Helmet Streamers

Helmet Streamer is a magnetically confined plasma structure in the solar corona that extends outward from active regions and is distinguished by its helmet-like shape and role in shaping the Sun’s outer atmosphere during periods of high solar activity.

84

Publications

5.2K

Citations

243

Authors

130

Institutions

Publications per year

2017–2026

14

Variants

Helmet Streamer

Authors

243

  1. AP
    A. P. Rouillard

    Centre National de la Recherche Scientifique, France

    7 publications · 459 citations

    7

    h-index

  2. BL
    B. Lavraud

    Institut de Recherche en Astrophysique et Planétologie, France

    6 publications · 443 citations

    6

    h-index

  3. JA
    J. A. Davies

    Rutherford Appleton Laboratory, United Kingdom

    6 publications · 597 citations

    6

    h-index

  4. NR
    N. R. Sheeley

    United States Naval Research Laboratory, United States

    6 publications · 869 citations

    6

    h-index

  5. VR
    V. Rušín

    Slovak Academy of Sciences, Slovakia

    4 publications · 133 citations

    4

    h-index

1–5 of 243

Venues

  1. The Astrophysical Journal

    ApJ · 41 publications · 2.5K citations

    29

    h-index

  2. Journal of Geophysical Research Atmospheres

    JGR · 15 publications · 1.3K citations

    14

    h-index

  3. Geophysical Research Letters

    5 publications · 478 citations

    5

    h-index

  4. Solar Physics

    5 publications · 211 citations

    5

    h-index

  5. The Astrophysical Journal Letters

    4 publications · 185 citations

    4

    h-index

1–5