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

Authors

1.1K

  1. JS
    J. Schou

    Stanford University, United States

    8 publications · 1.1K citations

    8

    h-index

  2. HM
    H. M. Antia

    Tata Institute of Fundamental Research, India

    8 publications · 865 citations

    8

    h-index

  3. RH
    R. Howe

    National Solar Observatory, United States

    7 publications · 778 citations

    7

    h-index

  4. FH
    F. Hill

    National Solar Observatory, United States

    6 publications · 762 citations

    6

    h-index

  5. SB
    Sarbani Basu

    Yale University, United States

    6 publications · 430 citations

    6

    h-index

1–5 of 1.1K

Venues

  1. The Astrophysical Journal

    ApJ · 50 publications · 3.1K citations

    30

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    28 publications · 1.6K citations

    20

    h-index

  3. Journal of Geophysical Research Atmospheres

    JGR · 23 publications · 1K citations

    19

    h-index

  4. Astronomy and Astrophysics

    19 publications · 874 citations

    16

    h-index

  5. Solar Physics

    16 publications · 478 citations

    12

    h-index

1–5