Flare Cooling

Flare Cooling is a physical process in solar physics describing the phase subsequent to a solar flare during which the highly energized plasma in the coronal loop loses thermal energy through radiation, conduction, and adiabatic expansion, distinguishing it from the impulsive and peak emission stages of flare evolution.

53

Publications

2.6K

Citations

299

Authors

113

Institutions

Publications per year

2017–2026

11

Authors

299

  1. SK
    S. K. Antiochos

    United States Naval Research Laboratory, United States

    7 publications · 422 citations

    7

    h-index

  2. JT
    J. T. Mariska

    United States Naval Research Laboratory, United States

    3 publications · 267 citations

    3

    h-index

  3. PJ
    P. J. Cargill

    Imperial College London, United Kingdom

    2 publications · 241 citations

    2

    h-index

  4. AG
    A. G. Emslie

    University of Alabama in Huntsville, United States

    2 publications · 133 citations

    2

    h-index

  5. SZ
    Shuo Zhang

    Columbia University, United States

    2 publications · 163 citations

    2

    h-index

1–5 of 299

Venues

  1. The Astrophysical Journal

    ApJ · 26 publications · 1.1K citations

    19

    h-index

  2. Solar Physics

    10 publications · 839 citations

    9

    h-index

  3. The Astrophysical Journal Letters

    3 publications · 76 citations

    3

    h-index

  4. 2

    h-index

  5. Astronomy and Astrophysics

    2 publications · 101 citations

    2

    h-index

1–5