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.

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