Coronal Density Structure

Coronal Density Structure is a physical model that characterizes the spatial distribution and variation of electron density within the solar corona, distinguished by its emphasis on quantitative descriptions of density gradients, inhomogeneities, and their temporal evolution in relation to coronal magnetic fields and thermal processes.

368

Publications

20.4K

Citations

857

Authors

325

Institutions

Publications per year

2017–2026

50

Authors

857

  1. SR
    S. R. Habbal

    Center for Astrophysics Harvard & Smithsonian, United States

    14 publications · 1.3K citations

    14

    h-index

  2. RR
    Richard R. Fisher

    Goddard Space Flight Center, United States

    10 publications · 608 citations

    10

    h-index

  3. RA
    R. A. Frazin

    University of Michigan, United States

    9 publications · 264 citations

    9

    h-index

  4. RW
    Richard Woo

    Jet Propulsion Laboratory, United States

    9 publications · 262 citations

    9

    h-index

  5. JC
    J. C. Raymond

    Center for Astrophysics Harvard & Smithsonian, United States

    9 publications · 1.1K citations

    9

    h-index

1–5 of 857

Venues

  1. The Astrophysical Journal

    ApJ · 142 publications · 9.9K citations

    51

    h-index

  2. Astronomy and Astrophysics

    53 publications · 2.9K citations

    28

    h-index

  3. Journal of Geophysical Research Atmospheres

    JGR · 29 publications · 2.1K citations

    22

    h-index

  4. Solar Physics

    38 publications · 1.3K citations

    22

    h-index

  5. Springer Link (Chiba Institute of Technology)

    Repository · 8 publications · 125 citations

    8

    h-index

1–5