11/19/2012

After you have typed 
"idlz"
(This will run IDL in a mode where no outputs are directed to the terminal screen.)

At the command prompt and gotten into idl type:
.r cycle_vu_stel_stel_diff_12_3_30Rs
(This should compile the main program (from the directory where you have typed "idlz".)

For this program I then ran:
cycle_vu_stel_stel_diff_12_3_30Rs,source='/home/bjackson/soft/for/development/ipstd20n_in-situ/test/MEXART_2082/',destination='/home/bjackson/soft/for/development/ipstd20n_in-situ/test/MEXART_2082/images/',/ecliptic,/density,filter='nv3h*',/speed,/ips_glevel,/hammer,/fisheye,/meridional,/stereo,/points
(This ran the cycle_vu_stel_stel_diff_12_3_30Rs IDL program taking files from the source directory (in ths case /home/bjackson/soft/for/development/ipstd20n_in-situ/test/MEXART_2082/) and placing them in the destination directory (in this case /home/bjackson/soft/for/development/ipstd20n_in-situ/test/MEXART_2082/images/).
The file output from the tomography program named nagoya.2009 (The same year as the Carrington rotation imaged) must be in the "source" directory in order that the source "points" that survived the edits and were used in the program be added to the "fisheye" and "Hammer-Aitoff" images. 

Another IDL program to compile and run is:
.r insitu_drive.pro
Then type:
insitu_drive, source='/home/bjackson/soft/for/development/ipstd20n_in-situ/test/MEXART_2082/',destination='/home/bjackson/soft/for/development/ipstd20n_in-situ/test/MEXART_2082/images/',/ace0,/ips
(This provides the plots of the ace level-zero data versus the different e3, E3, ea output files.)
To get these plots into png files (from the eps files output) type:
convert e3_2082.000_ACE_L0_ips_D_delt_1.00.eps -bordercolor white -border 0x0 e3_2082.000_ACE_L0_ips_D_delt_1.00.png