Sunspot Penumbrae

Sunspot Penumbrae is a structural component of a sunspot comprising the radially elongated, filamentary regions of intermediate brightness that surround the darker central umbra and exhibit inclined magnetic fields, partial brightness suppression, and organized plasma flows distinguishing it from both the umbra and the surrounding photosphere.

353

Publications

14.3K

Citations

440

Authors

195

Institutions

Publications per year

2017–2026

48

Authors

440

  1. RS
    R. Schlichenmaier

    Institut für Sonnenphysik, Germany

    30 publications · 1.3K citations

    23

    h-index

  2. SK
    S. K. Solanki

    Max Planck Institute for Solar System Research, Germany

    26 publications · 853 citations

    19

    h-index

  3. LR
    L. R. Bellot Rubio

    Instituto de Astrofísica de Andalucía, Spain

    18 publications · 863 citations

    17

    h-index

  4. BW
    B. W. Lites

    NSF NCAR High Altitude Observatory, United States

    12 publications · 883 citations

    12

    h-index

  5. AT
    A. Tritschler

    National Solar Observatory, United States

    11 publications · 393 citations

    11

    h-index

1–5 of 440

Venues

  1. Astronomy and Astrophysics

    73 publications · 3.3K citations

    38

    h-index

  2. The Astrophysical Journal

    ApJ · 96 publications · 4.4K citations

    37

    h-index

  3. Solar Physics

    55 publications · 2K citations

    24

    h-index

  4. The Astrophysical Journal Letters

    18 publications · 647 citations

    15

    h-index

  5. Springer Link (Chiba Institute of Technology)

    Repository · 11 publications · 285 citations

    11

    h-index

1–5