DOI: 10.1029/2018JA025311
Scopus记录号: 2-s2.0-85052455675
论文题名: The Largest Electron Differential Energy Flux Observed at Mars by the Mars Express Spacecraft, 2004–2016
作者: Frahm R.A. ; Winningham J.D. ; Coates A.J. ; Gérard J.-C. ; Holmström M. ; Barabash S.
刊名: Journal of Geophysical Research: Space Physics
ISSN: 21699380
出版年: 2018
卷: 123, 期: 8 起始页码: 6576
结束页码: 6590
语种: 英语
英文摘要: The goal of this paper is to understand the processes by which solar wind electrons are energized in the Martian magnetosphere and how this compares to processes at Venus and Earth. Each is unique in the source of its magnetic field topology and how this influences electron energization. To achieve this goal, 24 million spectra spanning 13 years have been examined using the electron spectrometer from the Mars Express spacecraft between about 12,000 km and about 250 km altitude, and from all latitudes and local times. The top 10 largest differential energy flux at energies above the differential energy flux peak have been found: seven spectra from the magnetosheath near noon, three from the dark tail (the largest two from the middle and ionospheric edge of the magnetosheath). Spectral comparisons show a decade range in the peak of the electron distributions; however, all distributions show a similar energy maximum dictated by solar wind/planet interaction. Similarly derived, the largest Venus spectrum occurred near the magnetosheath bow shock and had the same shape as the most intense Mars inner magnetosheath spectrum. The Mars and Venus dayside spectra compared to the Mars nightside spectrum that included an enhanced optical signal attributed to discrete “auroral” precipitation show a similar shape. These spectra are also compared to a selected auroral zone electron spectra from the Earth. The Mars and Venus results suggest that there is no more energy needed to generate electrons forming the nightside precipitation than is gained during the solar wind/planet interaction. ©2018. The Authors. Citation statistics:
资源类型: 期刊论文
标识符: http://119.78.100.158/handle/2HF3EXSE/113452
Appears in Collections: 气候减缓与适应
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作者单位: Southwest Research Institute, San Antonio, TX, United States; Mullard Space Science Laboratory, University College London, Surrey, United Kingdom; Laboratory of Planetary and Atmospheric Physics, Université de Liège, Liège, Belgium; Swedish Institute of Space Physics, Kiruna, Sweden
Recommended Citation:
Frahm R.A.,Winningham J.D.,Coates A.J.,et al. The Largest Electron Differential Energy Flux Observed at Mars by the Mars Express Spacecraft, 2004–2016[J]. Journal of Geophysical Research: Space Physics,2018-01-01,123(8)