Chromospheric Spectroscopy

Chromospheric Spectroscopy is a specialized observational method in solar physics that analyzes spectral emissions from the Sun's chromosphere to infer its physical properties, dynamics, and thermal structure through high-resolution wavelength-resolved measurements distinct from photospheric or coronal spectroscopic techniques.

303

Publications

20K

Citations

866

Authors

324

Institutions

Publications per year

2017–2026

40

Authors

866

  1. AF
    A. Frasca

    Osservatorio Astrofisico di Catania, Italy

    13 publications · 1.1K citations

    13

    h-index

  2. TR
    T. R. Ayres

    University of Colorado Boulder, United States

    11 publications · 689 citations

    11

    h-index

  3. KB
    K. Biazzo

    Osservatorio Astrofisico di Catania, Italy

    10 publications · 921 citations

    10

    h-index

  4. BW
    B. W. Bopp

    University of Toledo, United States

    8 publications · 326 citations

    8

    h-index

  5. LZ
    Liyun Zhang

    Chinese Academy of Sciences, China

    8 publications · 179 citations

    8

    h-index

1–5 of 866

Venues

  1. The Astrophysical Journal

    ApJ · 101 publications · 7.4K citations

    39

    h-index

  2. Astronomy and Astrophysics

    45 publications · 2.6K citations

    25

    h-index

  3. 18

    h-index

  4. The Astronomical Journal

    AJ · 22 publications · 3.4K citations

    18

    h-index

  5. Solar Physics

    24 publications · 788 citations

    17

    h-index

1–5