Coronal Brightness Distribution

Coronal Brightness Distribution is a scientific construct that characterizes the spatial variation of radiant intensity in the solar corona, distinguished by its quantification of brightness as a function of angular distance from the Sun's center, typically derived from white-light coronagraph observations.

305

Publications

15.8K

Citations

756

Authors

238

Institutions

Publications per year

2017–2026

35

Authors

756

  1. RA
    R. A. Howard

    United States Naval Research Laboratory, United States

    11 publications · 3.9K citations

    11

    h-index

  2. LG
    L. Golub

    Center for Astrophysics Harvard & Smithsonian, United States

    10 publications · 633 citations

    10

    h-index

  3. SR
    S. R. Habbal

    Center for Astrophysics Harvard & Smithsonian, United States

    9 publications · 408 citations

    9

    h-index

  4. RM
    R. M. MacQueen

    NSF NCAR High Altitude Observatory, United States

    9 publications · 337 citations

    9

    h-index

  5. PL
    P. Lamy

    Laboratoire d’Astrophysique de Marseille, France

    8 publications · 725 citations

    8

    h-index

1–5 of 756

Venues

  1. The Astrophysical Journal

    ApJ · 82 publications · 4K citations

    37

    h-index

  2. Solar Physics

    98 publications · 7K citations

    35

    h-index

  3. Journal of Geophysical Research Atmospheres

    JGR · 20 publications · 1.5K citations

    16

    h-index

  4. Astronomy and Astrophysics

    14 publications · 565 citations

    13

    h-index

  5. 8

    h-index

1–5