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- W2085849475 abstract "After deriving the Minnaert (1961) parameters for the five largest satellites of Uranus as functions of both wavelength and phase angle, the well-documented case of Titania is invoked to assess the usefulness of the Minnaert description vs the more rigorous approach of Hapke (1981). While the limb-darkening Minnaert parameter k possesses only a weak wavelength dependence, it exhibits a strong dependence on phase angle that varies to some extent from satellite to satellite; in the case of Titania, this dependence is similar to that for the earth's moon." @default.
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- W2085849475 date "1989-03-01" @default.
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- W2085849475 title "Minnaert photometric parameters for the satellites of Uranus" @default.
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- W2085849475 doi "https://doi.org/10.1016/0019-1035(89)90066-3" @default.
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