Interplanetary Coronal Mass Ejections
Interplanetary Coronal Mass Ejections is a large-scale transient phenomenon in the heliosphere characterized by the propagation of magnetized plasma clouds originating from the Sun, distinguishable from other solar wind disturbances by its enhanced magnetic field strength, low proton temperature, and coherent magnetic flux rope structure.
932
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2K
Authors
605
Institutions
Publications per year
2017–2026
265
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932
Interplanetary magnetic clouds At 1 AU
L. W. Klein, L. F. Burlaga · Journal of Geophysical Research Atmospheres · 1982 · 934 citations
J. T. Gosling · Journal of Geophysical Research Atmospheres · 1993 · 924 citations
Natural Sciences, Astronomy, Physics +17
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Goddard Space Flight Center
Greenbelt, United States
67 h-index
506 publications
41.1K citations
University of California, Berkeley
Berkeley, United States
47 h-index
212 publications
17.5K citations

United States Naval Research Laboratory
Washington, United States
42 h-index
118 publications
10.2K citations

University of New Hampshire
Durham, United States
37 h-index
175 publications
10.2K citations
Los Alamos National Laboratory
Los Alamos, United States
35 h-index
91 publications
7.8K citations
Catholic University of America
Washington D.C., United States
34 h-index
110 publications
8.5K citations
University of America
Murrieta, United States
34 h-index
115 publications
9.8K citations
University of Maryland, College Park
College Park, United States
33 h-index
59 publications
6K citations
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JGR · 183 publications · 19K citations
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ApJ · 169 publications · 8.8K citations
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74 publications · 5.1K citations
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81 publications · 5.3K citations
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81 publications · 3.5K citations
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