STRUCTURE OF VENUS ATMOSPHERE FROM MODELING OF NIGHT-SIDE INFRARED-SPECTRA
The surface and lower atmosphere of Venus lie below long path-lengths of carbon dioxide and water vapour, and thick cloud layers that were, until recently, thought to be essentially opaque to electromagnetic radiation at wavelengths shorter than a few millimetres. It was unexpected, therefore, when...
| Asıl Yazarlar: | , , |
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| Materyal Türü: | Journal article |
| Dil: | English |
| Baskı/Yayın Bilgisi: |
1988
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