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- L. D. Travis
- NASA Goddard Institute for Space Studies, Goddard Space Flight Center, New York 10025
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- D. L. Coffeen
- NASA Goddard Institute for Space Studies, Goddard Space Flight Center, New York 10025
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- A. D. Del Genio
- NASA Goddard Institute for Space Studies, Goddard Space Flight Center, New York 10025
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- J. E. Hansen
- NASA Goddard Institute for Space Studies, Goddard Space Flight Center, New York 10025
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- K. Kawabata
- NASA Goddard Institute for Space Studies, Goddard Space Flight Center, New York 10025
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- A. A. Lacis
- NASA Goddard Institute for Space Studies, Goddard Space Flight Center, New York 10025
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- W. A. Lane
- NASA Goddard Institute for Space Studies, Goddard Space Flight Center, New York 10025
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- S. S. Limaye
- NASA Goddard Institute for Space Studies, Goddard Space Flight Center, New York 10025
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- W. B. Rossow
- NASA Goddard Institute for Space Studies, Goddard Space Flight Center, New York 10025
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- P. H. Stone
- Department of Meteorology, Massachusetts Institute of Technology, Cambridge 02139
書誌事項
- 公開日
- 1979-07-06
- DOI
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- 10.1126/science.205.4401.74
- 公開者
- American Association for the Advancement of Science (AAAS)
この論文をさがす
説明
<jats:p>Ultraviolet images of Venus over a 3-month period show marked evolution of the planetary scale features in the cloud patterns. The dark horizontal Y feature recurs quasi-periodically, at intervals of about 4 days, but it has also been absent for periods of several weeks. Bow-shaped features observed in Pioneer Venus images are farther upstream from the subsolar point than those in Mariner 10 images.</jats:p>
収録刊行物
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- Science
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Science 205 (4401), 74-76, 1979-07-06
American Association for the Advancement of Science (AAAS)