Prominence Imaging

Prominence Imaging is a specialized observational technique in solar physics that employs high-resolution optical and multi-wavelength instrumentation to selectively visualize and analyze the thermal, dynamic, and magnetic structures of solar prominences within the Sun’s chromosphere and corona.

60

Publications

3.2K

Citations

213

Authors

131

Institutions

Publications per year

2017–2026

13

Authors

213

  1. BS
    B. Schmieder

    Observatoire de Paris, France

    4 publications · 139 citations

    4

    h-index

  2. SR
    S. R. Habbal

    Center for Astrophysics Harvard & Smithsonian, United States

    3 publications · 114 citations

    3

    h-index

  3. SG
    S. Gunár

    Czech Academy of Sciences, Astronomical Institute, Czechia

    3 publications · 106 citations

    3

    h-index

  4. NL
    N. Labrosse

    University of Glasgow, United Kingdom

    3 publications · 82 citations

    3

    h-index

  5. PH
    P. Heinzel

    Czech Academy of Sciences, Astronomical Institute, Czechia

    3 publications · 87 citations

    3

    h-index

1–5 of 213

Venues

  1. The Astrophysical Journal

    ApJ · 19 publications · 781 citations

    18

    h-index

  2. Astronomy and Astrophysics

    13 publications · 450 citations

    13

    h-index

  3. Journal of Geophysical Research Atmospheres

    JGR · 3 publications · 708 citations

    3

    h-index

  4. Solar Physics

    3 publications · 274 citations

    3

    h-index

  5. The Astrophysical Journal Letters

    2 publications · 179 citations

    2

    h-index

1–5