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pTC-1 observation of ion high-speed flow reversal in the near-Earth plasma sheet during substorm

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【作者】 H. RMEI. DANDOURASC. M. CARR

【Author】 DUAN SuPing1, LIU ZhenXing1, CAO JinBin1, LU Li1, H. RME2, I. DANDOURAS2 & C. M. CARR3 1 State Key Laboratory of Space Weather, Center for Space Science and Applied Research, Chinese Academy of Sciences, Beijing 100190, China; 2 Centre d’Etude Spatiale des Rayonnements, CEDEX 4, F-31028 Toulouse, France; 3 The Blackett Laboratory, Imperial College London, SW7 2BW, UK

【机构】 Centre d’Etude Spatiale des Rayonnements, CEDEX 4, F-31028 Toulouse, FranceCentre d’Etude Spatiale des Rayonnements, CEDEX 4, F-31028 Toulouse, FranceThe Blackett Laboratory, Imperial College London, SW7 2BW, UK

【摘要】 Based on measurements of FGM and HIA on board TC-1 at its apogee on Septem-ber 14, 2004, we analyzed the ion high-speed flows in the near-Earth plasma sheet observed during the substorm expansion phase. Strong tailward high-speed flows (Vx ~ -350 km/s) were first seen at about X ~ -13.2 RE in near-Earth magnetotail, one minute later the flows reversed from tailward to earthward. The reversal process occurred quickly after the substorm expansion onset. The near-Earth magnetotail plasma sheet was one of key regions for substorm onset. Our analysis showed that the ion flow reversal from tailward to earthward was likely to be in close relation with the substorm expansion initiation and might play an important role in trigger-ing the substorm expansion onset.

【Abstract】 Based on measurements of FGM and HIA on board TC-1 at its apogee on Septem-ber 14, 2004, we analyzed the ion high-speed flows in the near-Earth plasma sheet observed during the substorm expansion phase. Strong tailward high-speed flows (Vx ~ -350 km/s) were first seen at about X ~ -13.2 RE in near-Earth magnetotail, one minute later the flows reversed from tailward to earthward. The reversal process occurred quickly after the substorm expansion onset. The near-Earth magnetotail plasma sheet was one of key regions for substorm onset. Our analysis showed that the ion flow reversal from tailward to earthward was likely to be in close relation with the substorm expansion initiation and might play an important role in trigger-ing the substorm expansion onset.

【基金】 the National Natural Science Foundation of China (Grant Nos. 40620130094, 40731054, 40704027, 40390150)
  • 【文献出处】 Science in China(Series E:Technological Sciences) ,中国科学(E辑:技术科学)(英文版) , 编辑部邮箱 ,2008年10期
  • 【分类号】P353
  • 【被引频次】2
  • 【下载频次】12
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