Coronal Waves
Coronal Waves is a physical phenomenon in solar physics characterized as large-scale propagating disturbances in the Sun’s corona, distinguished from other coronal disturbances by their association with transient energy releases such as coronal mass ejections and their observable signatures in extreme ultraviolet and radio emissions.
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34.3K
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997
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360
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2017–2026
93
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572
B. Roberts, P. M. Edwin, A. O. Benz · The Astrophysical Journal · 1984 · 681 citations
Solar Flares and Coronal Mass Ejections
S. W. Kahler · Annual Review of Astronomy and Astrophysics · 1992 · 482 citations
Natural Sciences, Astronomy, Physics +16
Coronal Waves and Oscillations
V. M. Nakariakov, E. Verwichte · Living Reviews in Solar Physics · 2005 · 451 citations · Full text
Natural Sciences, Astronomy, Physics +17
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Goddard Space Flight Center
Greenbelt, United States
38 h-index
115 publications
9.6K citations

University of Warwick
Coventry, United Kingdom
33 h-index
80 publications
7.2K citations
Catholic University of America
Washington D.C., United States
26 h-index
48 publications
3.3K citations

University of St Andrews
St Andrews, United Kingdom
26 h-index
62 publications
3.3K citations
KU Leuven
Leuven, Belgium
25 h-index
79 publications
3.8K citations
Lockheed Martin (United States)
Bethesda, United States
25 h-index
57 publications
9.5K citations

United States Naval Research Laboratory
Washington, United States
24 h-index
77 publications
6.6K citations
University of Graz
Graz, Austria
24 h-index
51 publications
4.1K citations
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ApJ · 169 publications · 11.6K citations
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95 publications · 5K citations
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77 publications · 4.8K citations
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38 publications · 2.1K citations
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JGR · 24 publications · 1.6K citations
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