Coronal Plasma Diagnostics

Coronal Plasma Diagnostics is a systematic method in solar physics that analyzes X-ray emission spectra and intensity distributions to infer the physical conditions—such as temperature, density, and composition—of plasma in the solar corona.

190

Publications

10K

Citations

809

Authors

249

Institutions

Publications per year

2017–2026

37

Authors

809

  1. EL
    E. Landi

    United States Naval Research Laboratory, United States

    11 publications · 404 citations

    11

    h-index

  2. FR
    F. Reale

    Osservatorio Astronomico di Palermo, Italy

    8 publications · 308 citations

    8

    h-index

  3. GD
    G. Del Zanna

    University of Cambridge, United Kingdom

    8 publications · 352 citations

    8

    h-index

  4. LG
    L. Golub

    Center for Astrophysics Harvard & Smithsonian, United States

    7 publications · 932 citations

    7

    h-index

  5. VM
    V. M. Nakariakov

    University of Warwick, United Kingdom

    7 publications · 1.1K citations

    7

    h-index

1–5 of 809

Venues

  1. The Astrophysical Journal

    ApJ · 63 publications · 3K citations

    34

    h-index

  2. Astronomy and Astrophysics

    35 publications · 2K citations

    24

    h-index

  3. Solar Physics

    12 publications · 862 citations

    12

    h-index

  4. Physics of Plasmas

    6 publications · 201 citations

    6

    h-index

  5. The Astrophysical Journal Letters

    5 publications · 226 citations

    5

    h-index

1–5