Prominence Current Sheets

Prominence Current Sheets is a theoretical construct in solar physics denoting a thin, localized layer of intense electric current that develops within the magnetic field topology of a solar prominence, distinguishing itself by facilitating the dissipation of magnetic energy and enabling plasma instabilities critical to prominence dynamics and eruption mechanisms.

54

Publications

2.4K

Citations

128

Authors

78

Institutions

Publications per year

2017–2026

6

Authors

128

  1. BC
    B. C. Low

    NSF NCAR High Altitude Observatory, United States

    5 publications · 443 citations

    5

    h-index

  2. ER
    E. R. Priest

    University of St Andrews, United Kingdom

    5 publications · 195 citations

    5

    h-index

  3. АG
    А. G. Frank

    Prokhorov General Physics Institute, Russia

    3 publications · 115 citations

    3

    h-index

  4. TG
    T. G. Forbes

    University of New Hampshire, United States

    1 publications · 15 citations

    2

    h-index

  5. IM
    I. M. Podgorny

    P.N. Lebedev Physical Institute of the Russian Academy of Sciences, Russia

    1 publications · 17 citations

    2

    h-index

1–5 of 128

Venues

  1. The Astrophysical Journal

    ApJ · 11 publications · 665 citations

    11

    h-index

  2. Solar Physics

    9 publications · 297 citations

    10

    h-index

  3. Astronomy and Astrophysics

    5 publications · 202 citations

    5

    h-index

  4. Journal of Geophysical Research Atmospheres

    JGR · 5 publications · 316 citations

    5

    h-index

  5. Space Science Reviews

    2 publications · 146 citations

    3

    h-index

1–5