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.
CITATION STYLE
Hestroffer, D., & Magnan, C. (1998). Wavelength dependency of the Solar limb darkening. Astronomy and Astrophysics, 333(1), 338–342.
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