Coronal Spectroscopy

Coronal Spectroscopy is a specialized branch of solar spectroscopy that employs the analysis of electromagnetic radiation emitted by the Sun's corona to determine its physical properties, such as temperature, density, and composition, through the identification and interpretation of spectral lines formed in highly ionized states of atoms under extreme coronal conditions.

326

Publications

15K

Citations

882

Authors

301

Institutions

Publications per year

2017–2026

39

Authors

882

  1. GD
    G. Del Zanna

    University of Cambridge, United Kingdom

    12 publications · 711 citations

    12

    h-index

  2. UF
    U. Feldman

    United States Naval Research Laboratory, United States

    14 publications · 653 citations

    12

    h-index

  3. EL
    E. Landi

    United States Naval Research Laboratory, United States

    11 publications · 481 citations

    11

    h-index

  4. JJ
    J. J. Drake

    Center for Astrophysics Harvard & Smithsonian, United States

    9 publications · 597 citations

    9

    h-index

  5. GA
    G. A. Doschek

    United States Naval Research Laboratory, United States

    8 publications · 376 citations

    8

    h-index

1–5 of 882

Venues

  1. The Astrophysical Journal

    ApJ · 137 publications · 6.3K citations

    46

    h-index

  2. Astronomy and Astrophysics

    39 publications · 2.9K citations

    29

    h-index

  3. Solar Physics

    35 publications · 1.9K citations

    21

    h-index

  4. 14

    h-index

  5. Advances in Space Research

    11 publications · 475 citations

    11

    h-index

1–5