Rotation Rate Variability
Rotation Rate Variability is a solar physical metric that quantifies the differential changes in angular velocity of the Sun’s plasma across latitudes, longitudes, and time, distinguishing it from uniform rotational models by capturing spatiotemporal fluctuations in solar rotation.
262
Publications
14.2K
Citations
1.1K
Authors
378
Institutions
Publications per year
2017–2026
45
Parents
262
Differential Rotation and Dynamics of the Solar Interior
M. J. Thompson, Juri Toomre, E. Anderson et al. · Science · 1996 · 404 citations · Full text
1–5 of 262
1.1K
8
h-index
8
h-index
7
h-index
6
h-index
6
h-index
1–5 of 1.1K
378
Jet Propulsion Laboratory
Pasadena, United States
16 h-index
50 publications
22.3K citations
California Institute of Technology
Pasadena, United States
14 h-index
37 publications
3.7K citations
University of Colorado Boulder
Boulder, United States
13 h-index
31 publications
12.7K citations
Planetary Science Institute
Tucson, United States
12 h-index
141 publications
111.4K citations

Centre National de la Recherche Scientifique
Paris, France
12 h-index
44 publications
18K citations
Stanford University
Stanford, United States
11 h-index
16 publications
1.6K citations
Yale University
New Haven, United States
11 h-index
12 publications
626 citations
National Solar Observatory
Boulder, United States
10 h-index
24 publications
2.9K citations
1–8 of 378
ApJ · 50 publications · 3.1K citations
30
h-index
28 publications · 1.6K citations
20
h-index
JGR · 23 publications · 1K citations
19
h-index
19 publications · 874 citations
16
h-index
16 publications · 478 citations
12
h-index
1–5