Coates Andrew J
Mullard Space Science Laboratory, University College London, Holmbury St Mary, Dorking RH5 6NT, UK.
Philos Trans A Math Phys Eng Sci. 2009 Feb 28;367(1889):773-88. doi: 10.1098/rsta.2008.0248.
Titan is the only Moon in the Solar System with a significant permanent atmosphere. Within this nitrogen-methane atmosphere, an ionosphere forms. Titan has no significant magnetic dipole moment, and is usually located inside Saturn's magnetosphere. Atmospheric particles are ionized both by sunlight and by particles from Saturn's magnetosphere, mainly electrons, which reach the top of the atmosphere. So far, the Cassini spacecraft has made over 45 close flybys of Titan, allowing measurements in the ionosphere and the surrounding magnetosphere under different conditions. Here we review how Titan's ionosphere and Saturn's magnetosphere interact, using measurements from Cassini low-energy particle detectors. In particular, we discuss ionization processes and ionospheric photoelectrons, including their effect on ion escape from the ionosphere. We also discuss one of the unexpected discoveries in Titan's ionosphere, the existence of extremely heavy negative ions up to 10000amu at 950km altitude.
土卫六是太阳系中唯一拥有显著永久大气层的卫星。在这种氮 - 甲烷大气层中,会形成一个电离层。土卫六没有显著的磁偶极矩,并且通常位于土星的磁层内部。大气粒子会被太阳光以及来自土星磁层的粒子(主要是电子,这些电子会到达大气层顶部)电离。到目前为止,卡西尼号航天器已经对土卫六进行了超过45次近距离飞越,从而能够在不同条件下对电离层和周围磁层进行测量。在这里,我们利用卡西尼号低能粒子探测器的测量结果,回顾土卫六电离层与土星磁层是如何相互作用的。特别是,我们讨论了电离过程和电离层光电子,包括它们对离子从电离层逃逸的影响。我们还讨论了土卫六电离层中一个意外发现,即在950千米高度存在质量高达10000原子质量单位的极重负离子。