White-light Flares
White-Light Flares is a phenomenon in solar physics characterized by a transient enhancement of continuum radiation across the visible spectrum during a solar flare, distinguished from typical flares by the prominence of broadband white-light emission originating from the photosphere or chromosphere.
263
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12.7K
Citations
796
Authors
314
Institutions
Publications per year
2017–2026
80
Variants
White-light Solar Flares
Parents
263
Thick-target processes and white-light flares
H. S. Hudson · Solar Physics · 1972 · 235 citations
The Outer Solar Corona as Observed from Skylab: Preliminary Results
R. M. MacQueen, John A. Eddy, J. T. Gosling et al. · The Astrophysical Journal · 1974 · 213 citations
Natural Sciences, Astronomy, Physics +17
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Goddard Space Flight Center
Greenbelt, United States
20 h-index
40 publications
2.6K citations
University of California, Berkeley
Berkeley, United States
19 h-index
40 publications
3.5K citations
National Solar Observatory
Boulder, United States
19 h-index
31 publications
1.5K citations
Nanjing University
Nanjing, China
17 h-index
66 publications
2.3K citations
New Jersey Institute of Technology
Newark, United States
16 h-index
78 publications
3.9K citations
National Astronomical Observatory of Japan
Mitaka-shi, Japan
14 h-index
21 publications
1.1K citations

Kyoto University
Kyoto, Japan
13 h-index
45 publications
3.2K citations

United States Naval Research Laboratory
Washington, United States
13 h-index
37 publications
2.9K citations
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ApJ · 92 publications · 5.6K citations
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52 publications · 2.1K citations
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17 publications · 894 citations
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14 publications · 626 citations
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7 publications · 276 citations
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