Active Region Classification
Active Region Classification is a methodological construct in solar physics that categorizes solar active regions based on morphological, magnetic, and evolutionary characteristics to assess their potential for flare and coronal mass ejection productivity.
94
Publications
4.4K
Citations
261
Authors
122
Institutions
Publications per year
2017–2026
36
Variants
Solar Active Region Classification
Parents
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Chinese Academy of Sciences
Beijing, China
8 h-index
27 publications
1K citations
Northwest Research Associates
Redmond, United States
7 h-index
15 publications
873 citations
Stanford University
Stanford, United States
6 h-index
7 publications
482 citations
University of Michigan
Ann Arbor, United States
5 h-index
31 publications
2.3K citations

Special Astrophysical Observatory
Nizhniy Arkhyz, Russia
5 h-index
9 publications
189 citations
University of Chinese Academy of Sciences
Beijing, China
5 h-index
7 publications
273 citations
California Institute of Technology
Pasadena, United States
5 h-index
10 publications
1.2K citations

University of Bradford
Bradford, United Kingdom
5 h-index
13 publications
685 citations
1–8 of 122
ApJ · 25 publications · 1.8K citations
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16 publications · 650 citations
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10 publications · 575 citations
10
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7 publications · 496 citations
7
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5 publications · 100 citations
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