The scattering coefficient in the lower Venusian atmosphere from the results of photometric measurements onboard Venera 9 and 10

Details The scattering coefficient in the lower Venusian atmosphere from the results of photometric measurements onboard Venera 9 and 10 The scattering coefficient in the lower Venusian atmosphere from the results of photometric measurements onboard Venera 9 and 10

Jul 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978kosis..16..563g&link_type=abstract

Kosmicheskie Issledovaniia, vol. 16, July-Aug. 1978, p. 563-569. In Russian.

Physics

Optics

1

Astronomical Photometry, Rayleigh Scattering, Scattering Coefficients, Venera Satellites, Venus Atmosphere, Albedo, Atmospheric Optics, Carbon Dioxide, Lower Atmosphere, Optical Thickness, Planetology, Radiant Flux Density

Scientific paper

In the present paper, the scattering coefficient at heights up to 10 km
in the Venusian atmosphere is determined from spaceborne light-flux
measurements. It is shown that, within experimental uncertainty, there
is a good agreement with the Rayleigh coefficient.

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