Solar Corona

Solar Corona is the outermost layer of the Sun's atmosphere, distinguished from other atmospheric layers by its extremely high temperature and faint, diffuse plasma emission visible during total solar eclipses.

12K

Publications

685.3K

Citations

14.1K

Authors

2.2K

Institutions

Publications per year

2017–2026

2.1K

Authors

14.1K

  1. RA
    R. A. Howard

    United States Naval Research Laboratory, United States

    169 publications · 25.4K citations

    74

    h-index

  2. AV
    A. Vourlidas

    United States Naval Research Laboratory, United States

    149 publications · 13.4K citations

    66

    h-index

  3. NR
    N. R. Sheeley

    United States Naval Research Laboratory, United States

    99 publications · 10.4K citations

    54

    h-index

  4. DJ
    D. J. McComas

    Southwest Research Institute, United States

    88 publications · 10.5K citations

    51

    h-index

  5. JT
    J. T. Gosling

    Los Alamos National Laboratory, United States

    79 publications · 8.1K citations

    50

    h-index

1–5 of 14.1K

Venues

  1. The Astrophysical Journal

    ApJ · 3.9K publications · 253.7K citations

    198

    h-index

  2. Journal of Geophysical Research Atmospheres

    JGR · 833 publications · 63.9K citations

    124

    h-index

  3. Solar Physics

    1.2K publications · 77.5K citations

    109

    h-index

  4. Astronomy and Astrophysics

    1.1K publications · 49.6K citations

    98

    h-index

  5. Geophysical Research Letters

    292 publications · 19.3K citations

    76

    h-index

1–5