The shadow component of the phase brightness dependence of atmosphereless cosmic bodies

Details The shadow component of the phase brightness dependence of atmosphereless cosmic bodies The shadow component of the phase brightness dependence of atmosphereless cosmic bodies

Oct 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988kfnt....4...60s&link_type=abstract

Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 4, Sept.-Oct. 1988, p. 60-66. In Russian.

Computer Science

5

Atmospheric Attenuation, Celestial Bodies, Light Scattering, Phase Shift, Shadows, Autocorrelation, Brightness, Powder (Particles)

Scientific paper

A new theoretical model for the shadow effect of powdery surfaces is constructed using the autocorrelation function for the optical inhomogeneity of a scattered surface. A formula is obtained for the shadow component of the phase brightness distribution, which is in good agreement with observational data for small phase angles and low photometric longitude values.

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