Solar Granulation Dynamics
Solar Granulation Dynamics is a physical phenomenon in solar physics characterized by the organized convective motion and temporal evolution of granular-scale plasma structures in the solar photosphere, driven by subsurface convection and marked by distinct upwelling centers and downdraft intergranular lanes.
143
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8.2K
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242
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130
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2017–2026
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Simulations of Solar Granulation. I. General Properties
R. F. Stein, Åke Nordlund · The Astrophysical Journal · 1998 · 746 citations · Full text
Natural Sciences, Astronomy, Physics +15
Precise proper-motion measurement of solar granulation
L. J. November, George W. Simon · The Astrophysical Journal · 1988 · 461 citations
Natural Sciences, Astronomy, Physics +15
Topology of convection beneath the solar surface
R. F. Stein, Åke Nordlund · The Astrophysical Journal · 1989 · 301 citations
On Noise Arising from the Solar Granulation.
M. Schwarzschild · The Astrophysical Journal · 1948 · 241 citations
Natural Sciences, Astronomy, Physics +17
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Instituto de Astrofísica de Canarias
Tenerife, Spain
15 h-index
29 publications
1.4K citations

Centre National de la Recherche Scientifique
Paris, France
11 h-index
41 publications
2.1K citations
Max Planck Institute for Solar System Research
Göttingen, Germany
9 h-index
29 publications
1.4K citations
Institut für Sonnenphysik
Freiburg im Breisgau, Germany
8 h-index
20 publications
824 citations
Main Astronomical Observatory
Kyiv, Ukraine
7 h-index
9 publications
251 citations
Michigan State University
East Lansing, United States
6 h-index
6 publications
1.2K citations
University of Graz
Graz, Austria
6 h-index
12 publications
646 citations
Lockheed Martin (United States)
Bethesda, United States
6 h-index
9 publications
422 citations
1–8 of 130
ApJ · 48 publications · 4.7K citations
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35 publications · 1.3K citations
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12 publications · 414 citations
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6 publications · 84 citations
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6 publications · 293 citations
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