Closed ascbot closed 4 years ago
Original Redmine Comment Author Name: Moses Milazzo (Moses Milazzo) Original Date: 2011-06-08T16:31:30Z
The PGG Carto panel recommended looking at ISIS2 applications and selecting a number to quickly rewrite into ISIS3. This is an application that our own team needs, and that other users could use.
Original Redmine Comment Author Name: Moses Milazzo (Moses Milazzo) Original Date: 2011-06-14T21:59:52Z
Kris, Tom Stone should get together to complete some/most of this work.
Original Redmine Comment Author Name: Ella (Contractor) Lee (Ella (Contractor) Lee) Original Date: 2012-12-04T20:55:23Z
The following have been modified from ISIS2 to the work with the current version of photomet, and available in ISIS3 production version:
$ISIS3DATA/base/templates/photometry/ callisto.pvl europa.pvl ganymede.pvl general_photomet.pvl io.pvl marsblu.pvl mars_mdim2.1_blu_hapkenalbat##pvl mars_mdim2.1_blu_hapkentopat##pvl mars_mdim2.1_otherfilters_hapkenalbat##pvl mars_mdim2.1_otherfilters_hapkentopat##pvl mars.pvl marsred.pvl moon_clementine_uvvis_a.pvl moon_clementine_uvvis_b.pvl moon_clementine_uvvis_cde.pvl
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Author Name: Tammy Becker (Tammy Becker)
This is a functionality did exist in Isis2 where the user could select a prepared lookup table based on target body and wavelength. Bodies like the Galilean satellites have look up tables for empircally derived Lunar Lambert curves as a function of phase angle. Mars (MOC) data for Red and Blue channels had look up tables as well.
Refer to: $ISISDATA/photom*.sav for Callisto, Europa, Ganymede, Io, Mars