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- W2020196235 abstract "Opposition effect is a nonlinear increase in the brightness of an object close to astronomical opposition. We present a comparison and summary of the phase curves of some icy solar system objects, and terrestrial ice. We have constructed a method of approximating the height and width of the opposition peak and evaluating the practicality of the method in each case, with the aid of a four-parameter fit to a linear-exponential function and computing the a posteriori probability distribution of the height and width of the opposition peak. The procedure described is most applicable in finding a realistic fit and evaluating the suitability of data, even with moderate inaccuracy. We have studied the effect of the number of data points to the feasibility of the fit, in order to estimate the minimum amount of data required for a desired accuracy. Furthermore, we present an interpretation of the phase curves by means of two scattering mechanisms with important applications to the recent study of the opposition effect: shadowing and coherent backscattering." @default.
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- W2020196235 date "2001-08-01" @default.
- W2020196235 modified "2023-09-27" @default.
- W2020196235 title "Comparative study on opposition effect of icy solar system objects" @default.
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- W2020196235 doi "https://doi.org/10.1016/s0022-4073(01)00027-9" @default.
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