By comparing observations from the Cassini imaging system, UV spectrometer, and Huygens atmospheric structure instrument, we determine an apparent radius of ∼40 nm, an imaginary index <0.3 at 187.5 nm and a number density of ∼30 particles cm -3 for the detached haze layer at 520 km in Titan's mesosp
✦ LIBER ✦
The evolution of Titan's detached haze layer near equinox in 2009
✍ Scribed by West, Robert A.; Balloch, Jonathan; Dumont, Philip; Lavvas, Panayotis; Lorenz, Ralph; Rannou, Pascal; Ray, Trina; Turtle, Elizabeth P.
- Book ID
- 119680930
- Publisher
- American Geophysical Union
- Year
- 2011
- Tongue
- English
- Weight
- 296 KB
- Volume
- 38
- Category
- Article
- ISSN
- 1944-8007
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