Ion transport in Titan's upper atmosphere
نویسندگان
چکیده
منابع مشابه
Negative ion chemistry in Titan’s upper atmosphere
The Electron Spectrometer (ELS), one of the sensors making up the Cassini Plasma Spectrometer (CAPS) revealed the existence of numerous negative ions in Titan’s upper atmosphere. The observations at closest approach ( 1000 km) show evidence for negatively charged ions up to 10,000 amu/q, as well as two distinct peaks at 2274 and 4478 amu/q, and maybe a third one at 82714 amu/q. We present the f...
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High-energy photons, electrons, and ions initiate ion–neutral chemistry in Titan’s upper atmosphere by ionizing the major neutral species (nitrogen and methane). The Ion and Neutral Mass Spectrometer (INMS) onboard the Cassini spacecraft performed the first composition measurements of Titan’s ionosphere. INMS revealed that Titan has the most compositionally complex ionosphere in the Solar Syste...
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ژورنال
عنوان ژورنال: Journal of Geophysical Research: Space Physics
سال: 2010
ISSN: 0148-0227
DOI: 10.1029/2009ja014563