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D. G. Stankevich

Researcher at University of Kharkiv

Publications -  52
Citations -  938

D. G. Stankevich is an academic researcher from University of Kharkiv. The author has contributed to research in topics: Scattering & Light scattering. The author has an hindex of 14, co-authored 51 publications receiving 861 citations.

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Opposition effect from clementine data and mechanisms of backscatter

TL;DR: In this article, an analysis of Clementine data obtained from a UVVIS camera and simulating laboratory photometric and polarimetric measurements is presented with the use of a new photometric three-parameter function combining the shadow-hiding and coherent backscatter mechanisms.
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A Critical review of theoretical models of negatively polarized light scattered by atmosphereless solar system bodies

TL;DR: In this article, the phase-angle dependence of the degree of polarization observed at small phase angles has been analyzed and it was shown that interference or coherent backscattering mechanism is the most promising model.
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A critical assessment of the Hapke photometric model

TL;DR: In this paper, the Hapke model is used to study the surface structure and composition of atmosphereless celestial bodies using photometric measurements, but the model does not consider the dependence of the shadow-hiding effect of particles and coherent backscattering enhancement on illuminating/viewing geometry.
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Statistical Analysis of the Links among Lunar Mare Soil Mineralogy, Chemistry, and Reflectance Spectra

TL;DR: In this article, a statistical analysis of the variance across each measurement using principal component analysis (PCA) is performed for spectral properties of mare soils and their compositional properties (elemental abundance and mineralogy).
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Photometric properties of the lunar surface derived from Clementine observations

TL;DR: In this paper, the dependence of the surface brightness on the observation/illumination geometry was studied, and it was shown that the disk component of this dependence, that is, the variations of brightness at constant phase angle, is different for different mare areas.