Theoretical brightness curves of a planet and their comparison with brightness curves of Venus

Details Theoretical brightness curves of a planet and their comparison with brightness curves of Venus Theoretical brightness curves of a planet and their comparison with brightness curves of Venus

Jan 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976avest...9..147k&link_type=abstract

(Astronomicheskii Vestnik, vol. 9, July-Sept. 1975, p. 147-151.) Solar System Research, vol. 9, no. 3, Jan. 1976, p. 119-123. Tr

Astronomy and Astrophysics

Astronomy

Light Curve, Planetary Radiation, Venus Atmosphere, Anisotropic Media, Atmospheric Scattering, Light Scattering, Ubv Spectra, Venus (Planet)

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.

Affiliated with

Also associated with

No associations

Rating

Theoretical brightness curves of a planet and their comparison with brightness curves of Venus does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Theoretical brightness curves of a planet and their comparison with brightness curves of Venus, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Theoretical brightness curves of a planet and their comparison with brightness curves of Venus will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1572006