Change in Venusian atmosphere absorption coefficient with altitude

Details Change in Venusian atmosphere absorption coefficient with altitude Change in Venusian atmosphere absorption coefficient with altitude

Oct 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984rpspr...2...78y&link_type=abstract

In its USSR Rept.: Space (JPRS-USP-84-005) p 78 (SEE N85-11060 02-12) Transl. into ENGLISH from Kosm. Issled. (Moscow), v. 22

Computer Science

Absorptivity, Altitude, Venus Atmosphere, Light (Visible Radiation), Pioneer Venus Spacecraft, Venera Satellites

Scientific paper

A method is given of directly determining the distribution of absorption coefficient kappa (h) as a function of height in the Venusian atmosphere by measurement of the amount of light striking a horizontal area both from above and from below over a broad range of wavelengths between 0.5 and 1.2 microns. Such measurements were performed by the Venera-9, Venera-10 and Pioneer-Venus spacecraft. Such measurement is sufficiently reliable, allowing direct determination of the volumetric absorption coefficient kappa (h) and complete restoration of the field of radiation in the deeper layes of the atmosphere, using the equations presented.

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