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  5. Effects of the surface conductivity and IMF strength on dynamics of planetary ions in Mercury's

Effects of the surface conductivity and IMF strength on dynamics of planetary ions in Mercury's

来源 :International Symposium & Summer School on Planetary Science | 被引量 : 0次 | 上传用户：xin__yonghu
【摘 要】
：
A previous study of ion dynamics in the Mercurys magnetosphere, which uses a rescaled analytical model of the geomagnetic and electric fields for Mercury, shows that non-adiabatic motion of ions in th
【作 者】
：
K.SEKI N.TERADA M.YAGI D.C.DELCOURT F.LEBLANC T.OGINO 
【机 构】
：
Solar-Terrestrial Environment Laboratory,Nagoya University,Aichi 464-8601,Japan
【出 处】
：
International Symposium & Summer School on Planetary Science
【发表日期】
：
2013年4期
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　　A previous study of ion dynamics in the Mercurys magnetosphere, which uses a rescaled analytical model of the geomagnetic and electric fields for Mercury, shows that non-adiabatic motion of ions in the magnetotail can cause a narrow band of energetic (several keV) Na+ precipitation in each hemisphere [Delcourt et al., 2003].On the other hand, it is not evident that the magnetospheric configuration and global convection pattern in the Mercurys magnetosphere can be described with the rescaled geomagnetospheric model.
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