Tachocline Dynamics is a theoretical construct in solar physics that characterizes the mechanical and electromagnetic processes governing the thin, shear-dominated transition layer between the Sun's differentially rotating convective envelope and uniformly rotating radiative interior.
170
Publications
8.7K
Citations
185
Authors
147
Institutions
Publications per year
2017–2026
24
Parents
Publications
170
Solar Interior Rotation and its Variation
R. Howe · Living Reviews in Solar Physics · 2009 · 339 citations · Full text
1–5 of 170
Authors
185
- PA
21
h-index
- MD
19
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- MS
12
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- ASA. S. Brun
Commissariat à l'Énergie Atomique et aux Énergies Alternatives, France
9 publications · 1.5K citations
9
h-index
- JT
7
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1–5 of 185
Institutions
147
NSF National Center for Atmospheric Research
Boulder, United States
27 h-index
73 publications
4.9K citations
NSF NCAR High Altitude Observatory
Boulder, United States
27 h-index
78 publications
5K citations
U.S. National Science Foundation
Alexandria, United States
21 h-index
45 publications
3.1K citations
University of Colorado Boulder
Boulder, United States
13 h-index
21 publications
1.1K citations
University of California, Santa Cruz
Santa Cruz, United States
12 h-index
18 publications
541 citations
Centre National de la Recherche Scientifique
Paris, France
12 h-index
21 publications
1.1K citations
Leibniz Institute for Astrophysics Potsdam
Potsdam, Germany
11 h-index
27 publications
588 citations
University of Cambridge
Cambridge, United Kingdom
11 h-index
17 publications
591 citations
1–8 of 147
Venues
- The Astrophysical Journal
ApJ · 67 publications · 4.6K citations
36
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- Astronomy and Astrophysics
23 publications · 822 citations
17
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- Monthly Notices of the Royal Astronomical Society
13 publications · 473 citations
13
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- Astronomische Nachrichten
9 publications · 178 citations
9
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- Solar Physics
6 publications · 137 citations
6
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