Cme Shocks
CME Shock is a transient magnetohydrodynamic shock wave in the solar wind that is driven by a coronal mass ejection and characterized by a sudden increase in plasma density, temperature, and magnetic field strength at the interface between the ejecta and the ambient solar wind.
330
Publications
18.4K
Citations
824
Authors
337
Institutions
Publications per year
2017–2026
79
Variants
Cme Shock
Parents
330
Coronal Mass Ejections: Observations
D. F. Webb, Timothy Howard · Living Reviews in Solar Physics · 2012 · 690 citations · Full text
Natural Sciences, Astronomy, Physics +17
Coronal mass ejections and interplanetary shocks
N. R. Sheeley, R. A. Howard, M. J. Koomen et al. · Journal of Geophysical Research Atmospheres · 1985 · 409 citations
Natural Sciences, Astronomy, Physics +12
1–5 of 330
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337
Goddard Space Flight Center
Greenbelt, United States
39 h-index
202 publications
12.2K citations

United States Naval Research Laboratory
Washington, United States
25 h-index
52 publications
5.2K citations
Catholic University of America
Washington D.C., United States
24 h-index
75 publications
5.2K citations
University of America
Murrieta, United States
21 h-index
70 publications
5.7K citations
George Mason University
Fairfax, United States
18 h-index
27 publications
1.8K citations

Johns Hopkins University Applied Physics Laboratory
North Laurel, United States
18 h-index
39 publications
1.8K citations

University of Helsinki
Helsinki, Finland
18 h-index
51 publications
2.5K citations
National Space Science Center
Beijing, China
18 h-index
61 publications
2.3K citations
1–8 of 337
ApJ · 86 publications · 4.5K citations
37
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JGR · 44 publications · 4.2K citations
29
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32 publications · 1.3K citations
24
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24 publications · 1.6K citations
20
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25 publications · 1.2K citations
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