ISIS 3 Application Documentation
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Import PDS formatted Rosetta VIRTIS image into an ISIS cube.
Overview | Parameters |
DescriptionThis program will import and convert a PDS-formatted Rosetta VIRTIS-M or VIRTIS-H image into an ISIS cube. This program is designed to work with data available in the draft data area on PDS as of 04/25/2016 and with any officially released data as of 11/01/2016. The output cube will contain a substantial housekeeping data table named "HK." It contains, in order, the HK values for each line of the cube as described on pg 66-67 of the VIRTIS EAICD. Requirements
Instrument OverviewVIRTIS-M is a mapping spectrometer onboard the Rosetta mission comprised of two components: VIRTIS-M-VIS, and VIRTIS-M-IR. VIRTIS-M-VIS is the visible component, and VIRTIS-M-IR is the infrared component. VIRTIS-H is a high resolution infrared spectrometer (1840-4990 nm). Data ArchiveThe Rosetta data are available from the NASA PDS Small Bodies Node. ReferencesCategoriesHistory
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Parameter GroupsFiles
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Use this parameter to select the Rosetta VIRTIS filename.
Type | filename |
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File Mode | input |
Filter | *.qub |
Use this parameter to select the output filename.
Type | cube |
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File Mode | output |
Filter | *.cub |