In-Flight Calibration and Performance of the OSIRIS-REx Visible and IR Spectrometer (OVIRS)
Name:
remotesensing-10-01486.pdf
Size:
1.258Mb
Format:
PDF
Description:
Final Published Version
Author
Simon, AmyReuter, Dennis
Gorius, Nicolas
Lunsford, Allen
Cosentino, Richard
Wind, Galina
Lauretta, Dante
Affiliation
Univ Arizona, Lunar & Planetary LabIssue Date
2018-09-18
Metadata
Show full item recordPublisher
MDPICitation
Simon, A. A., Reuter, D. C., Gorius, N., Lunsford, A., Cosentino, R. G., Wind, G., & Lauretta, D. S. (2018). In-flight calibration and performance of the OSIRIS-REx Visible and IR Spectrometer (OVIRS). Remote Sensing, 10(9), 1486.Journal
REMOTE SENSINGRights
Copyright © 2018 by the authors. Licensee MDPI, Basel, Switzerland. This article is an open access article distributed under the terms and conditions of the Creative Commons Attribution (CC BY) license (http://creativecommons.org/licenses/by/4.0/).Collection Information
This item from the UA Faculty Publications collection is made available by the University of Arizona with support from the University of Arizona Libraries. If you have questions, please contact us at repository@u.library.arizona.edu.Abstract
Performance of the Origins, Spectral Interpretation, Resource Identification, Security-Regolith Explorer (OSIRIS-REx) Visible and InfraRed Spectrometer (OVIRS) instrument was validated, showing that it met all science requirements during extensive thermal vacuum ground testing. Preliminary instrument radiometric calibration coefficients and wavelength mapping were also determined before instrument delivery and launch using NIST-traceable sources. One year after launch, Earth flyby data were used to refine the wavelength map by comparing OVIRS spectra with atmospheric models. Near-simultaneous data from other Earth-orbiting satellites were used to cross-calibrate the OVIRS absolute radiometric response, particularly at visible wavelengths. Trending data from internal calibration sources and the Sun show that instrument radiometric performance has been stable to better than 1% in the 18 months since launch.Note
Open access journalISSN
2072-4292EISSN
2072-4292Version
Final published versionSponsors
NASA OSIRIS-REx Projectae974a485f413a2113503eed53cd6c53
10.3390/rs10091486
Scopus Count
Collections
Except where otherwise noted, this item's license is described as Copyright © 2018 by the authors. Licensee MDPI, Basel, Switzerland. This article is an open access article distributed under the terms and conditions of the Creative Commons Attribution (CC BY) license (http://creativecommons.org/licenses/by/4.0/).

