中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Solar and Magnetic Control of Minor Ion Peaks in the Dayside Martian Ionosphere

文献类型:期刊论文

作者Huang, J. -P.7; Cui, J.5,6,7; Hao, Y. -Q.1; Guo, J. -P.4; Wu, X. -S.5,6; Niu, D. -D.3; Wei, Y.2
刊名JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS
出版日期2020-08-01
卷号125期号:8页码:15
ISSN号2169-9380
DOI10.1029/2020JA028254
英文摘要The Neutral Gas and Ion Mass Spectrometer of the Mars Atmosphere and Volatile Evolution provides a large data set to explore the ion composition and structure of the Martian ionosphere. Here, the dayside measurements are used to investigate the minor ion density profiles with distinctive peaks above 150 km, revealing a systematic trend of decreasing peak altitude with increasing ion mass. We specifically focus on a subset of species including O+, N-2(+)/CO+, C+, N+, He+, and O++, all of which are mainly produced via direct photoionization of parent neutrals. Our analysis reveals weak or no variation with solar zenith angle (SZA) in both peak density and altitude, which is an expected result because these ion peaks are located within the optically thin regions subject to the same level of solar irradiance independent of SZA. In contrast, the solar cycle variations of peak density and altitude increase considerably with increasing solar activity, as a result of enhanced photoionization frequency and atmospheric expansion at high solar activities. He+ serves as an exception in that its peak density increases toward large SZA and meanwhile shows no systematic variation with solar activity. The thermospheric He distribution on Mars should play an important role in determining these observed variations. Finally, the peak altitudes for all species are elevated by at least several km within the weakly magnetized regions, possibly attributable to the suppression of vertical diffusion by preferentially horizontal magnetic fields in these regions.
WOS关键词ELECTRON-DENSITY PROFILES ; MARS GLOBAL SURVEYOR ; MONOCHROMATIC RADIATION ; TOPSIDE IONOSPHERE ; MAVEN OBSERVATIONS ; ATMOSPHERE ; VARIABILITY ; ABSORPTION ; ANOMALIES ; VIKING
资助项目B-type Strategic Priority Program - Chinese Academy of Sciences[XDB41000000] ; pre-research project on Civil Aerospace Technologies - China's National Space Administration[D020105] ; National Science Foundation of China[41525015] ; National Science Foundation of China[41525016] ; National Science Foundation of China[41774186] ; National Science Foundation of China[41904154]
WOS研究方向Astronomy & Astrophysics
语种英语
出版者AMER GEOPHYSICAL UNION
WOS记录号WOS:000577125000072
资助机构B-type Strategic Priority Program - Chinese Academy of Sciences ; B-type Strategic Priority Program - Chinese Academy of Sciences ; pre-research project on Civil Aerospace Technologies - China's National Space Administration ; pre-research project on Civil Aerospace Technologies - China's National Space Administration ; National Science Foundation of China ; National Science Foundation of China ; B-type Strategic Priority Program - Chinese Academy of Sciences ; B-type Strategic Priority Program - Chinese Academy of Sciences ; pre-research project on Civil Aerospace Technologies - China's National Space Administration ; pre-research project on Civil Aerospace Technologies - China's National Space Administration ; National Science Foundation of China ; National Science Foundation of China ; B-type Strategic Priority Program - Chinese Academy of Sciences ; B-type Strategic Priority Program - Chinese Academy of Sciences ; pre-research project on Civil Aerospace Technologies - China's National Space Administration ; pre-research project on Civil Aerospace Technologies - China's National Space Administration ; National Science Foundation of China ; National Science Foundation of China ; B-type Strategic Priority Program - Chinese Academy of Sciences ; B-type Strategic Priority Program - Chinese Academy of Sciences ; pre-research project on Civil Aerospace Technologies - China's National Space Administration ; pre-research project on Civil Aerospace Technologies - China's National Space Administration ; National Science Foundation of China ; National Science Foundation of China
源URL[http://ir.iggcas.ac.cn/handle/132A11/98312]  
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Cui, J.
作者单位1.Beijing Univ, Sch Earth & Space Sci, Beijing, Peoples R China
2.Chinese Acad Sci, Inst Geol & Geophys, Beijing, Peoples R China
3.Macau Univ Sci & Technol, Space Sci Inst, Macau, Peoples R China
4.Beijing Normal, Dept Astron, Beijing, Peoples R China
5.Chinese Acad Sci, Ctr Excellence Comparat Planetol, Hefei, Peoples R China
6.Chinese Acad Sci, Natl Astron Observ, Beijing, Peoples R China
7.Sun Yat Sen Univ, Sch Atmospher Sci, Planetary Environm & Astrobiol Res Lab PEARL, Zhuhai, Peoples R China
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GB/T 7714
Huang, J. -P.,Cui, J.,Hao, Y. -Q.,et al. Solar and Magnetic Control of Minor Ion Peaks in the Dayside Martian Ionosphere[J]. JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS,2020,125(8):15.
APA Huang, J. -P..,Cui, J..,Hao, Y. -Q..,Guo, J. -P..,Wu, X. -S..,...&Wei, Y..(2020).Solar and Magnetic Control of Minor Ion Peaks in the Dayside Martian Ionosphere.JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS,125(8),15.
MLA Huang, J. -P.,et al."Solar and Magnetic Control of Minor Ion Peaks in the Dayside Martian Ionosphere".JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS 125.8(2020):15.

入库方式: OAI收割

来源:地质与地球物理研究所

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