Radiometric performance results of the Juno ultraviolet spectrograph (Juno-UVS)

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

doi:10.1117/12.894274

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13 September 2011 Radiometric performance results of the Juno ultraviolet spectrograph (Juno-UVS)

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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Proceedings Volume 8146, UV/Optical/IR Space Telescopes and Instruments: Innovative Technologies and Concepts V; 814604 (2011) https://doi.org/10.1117/12.894274
Event: SPIE Optical Engineering + Applications, 2011, San Diego, California, United States

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.

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Michael W. Davis, G. Randall Gladstone, Thomas K. Greathouse, David C. Slater, Maarten H. Versteeg, Kristian B. Persson, Gregory S. Winters, Steven C. Persyn, and John S. Eterno "Radiometric performance results of the Juno ultraviolet spectrograph (Juno-UVS)", Proc. SPIE 8146, UV/Optical/IR Space Telescopes and Instruments: Innovative Technologies and Concepts V, 814604 (13 September 2011); https://doi.org/10.1117/12.894274

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