Inputs : arr - input data array which is to be converted
to a simple string.
Opt. Inputs : delim - an alternative positional parameter to specify the
delimiter.
Outputs : Function returns a simple string using the delimiter to
separate the elements of the original array.
Opt. Outputs:
Keywords : delimiter - specify the delimiter to be used, default
delimiter is ','
trim_str - If set, call STRTRIM when converting to string
compress - If set, call STRCOMPRESS after converting
no_duplicate If set, inhibit having string with consecutive
delimiters such as //
Category : Util, string
Prev. Hist. : Sam Freeland 11/19/91
(Various Slf,MDM,DP mods)
Written : Sam Freeland
Modified : Version 2, William Thompson, GSFC, 15 June 1995
Added /TRIM keyword to be compatible with Yohkoh
version. Added /COMPRESS keyword
Version 2.1, Sam Freeland, SSW merge
Version 3, Zarro (SAC/GSFC) - added /NO_DUPLICATE &
renamed TRIM keyword to TRIM_STR to avoid
name conflict with TRIM function
Modified, 17-Mar-03, Zarro (EER/GSFC) - changed loop variable
to long, change to use [], added error checks,
changed 'string' variable name to 'ostring' in case
of reserved name conflicts
CALLED BY
ADD_METHOD, ADD_PATH [1], ADD_PATH [2], BATSE_TIME_INPUT, BUILD_DRM_MER_CONT
CDS_PLAN_BRIEF, CHECK_KAP, CH_LINE_LIST, CLEAN_PATH, CRONTAB, CkFurFiles
Create_update_tar, DB_CHECK, DEF2C_FORMAT, DEF2STRUCT, DISCSP_BANDS, EIT_COPY
EIT_GBO, EIT_QUALITY [1], EIT_QUALITY [2], EVAL_SHERB, EXEC_STRUCT, EXP_DBASE
EXP_ZDBASE, FIND_CAT, FITS WRITER CLASS FOR ANY RHESSI DATA TYPES, FIX_DATE
FTP__DEFINE, GET_ANOMALY, GET_CDS_FOV, GET_CDS_XY, GET_SID, HESSI
HESSI CALIBRATED EVENTLIST CLASS DEFINITION [3]
HESSI PACKET FILE ABSTRACT CLASS, HESSI_DATA_PATHS [1], HESSI_DATA_PATHS [2]
HSI_CHK_DUPLICATE, HSI_EST_MEMMAX, HSI_EVENTLIST_SELECT_BY_ENERGY
HSI_EVENTLIST_SELECT_BY_TIME [1], HSI_EVENTLIST_SELECT_BY_TIME [2]
HSI_RD_FITS_SPECTRUM, HXFITS, LATEST_IMAGE, LIST_ANOMALY, LIST_GEV, LIST_NAR
LOCAL_DIFFS, Load_recs, MCURVEFIT, MDI_GBO, MERGE_DISCSP_HKG_OCC, MK_CDS_ANALYSIS
MK_CDS_PLAN, MK_MER_CONT, MK_PLAN_ORDER, MK_PLAN_WRITE, MK_RASTER
MkFnMapMake Filename Map, Modify_Merge_list [1], Modify_Merge_list [2]
OCC_DBASE, OP_COM [1], OP_COM [2], OVSA_EXPLORER formerly OVSA_PRESUB, OVSA_FIT
OVSA__DEFINE, PAIR_STRUCT, PARSE_GROSSC_ATTITUDE
POINT SPREAD FUNCTION CLASS DEFINITION, POINT [1], QUERY_ANOMALY
RATIO_PLOTTER [1], RD_IMAGE_FITS, READ_GDFILE_GD, REMOVE_PATH, RM_FILE
RM_PATH [1], RM_PATH [2], ROUTINE_NAME [4], ROUTINE_NAME [7], RTMVI [1], RdTap [1]
RdTap [2], RdTap [3], SEL_LINE_EVENT, SETUP_DRM, SET_CDS_FITS, SITE__DEFINE
SOHO_ITEMS_HTML, SPEX_BACKGROUND [1], SPEX_BACKGROUND [2], SPEX_COMMONS [2]
SPEX_COMMONS [4], SPEX_DRM__DEFINE, SPEX_ENV [2], SPEX_ENV [4], SPEX_ENV [5]
SPEX_FIT__DEFINE, SPEX_GEN__DEFINE, SPEX_HANDLES [1], SPEX_HANDLES [2]
SPEX_PROC [1], SPEX_PROC [2], SPEX_SAVE [1], SPEX_SAVE [2], SPEX_SAVE_DATA [1]
SPEX_SAVE_DATA [2], SPEX_SUMMARY [1], SPEX_SUMMARY [2], SPEX_THISTORY [1]
SPEX_THISTORY [2], SPEX__DEFINE, SSW_LOCAL_PATH, STRUCTURE TO VOTABLE, STR_CHOP
STR_DEBLANK, STR_FIND, STR_TRAIL, SXI_GBO, SYNOP_DEFINE, TEST_DIR2, TRACE_COPY
TRACE_GBO, TRACE_SSWHERE [1], UPDATE_CAMPAIGN, UPDATE_MPG, UPDATE_SXT_CO_INDEX
