Solar limb darkening function and solar diameter with eclipse observations

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Wavelength dependency of the Solar limb darkening

A single parameter model of the mean Solar limbdarkening is presented. This empirical law has the advantage to represent the limb darkening over a large spectrum at least as well as a quadratic or logarithmic law. Since it is less sensitive than high degree polynomial laws, it is recommended for subsequent analysis of average limb-darkening variations and comparisons.

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ژورنال

عنوان ژورنال: EAS Publications Series

سال: 2012

ISSN: 1633-4760,1638-1963

DOI: 10.1051/eas/1255056