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Basic Information on hermes
Task: hermes
Purpose: Make model images for Mercury.
Categories: image analysis, planets.
First calculates a Hermographic brightness temperature map,
then uses interpolation and coordinate rotations to find
the corresponding map in geocentric RA and DEC offsets from
the sub-earth point. Next, the Fresnel reflection coef-
ficients are applied to obtain the model map. Finally, a
set of CLEAN components are generated for use in the RAL
software package. This is the non-linear diffusion version.
$MIR/cat/hermes.in is a sample input file, and can be copied
to the user's own directory. A more complete discussion of
program HERMES can be found in file $MIR/cat/hermes.txt.
Key: in
Parameter file. Default is "hermes.in".
Key: imsize
Image size. Default is 64.
Key: log
Output log file. Default is "hermes.log".
Key: out
Output image. Units JY/PIXEL. No default.
Revision: 1.7, 2013/08/30 01:49:21 UTC
Generated by miriad@atnf.csiro.au on 21 Jun 2016