Polar Coronal Structures

Polar Coronal Structures is a large-scale solar atmospheric phenomenon characterized by magnetically confined, bright, ray-like formations extending from the Sun's polar regions into the corona, distinguishable by their persistent, radially organized plasma density enhancements observed primarily during solar minima.

278

Publications

16.1K

Citations

676

Authors

230

Institutions

Publications per year

2017–2026

22

Authors

676

  1. DJ
    D. J. McComas

    Southwest Research Institute, United States

    16 publications · 2.2K citations

    14

    h-index

  2. BE
    B. E. Goldstein

    Jet Propulsion Laboratory, United States

    12 publications · 2.2K citations

    12

    h-index

  3. SR
    S. R. Habbal

    Center for Astrophysics Harvard & Smithsonian, United States

    12 publications · 1.2K citations

    12

    h-index

  4. JT
    J. T. Gosling

    Los Alamos National Laboratory, United States

    10 publications · 2.1K citations

    10

    h-index

  5. NR
    N. R. Sheeley

    United States Naval Research Laboratory, United States

    9 publications · 682 citations

    9

    h-index

1–5 of 676

Venues

  1. The Astrophysical Journal

    ApJ · 84 publications · 5.4K citations

    41

    h-index

  2. Geophysical Research Letters

    28 publications · 3K citations

    25

    h-index

  3. Journal of Geophysical Research Atmospheres

    JGR · 33 publications · 2.4K citations

    23

    h-index

  4. Solar Physics

    30 publications · 1.2K citations

    20

    h-index

  5. Astronomy and Astrophysics

    20 publications · 751 citations

    17

    h-index

1–5