Global variations of the optical thickness of the Venus atmosphere. III - Analysis of the behavior of equivalent widths of CO2 lines for an inhomogeneous atmosphere model

Details Global variations of the optical thickness of the Venus atmosphere. III - Analysis of the behavior of equivalent widths of CO2 lines for an inhomogeneous atmosphere model Global variations of the optical thickness of the Venus atmosphere. III - Analysis of the behavior of equivalent widths of CO2 lines for an inhomogeneous atmosphere model

Aug 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993kfnt....9...30f&link_type=abstract

Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 9, no. 4, p. 30-42.

Physics

Atmospheric Models, Carbon Dioxide Concentration, Optical Thickness, Spectral Line Width, Venus Atmosphere, Venus Clouds, Inhomogeneity, Spectral Bands, Variations

Scientific paper

A two-layer model of the Venus atmosphere is considered. The higher layer is a gaseous aerosol slab with a fixed height of the lower boundary (h - 50 km) above the planetary surface. The lower layer is a gaseous slab consisting of pure CO2. The model is used to study observed oscillations of equivalent widths of the F(0) line of CO absorption bands of 788.3 and 868.9 nm. The optical thickness of the cloud layer is tau(x) = 34.4 for one hemisphere of the planet and tau(n) = 24.4 for the opposite one. The corresponding heights of the top boundary of the cloud layer are 68.4 and 75.8 km. The variations of height of the top boundary of the cloud layer coincide with observed variations of the degree of polarization of the Venusian disk in the UV region.

Affiliated with

Also associated with

No associations

Rating

Global variations of the optical thickness of the Venus atmosphere. III - Analysis of the behavior of equivalent widths of CO2 lines for an inhomogeneous atmosphere model 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 Global variations of the optical thickness of the Venus atmosphere. III - Analysis of the behavior of equivalent widths of CO2 lines for an inhomogeneous atmosphere model, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Global variations of the optical thickness of the Venus atmosphere. III - Analysis of the behavior of equivalent widths of CO2 lines for an inhomogeneous atmosphere model will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1493833