Using MEM_Sato

Just as in previous tutorials, start up the gui and enter the time of your favorite flare. In this example, I have used a 20-s interval of the 2002 July 4 flare. I use detectors 3F-8F, 1.5 arcsec pixels, and energy band 12-25 keV.

After setting the imaging algorithm to MEM_Sato,   pull down the "Set parameters" menu.

Note the option called "Smoothness constraint".
This is not really a smoothness parameter, but it
is supposed to weight the entropy term relative to the
chisquare term. The default value is 0.1. We have set the
parameter to 4 values, 0.025, 0.100, 0.400, and 1.0, and
made maps, as shown below.

There are no significant differences in these maps. Further, all 4 maps have similar values of chisquare. (Recall the 3-pixel likelihood hypercube.) This is an undesirable "feature" of MEM_Sato (noted by Andrew Conway in Dec/2001) in which the "entropy constraint" is effectively turned off for lnorm > 0.1. Another "feature" is the well-known super-resolution of MEM images. To see this, open the Plot_control menu, and create a column profile.

As shown here, the FWHM of the selected source is about 4.5". This is less than the 6.9" resolution of subcollimator 3, the finest used in these maps. This means that, if the mapped flux equals the true flux, then, in addition to underestimating the size of sources, the maps also overestimate the source intensity.