Titan's ionosphere in the magnetosheath: Cassini RPWS results during the T32 flyby

被引:22
作者
Garnier, P. [1 ,2 ,3 ]
Wahlund, J-E. [1 ]
Rosenqvist, L. [1 ]
Modolo, R. [1 ]
Agren, K. [1 ]
Sergis, N. [4 ]
Canu, P. [5 ]
Andre, M. [1 ]
Gurnett, D. A. [6 ]
Kurth, W. S. [6 ]
Krimigis, S. M. [7 ]
Coates, A. [8 ]
Dougherty, M. [9 ]
Waite, J. H. [10 ]
机构
[1] Swedish Inst Space Phys, S-75121 Uppsala, Sweden
[2] Univ Toulouse, UPS, CESR, F-31028 Toulouse 9, France
[3] CNRS, UMR5187, F-31028 Toulouse, France
[4] Acad Athens, Off Space Res & Applicat, Athens, Greece
[5] Inst Pierre Simon Laplace, Ctr Etud Environm Terr & Planetaires, Velizy Villacoublay, France
[6] Univ Iowa, Dept Phys & Astron, Iowa City, IA 52242 USA
[7] Johns Hopkins Univ, Appl Phys Lab, Laurel, MD USA
[8] Univ Coll London, Mullard Space Sci Lab, Dorking RH5 6NT, Surrey, England
[9] Univ London Imperial Coll Sci Technol & Med, Space & Atmospher Phys Grp, London SW7 2AZ, England
[10] SW Res Inst, Space Sci & Engn Div, San Antonio, TX 78228 USA
基金
英国科学技术设施理事会;
关键词
Ionosphere; Ionospheric irregularities; Planetary ionospheres; Magnetospheric physics; Magnetosheath; UPPER-ATMOSPHERE; PLASMA; ION; MODEL; SPECTROMETER; CHEMISTRY; VENUS; MAGNETOSPHERE; SATURN; MIMI;
D O I
10.5194/angeo-27-4257-2009
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The Cassini mission has provided much information about the Titan environment, with numerous low altitude encounters with the moon being always inside the magnetosphere. The only encounter taking place outside the magnetopause, in the magnetosheath, occurred the 13 June 2007 (T32 flyby). This paper is dedicated to the analysis of the Radio and Plasma Wave investigation data during this specific encounter, in particular with the Langmuir probe, providing a detailed picture of the cold plasma environment and of Titan's ionosphere with these unique plasma conditions. The various pressure terms were also calculated during the flyby. The comparison with the T30 flyby, whose geometry was very similar to the T32 encounter but where Titan was immersed in the kronian magnetosphere, reveals that the evolution of the incident plasma has a significant influence on the structure of the ionosphere, with in particular a change of the exo-ionospheric shape. The electrical conductivities are given along the trajectory of the spacecraft and the discovery of a polar plasma cavity is reported.
引用
收藏
页码:4257 / 4272
页数:16
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