Article ID | Journal | Published Year | Pages | File Type |
---|---|---|---|---|
1773709 | Icarus | 2012 | 12 Pages |
Abstract
⺠Dynamics in the upper atmosphere of Venus by measuring the Doppler shift. ⺠Narrow altitude region in Venus' atmosphere around 110 ± 10 km (1 lbar). ⺠The results show no significant zonal wind velocity at the equator. ⺠An increase with latitude up to 43 ± 13 m/s at a latitude of 33N was observed. ⺠Maximum cross terminator velocity of the sub-solar-to-antisolar flow at 72 ± 47 m/s.
Related Topics
Physical Sciences and Engineering
Earth and Planetary Sciences
Space and Planetary Science
Authors
M. Sornig, T.A. Livengood, G. Sonnabend, D. Stupar, P. Kroetz,