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Bayesian Infernce for Indentifying Solar Active RegionsThe 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.
Document ID
20060035320
Acquisition Source
Jet Propulsion Laboratory
Document Type
Preprint (Draft being sent to journal)
External Source(s)
Authors
Pap, Judit
Turmon, Michael
Mukhtar, Saleem
Date Acquired
August 23, 2013
Publication Date
August 13, 1997
Distribution Limits
Public
Copyright
Other
Keywords
solar active solar chromosphere plage network background

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