Solar radiation fluxes in the near infrared region of the spectrum in the Venusian lower atmosphere

Details Solar radiation fluxes in the near infrared region of the spectrum in the Venusian lower atmosphere Solar radiation fluxes in the near infrared region of the spectrum in the Venusian lower atmosphere

Sep 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975kosis..13..760g&link_type=abstract

Kosmicheskie Issledovaniia, vol. 13, Sept.-Oct. 1975, p. 760-764. In Russian.

Statistics

Computation

Lower Atmosphere, Near Infrared Radiation, Solar Flux, Venera Satellites, Venus Clouds, Atmospheric Attenuation, Atmospheric Models, Carbon Dioxide Concentration, Planetology, Venus Atmosphere

Scientific paper

Solar radiation fluxes incident on the Venusian atmosphere below the cloud layer are calculated in the near infrared. The computations are based on Venera data on the physical structure of the Venusian atmosphere and on recent data on the characteristics of absorption of the principal component (CO2) of the atmosphere. The results are tabulated with and without allowance for Rayleigh scattering.

Affiliated with

Also associated with

No associations

Rating

Solar radiation fluxes in the near infrared region of the spectrum in the Venusian lower 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 Solar radiation fluxes in the near infrared region of the spectrum in the Venusian lower atmosphere, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Solar radiation fluxes in the near infrared region of the spectrum in the Venusian lower atmosphere will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-911803