Radiative heat transfer and water content in Venusian atmosphere

Details Radiative heat transfer and water content in Venusian atmosphere Radiative heat transfer and water content in Venusian atmosphere

Jan 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986rpspr...1..123m&link_type=abstract

In its USSR Report: Space (JPRS-USP-86-001) p 123-124 (SEE N86-20178 10-88) Transl. into ENGLISH from Astronomicheskiy Vestni

Physics

Optics

Atmospheric Composition, Moisture Content, Radiative Heat Transfer, Venus Atmosphere, Absorption Spectra, Atmospheric Models, Carbon Dioxide, Sulfur Dioxides, Venus (Planet)

Scientific paper

Procedures for calculating the optical characteristics of the mean components and effective fluxes of the atmosphere of Venus are presented, and some theoretical results are compared with the available experimental data and other atmospheric optics models. Attention is given to the problem of correctly estimating the absorption spectra of the main gaseous components (CO2, H2O, and SO2) at their respective temperatures, pressures, and abundances. It is shown that the conditions of thermal equilibrium in the undercloud atmosphere of Venus correspond to a water vapor adundance of about 0.0001. Some possible sources of error in the theoretical calculations are discussed.

Affiliated with

Also associated with

No associations

Rating

Radiative heat transfer and water content in Venusian atmosphere 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 Radiative heat transfer and water content in Venusian atmosphere, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Radiative heat transfer and water content in Venusian atmosphere will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1847850