VALID_TIME, WHICH, WRT_GEN [1], WRT_GEN [2], WRT_GENX [1], WRT_GENX [2], W_HISTOGRAM
XACK, XCAMP, XCAT, XCRON, XLIST, XMATRIX, break_doc [1], break_doc [2], break_doc [3]
cal_fig_mich, ch_ss, check_dumps [1], check_ff_load, check_oldprocess [1]
check_oldprocess [2], check_oldprocess [3], check_oldprocess [4], cnvtimstr
copy_visible, db_gbo, disk_monitor [1], disk_monitor [2], disp_dt_genx
disp_therm_rs232, do_reg_backup, drm_4_spex [1], drm_4_spex [2]
eit_proton_summary, evt_grid, expand_dirs, extract_val, fidmap, fit_comp_kw
fitshead2struct, get_eit_info, get_ovsa_log, get_survey, getcurstr [1]
getcurstr [2], getwkprelst, go_batch [1], go_batch [2], go_ssw_batch
go_yo_prod_batch, goes_summary, gt2exe [1], gt2exe [2], help_merge [1]
help_merge [2], hist_summary, hkplot_info, hsi_a2d_list, hsi_coll_segment_list
hsi_gbo, hsi_get_flare_flags, hsi_getflare, hsi_image_plot
hsi_image_raw__define, hsi_imagemisc_widget, hsi_params_write_pro
hsi_plot_flux, hsi_select_flare, hsi_show_flags [2], hsi_spectrum__filewrite
hsi_ui_flarecat, hsi_ui_lc, hsi_ui_mon, hsi_ui_obs, hsi_ui_qlimage, hsi_ui_spec
html_get_files, hxt_images2ps, ihy_db, image2movie, image_summary, img_summary [1]
img_summary [2], ip_que_dmpver, is_alive [1], is_alive [2], is_bestnode [1]
is_bestnode [2], jitter_gif_xyimg, lastgki, list_mo_log [1], list_mo_log [2]
load_hd, mail [1], mail [2], make_mirror, mk_bad_pix_map_load, mk_lasteit_movie
mk_orbit_files, mk_sfc [1], mk_sfc [2], mk_ssc_batch [1], mk_ssc_batch [2]
mmap_imgnum, mo_patch, mon_sci5k, mtcmd [1], mtcmd [2], mwritefits, netscape_control
nob_img_copy, option_changer [1], option_changer [2], ospex_params_write_pro
ovsa_calib, ovsa_interact, parse_lines [1], parse_lines [2], path_ucon, pathfix
plot_fov [1], plot_goesp, plotman, plotman_imageoptions, point [2]
pr_his_index [1], pr_his_index [2], pr_his_index [3], pref_super, psk_correlate
ratio_plotter [2], rd_guf_ascii, rd_sxg, rd_sxs_pha [1], rd_sxs_pha [2]
rd_tr_seq_head, rdbda_smm, read_batse_4_spex [1], read_batse_4_spex [2], reads
redo_disploi, redo_mon_sci5k, required_tags, restgenx, save_idl_routines, savegenx
secchi_time2files, seq_cubes, set_fastpath [1], set_fastpath [2], set_logwindows
set_oldpath [1], set_oldpath [2], setssw_windows, soon_search [1]
soon_search [3], spec_plot [1], spec_plot [2], spec_plot [3], spec_plot [4]
special_movie, spex_convert_results [1], spex_convert_results [2]
spex_data__define, spex_delete [1], spex_delete [2], spex_evnt [1]
spex_evnt [2], spex_hold [1], spex_hold [2], spex_image__define, spex_merge [1]
spex_merge [2], spex_merge_control [1], spex_merge_control [2]
spex_preview [1], spex_preview [2], spex_source [1], spex_source [2]
spex_spec_plot [1], spex_spec_plot [2], spex_spec_plot [3], spex_spec_plot [4]
ssw_imapcoord2html, ssw_install [1], ssw_install [2], ssw_instr_info
ssw_javamovie, ssw_path, ssw_set_instr, ssw_setup_windows, ssw_start_rpcserver
ssw_swmap_info, str_pow_conv, str_replace [1], str_replace [2], strlist2html [1]
strlist2html [2], strpair2struct, sw_tape, sxt_orhis, sxt_prep_exe, synop_link
table2struct, timeavg [1], timeavg [2], timeline, timstr2ex [1], timstr2ex [2]
todays_targets, topsdb [1], topsdb [2], tr_decode_head [1], tr_decode_head [2]
