Cme Deflection
CME Deflection is a physical phenomenon in heliophysics whereby a coronal mass ejection deviates from its initially radial trajectory in the solar corona and inner heliosphere due to interactions with ambient solar wind structures, magnetic fields, or other coronal mass ejections.
29
Publications
1.9K
Citations
82
Authors
56
Institutions
Publications per year
2017–2026
8
Variants
Coronal Mass Ejection Deflection
Parents
29
Deflection of coronal mass ejection in the interplanetary medium
Yuming Wang, Chenglong Shen, S. Wang et al. · Solar Physics · 2004 · 172 citations
Natural Sciences, Astronomy, Physics +14
Quantitative Analysis of CME Deflections in the Corona
Solar Physics · 2011 · 132 citations · Full text
Natural Sciences, Astronomy, Physics +13
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Goddard Space Flight Center
Greenbelt, United States
8 h-index
21 publications
830 citations
Boston University
Boston, United States
7 h-index
14 publications
867 citations
University of Science and Technology of China
Hefei, China
5 h-index
26 publications
1.9K citations
National Space Science Center
Beijing, China
5 h-index
10 publications
612 citations

Chinese Academy of Sciences
Beijing, China
4 h-index
8 publications
540 citations
University of America
Murrieta, United States
3 h-index
12 publications
309 citations

University of New Hampshire
Durham, United States
3 h-index
5 publications
688 citations
Catholic University of America
Washington D.C., United States
3 h-index
12 publications
309 citations
1–8 of 56
ApJ · 13 publications · 930 citations
12
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6 publications · 410 citations
6
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3 publications · 191 citations
3
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2 publications · 76 citations
2
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1 publications · 18 citations
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