Implications of preliminary VEGA balloon results for the Venus atmosphere dynamics

Details Implications of preliminary VEGA balloon results for the Venus atmosphere dynamics Implications of preliminary VEGA balloon results for the Venus atmosphere dynamics

Feb 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986pazh...12...52b&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 12, Jan. 1986, p. 52-58) Soviet Astronomy Letters (ISSN 0360-0327), vol. 12, Jan.-Feb.

Computer Science

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2

Atmospheric Circulation, Balloon Sounding, Vega Project, Venus Atmosphere, Vertical Air Currents, Convective Heat Transfer, Radar Measurement, Solar Planetary Interactions, Wind Measurement

Scientific paper

Typical vertical wind velocities of (1 - 2) m/s measured by the Vega balloons appear to be caused by thermal convection. The observed temperature difference of 6.5K between Vega 1 and Vega 2 data can be caused by the synoptic or planetary scale disturbances. The mean wind velocities obtained from Doppler measurements exceed those of previous experiments. A solar-tied feature in the wind field is possible. Surface topography appears to have influenced the motion of the Vega 2 balloon.

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