Solar Interior Structure

Solar Interior Structure is a theoretical construct in solar physics that delineates the layered composition and physical conditions within the Sun, distinguished by its specification of the core, radiative zone, and convective zone as regions governing energy generation, transport, and fluid dynamics in stellar interiors.

314

Publications

24.8K

Citations

930

Authors

362

Institutions

Publications per year

2017–2026

52

Variants

Solar Internal Structure

Authors

930

  1. JC
    J. Christensen‐Dalsgaard

    Aarhus University, Denmark

    25 publications · 3.6K citations

    22

    h-index

  2. JS
    J. Schou

    Stanford University, United States

    14 publications · 3.2K citations

    13

    h-index

  3. DO
    D. O. Gough

    University of Cambridge, United Kingdom

    12 publications · 2.6K citations

    12

    h-index

  4. MJ
    M. J. Thompson

    Stanford University, United States

    10 publications · 1.4K citations

    10

    h-index

  5. SB
    Sarbani Basu

    Yale University, United States

    10 publications · 1K citations

    10

    h-index

1–5 of 930

Venues

  1. The Astrophysical Journal

    ApJ · 92 publications · 6.7K citations

    43

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    25 publications · 1.3K citations

    19

    h-index

  3. Science

    20 publications · 3.4K citations

    17

    h-index

  4. Astronomy and Astrophysics

    20 publications · 1.4K citations

    14

    h-index

  5. Solar Physics

    12 publications · 3.2K citations

    12

    h-index

1–5