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机译:Jumo / Jedi测量的木星的主要极光区域中沉淀电子能量通量和特征能
The Johns Hopkins University Applied Physics Laboratory Laurel MD USA;
National Institute of Information and Communications Technology Tokyo Japan;
The Johns Hopkins University Applied Physics Laboratory Laurel MD USA;
Department of Physics and Astronomy University of Leicester Leicester UK;
Institut für Geophysik und Meteorologie Universit?t zu K?ln Cologne Germany;
Department of Physics and Astronomy University of Leicester Leicester UK;
Southwest Research Institute San Antonio TX USA;
Southwest Research Institute San Antonio TX USA;
Laboratory for Atmospheric and Space Physics University of Colorado Boulder Boulder CO USA;
Southwest Research Institute San Antonio TX USA;
Space Sciences Technologies and Astrophysics Research Institute LPAP Universite de Liege Liege Belgium;
Goddard Space Flight Center Greenbelt MD USA;
Southwest Research Institute San Antonio TX USA;
Goddard Space Flight Center Greenbelt MD USA;
The Johns Hopkins University Applied Physics Laboratory Laurel MD USA;
Precipitating Electron; Energy Flux; Juno/JEDI;
机译:Jumo / Jedi测量的木星的主要极光区域中沉淀电子能量通量和特征能
机译:Jupiter高能量/高纬度电子环境来自朱诺的Jedi和UVS科学仪器背景噪音
机译:Hisaki / EXCEED观测到的木星极光的变化:1.与使用HST / STIS进行的观测相比,观测到的极光电子能量特征
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机译:Hisaki / EXCEED观测到的木星极光的变化:1.与使用HST / STIS进行的观测相比,观测到的极光电子能量特征