Mode Damping is a physical phenomenon in helioseismology characterized by the gradual dissipation of oscillatory energy in solar acoustic modes due to thermal conduction, radiative losses, and turbulent viscosity, distinguishing it from other mode properties such as frequency or amplitude by specifically describing the rate at which standing pressure waves decay in the Sun’s interior.
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876
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302
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2017–2026
39
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246
1–5 of 246
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876
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1–5 of 876
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302
University of Birmingham
Birmingham, United Kingdom
15 h-index
43 publications
2.5K citations
Centre National de la Recherche Scientifique
Paris, France
10 h-index
27 publications
1K citations
National Institute for Fusion Science
Toki, Japan
9 h-index
17 publications
1.1K citations
California Institute of Technology
Pasadena, United States
8 h-index
80 publications
3.7K citations
Sheffield Hallam University
Sheffield, United Kingdom
8 h-index
11 publications
580 citations
Université Paris Cité
Paris, France
7 h-index
22 publications
1K citations
Commissariat à l'Énergie Atomique et aux Énergies Alternatives
Paris, France
7 h-index
13 publications
814 citations
University of Sheffield
Sheffield, United Kingdom
6 h-index
13 publications
721 citations
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- The Astrophysical Journal
ApJ · 35 publications · 2.4K citations
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- Astronomy and Astrophysics
22 publications · 1.1K citations
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- Physics of Plasmas
19 publications · 731 citations
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- Monthly Notices of the Royal Astronomical Society
17 publications · 1K citations
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- Physical Review Letters
PRL · 8 publications · 561 citations
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