Photospheric Structure

Photospheric Structure is a physical construct in solar astrophysics that characterizes the spatially resolved, layered organization of temperature, density, and magnetic fields in the Sun's visible surface layer, distinguishing it from deeper interior or overlying chromospheric structures.

1.3K

Publications

74.1K

Citations

3.7K

Authors

887

Institutions

Publications per year

2017–2026

226

Authors

3.7K

  1. SK
    S. K. Solanki

    Max Planck Institute for Solar System Research, Germany

    24 publications · 813 citations

    19

    h-index

  2. PA
    P. A. Mazzali

    Max Planck Institute for Astrophysics, Germany

    14 publications · 1.2K citations

    14

    h-index

  3. JD
    J.‐F. Donati

    Centre National de la Recherche Scientifique, France

    13 publications · 1.5K citations

    13

    h-index

  4. SB
    S. Benetti

    Osservatorio Astronomico di Padova, Italy

    13 publications · 1.4K citations

    13

    h-index

  5. LR
    L. R. Bellot Rubio

    Instituto de Astrofísica de Andalucía, Spain

    13 publications · 488 citations

    12

    h-index

1–5 of 3.7K

Venues

  1. The Astrophysical Journal

    ApJ · 454 publications · 29.7K citations

    87

    h-index

  2. Astronomy and Astrophysics

    224 publications · 10.3K citations

    56

    h-index

  3. Monthly Notices of the Royal Astronomical Society

    149 publications · 9.2K citations

    51

    h-index

  4. Solar Physics

    96 publications · 5.8K citations

    38

    h-index

  5. The Astrophysical Journal Letters

    38 publications · 2.4K citations

    28

    h-index

1–5