Reference : In-flight characterization and calibration of the Juno-Ultraviolet Spectrograph (Juno-UVS)
Scientific congresses and symposiums : Poster
Physical, chemical, mathematical & earth Sciences : Space science, astronomy & astrophysics
http://hdl.handle.net/2268/224152
In-flight characterization and calibration of the Juno-Ultraviolet Spectrograph (Juno-UVS)
English
Hue, V. [Southwest Research Institute > > > >]
Kammer, J. D. [Southwest Research Institute > > > >]
Gladstone, G. R. [Southwest Research Institute > > > >]
Davis, M. K. [Southwest Research Institute > > > >]
Bonfond, Bertrand mailto [Université de Liège - ULiège > Département d'astrophys., géophysique et océanographie (AGO) > Labo de physique atmosphérique et planétaire (LPAP) >]
Versteeg, M. H. [Southwest Research Institute > > > >]
Grodent, Denis mailto [Université de Liège - ULiège > Département d'astrophys., géophysique et océanographie (AGO) > Labo de physique atmosphérique et planétaire (LPAP) >]
Gérard, Jean-Claude mailto [Université de Liège - ULiège > Département d'astrophys., géophysique et océanographie (AGO) > Département d'astrophys., géophysique et océanographie (AGO) >]
Bolton, S. J. [Southwest Research Institute > > > >]
Levin, S. M. [NASA, JPL > > > >]
Jun-2018
No
No
International
SPIE Astronomical Tescopes + Instrumentation Congress 2018
10-15 juin 2018
The International Society for Optics and Photonics
Austin, Texas
USA
[en] Juno UVS ; Jupiter
[en] The Juno mission, orbiting Jupiter since July 2016, offers an unprecedented opportunity to study Jupiter, from its internal structure to its magnetospheric environment. Juno-UVS is a ultraviolet (UV) photon counting spectrograph with a bandpass of 68<λ<210 nm. The main purpose of Juno-UVS is to observe and characterize Jupiter’s UV auroral emissions and provide global context for Juno’s in-situ particles and fields instruments. Juno is a spinning spacecraft that nominally spins at 2 rpm, so it spends a significant amount of time observing the sky background, including stars, interplanetary medium and extragalactic sources. We present here how we use this information to: (i) characterize and calibrate Juno-UVS; and (ii) monitor the detector response over the mission.
Space sciences, Technologies and Astrophysics Research - STAR
Researchers ; Professionals
http://hdl.handle.net/2268/224152
https://spie.org/AS/conferencedetails/space-telescopes-and-instrumentation-uv-to-gamma#session-b
Paper 10699-108

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