Euv Coronal Imaging

EUV Coronal Imaging is a specialized observational technique in solar physics that employs extreme ultraviolet (EUV) wavelengths to capture high-resolution images of the Sun's corona, enabling the detailed study of its thermal structure, plasma dynamics, and transient phenomena.

144

Publications

8.8K

Citations

385

Authors

166

Institutions

Publications per year

2017–2026

25

Authors

385

  1. LK
    L. K. Harra

    University College London, United Kingdom

    10 publications · 928 citations

    10

    h-index

  2. FA
    F. Auchère

    Institut d'Astrophysique Spatiale, France

    8 publications · 215 citations

    8

    h-index

  3. PR
    Peter R. Young

    New Frontier, United States

    8 publications · 859 citations

    8

    h-index

  4. HH
    Hirohisa Hara

    National Astronomical Observatory of Japan, Japan

    6 publications · 765 citations

    6

    h-index

  5. DH
    David H. Brooks

    George Mason University, United States

    6 publications · 338 citations

    6

    h-index

1–5 of 385

Venues

  1. The Astrophysical Journal

    ApJ · 76 publications · 5.5K citations

    40

    h-index

  2. Astronomy and Astrophysics

    16 publications · 1.1K citations

    15

    h-index

  3. Solar Physics

    11 publications · 598 citations

    11

    h-index

  4. The Astrophysical Journal Letters

    9 publications · 671 citations

    9

    h-index

  5. Journal of Geophysical Research Atmospheres

    JGR · 4 publications · 144 citations

    4

    h-index

1–5