Isis 2 Documentation
unfazed - Undo phase correction This program will undo the phase correction part of the photometric normalization that was applied to Clementine UVVIS mosaics so that a new phase correction can be applied with "photomet". This program is most appropriately applied to the special "A" verion of the Clementine UVVIS data. These data are available online via ftp from pdsimage.wr.usgs.gov, and can be found on /cdroms/CL_4XXXA for the appropriate quad and location on the Moon. The "A" data have had the full photometric correction applied (with photom/photompr/moonpr), but have not had the later empirical "fixes" applied to correct for the month1/month2 brightness differences (MONTH1_2, NOTE: Old name was CLEMFIX) and the bug in the application of the photometric correction (PHOTBUG, NOTE: Old name wasCLEMFIX2). "unfazed" is applied to these data to avoid the need for undoing these corrections. The "A" data have the required phase-angle backplane information for these calculations. "unfazed" works on each band of an input cube to remove the phase function portion of the photometric correction and leave the lambertian correction untouched. Bands 1, 2, and (3,4,5) in the UVVIS data each had different coefficients applied to perform the phase function correction, so they must be processed separately. Information on the photometric correction applied to the Clementine UVVIS data can be found in the "volinfo" document on each cdrom and on the pdsimage.wr.usgs.gov site. The result of running "unfazed" on "A" data should be directly comparable to running "photom/photompr/moonpr" (with the "noalbedo" option) to perform the lambertian correction only. The user can apply a new, user-defined phase function correction using "photomet". Programmer: Tracie L Sucharski, U.S.G.S., Flagstaff, AZ
Parm | Description | Default |
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FROM | Input cube file name (Default extension is .cub) | NONE |
SFROM | Input subcube specifier | -- |
TO | Output cube file name (Default extension is .cub) |
ADDITIONAL NOTES:
Parm | Description |
---|---|
FROM | Input cube file name. If the file extension is omitted, then ".cub" will be assumed. |
SFROM | SFROM specifies the subcube using a single string for all three dimensions of the cube. The order of the three dimensions is always "samples:lines:bands". If a dimension is left blank, all the data for that dimension is selected. The default value of NULL for SFROM selects the entire cube. Any application below can be used for any dimension. To select specific data from any dimension: "10-100(3):11,12,15-20:1-10(2)" = This example will select every third sample starting with sample 10 thru 100. It selects lines 11 and 12, and 15-20. It selects every other band, starting with band 1 thru 10. There are special characters that can be used for selecting a subcube efficiently, such as "*","#", and "~". For examples type "help sfrom" in TAE. **NOTE** For more examples and explanation of the many features of the SFROM parameter, tutor the sfrom.pdf or refer to Introduction To ISIS, Section 6, of the ISIS User's Manual ** |
TO | Output cube file name. If the file extension is omitted, then ".cub" will be assumed. |
Contact us online at the Isis Support Center: http://isisdist.wr.usgs.gov