Line Profile Fitting

Line Profile Fitting is a spectroscopic analysis method that belongs to the class of data inversion techniques in helioseismology, distinguished by its focus on modeling the shape of spectral line profiles to infer physical parameters of solar oscillations such as velocity, intensity, and linewidth.

666

Publications

36.5K

Citations

2.1K

Authors

715

Institutions

Publications per year

2017–2026

126

Authors

2.1K

  1. FB
    F. Borsa

    Brera Astronomical Observatory, Italy

    24 publications · 750 citations

    18

    h-index

  2. AS
    A. Sozzetti

    Osservatorio Astrofisico di Torino, Italy

    27 publications · 781 citations

    18

    h-index

  3. AS
    A. S. Bonomo

    Osservatorio Astrofisico di Torino, Italy

    25 publications · 740 citations

    17

    h-index

  4. EP
    E. Poretti

    Brera Astronomical Observatory, Italy

    25 publications · 774 citations

    17

    h-index

  5. AB
    A. Bignamini

    Trieste Astronomical Observatory, Italy

    25 publications · 744 citations

    17

    h-index

1–5 of 2.1K

Venues

  1. The Astrophysical Journal

    ApJ · 120 publications · 8.2K citations

    46

    h-index

  2. Astronomy and Astrophysics

    83 publications · 4K citations

    36

    h-index

  3. Monthly Notices of the Royal Astronomical Society

    79 publications · 2.9K citations

    33

    h-index

  4. Journal of Quantitative Spectroscopy and Radiative Transfer

    JQSRT · 35 publications · 2.1K citations

    20

    h-index

  5. Journal of Applied Crystallography

    20 publications · 4.3K citations

    17

    h-index

1–5