Published March 21, 1986
| public
Journal Article
VEGA Balloon Dynamics and Vertical Winds in the Venus Middle Cloud Region
Chicago
Abstract
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.
Additional Information
© 1986 American Association for the Advancement of Science. Received for publication 23 October 1985. Accepted for publication 24 January 1986. Funding partially by National Aeronautics and Space Administration Ames Research Center and the Jet Propulsion Laboratory.Additional details
- Eprint ID
- 38069
- DOI
- 10.1126/science.231.4744.1417
- Resolver ID
- CaltechAUTHORS:20130423-070919900
- NASA Ames Research Center
- JPL
- Created
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2013-04-23Created from EPrint's datestamp field
- Updated
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2021-11-09Created from EPrint's last_modified field
- Caltech groups
- Division of Geological and Planetary Sciences (GPS)