Flux Cancellation

Flux Cancellation is a physical process in solar magnetohydrodynamics wherein adjacent regions of opposite magnetic polarity in the solar photosphere undergo mutual neutralization through converging motions, leading to the apparent disappearance of magnetic flux and often associated with the formation or evolution of solar active regions.

149

Publications

7.9K

Citations

370

Authors

202

Institutions

Publications per year

2017–2026

62

Authors

370

  1. JC
    Jongchul Chae

    Seoul National University, South Korea

    7 publications · 358 citations

    7

    h-index

  2. FC
    Fred C. Lee

    Virginia Tech, United States

    5 publications · 403 citations

    5

    h-index

  3. ER
    E. R. Priest

    University of St Andrews, United Kingdom

    5 publications · 364 citations

    5

    h-index

  4. AA
    A. A. van Ballegooijen

    Center for Astrophysics Harvard & Smithsonian, United States

    5 publications · 1K citations

    5

    h-index

  5. JW
    Jingxiu Wang

    National Astronomical Observatories, China

    4 publications · 251 citations

    4

    h-index

1–5 of 370

Venues

  1. The Astrophysical Journal

    ApJ · 69 publications · 3.8K citations

    36

    h-index

  2. Astronomy and Astrophysics

    18 publications · 805 citations

    15

    h-index

  3. The Astrophysical Journal Letters

    6 publications · 277 citations

    6

    h-index

  4. Springer Link (Chiba Institute of Technology)

    Repository · 4 publications · 184 citations

    4

    h-index

  5. Journal of Geophysical Research Atmospheres

    JGR · 3 publications · 314 citations

    3

    h-index

1–5