Solar Supergranulation
Solar Supergranulation is a large-scale convective flow pattern in the solar photosphere characterized by horizontal plasma motions organized into cellular structures approximately 30,000 kilometers in diameter, distinguishing it from smaller-scale granulation and mesogranulation features through its size, lifetime, and role in advecting magnetic fields across the Sun’s surface.
267
Publications
14.9K
Citations
409
Authors
214
Institutions
Publications per year
2017–2026
27
Parents
267
Transport of Magnetic Fields on the Sun.
Robert B. Leighton · The Astrophysical Journal · 1964 · 708 citations
Natural Sciences, Astronomy, Physics +16
Precise proper-motion measurement of solar granulation
L. J. November, George W. Simon · The Astrophysical Journal · 1988 · 461 citations
Natural Sciences, Astronomy, Physics +15
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Instituto de Astrofísica de Canarias
Tenerife, Spain
20 h-index
39 publications
2.4K citations

Centre National de la Recherche Scientifique
Paris, France
18 h-index
72 publications
3.2K citations
Max Planck Institute for Solar System Research
Göttingen, Germany
18 h-index
69 publications
2.8K citations
Instituto de Astrofísica de Andalucía
Granada, Spain
17 h-index
27 publications
1.4K citations
NSF NCAR High Altitude Observatory
Boulder, United States
15 h-index
19 publications
842 citations
University of Colorado Boulder
Boulder, United States
15 h-index
26 publications
1.2K citations
Lockheed Martin (United States)
Bethesda, United States
15 h-index
22 publications
1.3K citations

NSF National Center for Atmospheric Research
Boulder, United States
13 h-index
16 publications
741 citations
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ApJ · 111 publications · 8.9K citations
48
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43 publications · 1.4K citations
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22 publications · 670 citations
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12 publications · 480 citations
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10 publications · 368 citations
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