Solar X-ray Variability

Solar X-Ray Variability is a temporal phenomenon characterized by changes in the intensity and spectral properties of solar X-ray emissions over various timescales, distinguishing it from steady-state solar X-ray emission within the study of solar atmospheric dynamics.

206

Publications

8.4K

Citations

615

Authors

263

Institutions

Publications per year

2017–2026

32

Authors

615

  1. TN
    T. N. Woods

    Laboratory for Atmospheric and Space Physics, United States

    8 publications · 416 citations

    8

    h-index

  2. JH
    J. H. M. M. Schmitt

    Universität Hamburg, Germany

    7 publications · 185 citations

    7

    h-index

  3. GR
    G. R. Gladstone

    Southwest Research Institute, United States

    6 publications · 212 citations

    6

    h-index

  4. GB
    G. Branduardi‐Raymont

    University College London, United Kingdom

    5 publications · 169 citations

    5

    h-index

  5. SS
    S. Sciortino

    Osservatorio Astronomico di Palermo, Italy

    5 publications · 156 citations

    5

    h-index

1–5 of 615

Venues

  1. The Astrophysical Journal

    ApJ · 49 publications · 2.5K citations

    31

    h-index

  2. Solar Physics

    27 publications · 1.5K citations

    20

    h-index

  3. Journal of Geophysical Research Atmospheres

    JGR · 17 publications · 889 citations

    13

    h-index

  4. Astronomy and Astrophysics

    10 publications · 284 citations

    11

    h-index

  5. Geophysical Research Letters

    9 publications · 685 citations

    9

    h-index

1–5