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
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1–5 of 149
370
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Center for Astrophysics Harvard & Smithsonian, United States
5 publications · 1K citations
5
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4
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202

Chinese Academy of Sciences
Beijing, China
17 h-index
59 publications
2.1K citations
National Astronomical Observatories
Beijing, China
16 h-index
52 publications
2K citations

University of St Andrews
St Andrews, United Kingdom
15 h-index
28 publications
1.7K citations

Centre National de la Recherche Scientifique
Paris, France
13 h-index
20 publications
977 citations
Université Paris Cité
Paris, France
13 h-index
17 publications
844 citations
Laboratoire d’études spatiales et d’instrumentation en astrophysique
Meudon, France
11 h-index
14 publications
646 citations

Yunnan Observatories
Kunming, China
11 h-index
45 publications
1.4K citations
University College London
London, United Kingdom
11 h-index
22 publications
1.5K citations
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ApJ · 69 publications · 3.8K citations
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18 publications · 805 citations
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6 publications · 277 citations
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Repository · 4 publications · 184 citations
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JGR · 3 publications · 314 citations
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