On the wavelength dependency of solar limb darkening (λλ303 to 1099 nm)

Details On the wavelength dependency of solar limb darkening (λλ303 to 1099 nm) On the wavelength dependency of solar limb darkening (λλ303 to 1099 nm)

Aug 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996soph..167....9n&link_type=abstract

Solar Physics, Volume 167, Issue 1-2, pp. 9-23

Physics

17

Scientific paper

The limb-darkening data published by Neckel and Labs (1994) (5th-order polynomials P 5(μ), μ = cos θ) are used to represent the limb darkening by the functions L n(μ), proposed first by Kourganoff (1949a). When plotted against wavelength, the coefficients of these functions show a rather low scatter and appear to be linear functions of either λ -1 or λ #x2212;5.

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