trace_cosmic2filename, trace_cosmic2hist_accum, trace_dph2struct [1]
trace_scale, trace_sswhere [2], trace_sswhere [3], trace_sswhere [4]
track_proc [1], track_proc [2], ucon_path, url_decode, url_encode, vso_format
wbs_response [1], wbs_response [2], web_seq, where_pattern [1]
where_pattern [2], where_title [1], where_title [2], write_genxcat
write_ovsa_fits, write_trace, write_trace_bin, wrt_rate_ext, wwwidl_server_check
wwwidl_watchdog [1], wwwidl_watchdog [2], xcheckip, xdisp_fits, xdisp_trace [1]
xdisp_trace2, xdisp_trace3, xhkplot, xread_hist, xset_chain [1], xset_chain [2]
xso_butevents [1], xso_butevents [2], xsxt_prep_event, ys_contrib [1]
ys_contrib [2], zformat [1], zformat [2]
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Name: arr_diff
Purpose: boolean function - arrays different? (string/struct/numeric OK)
Input Parameteters:
arr1, arr2 - to arrays to compare
Output Parameters:
ndiff - number of differences
Output:
function returns 1 if there are ANY differences
Keyword Parameters:
ignore_type - ignore numeric type (dont worry about TYPE only differences
for numeric comparisons)
Calling Sequence:
IDL> different=array_diff(array1, array2)
Calling Examples:
IDL> print,array_diff(replicate(!x,10),replicate(!y,10)) ;structure
1
IDL> print,array_diff(replicate(!x,10),replicate(!x,10))
0
IDL> print,array_diff(sindgen(10),sindgen(10)) ;striings
0
IDL> print,array_diff(sindgen(10),alphagen(10))
1
IDL> print,array_diff(indgen(10),findgen(10)) ;numeric
1
IDL> print,array_diff(indgen(10),findgen(10),/ignore_type)
0
CALLS: ***
ARRAY_DIFF, BOX_MESSAGE, STR_DIFF, data_chk [1], data_chk [2]
History:
12-August-2000 - S.L. Freeland - package a few useful checks
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PROJECT:
GENERAL
NAME:
array_concat
PURPOSE:
concatenate a dynamic array with subarrays of variable lengths
x0=fltarr(n0)
x1=fltarr(n1)
The concatenated array is
x_=[x0,x1]
with index ranges
x_(i1:i2)=xj, i1=x_ind(0,j), i2=x_ind(1,j)
CALLING SEQUENCE:
array_concat,i1,i,x,x_,x_ind,n_ind
INPUTS:
i1 = ID number of first subarray
i = ID number of subsequent subarrays
x = subarray of any length
OUTPUTS:
x_ = concatenated array x_=[x_0,x_1,...,x_i]
x_ind(2,n_ind) = start and stop indices of subarrays in concatenated array
n_ind = number of concatenated subarrays
MODIFICATION HISTORY:
Version 1, aschwanden@lmsal.com, Written, 1999 Dec 1
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NAME:
array_decat
PURPOSE:
decatenates a dynamic array into subarrays of variable lengths
This procedure is inverse to FWC_CONCATENATE and uses its arguments
CALLING SEQUENCE:
array_decat,i,x_ind,x_,x,ni
INPUTS:
i = ID number of subsequent subarrays
x_ind(2,n_ind) = start and stop indices of subarrays in concatenated array
x_ = concatenated array x_=[x_0,x_1,...,x_i]
OUTPUTS:
x = subarray with index i
MODIFICATION HISTORY:
Version 1, aschwanden@lmsal.com, Written, 1999 Dec 1
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NAME:
Array_Despike
PURPOSE:
Remove isolated HIGH SIGNAL/NOISE elements from a 2D array, replacing
them with a local mean. This routine iterates until convergence or
a user-supplied maximum number. Only
points passing the S/N cut are affected.
