Solar Surface Flows
Solar Surface Flows is a physical phenomenon within solar physics that denotes the large-scale horizontal motions of plasma across the Sun's photosphere, distinguished by their role in advecting magnetic fields and contributing to the evolution of surface magnetic topology.
400
Publications
21.1K
Citations
779
Authors
354
Institutions
Publications per year
2017–2026
80
Parents
400
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
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779
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354
Max Planck Institute for Solar System Research
Göttingen, Germany
26 h-index
91 publications
4.5K citations
Stanford University
Stanford, United States
23 h-index
49 publications
3.8K citations
NSF NCAR High Altitude Observatory
Boulder, United States
20 h-index
29 publications
1.8K citations
Goddard Space Flight Center
Greenbelt, United States
19 h-index
34 publications
2.7K citations
National Solar Observatory
Boulder, United States
18 h-index
52 publications
3.6K citations
Instituto de Astrofísica de Canarias
Tenerife, Spain
17 h-index
31 publications
1.6K citations

Centre National de la Recherche Scientifique
Paris, France
17 h-index
47 publications
2.1K citations

Czech Academy of Sciences, Astronomical Institute
Ondřejov, Czechia
15 h-index
27 publications
797 citations
1–8 of 354
ApJ · 102 publications · 7.5K citations
43
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61 publications · 2.3K citations
28
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33 publications · 1.4K citations
21
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12 publications · 466 citations
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JGR · 12 publications · 889 citations
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