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- W3149019203 abstract "在 2004 年 7 月 22 日， WIND 太空船检测了典型星际间的震动。在 preshock 区域正在支撑弱向南方的磁场，向南方的领域突然越过吃惊前面被提高(即，向南方的拐弯处) 。当吃惊在磁气圈上侵犯了时，磁电机球的血浆传送对流突然地在中央血浆表被提高，它被位于不同区域的 TC-1 和簇太空船直接观察。同时，簇太空船观察到 dawn-to-dusk 电场突然地被提高。磁场的变化由 TC-1，簇， GOES-10 和 GOES-12 观察到那在血浆表在不同区域被散布，在 geosynchronous，轨道显然是不同的。TC-1 观察证明磁性的紧张保持几乎未改变，举起角度减少了，但是簇太空船，也在血浆表并且从赤道是进一步的，观察到磁场是显然提高了。同时，在午夜附近定位的 GOES-12 观察到磁性的紧张严厉地增加了，举起角度减少了，但是位于黎明方面的 GOES-10 观察到磁场都仅仅严厉地与它的三个部件被压缩增加。而且，在将近隧道由五颗 LANL 卫星观察了的所有的精力充沛的质子和电子流动在所有由于吃惊的压缩看了冲动的改进的不同磁性的本地时间(MLT ) 定位了。精力充沛的粒子的回答比夜面上的那些在行星的光面上是明显的。特别午夜附近的回答是相当弱的。在这篇论文，到上面的观察的可能的合理物理解释也被讨论。所有导致吃惊的回答是太阳的风的联合效果动态压力脉搏和磁场向南方的拐弯处。" @default.
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- W3149019203 date "2009-01-01" @default.
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- W3149019203 title "Responses of properties in the plasma sheet and at the geosynchronous orbit to interplanetary shock" @default.
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