CALLING SEQUENCE:
Newarray = Array_Despike( array, kernel=kernel, $
Sigma=Sigma, threshold=threshold, itmax=itmax, verbose=verbose
INPUT ARGUMENT:
array = the array to despike. Units are counts because sqrt(mean) used
to determine number of standard deviations per spike
OPTIONAL INPUT ARGUMENT:
kernel = local mean computed by convol( array, kernel, /normalize,/edge_truncate)
default kernel is the 8 cells surrounding a cell
SIGMA = the number of standard deviations by which a pixel must
exceed the local background for it to be replaced. DEFAULT = 5.0
ITMAX = the maximum number of iterations. DEFAULT = 20
SCALE = If any scaling is needed for cells, scale is used.
it should have the same size as array. For example, if
array columns have different accumulation times (livetimes)
then this scaling can be applied here. Expectation values
should scale with array/scale.
NOLOW = If set, then negative spikes are not removed
OUTPUT:
Array_Despike returns the array, with spikes removed.
REVISION HISTORY:
7-jul-2006, richard.schwartz@gsfc.nasa.gov
12-jul-2006, richard.schwartz@gsfc.nasa.gov, added scale array input
and fixed problem with totally isolated spikes, minimum
sigma is 1 to keep f_div from reporting 0 for diff/sigma
19-jul-2006, ras, Added removal of negative spikes and NOLOW keyword to disable this
new feature
CALLS:
CALLED BY
read_soxs_4_ospex
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NAME: array_insert
PURPOSE: Insert an array into another array at a specified point.
Output array is dimension of original plus inserted array.
If arr_a is 1-D, arr_b must be 1-D and will be inserted at element 'index'.
If arr_a is 2-D, arr_b can be 1-D or 2-D:
if arr_b is 1-D, the same elements are inserted into every row of arr_a
if arr_b is 2-D, the second dimension must match the second dimension of arr_a
INPUT:
arr_a - destination array
arr_b - array to insert
index - column # in arr_a to place arr_b into
OUTPUT: array of combined arrays. Returns -1 if error.
CALLED BY:
SPEX_FIT__DEFINE, spex_convert_results [1], spex_convert_results [2]
EXAMPLES:
1. arr_a and arr_b are 1-D
print, array_insert (indgen(6), indgen(3), 4)
0 1 2 3 0 1 2 4 5
2. arr_a is 2-D and arr_b is 1-D
print, array_insert (indgen(2,3), [33,34], 1)
0 33 34 1
2 33 34 3
4 33 34 5
3. arr_a and arr_b are 2-D.
print, array_insert (indgen(2,3), transpose([33,34,35]), 1) ; arr_b is 1x3
0 33 1
2 34 3
4 35 5
CALLS: ***
CHECKVAR [1], REPRODUCE, checkvar [2]
Restrictions: Can't handle higher dimensions than 2-D arrays
HISTORY:
Written 5-May-2006, Kim Tolbert
8-Nov-2006, Kim. Use reproduce instead of rebin, so it will work on strings too.
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NAME:
ARRAY_JHUAPL
PURPOSE:
Force given argument to be an array.
