Solar Filaments
Solar filaments are cool, dense plasma structures suspended in the Sun's corona that appear as dark, thread-like formations when observed in Hα emission against the bright solar disk, distinguished from other chromospheric features by their association with magnetic neutrality lines and their potential to erupt as coronal mass ejections.
842
Publications
41.7K
Citations
1.6K
Authors
503
Institutions
Publications per year
2017–2026
192
842
Filamentary structure in the Orion molecular cloud
John Bally, A. A. Stark, R. W. Wilson et al. · The Astrophysical Journal · 1987 · 509 citations
Natural Sciences, Astronomy, Physics +15
CRISP Spectropolarimetric Imaging of Penumbral Fine Structure
The Astrophysical Journal · 2008 · 477 citations · Full text
Natural Sciences, Astronomy, Physics +17
RADIATIVE MAGNETOHYDRODYNAMIC SIMULATION OF SUNSPOT STRUCTURE
M. Rempel, M. Knölker · The Astrophysical Journal · 2009 · 352 citations · Full text
Natural Sciences, Astronomy, Physics +15
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503

Chinese Academy of Sciences
Beijing, China
40 h-index
420 publications
17.5K citations
National Astronomical Observatories
Beijing, China
38 h-index
300 publications
13K citations

Yunnan Observatories
Kunming, China
31 h-index
318 publications
12.7K citations
Nanjing University
Nanjing, China
31 h-index
139 publications
5.7K citations
Goddard Space Flight Center
Greenbelt, United States
31 h-index
88 publications
4.9K citations
Max Planck Institute for Solar System Research
Göttingen, Germany
30 h-index
137 publications
6.4K citations

Centre National de la Recherche Scientifique
Paris, France
29 h-index
127 publications
9.5K citations

Observatoire de Paris
Paris, France
29 h-index
102 publications
5.8K citations
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ApJ · 360 publications · 20.6K citations
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98 publications · 4K citations
36
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75 publications · 3.6K citations
35
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48 publications · 2.2K citations
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JGR · 18 publications · 1.6K citations
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