As shown by the following script, this is very simple. Here we make visibilities for the 2002/Feb/20 flare:
det_index_mask = [1,1,1, 1,1,1, 1,1,1] xyoffset = [905.64,260.42] time_range = ' 20-Feb-2002 '+['11:06:00','11:06:36'] energy_band = [25.,50.] hsi_vis = hsi_vis_usershell(det_index_mask=det_index_mask,xyoffset=xyoffset, $ time_range=time_range,energy_band=energy_band)
This will create a named visibility structure with the following tags:
** Structure HSI_VIS, 11 tags, length=64, data length=64: ISC INT 0 HARM INT 1 ERANGE FLOAT Array[2] TRANGE DOUBLE Array[2] U FLOAT 0.219972 V FLOAT 0.0214038 OBSVIS COMPLEX ( 6.41359, -10.3197) TOTFLUX FLOAT 35.3267 SIGAMP FLOAT 6.44080 CHI2 FLOAT 1.48733 XYOFFSET FLOAT Array[2]
grids=[2,7] ; subcollimators 3,4,5,6,7,8 pixel_size=2 ; 2 x 2 arcsec flux=-1. ; establishes the variable name mem_map,hsi_vis,vis_out, hsi_vis.u, hsi_vis.v,image,grids,pixel_size,flux,/showThe command produces an image structure with the following tags:
** Structure <9ac442c>, 16 tags, length=69012, data length=69012, refs=1: MAP FLOAT Array[128, 128] X FLOAT Array[128] Y FLOAT Array[128] XTIT STRING '[arcsec]' YTIT STRING '[arcsec]' FLUX FLOAT 96.1096 FERR FLOAT 2.88329 IMSIZ LONG 128 MISC STRING Array[5] SVIS FLOAT Array[150] TOL FLOAT 0.0300000 XYINT FLOAT 3.40972 ENTROPY FLOAT 91.1800 CHI2 FLOAT 78.0868 LAMBDA DOUBLE 1.1676755 VISOBSK STRUCT ->Array[1]
In the present version (Aug. 2006), mem_map will pop up a graphical widget showing the u,v coverage, and a response widget prompting you to respond whether you like the coverage. Just click "yes". A surface plot of the iterated MEM map appears with measures of the normalized gradients and chisquared values.
Q: How do you specify tolerance (TOL)? A: Q: How do you change the input flux? A: Q: What are the quantities alpha and beta in the vis_out.misc string? A: Q: What is vis_out.lambda? A: