Temperature and zonal circulation of the Venus atmosphere from radio occultation data

Details Temperature and zonal circulation of the Venus atmosphere from radio occultation data Temperature and zonal circulation of the Venus atmosphere from radio occultation data

May 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980kosis..18..435c&link_type=abstract

Kosmicheskie Issledovaniia, vol. 18, May-June 1980, p. 435-441. In Russian.

Physics

1

Atmospheric Circulation, Atmospheric Temperature, Atmospheric Turbulence, Radio Occultation, Venus Atmosphere, Zonal Flow (Meteorology), Daytime, Night, Space Exploration, Temperature Profiles, Wind Velocity

Scientific paper

Radio occultation data obtained in various regions of the day and night sides of Venus are used to analyze the height dependence of temperature in the Venus atmosphere. A method for determining the zonal transport velocity of atmospheric masses from temperature data is presented. Attention is given to the height dependence of the zonal wind velocity for various near-equatorial regions and for midlatitude regions on the day and night sides of the planet. The presence of a jet stream at heights of 60-70 km is suggested.

Affiliated with

Also associated with

No associations

Rating

Temperature and zonal circulation of the Venus atmosphere from radio occultation data 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 Temperature and zonal circulation of the Venus atmosphere from radio occultation data, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Temperature and zonal circulation of the Venus atmosphere from radio occultation data will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1360065