CATEGORY:
CALLING SEQUENCE:
y = array_jhuapl(x)
INPUTS:
x = input which may be an array or scalar. in
KEYWORD PARAMETERS:
OUTPUTS:
y = out which is an array. out
CALLS: ***
DATATYPE [1], DATATYPE [2], DATATYPE [3]
CALLED BY:
RECPOL [1], RECPOL [2], RECPOL [3], STRSEC [1], STRSEC [2]
COMMON BLOCKS:
NOTES:
MODIFICATION HISTORY:
R. Sterner, JHU-APL, 28 Jan, 1986.
Converted to SUN 14 Aug, 1989 --- R. Sterner.
30-Apr-92 (MDM) - Renamed from "array.pro" to "array_jhuapl.pro"
Copyright (C) 1986, Johns Hopkins University/Applied Physics Laboratory
This software may be used, copied, or redistributed as long as it is not
sold and this copyright notice is reproduced on each copy made. This
routine is provided as is without any express or implied warranties
whatsoever. Other limitations apply as described in the file disclaimer.txt.
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Project : SOHO - CDS
Name : ARRAY_MATCH()
Purpose : Detect if a vector matches any row or column of a 2D array
Explanation : Search through a 2D array to see if any row (or column, if
keyword COLUMN is set) of it is identical to (or matches)
a given vector.
This routine is called by XCDS to check if the current
study has been selected previously.
Use : Result = array_match(A, B [,/column])
IF (array_match(a,b [,/column])) THEN ...
Inputs : A -- a 2D array with n x m elements
B -- a vector with n elements (or m elements if keyword COLUMN
is to be set)
Opt. Inputs : None.
Outputs : Result -- 1 if vector B matches either row (or column when
COLUMN is set) of array A; 0 otherwise
Opt. Outputs: None.
Keywords : COLUMN -- If set, comparison is made through column of A
Calls : None.
CALLED BY:
hsi_range_widget, hsi_select_flare, hsi_time_widget
Common : None.
Restrictions: Number of elements of vector B must be equal to the column
number (or row number, if the keyword COLUMN is set) of
array A
Side effects: None.
Category : Utilities, array manipulation
Prev. Hist. : None.
Written : Liyun Wang, GSFC/ARC, August 23, 1994
Modified : Liyun Wang, GSFC/ARC, August 24, 1994
Fixed a bug that only checks for a maximum of two rows
Liyun Wang, GSFC/ARC, August 30, 1994
Added keyword COLUMN to allow comparison of one vector with
each column of a 2D array.
Version : Version 1.0, August 30, 1994
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Project : SOHO - CDS
Name : ARRAY_XOR()
Purpose : Returns the XOR elements of two arrays.
Explanation : Given 2 arrays it returns an array containing the elements
that are in either array but not both.
Use : IDL> x = [0,1,2,3,4,8]
IDL> y = [2,3,4,9]
IDL> print,array_xor(x,y) --> 0 1 8 9
Inputs : x,y - two arrays (any type ecept complex and structure)
Opt. Inputs : None
Outputs : Function returns exclusive array
Opt. Outputs: None
Keywords : None
Calls : ***
DATATYPE [1], DATATYPE [2], DATATYPE [3], FIND_COMMON, REM_DUP [1], REM_DUP [2]
REM_DUP [3], REST_MASK
Common : None
Restrictions: Input arrays must be same type
Side effects: None
Category : Util
Prev. Hist. : None
Written : C D Pike, RAL. 22-Apr-97
Modified :
Version : Version 1, 22-Apr-97
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NAME: ARROW
PURPOSE: Draw a vector(s) with an arrow head
CATEGORY: Graphics
CALLING SEQUENCE:
ARROW, x0, y0, x1, y1
INPUTS:
(x0, y0) = coordinates of beginning of vector(s). May be arrays
or scalars. Coordinates are in DEVICE coordinates
unless otherwise specified.
(x1, y1) = coordinates of endpoint (head) of vector.
x0, y0, x1, y1 must all have the same number of elements.
KEYWORD PARAMETERS:
DATA - if set, implies that coordinates are in data coords.
NORMALIZED - if set, coordinates are specified in normalized coords.
