Solar Velocity Fields
Solar Velocity Fields is a physical construct in solar spectroscopy that represents the spatially resolved line-of-sight and horizontal motions of plasma on the Sun's surface, derived from Doppler shifts in spectral lines, to characterize dynamic atmospheric processes such as convection, oscillations, and flows.
126
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6.5K
Citations
256
Authors
124
Institutions
Publications per year
2017–2026
5
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126
Large-scale solar velocity fields
T. L. Duvall · Solar Physics · 1979 · 182 citations
Natural Sciences, Astronomy, Physics +10
Velocity fields in the solar atmosphere
Robert Howard · Solar Physics · 1967 · 151 citations
Natural Sciences, Astronomy, Physics +14
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Fraunhofer Institute for Physical Measurement Techniques, Germany
4 publications · 148 citations
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4
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1–5 of 256
124

Centre National de la Recherche Scientifique
Paris, France
8 h-index
31 publications
1.3K citations

Kitt Peak National Observatory
Tucson, United States
8 h-index
9 publications
284 citations
Max Planck Institute for Solar System Research
Göttingen, Germany
8 h-index
12 publications
566 citations
Carnegie Observatories
Pasadena, United States
6 h-index
6 publications
382 citations

Observatoire de Paris
Paris, France
6 h-index
12 publications
553 citations
Institut für Sonnenphysik
Freiburg im Breisgau, Germany
6 h-index
14 publications
360 citations

Czech Academy of Sciences, Astronomical Institute
Ondřejov, Czechia
6 h-index
8 publications
196 citations
Université de Versailles Saint-Quentin-en-Yvelines
Versailles, France
5 h-index
10 publications
513 citations
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ApJ · 33 publications · 2.7K citations
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28 publications · 1.5K citations
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19 publications · 774 citations
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5 publications · 84 citations
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3 publications · 169 citations
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