Solar Eigenfunctions
Solar Eigenfunctions is a mathematical construct in helioseismology that represents the spatial patterns of oscillation modes in the Sun, derived as solutions to the linearized equations of stellar pulsation under spherical symmetry and stratified structure.
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2.9K
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133
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86
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2017–2026
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Solar seismology. I - The stability of the solar p-modes
P. Goldreich, Douglas A. Keeley · The Astrophysical Journal · 1977 · 230 citations
Natural Sciences, Astronomy, Physics +15
A dispersion law for solar oscillations
T. L. Duvall · Nature · 1982 · 111 citations
Natural Sciences, Astronomy, Physics +13
The quest for the solar g modes
The Astronomy and Astrophysics Review · 2010 · 109 citations · Full text
Natural Sciences, Astronomy, Physics +12
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86

University of Birmingham
Birmingham, United Kingdom
7 h-index
30 publications
1.1K citations
NSF NCAR High Altitude Observatory
Boulder, United States
6 h-index
6 publications
332 citations

European Space Research and Technology Centre
Noordwijk-Binnen, The Netherlands
5 h-index
6 publications
195 citations
CEA Paris-Saclay
Gif-sur-Yvette, France
5 h-index
6 publications
300 citations

Joint Institute for Laboratory Astrophysics
Boulder, United States
5 h-index
7 publications
196 citations
Commissariat à l'Énergie Atomique et aux Énergies Alternatives
Paris, France
5 h-index
6 publications
300 citations
Institut für Sonnenphysik
Freiburg im Breisgau, Germany
5 h-index
10 publications
244 citations
Stanford University
Stanford, United States
5 h-index
8 publications
463 citations
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ApJ · 24 publications · 1.2K citations
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13 publications · 420 citations
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10 publications · 271 citations
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4 publications · 79 citations
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4 publications · 83 citations
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