HSIZE = size of arrowhead. Default = 1/64th the width of the device,
(!D.X_SIZE / 64.).
If the size is positive, it is assumed to be in device
coordinate units. If it is NEGATIVE, then the head length
is set to the vector length * abs(hsize), giving heads
proportional in size to the bodies. The size is defined as
the length of each of the lines (separated by 60 degrees)
that make the head.
COLOR = drawing color. Default = highest color index.
HTHICK = thickness of heads. Default = 1.0.
SOLID = if set, make a solid arrow, using polygon fills, looks better
for thick arrows.
THICK = thickness of body. Default = 1.0.
OUTPUTS:
No explicit outputs.
CALLED BY:
NEAR_CONJ, POINTING3, STARFIELD, TERM_QUICK, TERM_REVIEW, TERM_REVIEW_GIF, VIEW_RAW
XFLOW_DIAG [1], arrow2, help_roll, mdipdist, qNagoya_Skymap, xflow_diag [2]
SIDE EFFECTS:
RESTRICTIONS:
PROCEDURE:
Straightforward.
Examples:
Draw an arrow from (100,150) to (300,350) in DEVICE units.
ARROW, 100, 150, 300, 350
Draw a sine wave with arrows from the line Y=0 to
sin(x/4).
X = FINDGEN(50)
Y = SIN(x/4) ;Make sin wave
PLOT, X, Y
ARROW, X, REPLICATE(0,50), X, Y, /DATA
MODIFICATION HISTORY:
DMS, Feb, 1992.
DMS, Sept, 1992. Added /SOLID.
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NAME:
arrow2
PURPOSE:
Wrapper routine for IDL user library ARROW routine.
arrow2 works with tv2 to provide easier PostScript placement.
CALLING SEQUENCE:
arrow2, x0, y0, x1, y1 ; Provide head & tail coordinates
arrow2, x0, y0, angle, length, /angle ; x0,y0 = arrow's tail
arrow2, x0, y0, angle, length, /angle, /head ; x0,y0 = arrow's head
arrow2, x0, y0, angle, length, /angle, /tv2 ; Assume tv2,/init has been
previously called (see below).
INPUTS:
x0, y0 - Defines the tail of the arrow, or if /head is set, the
head of the arrow.
x1, y1 - Defines the head of the arrow, or if /head is set, the
the tail.
angle - if /angle is set, is the angle in degrees, counter
clockwise. 0.0 points to the right.
length - If /angle is set, is the length of the arrow in device,
data or normalized coordinates.
OPTIONAL INPUT PARAMETERS:
/angle - If set, 3rd and 4th parameters are the angle and length
of the arrow, respectively.
/head - To change x0, y0 to define the head of the arrow.
HSIZE, COLOR, HTHICK, THICK, SOLID are the same as in ARROW
DATA - if set, implies that coordinates are in data coords.
NORMALIZED - if set, coordinates are specified in normalized coords.
DEVICE - if set, coordinates are specified in device coords.
/tv2 - if set, assumes tv2,/init, xsiz_pix, ysiz_pix has
be previously called. In this case, /data, /norm and
and /dev will have no effect, since /dev will be assumed for
X-output and the pseudo window pixel coordinates will be
assumed for PostScript output.
CALLS: ***
ARROW
CALLED BY:
MARK_POINT, evt_grid
COMMON BLOCKS:
tv2_blk (which is created by tv2,/init).
METHOD:
arrow2 requires the PostScript plotting size to be set by a previous call
to tv2/init,xsiz_pix,ysiz_pix (see the document header of tv2 for more
information), which stores various parameters in common.
See also the following routines:
tv2, ocontour, draw_grid (sxt_grid), plots2
MODIFICATION HISTORY:
23-Jan-1996, J. R. Lemen (LPARL), Written.
24-Jan-2002, Kim Tolbert. Ensure that !p.psym is 0 before drawing arrow.
26-Dec-2002, Zarro (EER/GSFC) - removed unsupported /device in arrow call
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NAME:
ARROWS
PURPOSE:
To display "weathervane" directional arrows on an astronomical image
EXPLANATION:
Overlays a graphic showing orientation of North and East.
