Map of Jupiter's Radiation Environment From Juno's In-Situ Observations

IF 4 1区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS Journal of Geophysical Research: Planets Pub Date : 2025-02-28 DOI:10.1029/2024JE008549
M. Herceg, T. Denver, J. Sushkova, J. L. Jørgensen, M. Benn, L. Ghizoni, P. S. Jørgensen, S. Kotsiaros, J. E. P. Connerney, S. J. Bolton
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Abstract

Since its orbit insertion on 4 July 2016, the Juno spacecraft has orbited Jupiter in a highly elliptical, polar orbit. With every orbit, Juno's line of apsides migrates, increasing the angle relative to the Jovian equator. Therefore, the spacecraft traverses across the inner regions of the radiation belt, where energetic particles are trapped. The most energetic particle fluxes (electrons with energy >20 MeV) are continuously monitored by an instrument that is part of the Magnetic Field investigation, the micro Advanced Stellar Compass (μASC), which serves as an attitude reference for the magnetic sensor. In the regions traversed thus far in the mission, the μASC has obtained in-situ measurements of high-energy particle fluxes from those on open field lines to Io's L-shell, densely covering the flux environment. We present a map of the radiation environment within Jupiter's magnetosphere based on in-situ measurements acquired in regions not well sampled by prior missions.

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朱诺号现场观测的木星辐射环境图
自2016年7月4日进入轨道以来,朱诺号航天器一直在一个高度椭圆的极地轨道上绕木星运行。在每一次轨道运行中,朱诺号的倾斜线都会移动,增加相对于木星赤道的角度。因此,宇宙飞船穿越辐射带的内部区域,高能粒子被困在那里。最高能量的粒子通量(能量为20 MeV的电子)由磁场研究的一部分,微型先进恒星指南针(μASC)连续监测,该仪器作为磁传感器的姿态参考。在迄今为止的任务中所穿越的区域,μASC已经获得了从开放场线上到木卫一l壳层的高能粒子通量的原位测量,密集地覆盖了通量环境。我们提出了一幅木星磁层内辐射环境的地图,这是基于在以前的任务中没有很好采样的地区获得的原位测量结果。
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来源期刊
Journal of Geophysical Research: Planets
Journal of Geophysical Research: Planets Earth and Planetary Sciences-Earth and Planetary Sciences (miscellaneous)
CiteScore
8.00
自引率
27.10%
发文量
254
期刊介绍: The Journal of Geophysical Research Planets is dedicated to the publication of new and original research in the broad field of planetary science. Manuscripts concerning planetary geology, geophysics, geochemistry, atmospheres, and dynamics are appropriate for the journal when they increase knowledge about the processes that affect Solar System objects. Manuscripts concerning other planetary systems, exoplanets or Earth are welcome when presented in a comparative planetology perspective. Studies in the field of astrobiology will be considered when they have immediate consequences for the interpretation of planetary data. JGR: Planets does not publish manuscripts that deal with future missions and instrumentation, nor those that are primarily of an engineering interest. Instrument, calibration or data processing papers may be appropriate for the journal, but only when accompanied by scientific analysis and interpretation that increases understanding of the studied object. A manuscript that describes a new method or technique would be acceptable for JGR: Planets if it contained new and relevant scientific results obtained using the method. Review articles are generally not appropriate for JGR: Planets, but they may be considered if they form an integral part of a special issue.
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