Structured ionospheric outflow during the Cassini T55-T59 Titan flybys

被引：32

作者：

Edberg, N. J. T. ^{[1
]}

Agren, K. ^{[1
]}

Wahlund, J. -E. ^{[1
]}

Morooka, M. W. ^{[1
]}

Andrews, D. J. ^{[2
]}

Cowley, S. W. H. ^{[2
]}

Wellbrock, A. ^{[3
]}

Coates, A. J. ^{[3
]}

Bertucci, C. ^{[4
]}

Dougherty, M. K. ^{[5
]}

机构：

[1] Swedish Inst Space Phys, S-75121 Uppsala, Sweden

[2] Univ Leicester, Dept Phys & Astron, Leicester LE1 7RH, Leics, England

[3] Univ Coll London, Mullard Space Sci Lab, Dorking RH5 6NT, Surrey, England

[4] Inst Astron & Space Phys, Buenos Aires, DF, Argentina

[5] Univ London Imperial Coll Sci Technol & Med, Blackett Lab, Space & Atmospher Phys Grp, London SW7 2BW, England

来源：

PLANETARY AND SPACE SCIENCE | 2011年 / 59卷 / 08期

基金：

瑞典研究理事会;

关键词：

Cassini; Titan; Atmospheric escape; Ionosphere; KINETIC ALFVEN WAVES; HYBRID SIMULATION; PLASMA ENVIRONMENT; UPPER-ATMOSPHERE; ION CHEMISTRY; VENUS; ESCAPE; MAGNETOSPHERE; DENSITY; RADIO;

D O I：

10.1016/j.pss.2011.03.007

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

During the final three of the five consecutive and similar Cassini Titan flybys T55-T59 we observe a region characterized by high plasma densities (electron densities of 1-8 cm(-3)) in the tail/nightside of Titan. This region is observed progressively farther downtail from pass to pass and is interpreted as a plume of ionospheric plasma escaping Titan, which appears steady in both location and time. The ions in this plasma plume are moving in the direction away from Titan and are a mixture of both light and heavy ions with composition revealing that their origin are in Titan's ionosphere, while the electrons are more isotropically distributed. Magnetic field measurements indicate the presence of a current sheet at the inner edge of this region. We discuss the mechanisms behind this outflow, and suggest that it could be caused by ambipolar diffusion, magnetic moment pumping or dispersive Alfven waves. (C) 2011 Elsevier Ltd. All rights reserved.

引用

页码：788 / 797

页数：10

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