Solar Absorption Lines

Solar Absorption Lines is a spectroscopic phenomenon consisting of narrow, dark features in the solar spectrum that result from the selective absorption of continuum radiation by atomic or molecular species in the Sun's atmosphere.

412

Publications

19.2K

Citations

1.1K

Authors

359

Institutions

Publications per year

2017–2026

25

Variants

Fraunhofer Lines

Authors

1.1K

  1. CP
    C. P. Rinsland

    Langley Research Center, United States

    18 publications · 770 citations

    15

    h-index

  2. DG
    D. G. Murcray

    University of Denver, United States

    14 publications · 347 citations

    12

    h-index

  3. AS
    Alan S. Goldman

    Rutgers, The State University of New Jersey, United States

    11 publications · 340 citations

    11

    h-index

  4. CB
    C. B. Farmer

    Jet Propulsion Laboratory, United States

    11 publications · 551 citations

    10

    h-index

  5. FJ
    F. J. Murcray

    University of Denver, United States

    9 publications · 278 citations

    9

    h-index

1–5 of 1.1K

Venues

  1. The Astrophysical Journal

    ApJ · 100 publications · 5.6K citations

    38

    h-index

  2. Journal of Geophysical Research Atmospheres

    JGR · 29 publications · 1.4K citations

    21

    h-index

  3. Solar Physics

    30 publications · 841 citations

    18

    h-index

  4. Monthly Notices of the Royal Astronomical Society

    24 publications · 1.4K citations

    17

    h-index

  5. Geophysical Research Letters

    17 publications · 610 citations

    14

    h-index

1–5