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Observational connection between local high-temperature phenomena within magnetic clouds and the Sun

Observational connection between local high-temperature phenomena within magnetic clouds and the Sun

作     者:WANG JieMin FENG HengQiang 

作者机构:Institute of Space Physics Luoyang Normal University 

出 版 物:《Science China Earth Sciences》 (中国科学(地球科学英文版))

年 卷 期:2016年第59卷第5期

页      面:1051-1056页

核心收录:

学科分类:070802[理学-空间物理学] 07[理学] 0708[理学-地球物理学] 

基  金:supported by the National Natural Science Foundation of China (Grant Nos. 41274180 & 41231068) the Program for Science and Technology Innovation Research Team in University of Henan Province (Grant No. 13IRTSTHN020) 

主  题:Magnetic cloud Ion ionization state High temperature proton 

摘      要:Magnetic clouds(MCs) frequently show abnormal high-ionization states of heavy ions. The abnormal high-charge distributions are related to the coronal temperature of their source regions. We examined the plasma and magnetic field data of 74 MCs observed by the Advanced Composition Explorer from February 1998 to December 2008. We determined that 14 of the 74 events showed local high-temperature phenomena. We analyzed the correlation between proton temperature and O7/O6ratio(or high mean Fe charge state ?Fe?) within the local high-temperature regions in the 14 MCs. Results show that proton temperature and O7/O6 ratio(or high mean Fe charge state) had good correlations in nine MCs, but had no evident correlation in the other five MCs. The local high-temperature phenomena within the nine MCs have resulted from the Sun.

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