Continuum Intensity Variation

Continuum Intensity Variation is a photometric measurement representing the spatial and temporal fluctuations in the intensity of continuous spectral radiation emitted by the solar photosphere, distinguished from spectral line variations by its origin in the broadband opacity-driven emission from photospheric plasma.

278

Publications

12.4K

Citations

913

Authors

347

Institutions

Publications per year

2017–2026

22

Authors

913

  1. SK
    S. K. Solanki

    Max Planck Institute for Solar System Research, Germany

    8 publications · 557 citations

    8

    h-index

  2. LR
    L. R. Bellot Rubio

    Instituto de Astrofísica de Andalucía, Spain

    5 publications · 226 citations

    5

    h-index

  3. LČ
    Luka Č. Popović

    Astronomical Observatory, Serbia

    5 publications · 142 citations

    5

    h-index

  4. AM
    A. M. Title

    Lockheed Martin (United States), United States

    4 publications · 392 citations

    4

    h-index

  5. TD
    T. D. Tarbell

    Lockheed Martin (United States), United States

    4 publications · 343 citations

    4

    h-index

1–5 of 913

Venues

  1. The Astrophysical Journal

    ApJ · 75 publications · 4K citations

    32

    h-index

  2. Astronomy and Astrophysics

    47 publications · 2K citations

    26

    h-index

  3. Monthly Notices of the Royal Astronomical Society

    29 publications · 1.3K citations

    20

    h-index

  4. Solar Physics

    10 publications · 400 citations

    9

    h-index

  5. The Journal of Chemical Physics

    8 publications · 306 citations

    8

    h-index

1–5