タイトル | Ultraviolet observations of Titan from OAO-2 |
本文(外部サイト) | http://hdl.handle.net/2060/19740012374 |
著者(英) | Caldwell, J. J. |
著者所属(英) | Princeton Univ. |
発行日 | 1974-01-01 |
言語 | eng |
内容記述 | High altitude deposition of energy in Titan's atmosphere can have a significant effect on the spectral distribution of emitted thermal radiation from the satellite. This reasoning led to the prediction of emission peaks at wavelengths corresponding to allowed bands of CH4 and trace photolysis products such as C2H6. Intermediate resolution infrared spectrophotometry has encouraged this interpretation of the infrared properties of Titan, and provided the basis for initial, detailed model. |
NASA分類 | SPACE SCIENCES |
レポートNO | 74N20487 |
権利 | No Copyright |
URI | https://repository.exst.jaxa.jp/dspace/handle/a-is/570468 |
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