Coronal Temperature Structure

Coronal Temperature Structure is a theoretical construct that characterizes the spatially non-uniform thermal distribution within the solar corona, distinguished by its capacity to explain the anomalous increase in temperature with altitude despite decreasing thermal pressure.

559

Publications

32.4K

Citations

1.1K

Authors

370

Institutions

Publications per year

2017–2026

52

Authors

1.1K

  1. LG
    L. Golub

    Center for Astrophysics Harvard & Smithsonian, United States

    14 publications · 1.1K citations

    14

    h-index

  2. AR
    Amy R. Winebarger

    Marshall Space Flight Center, United States

    13 publications · 896 citations

    13

    h-index

  3. JT
    J. T. Schmelz

    University of Memphis, United States

    13 publications · 489 citations

    13

    h-index

  4. MJ
    Markus J. Aschwanden

    Lockheed Martin (United States), United States

    12 publications · 1.1K citations

    11

    h-index

  5. HP
    Harry P. Warren

    United States Naval Research Laboratory, United States

    11 publications · 824 citations

    11

    h-index

1–5 of 1.1K

Venues

  1. The Astrophysical Journal

    ApJ · 217 publications · 17.2K citations

    65

    h-index

  2. Solar Physics

    101 publications · 4.1K citations

    34

    h-index

  3. Astronomy and Astrophysics

    48 publications · 2.1K citations

    26

    h-index

  4. Journal of Geophysical Research Atmospheres

    JGR · 23 publications · 1.6K citations

    19

    h-index

  5. Monthly Notices of the Royal Astronomical Society

    25 publications · 1.8K citations

    19

    h-index

1–5