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: http://www.atnf.csiro.au/computing/software/miriad/doc/hermes.html
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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