Prominence Heating
Prominence Heating is a physical process in solar physics that refers to the mechanism by which energy is transferred and dissipated within solar prominences, maintaining their observed thermal structure against radiative and conductive losses.
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1.9K
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46
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41
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2017–2026
2
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Physics of Solar Prominences: I—Spectral Diagnostics and Non-LTE Modelling
N. Labrosse, P. Heinzel, J. C. Vial et al. · Space Science Reviews · 2010 · 431 citations · Full text
Natural Sciences, Astronomy, Physics +16
The Dynamic Formation of Prominence Condensations
The Astrophysical Journal · 1999 · 235 citations · Full text
Natural Sciences, Astronomy, Physics +14
A model for the formation of solar prominences
S. K. Antiochos, J. A. Klimchuk · The Astrophysical Journal · 1991 · 180 citations
Natural Sciences, Astronomy, Physics +15
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Goddard Space Flight Center
Greenbelt, United States
5 h-index
5 publications
897 citations

United States Naval Research Laboratory
Washington, United States
4 h-index
9 publications
1.1K citations
KU Leuven
Leuven, Belgium
3 h-index
5 publications
358 citations
RTX (United States)
Arlington, United States
2 h-index
2 publications
377 citations
Max Planck Society
Munich, Germany
2 h-index
3 publications
44 citations
Lockheed Martin (United States)
Bethesda, United States
2 h-index
2 publications
271 citations
National Sagamihara Hospital
Zama, Japan
2 h-index
2 publications
271 citations

Czech Academy of Sciences, Astronomical Institute
Ondřejov, Czechia
2 h-index
3 publications
916 citations
1–8 of 41
ApJ · 13 publications · 1.1K citations
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2 publications · 114 citations
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2 publications · 73 citations
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1 publications · 431 citations
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Repository · 1 publications · 142 citations
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