Wind Streaks on Venus: Clues to Atmospheric Circulation
Hadley cell
Streak
Atmospheric Circulation
Global wind patterns
Atmosphere of Venus
DOI:
10.1126/science.263.5145.358
Publication Date:
2006-10-06T00:01:25Z
AUTHORS (8)
ABSTRACT
Magellan images reveal surface features on Venus attributed to wind processes. Sand dunes, wind-sculpted hills, and more than 5830 streaks have been identified. The serve as local "wind vanes," representing direction at the time of streak formation allowing first global mapping near-surface patterns Venus. Wind are oriented both toward equator west. When associated with transient events, such impact cratering, deleted, westward component is mostly lost but equatorward remains. This pattern consistent a Hadley circulation lower atmosphere.
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