CALLING SEQUENCE:
ARROWS,h, [ xcen, ycen, ARROWLEN= , CHARSIZE= COLOR= , /DATA
FONT=, /NORMAL, /NOTVERTEX, THICK= ]
INPUTS:
h - FITS header array, must include astrometry
OPTIONAL INPUTS:
xcen,ycen - numeric scalars, specifying the center position of
arrows. Position in device units unless the /NORMALIZED
keyword is specified. If not supplied, then ARROWS
will prompt for xcen and ycen
OPTIONAL KEYWORD INPUTS:
arrowlen - length of arrows in terms of normal Y size of vector-drawn
character, default = 3.5, floating point scalar
charsize - character size, default = 2.0, floating point scalar
color - color that the arrows and NE letters should be. Default
value is !P.COLOR
Data - if this keyword is set and nonzero, the input center (xcen,
ycen) is understood to be in data coordinates
font - IDL vector font number (1-20) to use to display NE letters.
For example, set font=13 to use complex italic font.
NotVertex - Normally (historically) the specified xcen,ycen indicated
the position of the vertex of the figure. If this
keyword is set, the xcen,ycen coordinates refer to a sort
of 'center of mass' of the figure. This allows the
figure to always appear with the area irregardless of
the rotation angle.
Normal - if this keyword is set and nonzero, the input center
(xcen,ycen) is taken to be in normalized coordinates. The
default is device coordinates.
thick - line thickness, default = 2.0, floating point scalar
OUTPUTS:
none
CALLS: ***
GETROT, ONE_ARROW, ZPARCHECK [1], ZPARCHECK [2], ZPARCHECK [3]
CALLED BY:
ATV, TVLASER
EXAMPLE:
Draw a weathervane at (400,100) on the currently active window,
showing the orientation of the image associated with a FITS header, hdr
IDL> arrows, hdr, 400, 100
METHOD:
Uses EXTAST to EXTract ASTrometry from the FITS header. The
directions of North and East are computed and the procedure
ONE_ARROW called to create the "weathervane".
PROCEDURES USED:
GETROT - Computes rotation from the FITS header
ONE_ARROW - Draw a labeled arrow
ZPARCHECK
REVISON HISTORY:
written by B. Boothman 2/5/86
Recoded with new procedures ONE_ARROW, ONE_RAY. R.S.Hill,HSTX,5/20/92
Added separate determination for N and E arrow to properly display
arrows irregardless of handedness or other peculiarities and added
/NotVertex keyword to improve positioning of figure. E.Deutsch 1/10/93
Added /DATA and /NORMAL keywords W. Landsman July 1993
Recognize GSSS header W. Landsman June 1993
Added /FONT keyword W. Landsman April 1995
Modified to work correctly for COLOR=0 J.Wm.Parker, HITC 1995 May 25
Work correctly for negative CDELT values W. Landsman Feb. 1996
Converted to IDL V5.0 W. Landsman September 1997
Use GETROT to compute rotation W. Landsman June 2003
Restored /NotVertex keyword which was not working after June 2003 change
W. Landsman January 2004
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NAME:
ASCII
PURPOSE:
Print ASCII characters based on its numerical decimal value.
EXPLANATION:
CALLING SEQUENCE:
ASCII [,/ext]
INPUTS:
None.
OPTIONAL INPUTS:
None.
OUTPUTS:
None.
OPTIONAL OUTPUTS:
None.
KEYWORD PARAMETERS:
EXT -- Prints only extended ASCII characters.
CALLS:
None.
COMMON BLOCKS:
None.
RESTRICTIONS:
None.
SIDE EFFECTS:
None.
MODIFICATION HISTORY:
Written September 12, 1994, by Liyun Wang, GSFC/ARC
VERSION: Version 1, September 12, 1994
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NAME:
ASINH
PURPOSE:
Return the inverse hyperbolic sine of the argument
EXPLANATION:
The inverse hyperbolic sine is used for the calculation of asinh
magnitudes, see Lupton et al. (1999, AJ, 118, 1406)
CALLING SEQUENCE
result = asinh( x)
INPUTS:
X - hyperbolic sine, numeric scalar or vector or multidimensional array
(not complex)
OUTPUT:
result - inverse hyperbolic sine, same number of elements as X
double precision if X is double, otherwise floating pt.
