Solar Spicules

Solar Spicules is a dynamic chromospheric phenomenon characterized by narrow, jet-like protrusions of plasma extending from the solar limb, distinguished by their rapid vertical motion and short-lived nature within the Sun's lower atmosphere.

168

Publications

9.2K

Citations

290

Authors

154

Institutions

Publications per year

2017–2026

26

Authors

290

  1. BD
    Bart De Pontieu

    Lockheed Martin (United States), United States

    14 publications · 1.7K citations

    14

    h-index

  2. RE
    R. Erdélyi

    University of Sheffield, United Kingdom

    13 publications · 1.2K citations

    13

    h-index

  3. LR
    L. Rouppe van der Voort

    University of Oslo, Norway

    10 publications · 751 citations

    10

    h-index

  4. AC
    Alphonse C. Sterling

    Marshall Space Flight Center, United States

    7 publications · 291 citations

    7

    h-index

  5. RG
    R. G. Athay

    NSF NCAR High Altitude Observatory, United States

    7 publications · 286 citations

    7

    h-index

1–5 of 290

Venues

  1. The Astrophysical Journal

    ApJ · 73 publications · 3.6K citations

    34

    h-index

  2. Astronomy and Astrophysics

    24 publications · 907 citations

    18

    h-index

  3. The Astrophysical Journal Letters

    16 publications · 1K citations

    15

    h-index

  4. Solar Physics

    12 publications · 394 citations

    11

    h-index

  5. 5

    h-index

1–5