Theoretical light curves of a planet and a comparison with the light curves of Venus

Details Theoretical light curves of a planet and a comparison with the light curves of Venus Theoretical light curves of a planet and a comparison with the light curves of Venus

Sep 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975avest...9..147k&link_type=abstract

Astronomicheskii Vestnik, vol. 9, July-Sept. 1975, p. 147-151. In Russian.

Astronomy and Astrophysics

Astronomy

Light Curve, Planetary Radiation, Venus Atmosphere, Anisotropic Media, Atmospheric Scattering, Light Scattering

Scientific paper

The theory of anisotropic light scattering is used to compute theoretical light curves of a planet. A plane-parallel homogeneous semi-infinite model atmosphere with a Henyey-Greenstein scattering indicatrix is assumed. Optical characteristics of scattering particles in the atmosphere of Venus are estimated by comparing the theoretical light curves with observational data.

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