PDS_VERSION_ID = PDS3 RECORD_TYPE = STREAM SPACECRAFT_NAME = "PHOBOS_2" OBJECT = TEXT NOTE = "Description of the GEOMETRY directory contents" PUBLICATION_DATE = 1998-08-2 END_OBJECT = TEXT END GEOMETRY directory contents The GEOMETRY directory contains coordinate files for the ISM sessions, and altimetric contours files for Mars and Phobos used by the mapping routines. All these files are in binary format, except where indicated. Their detailed format is described in labels contained in the directory /Label (Mar_coor.lbl and Pho_coor.lbl). The following files are found in this directory: 1. Coordinates and angles for ISM Mars sessions XXX_COOR.DAT, where XXX is the nickname of the session (11 files) Coordinates and angles are computed by "Coord.for" from orbital parameters and instrument characteristics. Longitude and latitude of the four pixel corners are given in sequence. Longitudes are given using the terrestrial convention (-180 to 180 degrees eastward) to allow representation as 16-bits signed integers. Incidence and emergence angles are given relative to the average normal (direction of Mars' center). The coordinates contained in these files are computed for the second order, even, channels, and can be used for all practical purpose; coordinates corresponding to the other detector arrays can be computed using "Coord.for" (uncomment the corresponding lines in the source program). The files are used in particular by Pixtrace.for and IDL_map.pro to plot maps of spectral ratios. 2 Coordinates and angles for the main Phobos image cube Pho_coor.dat Geographic coordinates and angles for Phobos. Used by ISM_pho.pro Pho_scor.dat Screen coordinates and angles for Phobos, exact pixel shapes. Pho_scrn.dat Screen coordinates and angles for Phobos, coordinates are adapted to get adjacent pixels and continous maps. Used by ISM_map.pro. Pixloc.ctr Screen coordinates of pixels centers in the plane perpendicular to the line of sight, regardless of whether they are on the disk or not. Distances are given in kilometers from the center of Phobos. Geographic coordinates are given according to the terrestrial convention (longitude ranges from -180 to 180 degrees eastward). Incidence and emergence angles are computed relative to the local normal, as computed from T. Duxbury's model of Phobos (1991); their values are probably not very accurate near the limb. Phase angle is estimated from its average value, movement of the spacecraft, and position of the entrance mirror, and is not only indicative (see description of the geometry of observation in "DocISM.pdf"). 3. Altimetric contours for Mars Mars%%h.dat where %% ranges from 08 to 23 These files contain altimetric contours hand-digitized from the Mariner 9 altimetric map of Mars. They are used by Pixtrace.for to superimpose Martian contours to the ISM maps. 4. Reference contours for Phobos Gricor.dat This file contains reference contours from T. Duxbury's 1991 model of PHobos. It is used by Photrace.for to superimpose a contour to the ISM maps of Phobos.