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  • 1
    Publication Date: 2005-02-26
    Description: The Magnetospheric Imaging Instrument (MIMI) onboard the Cassini spacecraft observed the saturnian magnetosphere from January 2004 until Saturn orbit insertion (SOI) on 1 July 2004. The MIMI sensors observed frequent energetic particle activity in interplanetary space for several months before SOI. When the imaging sensor was switched to its energetic neutral atom (ENA) operating mode on 20 February 2004, at approximately 10(3) times Saturn's radius RS (0.43 astronomical units), a weak but persistent signal was observed from the magnetosphere. About 10 days before SOI, the magnetosphere exhibited a day-night asymmetry that varied with an approximately 11-hour periodicity. Once Cassini entered the magnetosphere, in situ measurements showed high concentrations of H+, H2+, O+, OH+, and H2O+ and low concentrations of N+. The radial dependence of ion intensity profiles implies neutral gas densities sufficient to produce high loss rates of trapped ions from the middle and inner magnetosphere. ENA imaging has revealed a radiation belt that resides inward of the D ring and is probably the result of double charge exchange between the main radiation belt and the upper layers of Saturn's exosphere.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Krimigis, S M -- Mitchell, D G -- Hamilton, D C -- Krupp, N -- Livi, S -- Roelof, E C -- Dandouras, J -- Armstrong, T P -- Mauk, B H -- Paranicas, C -- Brandt, P C -- Bolton, S -- Cheng, A F -- Choo, T -- Gloeckler, G -- Hayes, J -- Hsieh, K C -- Ip, W-H -- Jaskulek, S -- Keath, E P -- Kirsch, E -- Kusterer, M -- Lagg, A -- Lanzerotti, L J -- Lavallee, D -- Manweiler, J -- McEntire, R W -- Rasmuss, W -- Saur, J -- Turner, F S -- Williams, D J -- Woch, J -- New York, N.Y. -- Science. 2005 Feb 25;307(5713):1270-3.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Applied Physics Laboratory, Johns Hopkins University, Laurel, MD 20723, USA. tom.krimigis@jhuapl.edu〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/15731445" target="_blank"〉PubMed〈/a〉
    Keywords: Atmosphere ; Extraterrestrial Environment ; *Gases ; Hydrogen ; *Ions ; *Magnetics ; Nitrogen ; Oxygen ; *Saturn ; Spacecraft ; Spectrum Analysis ; *Water
    Print ISSN: 0036-8075
    Electronic ISSN: 1095-9203
    Topics: Biology , Chemistry and Pharmacology , Computer Science , Medicine , Natural Sciences in General , Physics
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  • 2
    Publication Date: 2005-05-14
    Description: 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-nitrile 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.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Waite, J Hunter Jr -- Niemann, Hasso -- Yelle, Roger V -- Kasprzak, Wayne T -- Cravens, Thomas E -- Luhmann, Janet G -- McNutt, Ralph L -- Ip, Wing-Huen -- Gell, David -- De La Haye, Virginie -- Muller-Wordag, Ingo -- Magee, Brian -- Borggren, Nathan -- Ledvina, Steve -- Fletcher, Greg -- Walter, Erin -- Miller, Ryan -- Scherer, Stefan -- Thorpe, Rob -- Xu, Jing -- Block, Bruce -- Arnett, Ken -- New York, N.Y. -- Science. 2005 May 13;308(5724):982-6.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Department of Atmospheric, Oceanic, and Space Sciences, University of Michigan, Ann Arbor, MI 48109-2143, USA.〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/15890873" target="_blank"〉PubMed〈/a〉
    Keywords: Argon ; Atmosphere ; Carbon Isotopes ; *Elements ; Evolution, Planetary ; Extraterrestrial Environment ; *Hydrocarbons ; Hydrogen ; Isotopes ; Mass Spectrometry ; Methane ; Nitriles ; Nitrogen ; Nitrogen Isotopes ; *Saturn ; Spacecraft ; Temperature
    Print ISSN: 0036-8075
    Electronic ISSN: 1095-9203
    Topics: Biology , Chemistry and Pharmacology , Computer Science , Medicine , Natural Sciences in General , Physics
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