中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Cross-Terminator Variations of the Photoelectron Energy Distribution in the Martian Ionosphere

文献类型:期刊论文

作者Cheng, Y. M.1,2; Wu, X. S.3,4; Cui, J.3,4; Cao, Y. T.3; Ni, B. B.5; Wei, Y.6,7
刊名JOURNAL OF GEOPHYSICAL RESEARCH-PLANETS
出版日期2022-02-01
卷号127期号:2页码:20
关键词Martian ionosphere photoelectrons transport atmospheric absorption MAVEN
ISSN号2169-9097
DOI10.1029/2021JE007136
英文摘要Photoelectrons are produced on the dayside of Mars via solar Extreme Ultraviolet (EUV) and X-ray ionization and are also frequently observed on the nightside as a result of field-aligned transport. Based on the Solar Wind Electron Analyzer (SWEA) measurements made on board the Mars Atmosphere and Volatile EvolutioN (MAVEN) spacecraft, we show that the shape of the photoelectron energy distribution exhibits interesting cross-terminator variations, in that the He II peak becomes less pronounced and the 10 - 50 eV smooth background becomes hardened, both more evident at lower altitudes. These observations could be understood as the outcome of "atmospheric absorption" via photoelectron collisions with ambient neutrals during day-to-night transport. Such a scenario could successfully interpret the diversity of the MAVEN SWEA observations such as the dawn-dusk and north-south asymmetries, the impacts of crustal magnetization, upstream solar wind conditions, and solar EUV and X-ray radiation, all using the 10-50 eV spectral hardness as a diagnostic. In particular, the magnetic control of the cross-terminator spectral reshaping is proposed as the outcome of varying day-to-night magnetic connectivity which naturally implies varying field-aligned atmospheric column for "absorption." Crude estimates suggest that an "absorbing" atmospheric column of approximate to 1.5 x 10(15) cm(-2) is required for a significant photoelectron spectral reshaping beyond the EUV terminator. Therefore the observations reported here may shed light on the extension of the cross-terminator magnetic field lines, as complementary to the day-to-night magnetic connectivity inferred from the occurrence of nightside photoelectrons.
WOS关键词SUPRATHERMAL ELECTRON DEPLETIONS ; SOLAR-CYCLE VARIATION ; MARS GLOBAL SURVEYOR ; NIGHTSIDE IONOSPHERE ; PEAKS ; PRECIPITATION ; PREDICTIONS ; DEPENDENCE ; SPECTRA ; WINDS
资助项目National Natural Science Foundation of China[42030201] ; National Natural Science Foundation of China[41904154] ; Institute of Geology & Geophysics, Chinese Academy of Sciences (CAS)[IGGCAS-201904] ; CAS B-type Strategic Priority Program[XDB41000000] ; pre-research projects on Civil Aerospace Technologies - China's National Space Administration[D020104] ; pre-research projects on Civil Aerospace Technologies - China's National Space Administration[D020105]
WOS研究方向Geochemistry & Geophysics
语种英语
WOS记录号WOS:000765623000017
出版者AMER GEOPHYSICAL UNION
资助机构National Natural Science Foundation of China ; National Natural Science Foundation of China ; Institute of Geology & Geophysics, Chinese Academy of Sciences (CAS) ; Institute of Geology & Geophysics, Chinese Academy of Sciences (CAS) ; CAS B-type Strategic Priority Program ; CAS B-type Strategic Priority Program ; pre-research projects on Civil Aerospace Technologies - China's National Space Administration ; pre-research projects on Civil Aerospace Technologies - China's National Space Administration ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Institute of Geology & Geophysics, Chinese Academy of Sciences (CAS) ; Institute of Geology & Geophysics, Chinese Academy of Sciences (CAS) ; CAS B-type Strategic Priority Program ; CAS B-type Strategic Priority Program ; pre-research projects on Civil Aerospace Technologies - China's National Space Administration ; pre-research projects on Civil Aerospace Technologies - China's National Space Administration ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Institute of Geology & Geophysics, Chinese Academy of Sciences (CAS) ; Institute of Geology & Geophysics, Chinese Academy of Sciences (CAS) ; CAS B-type Strategic Priority Program ; CAS B-type Strategic Priority Program ; pre-research projects on Civil Aerospace Technologies - China's National Space Administration ; pre-research projects on Civil Aerospace Technologies - China's National Space Administration ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Institute of Geology & Geophysics, Chinese Academy of Sciences (CAS) ; Institute of Geology & Geophysics, Chinese Academy of Sciences (CAS) ; CAS B-type Strategic Priority Program ; CAS B-type Strategic Priority Program ; pre-research projects on Civil Aerospace Technologies - China's National Space Administration ; pre-research projects on Civil Aerospace Technologies - China's National Space Administration
源URL[http://ir.iggcas.ac.cn/handle/132A11/105054]  
专题地质与地球物理研究所_中国科学院地球与行星物理重点实验室
通讯作者Wu, X. S.
作者单位1.Chinese Acad Sci, Natl Astron Observ, Key Lab Lunar & Deep Space Explorat, Beijing, Peoples R China
2.Univ Chinese Acad Sci, Sch Astron & Space Sci, Beijing, Peoples R China
3.Sun Yat Sen Univ, Planetary Environm & Astrobiol Res Lab PEARL, Sch Atmospher Sci, Zhuhai, Peoples R China
4.Chinese Acad Sci, Ctr Excellence Comparat Planetol, Hefei, Peoples R China
5.Wuhan Univ, Sch Elect Informat, Dept Space Phys, Wuhan, Peoples R China
6.Chinese Acad Sci, Key Lab Earth & Planetary Phys, Inst Geol & Geophys, Beijing, Peoples R China
7.Univ Chinese Acad Sci, Sch Earth & Planetary Sci, Beijing, Peoples R China
推荐引用方式
GB/T 7714
Cheng, Y. M.,Wu, X. S.,Cui, J.,et al. Cross-Terminator Variations of the Photoelectron Energy Distribution in the Martian Ionosphere[J]. JOURNAL OF GEOPHYSICAL RESEARCH-PLANETS,2022,127(2):20.
APA Cheng, Y. M.,Wu, X. S.,Cui, J.,Cao, Y. T.,Ni, B. B.,&Wei, Y..(2022).Cross-Terminator Variations of the Photoelectron Energy Distribution in the Martian Ionosphere.JOURNAL OF GEOPHYSICAL RESEARCH-PLANETS,127(2),20.
MLA Cheng, Y. M.,et al."Cross-Terminator Variations of the Photoelectron Energy Distribution in the Martian Ionosphere".JOURNAL OF GEOPHYSICAL RESEARCH-PLANETS 127.2(2022):20.

入库方式: OAI收割

来源:地质与地球物理研究所

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