rosvirtis2isis
Import PDS formatted Rosetta VIRTIS image into an ISIS cube.
This 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
- Input PDS file (.qub) (FROM)
- Output ISIS file name (.cub) (TO)
Instrument Overview
VIRTIS-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 Archive
The Rosetta data are available from the NASA PDS Small Bodies Node.
References
Categories
History
| Kristin Berry | 2016-04-25 | Original version |
| Kristin Berry | 2016-11-01 | Add ability to ingest housekeeping data. |
| Kaj Williams | 2017-08-24 | Add ability to ingest VIRTIS-H files. References #5130. |
| Kris Becker and Kaj Williams | 2017-08-24 | Fix issues with the translation of housekeeping data. Fixes #5131. |
| Jesse Mapel | 2018-05-14 | Fixed compiler warnings from new lvl3 ingestion code. |
| Jesse Mapel | 2018-05-14 | Nulled dark current scans in level 2 data. Fixes #5421. |