METHOD:
Expression given in Numerical Recipes, Press et al. (1992), eq. 5.6.7
Note that asinh(-x) = -asinh(x) and that asinh(0) = 0. and that
if y = asinh(x) then x = sinh(y).
REVISION HISTORY:
Written W. Landsman February, 2001
Work for multi-dimensional arrays W. Landsman August 2002
Simplify coding, and work for scalars again W. Landsman October 2003
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Project : SOHO - CDS
Name :
ASK
Purpose :
Gets a single letter response from the keyboard.
Explanation :
Gets a single letter response from the keyboard. Only responses in the
array VALID are allowed. The prompt string is printed, and GET_KBRD is
called to read in the result.
Use :
ASK, PROMPT, ANSWER [, VALID ]
CALLED BY:
CONCAT4DOS [1], CONCAT4DOS [2], TVPOINTS, XCOR_CDS
Example: ASK, 'Do you want to continue? ', ANSWER
Inputs :
PROMPT = Prompt to ask for input.
Opt. Inputs :
VALID = List of valid responses, put together into one character
string. If not passed, then "YN" is assumed. All characters
are converted to uppercase.
Outputs :
ANSWER = Single letter answer. This is always returned as uppercase.
Opt. Outputs:
None.
Keywords :
FONT = Font to use when displaying the prompt widget. Only
meaningful when the prompt is displayed in a text widget
(currently only in IDL for Windows). If not passed, then the
first available 20 point font is used.
Calls : ***
FILEPATH, SETPLOT [1], SETPLOT [2]
Common :
None.
Restrictions:
Any non-printing key will act just like the return key when used with
IDL for Microsoft Windows. This includes the delete and backspace
keys, which otherwise would erase the previous selected character.
Side effects:
None.
Category :
Utilities, User_interface.
Prev. Hist. :
W.T.T., Oct. 1989.
William Thompson, 11 May 1993, converted to use widgets when available.
This makes it compatible with IDL for Windows, together with a
small change for carriage returns. Also added FONT keyword.
William Thompson, 22 June 1993, converted to use widgets only with IDL
for Windows.
Written :
William Thompson, GSFC, October 1989.
Modified :
Version 1, William Thompson, GSFC, 9 July 1993.
Incorporated into CDS library.
Version 2, William Thompson, GSFC, 11-Aug-1997
Changed to be more compatible with IDL v4.
Version :
Version 2, 11-Aug-1997
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Project : SOHO - CDS
Name : ASMOOTH()
Purpose : Smooths a one or two-dimensional array.
Category : Image-processing, SU:SERTSIM, Class3
Explanation : Does the same thing as the IDL built-in SMOOTH function, except
that:
1. The effect tapers off at the edges of the array, instead
of abruptly stopping as in SMOOTH.
2. Missing pixels are handled.
Syntax : Result = ASMOOTH( ARRAY, WIDTH )
Examples :
Inputs : ARRAY = One or two-dimensional array to be smoothed.
WIDTH = Width of the smoothing box. If an even number, then
WIDTH+1 is used.
Opt. Inputs : None.
Outputs : The result of the function is the smoothed array.
Opt. Outputs: None.
Keywords : MISSING = The value representing missing pixels.
Calls : ***
FLAG_MISSING, GET_IM_KEYWORD, IS_NOT_MISSING
Common : None.
Restrictions: ARRAY must be one or two-dimensional.
Side effects: None.
Prev. Hist. : Originally written for the SERTS project, February 1993.
History : Version 1, 14-Aug-1998, William Thompson, GSFC
Version 2, 29-Oct-1998, William Thompson, GSFC
Fixed bug at edges of array when MISSING is not used.
Version 3, 02-Dec-1998, William Thompson, GSFC
Fixed bug when WIDTH is even, and MISSING not passed.
Version 4, 24-Dec-2002, William Thompson, GSFC
Sped up by using built-in SMOOTH function.
Version 5, 11-May-2005, William Thompson, GSFC
Handle NaN values
Contact : WTHOMPSON
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NAME:
ASTDI