Flare Cooling
Flare Cooling is a physical process in solar physics describing the phase subsequent to a solar flare during which the highly energized plasma in the coronal loop loses thermal energy through radiation, conduction, and adiabatic expansion, distinguishing it from the impulsive and peak emission stages of flare evolution.
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2.6K
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299
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113
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2017–2026
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Kink instability of solar coronal loops as the cause of solar flares
A. W. Hood, E. R. Priest · Solar Physics · 1979 · 363 citations
Natural Sciences, Astronomy, Physics +15
Simultaneous X-Ray and T[CLC]e[/CLC]V Observations of a Rapid Flare from Markarian 421
L. Maraschi, G. Fossati, F. Tavecchio et al. · The Astrophysical Journal · 1999 · 125 citations · Full text
Natural Sciences, Astronomy, Physics +12
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United States Naval Research Laboratory
Washington, United States
6 h-index
7 publications
154 citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
5 h-index
9 publications
688 citations
Stanford University
Stanford, United States
5 h-index
8 publications
376 citations
Institute of Space and Astronautical Science
Tokyo, Japan
4 h-index
9 publications
486 citations

Rice University
Houston, United States
4 h-index
4 publications
148 citations
National Astronomical Observatory of Japan
Mitaka-shi, Japan
4 h-index
7 publications
223 citations

University of Glasgow
Glasgow, United Kingdom
3 h-index
7 publications
196 citations
Goddard Space Flight Center
Greenbelt, United States
3 h-index
6 publications
243 citations
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ApJ · 26 publications · 1.1K citations
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10 publications · 839 citations
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3 publications · 76 citations
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2 publications · 69 citations
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2 publications · 101 citations
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