Damping Processes
Damping Processes is a physical mechanism within the study of pulsating stars that describes the dissipation of pulsational energy through radiative losses, turbulent viscosity, or non-adiabatic effects, thereby reducing the amplitude of stellar oscillations over time.
216
Publications
9.4K
Citations
672
Authors
294
Institutions
Publications per year
2017–2026
35
Parents
216
M.‐A. Dupret, A. Grigahcène, R. Garrido et al. · Astronomy and Astrophysics · 2005 · 293 citations · Full text
Natural Sciences, Astronomy, Physics +17
1–5 of 216
672
Laboratoire d’études spatiales et d’instrumentation en astrophysique, France
4 publications · 148 citations
4
h-index
3
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3
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3
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National Agency for New Technologies, Energy and Sustainable Economic Development, Italy
3 publications · 70 citations
3
h-index
1–5 of 672
294

Centre National de la Recherche Scientifique
Paris, France
11 h-index
41 publications
1.4K citations

Princeton Plasma Physics Laboratory
Princeton, United States
10 h-index
32 publications
1.5K citations
Max Planck Institute for Plasma Physics
Garching, Germany
9 h-index
23 publications
669 citations

Sorbonne Université
Paris, France
7 h-index
20 publications
622 citations
The University of Texas at Austin
Austin, United States
7 h-index
19 publications
1.5K citations
National Institute for Fusion Science
Toki, Japan
6 h-index
124 publications
4K citations

Oak Ridge National Laboratory
Oak Ridge, United States
6 h-index
9 publications
346 citations
General Atomics (United States)
San Diego, United States
6 h-index
12 publications
872 citations
1–8 of 294
17 publications · 634 citations
15
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PRL · 12 publications · 922 citations
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11 publications · 304 citations
11
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ApJ · 9 publications · 394 citations
10
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11 publications · 253 citations
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