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Proceedings Paper

Radiometric performance results of the Juno ultraviolet spectrograph (Juno-UVS)
Author(s): Michael W. Davis; G. Randall Gladstone; Thomas K. Greathouse; David C. Slater; Maarten H. Versteeg; Kristian B. Persson; Gregory S. Winters; Steven C. Persyn; John S. Eterno
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Paper Abstract

We describe the radiometric performance and ground calibration results of the Juno mission's Ultraviolet Spectrograph (Juno-UVS) flight model. Juno-UVS is a modest power (9.0 W) ultraviolet spectrograph based on the Alice instruments now in flight aboard the European Space Agency's Rosetta spacecraft, NASA's New Horizons spacecraft, and the LAMP instrument aboard NASA's Lunar Reconnaissance Orbiter. Its primary job will be to characterize Jupiter's UV auroral emissions and relate them to in situ particle measurements.

Paper Details

Date Published: 14 September 2011
PDF: 13 pages
Proc. SPIE 8146, UV/Optical/IR Space Telescopes and Instruments: Innovative Technologies and Concepts V, 814604 (14 September 2011); doi: 10.1117/12.894274
Show Author Affiliations
Michael W. Davis, Southwest Research Institute (United States)
G. Randall Gladstone, Southwest Research Institute (United States)
Thomas K. Greathouse, Southwest Research Institute (United States)
David C. Slater, Southwest Research Institute (United States)
Maarten H. Versteeg, Southwest Research Institute (United States)
Kristian B. Persson, Southwest Research Institute (United States)
Gregory S. Winters, Southwest Research Institute (United States)
Steven C. Persyn, Southwest Research Institute (United States)
John S. Eterno, Southwest Research Institute (United States)


Published in SPIE Proceedings Vol. 8146:
UV/Optical/IR Space Telescopes and Instruments: Innovative Technologies and Concepts V
Howard A. MacEwen; James B. Breckinridge, Editor(s)

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