Physics
Scientific paper
Feb 1991
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991p%26ss...39..327m&link_type=abstract
(Colloquium on Phobos-Mars Mission, Paris, France, Oct. 23-27, 1989, Proceedings. A91-29558 11-91) Planetary and Space Science (
Physics
1
Luminous Intensity, Phobos, Photogrammetry, Satellite Surfaces, Scattering Functions, Surface Roughness, Imaging Techniques, Light Scattering, Standard Deviation, Statistical Distributions, Mars, Satellites, Phobos, Surface, Scattering, Particles, Brightness, Statistical Methods, Theoretical Studies, Calculations, Roughness, Procedure, Techniques, Analysis
Scientific paper
It has been suggested that slope fluctuations on the scale of pixel dimensions could be determined by statistical photoclinometry. A closer study of the surface of Phobos reveals variations in the scattering properties of single particles and microstructures formed by the particles. In the present context, the photoclinometric method of brightness moments is extended to account for these variations by allowing statistical fluctuations in the phase function of the assumed Lommel-Seeliger scattering law. The mean slope on the investigated regions of Phobos has been found to vary from about 12 deg on a 61 m scale to about 7 deg on a 216 - 272 m scale. On the same scales, a value of the order of 2 percent has been obtained for the standard deviation of the scattering phase function. Hints of a fractal-like scale-invariance have been noticed in the covariance function of brightness.
Irvine William M.
Lumme Kari
Muinonen Karri
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