VEGA balloon dynamics and vertical winds in the Venus middle cloud region

Details VEGA balloon dynamics and vertical winds in the Venus middle cloud region VEGA balloon dynamics and vertical winds in the Venus middle cloud region

Mar 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986sci...231.1417l&link_type=abstract

Science (ISSN 0036-8075), vol. 231, March 21, 1986, p. 1417-1419. NASA-supported research.

Other

27

Balloon Flight, Vega Project, Venus Atmosphere, Venus Clouds, Vertical Air Currents, Wind Profiles, Vertical Distribution, Wind Direction, Wind Velocity Measurement, Venus, Vega 1, Vega 2, Probes, Experiments, Atmosphere, Meteorology, Dynamics, Wind, Clouds, Altitude, Velocity, Procedure, Techniques

Scientific paper

The VEGA balloons provided a long-term record of vertical wind fluctuations in a planetary atmosphere other than Earth's. The vertical winds were calculated from the observed displacement of the balloon relative to its equilibrium float altitude. The winds were intermittent; a large burst lasted several hours, and the peak velocity was 3 meters per second.

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