Coronal Acceleration Regions

Coronal Acceleration Region is a localized zone within the solar corona where intense electromagnetic fields and plasma waves differentially energize charged particles to high velocities, distinguishing it from other coronal structures by its role in the primary acceleration of solar energetic particles.

51

Publications

2.4K

Citations

499

Authors

138

Institutions

Publications per year

2017–2026

6

Authors

499

  1. JV
    Joseph V. Hollweg

    University of New Hampshire, United States

    2 publications · 68 citations

    2

    h-index

  2. KK
    Karl‐Ludwig Klein

    Observatoire de Paris, France

    2 publications · 43 citations

    2

    h-index

  3. GR
    G. R. Gupta

    Indian Institute of Astrophysics, India

    2 publications · 132 citations

    2

    h-index

  4. DB
    Dipankar Banerjee

    Indian Institute of Astrophysics, India

    2 publications · 132 citations

    2

    h-index

  5. HA
    H. Auraß

    Observatoire de Paris, France

    2 publications · 72 citations

    2

    h-index

1–5 of 499

Venues

  1. The Astrophysical Journal

    ApJ · 14 publications · 972 citations

    13

    h-index

  2. Solar Physics

    12 publications · 496 citations

    12

    h-index

  3. Astronomy and Astrophysics

    7 publications · 183 citations

    7

    h-index

  4. Journal of Geophysical Research Atmospheres

    JGR · 2 publications · 199 citations

    2

    h-index

  5. Space Science Reviews

    2 publications · 117 citations

    2

    h-index

1–5