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Statistical study of magnetotail flux ropes near the lunar orbit 总被引:1,自引:0,他引:1
SiQi Zhao AnMin Tian QuanQi Shi ChiJie Xiao SuiYan Fu QiuGang Zong HuiZi Wang Shuai Zhang ShaoJie Zhao DongXiao Pan ShangChun Teng YiXing Liu Kun Tan 《中国科学:技术科学(英文版)》2016,59(10):1591-1596
Flux-rope/TCR events near the magnetotail lunar orbit(-67R_E GSM X* -39RE) were studied using magnetic-field and plasma data measured by THEMIS B and C between January 2011 and March 2012. The aberrant coordinate GSM*, where the X* axis is rotated 4° relative to GSM-X, was used to count the occurrence rate. The number ratio of earthward to tailward events was about 3:5. Moreover, the event occurrence rate distribution showed a clear dawn-dusk asymmetry distribution, with dusk-side events accounting for 57.98%. A superposed epoch analysis of the flux-rope events showed that earthward events had a shorter duration in the leading than in the trailing part. Earthward events also displayed a lower temperature and a lower flow speed than tailward events. We studied the relationship between the event occurrence rate and geomagnetic activity level even further. The occurrence rate of tailward flux-rope/TCR events increases with increasing AE-index, whereas earthward events occur mainly in the relatively quiet period of geomagnetic activity(AE ~ 100–300 n T). Flux-rope/TCR events identified within a 10 mm time frame were treated as belonging to a single reconnection event. By comparing the occurrence rates of earthward and tailward events along X*, we estimated the most likely location of the near-Earth reconnection site as X* = -36R_E. 相似文献
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介绍田庄选煤厂内部生产调控中采用灰分快速测定方法,并运用成对对比法对其应用情况进行分析;阐述了方法的可行性,为同类厂提供参考。 相似文献
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