Ion Neutral Mass Spectrometer results from the first flyby of Titan

J. Hunter Waite, Hasso Niemann, Roger V. Yelle, Wayne T. Kasprzak, Thomas E. Cravens, Janet G. Luhmann, Ralph L. McNutt, Wing Huen Ip, David Gell, Virginie De La Haye, Ingo Müller-Wordag, Brian Magee, Nathan Borggren, Steve Ledvina, Greg Fletcher, Erin Walter, Ryan Miller, Stefan Scherer, Rob Thorpe, Jing XuBruce Block, Ken Arnett

研究成果: 雜誌貢獻期刊論文同行評審

361 引文 斯高帕斯(Scopus)

摘要

The Cassini Ion Neutral Mass Spectrometer (INMS) has obtained the first in situ composition measurements of the neutral densities of molecular nitrogen, methane, molecular hydrogen, argon, and a host of stable carbon-nitrite compounds in Titan's upper atmosphere. INMS in situ mass spectrometry has also provided evidence for atmospheric waves in the upper atmosphere and the first direct measurements of isotopes of nitrogen, carbon, and argon, which reveal interesting clues about the evolution of the atmosphere. The bulk composition and thermal structure of the moon's upper atmosphere do not appear to have changed considerably since the Voyager 1 flyby.

原文???core.languages.en_GB???
頁(從 - 到)982-986
頁數5
期刊Science
308
發行號5724
DOIs
出版狀態已出版 - 13 5月 2005

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