Coronal Waves

Coronal Waves is a physical phenomenon in solar physics characterized as large-scale propagating disturbances in the Sun’s corona, distinguished from other coronal disturbances by their association with transient energy releases such as coronal mass ejections and their observable signatures in extreme ultraviolet and radio emissions.

572

Publications

34.3K

Citations

997

Authors

360

Institutions

Publications per year

2017–2026

93

Authors

997

  1. VM
    V. M. Nakariakov

    University of Warwick, United Kingdom

    28 publications · 2.5K citations

    25

    h-index

  2. LO
    L. Ofman

    Goddard Space Flight Center, United States

    22 publications · 1.8K citations

    20

    h-index

  3. ID
    I. De Moortel

    University of St Andrews, United Kingdom

    19 publications · 959 citations

    18

    h-index

  4. BV
    B. Vršnak

    Croatian Geological Survey, Croatia

    16 publications · 1.4K citations

    16

    h-index

  5. AV
    Astrid Veronig

    University of Graz, Austria

    16 publications · 1.1K citations

    15

    h-index

1–5 of 997

Venues

  1. The Astrophysical Journal

    ApJ · 169 publications · 11.6K citations

    57

    h-index

  2. Astronomy and Astrophysics

    95 publications · 5K citations

    41

    h-index

  3. Solar Physics

    77 publications · 4.8K citations

    35

    h-index

  4. The Astrophysical Journal Letters

    38 publications · 2.1K citations

    24

    h-index

  5. Journal of Geophysical Research Atmospheres

    JGR · 24 publications · 1.6K citations

    20

    h-index

1–5