Solar Spectroscopy

Solar Spectroscopy is a branch of astronomical spectroscopy that analyzes the Sun's electromagnetic radiation to determine its physical properties, chemical composition, and dynamic processes by examining the intensity and wavelength distribution of spectral lines.

3.6K

Publications

175.6K

Citations

8.1K

Authors

1.5K

Institutions

Publications per year

2017–2026

490

Authors

8.1K

  1. UF
    U. Feldman

    United States Naval Research Laboratory, United States

    89 publications · 4.9K citations

    40

    h-index

  2. CP
    C. P. Rinsland

    Langley Research Center, United States

    67 publications · 3.5K citations

    37

    h-index

  3. GA
    G. A. Doschek

    United States Naval Research Laboratory, United States

    63 publications · 3.3K citations

    33

    h-index

  4. MA
    M. Asplund

    Australian National University, Australia

    39 publications · 5.4K citations

    32

    h-index

  5. SK
    S. K. Solanki

    Max Planck Institute for Solar System Research, Germany

    68 publications · 3.1K citations

    31

    h-index

1–5 of 8.1K

Venues

  1. The Astrophysical Journal

    ApJ · 854 publications · 37.8K citations

    89

    h-index

  2. Astronomy and Astrophysics

    398 publications · 21.1K citations

    72

    h-index

  3. Journal of Geophysical Research Atmospheres

    JGR · 176 publications · 10.1K citations

    57

    h-index

  4. Solar Physics

    239 publications · 15.7K citations

    53

    h-index

  5. Monthly Notices of the Royal Astronomical Society

    147 publications · 6.8K citations

    43

    h-index

1–5