Continuum Intensity Variation
Continuum Intensity Variation is a photometric measurement representing the spatial and temporal fluctuations in the intensity of continuous spectral radiation emitted by the solar photosphere, distinguished from spectral line variations by its origin in the broadband opacity-driven emission from photospheric plasma.
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12.4K
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913
Authors
347
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2017–2026
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Instituto de Astrofísica de Canarias
Tenerife, Spain
14 h-index
27 publications
1.1K citations

NSF National Center for Atmospheric Research
Boulder, United States
13 h-index
24 publications
1.1K citations
Max Planck Institute for Solar System Research
Göttingen, Germany
13 h-index
41 publications
2K citations
Institut für Sonnenphysik
Freiburg im Breisgau, Germany
13 h-index
38 publications
1.3K citations
NSF NCAR High Altitude Observatory
Boulder, United States
13 h-index
22 publications
1K citations

Chinese Academy of Sciences
Beijing, China
9 h-index
21 publications
531 citations
Max Planck Society
Munich, Germany
9 h-index
20 publications
2.2K citations
Instituto de Astrofísica de Andalucía
Granada, Spain
9 h-index
10 publications
414 citations
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ApJ · 75 publications · 4K citations
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