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ISIS 3 Application Documentation


rosvirtis2isis

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Import PDS formatted Rosetta VIRTIS image into an ISIS cube.

Overview Parameters

Description

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 Berry2016-04-25 Original version
Kristin Berry2016-11-01 Add ability to ingest housekeeping data.
Kaj Williams2017-08-24 Add ability to ingest VIRTIS-H files. References #5130.
Kris Becker and Kaj Williams2017-08-24 Fix issues with the translation of housekeeping data. Fixes #5131.

Parameter Groups

Files

Name Description
FROM Input PDS formatted Rosetta VIRTIS image file
TO Output Isis cube
X

Files: FROM


Description

Use this parameter to select the Rosetta VIRTIS filename.

Type filename
File Mode input
Filter *.qub
Close Window
X

Files: TO


Description

Use this parameter to select the output filename.

Type cube
File Mode output
Filter *.cub
Close Window