ISIS 3 Application Documentation
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Import PDS formatted Rosetta OSIRIS image into an ISIS cube
Overview | Parameters |
DescriptionThis program will import and convert a PDS-formatted Rosetta OSIRIS image into an ISIS cube. The input file can be in compressed or decompressed form, and can be from OSIRIS's Wide-Angle Camera (WAC) or its Narrow-Angle Camera (NAC.) Input PDS files are converted to 32-bit if they are not already 32-bit. Requirements
Instrument OverviewOSIRIS contains a high-resolution Narrow-Angle Camera (NAC) and a Wide-Angle Camera (WAC) that share a common shutter, filter wheel, and detector. The detector is a custom backside-illuminated 2048 x 2048 CCD with a UV-antireflection coating. OSIRIS-NAC has an off-axis three mirror system that minimizes the stray light hitting the CCD, and a field of view of 2.20 x 2.22 degrees. OSIRIS-WAC has an off-axis two mirror system which is also designed to minimize stray light and has a wider field of view of 11.34 x 12.11 degrees. OSIRIS-NAC has 12 filters that cover wavelengths 250-1000 nm at a resolution of 18.6 microradians/pixel, and OSIRIS-WAC has 14 filters over 240 - 720 nm at a resolution of 101 microradians/pixel. More detailed filter specifications are provided in the tables below. Narrow-Angle FiltersThe following table provides the specifications for each of the 16 OSIRIS-NAC filters.
Wide-Angle FiltersThe following table provides the specifications for each of the 14 OSIRIS-WAC filters. One of the filter wheels is always set to Empty because of hardware constraints. The wavelengths and full-width half maximums (FWHMs) for the Empty filters are set to 0 in the ISIS cube label.
Data ArchiveThe Rosetta data are available from the NASA PDS Small Bodies Node. The file-naming convention for OSIRIS images on the PDS archive is: {C}{YYYYMM DD}T{HHMMSSUUU}{FF}{L}{I}F{A}{B}.img, where: {C} is set to either N or W to indicate a NAC or WAC image, respectively, {YYYYMM DD} is the year, month, and day, of image acquisition; T is a separator that stands for "Time", and {HHMMSSUUU} is the hour, minute, second, and milli-second of acquisition. {FF} indicates the image file type: ID is a normal image, TH is a thumbnail image, and PA, PB, and OL indicate different kinds of calibration data; {L} is the processing level of the image; {I} is the instance id of the image, F is a separator that stands for "Filter", {A} indicates the position of filter wheel #1, and {B} indicates the position of filter wheel #2. ReferencesHviid, Stubbe F. "Osiris Experiment Data Record and Software Interface Specification (EDR/SIS) " Issue 3, 04/04/2011H. U. Keller et al. "OSIRIS - The Scientific Camera System Onboard Rosetta." Space Science Reviews. Volume 128, Issue 1-4, pp 433-506. CategoriesHistory
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Parameter GroupsFiles
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Use this parameter to select the Rosetta Osiris filename.
Type | filename |
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File Mode | input |
Filter | *.imq *.img |
Use this parameter to select the output filename.
Type | cube |
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File Mode | output |
Filter | *.cub |