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Temperature variation with latitude in the upper solar photosphere: Relevance to solar oblateness measurements and facular models
Authors:Ingersoll  Andrew P  Chapman  Gary A
Institution:1.Division of Geological and Planetary Sciences, California Institute of Technology, Calif., U.S.A.
;2.San Fernando Observatory, Space Physics Laboratory, The Aerospace Corporation, U.S.A.
;
Abstract:Solar Physics - Altrock and Canfield's observations of temperature variation with latitude in the upper solar photosphere refer to higher levels (smaller optical depths) than those to which...
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