中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Solar Illumination Control of the Polar Wind

文献类型:期刊论文

作者Maes, L.1,2; Maggiolo, R.1; De Keyser, J.1,3; Andre, M.4; Eriksson, A. I.4; Haaland, S.2,5; Li, K.6,7; Poedts, S.3
刊名JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS
出版日期2017-11-01
卷号122期号:11页码:11468-11480
ISSN号2169-9380
DOI10.1002/2017JA024615
文献子类Article
英文摘要Polar wind outflow is an important process through which the ionosphere supplies plasma to the magnetosphere. The main source of energy driving the polar wind is solar illumination of the ionosphere. As a result, many studies have found a relation between polar wind flux densities and solar EUV intensity, but less is known about their relation to the solar zenith angle at the ionospheric origin, certainly at higher altitudes. The low energy of the outflowing particles and spacecraft charging means it is very difficult to measure the polar wind at high altitudes. We take advantage of an alternative method that allows estimations of the polar wind flux densities far in the lobes. We analyze measurements made by the Cluster spacecraft at altitudes from 4 up to 20 RE. We observe a strong dependence on the solar zenith angle in the ion flux density and see that both the ion velocity and density exhibit a solar zenith angle dependence as well. We also find a seasonal variation of the flux density.
WOS关键词MASS-SPECTROMETER OBSERVATIONS ; ELECTRIC-FIELD ; IONOSPHERIC OUTFLOWS ; ION OUTFLOW ; CLUSTER ; PLASMA ; MAGNETOSPHERE ; TAIL ; MAGNETOTAIL ; INSTRUMENT
WOS研究方向Astronomy & Astrophysics
语种英语
出版者AMER GEOPHYSICAL UNION
WOS记录号WOS:000419938600035
资助机构Interuniversity Attraction Pole Planet TOPERS ; Interuniversity Attraction Pole Planet TOPERS ; Solar-Terrestrial Centre of Excellence ; Solar-Terrestrial Centre of Excellence ; Belgian Science Policy Office ; Belgian Science Policy Office ; ESA through PRODEX(PEA C4000109739 ; ESA through PRODEX(PEA C4000109739 ; Research Council of Norway/CoE(223252/F50) ; Research Council of Norway/CoE(223252/F50) ; Deutsches Zentrum fur Luft-und Raumfahrt(50OC1401) ; Deutsches Zentrum fur Luft-und Raumfahrt(50OC1401) ; SNSB (Swedish National Space Board)(72/12 ; SNSB (Swedish National Space Board)(72/12 ; PEAC4000119635) ; PEAC4000119635) ; 170/12) ; 170/12) ; Interuniversity Attraction Pole Planet TOPERS ; Interuniversity Attraction Pole Planet TOPERS ; Solar-Terrestrial Centre of Excellence ; Solar-Terrestrial Centre of Excellence ; Belgian Science Policy Office ; Belgian Science Policy Office ; ESA through PRODEX(PEA C4000109739 ; ESA through PRODEX(PEA C4000109739 ; Research Council of Norway/CoE(223252/F50) ; Research Council of Norway/CoE(223252/F50) ; Deutsches Zentrum fur Luft-und Raumfahrt(50OC1401) ; Deutsches Zentrum fur Luft-und Raumfahrt(50OC1401) ; SNSB (Swedish National Space Board)(72/12 ; SNSB (Swedish National Space Board)(72/12 ; PEAC4000119635) ; PEAC4000119635) ; 170/12) ; 170/12) ; Interuniversity Attraction Pole Planet TOPERS ; Interuniversity Attraction Pole Planet TOPERS ; Solar-Terrestrial Centre of Excellence ; Solar-Terrestrial Centre of Excellence ; Belgian Science Policy Office ; Belgian Science Policy Office ; ESA through PRODEX(PEA C4000109739 ; ESA through PRODEX(PEA C4000109739 ; Research Council of Norway/CoE(223252/F50) ; Research Council of Norway/CoE(223252/F50) ; Deutsches Zentrum fur Luft-und Raumfahrt(50OC1401) ; Deutsches Zentrum fur Luft-und Raumfahrt(50OC1401) ; SNSB (Swedish National Space Board)(72/12 ; SNSB (Swedish National Space Board)(72/12 ; PEAC4000119635) ; PEAC4000119635) ; 170/12) ; 170/12) ; Interuniversity Attraction Pole Planet TOPERS ; Interuniversity Attraction Pole Planet TOPERS ; Solar-Terrestrial Centre of Excellence ; Solar-Terrestrial Centre of Excellence ; Belgian Science Policy Office ; Belgian Science Policy Office ; ESA through PRODEX(PEA C4000109739 ; ESA through PRODEX(PEA C4000109739 ; Research Council of Norway/CoE(223252/F50) ; Research Council of Norway/CoE(223252/F50) ; Deutsches Zentrum fur Luft-und Raumfahrt(50OC1401) ; Deutsches Zentrum fur Luft-und Raumfahrt(50OC1401) ; SNSB (Swedish National Space Board)(72/12 ; SNSB (Swedish National Space Board)(72/12 ; PEAC4000119635) ; PEAC4000119635) ; 170/12) ; 170/12)
源URL[http://ir.iggcas.ac.cn/handle/132A11/82544]  
专题中国科学院地质与地球物理研究所
通讯作者Maes, L.
作者单位1.Royal Belgian Inst Space Aeron, Brussels, Belgium
2.Max Planck Inst Solar Syst Res, Gottingen, Germany
3.Katholieke Univ Leuven, Ctr Math Astrophys, Leuven, Belgium
4.Swedish Inst Space Phys, Uppsala, Sweden
5.Univ Bergen, Dept Phys & Technol, Bergen, Norway
6.Chinese Acad Sci, Inst Geol & Geophys, Key Lab Earth & Planetary Phys, Beijing, Peoples R China
7.Chinese Acad Sci, State Key Lab Space Weather, Beijing, Peoples R China
推荐引用方式
GB/T 7714
Maes, L.,Maggiolo, R.,De Keyser, J.,et al. Solar Illumination Control of the Polar Wind[J]. JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS,2017,122(11):11468-11480.
APA Maes, L..,Maggiolo, R..,De Keyser, J..,Andre, M..,Eriksson, A. I..,...&Poedts, S..(2017).Solar Illumination Control of the Polar Wind.JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS,122(11),11468-11480.
MLA Maes, L.,et al."Solar Illumination Control of the Polar Wind".JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS 122.11(2017):11468-11480.

入库方式: OAI收割

来源:地质与地球物理研究所

浏览0
下载0
收藏0
其他版本

除非特别说明,本系统中所有内容都受版权保护,并保留所有权利。