Ionospheric electrons in Titan's tail: Plasma structure during the cassini T9 encounter

被引:73
作者
Coates, A. J.
Crary, F. J.
Young, D. T.
Szego, K.
Arridge, C. S.
Bebesi, Z.
Sittler, E. C., Jr.
Hartle, R. E.
Hill, T. W.
机构
[1] UCL, Mullard Space Sci Lab, London WC1E 6BT, England
[2] SW Res Inst, Space Sci & Engn, San Antonio, TX 78228 USA
[3] Hungarian Acad Sci, Cent Re Inst Phys, Res Inst Particle & Nucl Phys, Budapest, Hungary
[4] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA
[5] Rice Univ, Dept Phys & Astron, Houston, TX 77005 USA
关键词
D O I
10.1029/2007GL030919
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
We present results from the CAPS electron spectrometer obtained during the downstream flyby of Titan on 26 December 2005, which occurred during a period of enhanced plasma pressure inside the magnetosphere. The electron data show an unusual split signature with two principal intervals of interest outside the nominal corotation wake. Interval 1 shows direct evidence for ionospheric plasma escape at several RT in Titan's tail. Interval 2 shows a complex plasma structure, a mix between plasma of ionospheric and magnetospheric origin. We suggest a mechanism for plasma escape based on ambipolar electric fields set up by suprathermal ionospheric photoelectrons.
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页数:6
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