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The Juno Radiation Monitoring (RM) Investigation
Authors:H N Becker  J W Alexander  A Adriani  A Mura  A Cicchetti  R Noschese  J L Jørgensen  T Denver  J Sushkova  A Jørgensen  M Benn  J E P Connerney  S J Bolton  The Selex Galileo Juno SRU Team  J Allison  S Watts  V Adumitroaie  E A Manor-Chapman  I J Daubar  C Lee  S Kang  W J McAlpine  T Di Iorio  C Pasqui  A Barbis  P Lawton  L Spalsbury  S Loftin  J Sun
Institution:1.Jet Propulsion Laboratory,California Institute of Technology,Pasadena,USA;2.IAPS-INAF,Rome,Italy;3.Technical University of Denmark,Kgs Lyngby,Denmark;4.NASA Goddard Space Flight Center,Greenbelt,USA;5.Space Research Corporation,Annapolis,USA;6.Southwest Research Institute,San Antonio,USA;7.Leonardo Finmeccanica S.p.A. (formerly Selex Galileo S.p.A),Florence,Italy;8.The University of Manchester,Manchester,UK;9.ENEA,Rome,Italy;10.ADNET Systems, Inc.,Bethesda,USA
Abstract:The Radiation Monitoring Investigation of the Juno Mission will actively retrieve and analyze the noise signatures from penetrating radiation in the images of Juno’s star cameras and science instruments at Jupiter. The investigation’s objective is to profile Jupiter’s \(>10\mbox{-MeV}\) electron environment in regions of the Jovian magnetosphere which today are still largely unexplored. This paper discusses the primary instruments on Juno which contribute to the investigation’s data suite, the measurements of camera noise from penetrating particles, spectral sensitivities and measurement ranges of the instruments, calibrations performed prior to Juno’s first science orbit, and how the measurements may be used to infer the external relativistic electron environment.
Keywords:
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