;+ ; hsi_image script - created Tue Oct 4 12:44:21 2022 by hsi_params2script.pro ; Includes only parameters changed from default settings. ; ; Note: This script simply sets control parameters in the hsi_image object as they ; were when you wrote the script. To make the object do anything in this script, ; you need to add some action commands. For instance, the command ; image= obj->getdata() ; would generate and return the image. ; ; For a complete list of control parameters look at the tables in ; http://hesperia.gsfc.nasa.gov/ssw/hessi/doc/hsi_params_all.htm ; ; There are several ways to use this script: ; ; A. Run this procedure via this command (compile first if it's not in your IDL path): ; hsi_image_script_nondefault_params_bproj_image_20030429_0415_40tx2e, obj=obj ; Note: you can set additional parameters or override parameters in script via: ; hsi_image_script_nondefault_params_bproj_image_20030429_0415_40tx2e, obj=obj, $ ; param1=param1, param2=param2,... ; or ; B. Compile and execute it as a main program by: ; 1. Comment out the "pro" line and save. ; 2. From the command line, $ ; type .run hsi_image_script_nondefault_params_bproj_image_20030429_0415_40tx2e. ; In the IDLDE, click Compile, then Execute. ; 3. Use .GO to restart at the beginning of the script ; or ; C. Execute it as a batch file via: ; 1. Comment out the "pro" and "end" lines and save. ; 2. Run the commands via @hsi_image_script_nondefault_params_bproj_image_20030429_0415_40tx2e ; ; Once you have run the script (via one of those 3 methods), you will have an ; hsi_image object called obj that is set up as it was when you wrote the script. ; You can proceed using obj from the command line or the hessi GUI. ; To use it in the GUI, type ; hessi,obj ; To use it from the command line, here are a few examples of commands: ; data = obj->getdata() ; retrieve the last image made ; data = obj->getdata(use_single=0) ; retrieve all images in cube ; obj->plot ; plot the last image ; obj->plotman ; plot the last image in plotman ; obj->plotman, /choose ; choose which image(s) in cube to plot in plotman ;- pro hsi_image_script_nondefault_params_bproj_image_20030429_0415_40tx2e, obj=obj, $ _extra=_extra obj = hsi_image() obj-> set, cbe_normalize= 1 obj-> set, image_algorithm= 'BPROJ' ;obj-> set, snr_chk= 1 ;obj-> set, $ ; snr_vis_file= '/data/rhessi_extras/visibility_fits_v2/2003/04/29/hsi_vis_20030429_0415_0512_40tx2e.fits' obj-> set, mpat_coord= 'CART' obj-> set, image_dim= [101, 101] obj-> set, pixel_size= [1.50000, 1.50000] obj-> set, im_time_interval= [['29-Apr-2003 04:15:04.200', '29-Apr-2003 04:16:34.916'], $ ['29-Apr-2003 04:16:34.916', '29-Apr-2003 04:18:04.916'], ['29-Apr-2003 04:18:04.916', $ '29-Apr-2003 04:19:34.916'], ['29-Apr-2003 04:19:34.916', '29-Apr-2003 04:21:04.916'], $ ['29-Apr-2003 04:21:04.916', '29-Apr-2003 04:22:34.916'], ['29-Apr-2003 04:22:34.916', $ '29-Apr-2003 04:24:04.916'], ['29-Apr-2003 04:24:04.916', '29-Apr-2003 04:25:34.916'], $ ['29-Apr-2003 04:25:34.916', '29-Apr-2003 04:27:04.916'], ['29-Apr-2003 04:28:16.916', $ '29-Apr-2003 04:30:16.916'], ['29-Apr-2003 04:30:16.916', '29-Apr-2003 04:31:27.916'], $ ['29-Apr-2003 04:31:27.916', '29-Apr-2003 04:32:34.916'], ['29-Apr-2003 04:32:34.916', $ '29-Apr-2003 04:33:34.916'], ['29-Apr-2003 04:33:34.916', '29-Apr-2003 04:34:34.916'], $ ['29-Apr-2003 04:34:34.916', '29-Apr-2003 04:35:34.916'], ['29-Apr-2003 04:35:34.916', $ '29-Apr-2003 04:36:34.916'], ['29-Apr-2003 04:36:34.916', '29-Apr-2003 04:37:34.916'], $ ['29-Apr-2003 04:37:34.916', '29-Apr-2003 04:38:34.916'], ['29-Apr-2003 04:38:34.916', $ '29-Apr-2003 04:39:34.916'], ['29-Apr-2003 04:39:58.702', '29-Apr-2003 04:40:58.922'], $ ['29-Apr-2003 04:40:58.922', '29-Apr-2003 04:42:01.922'], ['29-Apr-2003 04:42:01.922', $ '29-Apr-2003 04:43:01.922'], ['29-Apr-2003 04:44:25.571', '29-Apr-2003 04:45:25.917'], $ ['29-Apr-2003 04:45:25.917', '29-Apr-2003 04:46:25.917'], ['29-Apr-2003 04:46:25.917', $ '29-Apr-2003 04:47:25.917'], ['29-Apr-2003 04:48:52.794', '29-Apr-2003 04:49:52.916'], $ ['29-Apr-2003 04:49:52.916', '29-Apr-2003 04:50:55.916'], ['29-Apr-2003 04:50:55.916', $ '29-Apr-2003 04:51:57.916'], ['29-Apr-2003 04:53:19.727', '29-Apr-2003 04:54:19.916'], $ ['29-Apr-2003 04:54:19.916', '29-Apr-2003 04:55:19.916'], ['29-Apr-2003 04:55:19.916', $ '29-Apr-2003 04:56:19.916'], ['29-Apr-2003 04:57:46.701', '29-Apr-2003 04:58:46.916'], $ ['29-Apr-2003 04:58:46.916', '29-Apr-2003 04:59:46.916'], ['29-Apr-2003 04:59:46.916', $ '29-Apr-2003 05:00:46.916'], ['29-Apr-2003 05:02:13.699', '29-Apr-2003 05:03:43.924'], $ ['29-Apr-2003 05:03:43.924', '29-Apr-2003 05:05:13.924'], ['29-Apr-2003 05:06:15.568', $ '29-Apr-2003 05:07:15.800'], ['29-Apr-2003 05:07:15.800', '29-Apr-2003 05:08:15.800'], $ ['29-Apr-2003 05:08:15.800', '29-Apr-2003 05:09:45.800'], ['29-Apr-2003 05:09:45.800', $ '29-Apr-2003 05:11:15.800'], ['29-Apr-2003 05:11:15.800', '29-Apr-2003 05:12:45.800']] obj-> set, use_flux_var= 0L obj-> set, use_phz_stacker= 1L obj-> set, xyoffset= [769.992, -216.084] obj-> set, im_energy_binning= [[6.00000, 12.0000], [12.0000, 25.0000]] obj-> set, time_bin_def= [1.00000, 2.00000, 4.00000, 8.00000, 8.00000, 16.0000, 32.0000, $ 64.0000, 128.000] obj-> set, time_bin_min= 512L obj-> set, det_index_mask= [0B, 0B, 1B, 1B, 1B, 1B, 1B, 1B, 1B] zzz = {HSI_VIS_SRC_STRUCTURE, $ SRCTYPE: 'circle', $ SRCFLUX: 1.00000, $ SRCX: 0.00000, $ SRCY: 0.00000, $ SRCFWHM: 10.0000, $ ECCEN: 0.00000, $ SRCPA: 0.00000, $ LOOP_ANGLE: 0.00000, $ ALBEDO_RATIO: 0.100000, $ SRCHEIGHT: 10.0000, $ ALBEDO_APPLY: 1, $ FITMASK: [1, 1, 1, 1, 1, 1, 1, 1, 1, 1] } obj-> set, vf_srcin= zzz obj-> set, vis_cs_abort_numerical_issues= 1 obj-> set, vis_cs_sparseness= 0.700000 if keyword_set(_extra) then obj->set, _extra=_extra end