Coronal Abundance Diagnostics

Coronal Abundance Diagnostics is a systematic method in solar physics that determines the relative elemental composition of the solar corona by analyzing emission line intensities in extreme ultraviolet and X-ray spectra, distinguishing itself from other diagnostic techniques through its specific focus on abundance-derived signatures of plasma conditions and fractionation processes.

82

Publications

3.9K

Citations

212

Authors

96

Institutions

Publications per year

2017–2026

7

Authors

212

  1. UF
    U. Feldman

    United States Naval Research Laboratory, United States

    8 publications · 445 citations

    8

    h-index

  2. GD
    G. Del Zanna

    University of Cambridge, United Kingdom

    4 publications · 202 citations

    6

    h-index

  3. JM
    J. M. Laming

    United States Naval Research Laboratory, United States

    6 publications · 411 citations

    6

    h-index

  4. BJ
    B. J. I. Bromage

    Rutherford Appleton Laboratory, United Kingdom

    4 publications · 688 citations

    5

    h-index

  5. KG
    K. G. Widing

    United States Naval Research Laboratory, United States

    4 publications · 396 citations

    4

    h-index

1–5 of 212

Venues

  1. The Astrophysical Journal

    ApJ · 26 publications · 1.3K citations

    23

    h-index

  2. Solar Physics

    15 publications · 926 citations

    14

    h-index

  3. Astronomy and Astrophysics

    13 publications · 685 citations

    12

    h-index

  4. Advances in Space Research

    6 publications · 368 citations

    6

    h-index

  5. 4

    h-index

1–5