Prominence Morphology
Prominence Morphology is a scientific construct in solar physics that characterizes the structural form and spatial configuration of solar prominences, distinguishing it from other prominence properties by focusing specifically on their observable shape, fine-scale organization, and topological arrangement within the solar corona.
260
Publications
12.9K
Citations
552
Authors
254
Institutions
Publications per year
2017–2026
24
Parents
260
A magnetic cloud containing prominence material: January 1997
L. F. Burlaga, R. J. Fitzenreiter, R. P. Lepping et al. · Journal of Geophysical Research Atmospheres · 1998 · 282 citations · Full text
Natural Sciences, Astronomy, Physics +17
Solar Prominences: Observations
S. Parenti · Living Reviews in Solar Physics · 2014 · 275 citations · Full text
Natural Sciences, Astronomy, Physics +17
1–5 of 260
552
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254

Centre National de la Recherche Scientifique
Paris, France
15 h-index
27 publications
1.2K citations

Observatoire de Paris
Paris, France
14 h-index
26 publications
1.3K citations

Czech Academy of Sciences, Astronomical Institute
Ondřejov, Czechia
13 h-index
28 publications
936 citations
Laboratoire d’études spatiales et d’instrumentation en astrophysique
Meudon, France
13 h-index
26 publications
1.6K citations
NSF NCAR High Altitude Observatory
Boulder, United States
12 h-index
32 publications
2.9K citations

University of St Andrews
St Andrews, United Kingdom
12 h-index
26 publications
678 citations

NSF National Center for Atmospheric Research
Boulder, United States
12 h-index
29 publications
2.9K citations
Goddard Space Flight Center
Greenbelt, United States
12 h-index
21 publications
877 citations
1–8 of 254
77 publications · 3.3K citations
32
h-index
ApJ · 31 publications · 2K citations
22
h-index
16 publications · 661 citations
15
h-index
8 publications · 637 citations
8
h-index
7 publications · 223 citations
7
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