Wave-Heating Models is a theoretical framework in solar physics that explains the heating of the solar corona through the dissipation of magnetohydrodynamic waves propagating from the photosphere, distinguishing it from alternative coronal heating mechanisms by attributing thermal energy gain primarily to wave-induced plasma oscillations and turbulence.
72
Publications
4.6K
Citations
160
Authors
105
Institutions
Publications per year
2017–2026
12
Parents
Publications
72
On resonant heating below the cyclotron frequency
Liu Chen, Zhihong Lin, R. B. White · Physics of Plasmas · 2001 · 166 citations
1–5 of 72
Authors
160
- ZE
7
h-index
- WR
6
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- PU
6
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4
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- MC
4
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1–5 of 160
Institutions
105
Heidelberg University
Heidelberg, Germany
8 h-index
20 publications
739 citations
The University of Texas at Arlington
Arlington, United States
8 h-index
9 publications
301 citations
Max Planck Society
Munich, Germany
5 h-index
9 publications
671 citations
University of Colorado Boulder
Boulder, United States
4 h-index
5 publications
183 citations
Goddard Space Flight Center
Greenbelt, United States
4 h-index
5 publications
285 citations
University of Warsaw
Warsaw, Poland
4 h-index
4 publications
150 citations
KU Leuven
Leuven, Belgium
3 h-index
8 publications
280 citations
University of Wisconsin–Madison
Madison, United States
3 h-index
6 publications
156 citations
1–8 of 105
Venues
- The Astrophysical Journal
ApJ · 21 publications · 1K citations
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- Journal of Geophysical Research Atmospheres
JGR · 7 publications · 488 citations
7
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- Astronomy and Astrophysics
5 publications · 192 citations
5
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- Geophysical Research Letters
5 publications · 113 citations
5
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- The Astrophysical Journal Letters
3 publications · 112 citations
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1–5