By comparing observations from the Cassini imaging system, UV spectrometer, and Huygens atmospheric structure instrument, we determine an apparent radius of βΌ40 nm, an imaginary index <0.3 at 187.5 nm and a number density of βΌ30 particles cm -3 for the detached haze layer at 520 km in Titan's mesosp
β¦ LIBER β¦
A tidal explanation for the Titan haze layers
β Scribed by Richard L. Walterscheid; Gerald Schubert
- Book ID
- 108138672
- Publisher
- Elsevier Science
- Year
- 2006
- Tongue
- English
- Weight
- 189 KB
- Volume
- 183
- Category
- Article
- ISSN
- 0019-1035
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