Coronal Activity
Coronal Activity is a stellar phenomenon characterized by the emission of high-energy radiation and plasma ejections from the outer atmosphere of a star, distinguished by its origin in the magnetically driven processes within the stellar corona.
603
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36K
Citations
1.4K
Authors
466
Institutions
Publications per year
2017–2026
60
Parents
603
Interplanetary magnetic clouds At 1 AU
L. W. Klein, L. F. Burlaga · Journal of Geophysical Research Atmospheres · 1982 · 934 citations
The association of coronal mass ejection transients with other forms of solar activity
R. H. Munro, J. T. Gosling, E. Hildner et al. · Solar Physics · 1979 · 487 citations
Natural Sciences, Astronomy, Physics +15
Coronal Mass Ejections and Forbush Decreases
H. V. Cane · Space Science Reviews · 2000 · 469 citations
Natural Sciences, Astronomy, Physics +10
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466
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
34 h-index
120 publications
6.3K citations

United States Naval Research Laboratory
Washington, United States
30 h-index
99 publications
5.7K citations
Goddard Space Flight Center
Greenbelt, United States
30 h-index
77 publications
6.5K citations
NSF NCAR High Altitude Observatory
Boulder, United States
27 h-index
78 publications
7.1K citations

Centre National de la Recherche Scientifique
Paris, France
24 h-index
68 publications
3.7K citations
Lockheed Martin (United States)
Bethesda, United States
22 h-index
53 publications
4.3K citations

NSF National Center for Atmospheric Research
Boulder, United States
21 h-index
49 publications
6.1K citations
Laboratoire d’études spatiales et d’instrumentation en astrophysique
Meudon, France
19 h-index
38 publications
2.5K citations
1–8 of 466
ApJ · 173 publications · 11.9K citations
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83 publications · 4.6K citations
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99 publications · 5K citations
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JGR · 27 publications · 3.9K citations
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24 publications · 1.1K citations
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