Coronal Brightness Distribution
Coronal Brightness Distribution is a scientific construct that characterizes the spatial variation of radiant intensity in the solar corona, distinguished by its quantification of brightness as a function of angular distance from the Sun's center, typically derived from white-light coronagraph observations.
305
Publications
15.8K
Citations
756
Authors
238
Institutions
Publications per year
2017–2026
35
Parents
305
The Large Angle Spectroscopic Coronagraph (LASCO)
G. E. Brueckner, R. A. Howard, M. J. Koomen et al. · Solar Physics · 1995 · 2.8K citations
Natural Sciences, Astronomy, Physics +10
A study of the background corona near solar minimum
Kuniji Saito, A. I. Poland, R. H. Munro · Solar Physics · 1977 · 283 citations
Natural Sciences, Astronomy, Physics +14
1–5 of 305
756
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Center for Astrophysics Harvard & Smithsonian, United States
9 publications · 408 citations
9
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9
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8
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1–5 of 756
238
NSF NCAR High Altitude Observatory
Boulder, United States
18 h-index
43 publications
3K citations
Goddard Space Flight Center
Greenbelt, United States
18 h-index
40 publications
3K citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
16 h-index
42 publications
3.4K citations

NSF National Center for Atmospheric Research
Boulder, United States
16 h-index
41 publications
2.9K citations

United States Naval Research Laboratory
Washington, United States
13 h-index
47 publications
24.9K citations

Centre National de la Recherche Scientifique
Paris, France
12 h-index
52 publications
2.7K citations
Max Planck Institute for Solar System Research
Göttingen, Germany
11 h-index
16 publications
1.2K citations
Jet Propulsion Laboratory
Pasadena, United States
10 h-index
13 publications
786 citations
1–8 of 238
ApJ · 82 publications · 4K citations
37
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98 publications · 7K citations
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JGR · 20 publications · 1.5K citations
16
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14 publications · 565 citations
13
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8 publications · 411 citations
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