NASA NTRS · 20060035320
Bayesian Infernce for Indentifying Solar Active Regions
Abstract
The solar chromosphere consists of three classes-- plage, network, background -- which contribute differently to ultraviolet radiation reaching the earth. Solar physicists are interested in relating plage area and intensity to UV irradiance, as well as understanding the spatial and temporal evolution of plage shapes.
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Pap, Judit, Turmon, Michael, Mukhtar, Saleem. 1997-08-13. Bayesian Infernce for Indentifying Solar Active Regions. https://ntrs.nasa.gov/citations/20060035320
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