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Cluster observations of high-altitude cusp during multiple fast-turning IMF
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作者 CaI HongTao Ma ShuYing +3 位作者 DUNLOP M W BOGDaNOVa Y davies j a PITOUT F 《Chinese Science Bulletin》 SCIE EI CAS 2010年第12期1178-1185,共8页
Using coordinated observations from the Cluster,DMSP and ESR radar,high-altitude cusp was investigated for a time period characterized by four fast reversals of the IMF BZ.On February 12,2003,Cluster was flying sunwar... Using coordinated observations from the Cluster,DMSP and ESR radar,high-altitude cusp was investigated for a time period characterized by four fast reversals of the IMF BZ.On February 12,2003,Cluster was flying sunward at duskside over the Northern Hemisphere,across the high-altitude northern cusp twice.Both the two crossings are during steady northward IMF interval,whereas ion fluxes detected during the time period are quite different.The cusp in the first crossing is a "typical" northward-IMF one,with short-lived ion injections of evident "reversed" dispersion signatures.In the second crossing,however,the cusp appears to be a region reminiscent of the Stagnant Exterior Cusp (SEC).In addition,evident upward-flowing O+ ion bursts,possibly original from polar ionosphere,are also detected during the second cusp crossing,together with enhancement of trapped magnetospheric-like electron fluxes.We suggest that the SEC-like cusp is likely on newly closed field lines,which were first reconnected (being opened) at low latitudes and later reconnected again (being closed) poleward of the northern cusp. 展开更多
关键词 国际货币基金组织 高海拔 群集 观测 十字路口 离子检测 低纬度地区 气象卫星
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IMF Bz多次快速反向期间极尖区的Cluster观测
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作者 蔡红涛 马淑英 +3 位作者 Dunlop M W Bogdanova Y davies j a Pitout F 《科学通报》 EI CAS CSCD 北大核心 2009年第22期3582-3582,共1页
2003年2月12日,ACE卫星观测到IMFBz分量的4次快速反向:从稳定的北向(Bz~9nT)快速转为稳定的南向(Bz~-8nT);在持续南向约34min后Bz再次转为稳定北向(Bz-5nT);约22min后,ACE卫星观测到南向的IMF;IMF保持南向约46min后第二次... 2003年2月12日,ACE卫星观测到IMFBz分量的4次快速反向:从稳定的北向(Bz~9nT)快速转为稳定的南向(Bz~-8nT);在持续南向约34min后Bz再次转为稳定北向(Bz-5nT);约22min后,ACE卫星观测到南向的IMF;IMF保持南向约46min后第二次转回稳定的北向(Bz-6nT). 展开更多
关键词 卫星观测 CLUSTER IMF 反向 极尖区 ACE 稳定 Z分量
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