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Analysis of the Distribution,Rotation and Scale Characteristics of Solar Wind Switchbacks:Comparison between the First and Second Encounters of Parker Solar Probe

Analysis of the Distribution, Rotation and Scale Characteristics of Solar Wind Switchbacks: Comparison between the First and Second Encounters of Parker Solar Probe

作     者:Ming-Ming Meng Ying D.Liu Chong Chen Rui Wang Ming-Ming Meng;Ying D.Liu;Chong Chen;Rui Wang

作者机构:State Key Laboratory of Space WeatherNational Space Science CenterChinese Academy of SciencesBeijing 100190China University of Chinese Academy of SciencesBeijing 100049China 

出 版 物:《Research in Astronomy and Astrophysics》 (天文和天体物理学研究(英文版))

年 卷 期:2022年第22卷第3期

页      面:178-185页

核心收录:

学科分类:08[工学] 082503[工学-航空宇航制造工程] 0825[工学-航空宇航科学与技术] 

基  金:supported by NSFC under Grant Nos.41774179 and 12073032 Beijing Municipal Science and Technology Commission(Z191100004319003) the Specialized Research Fund for State Key Laboratories of China 

主  题:ISM:magnetic fields methods:statistical (Sun:)solar wind 

摘      要:The S-shaped magnetic structure in the solar wind formed by the twisting of magnetic field lines is called a switchback,whose main characteristics are the reversal of the magnetic field and the significant increase in the solar wind radial *** identify 242 switchbacks during the first two encounters of Parker Solar *** methods are applied to analyze the distribution and the rotation angle and direction of the magnetic field rotation of the *** diameter of switchbacks is estimated with a minimum variance analysis(MVA)method based on the assumption of a cylindrical magnetic *** also make a comparison between switchbacks from inside and the boundary of coronal *** main conclusions are as follows:(1)the rotation angles of switchbacks observed during the first encounter seem larger than those of the switchbacks observed during the second encounter in general;(2)the tangential component of the velocity inside the switchbacks tends to be more positive(westward)than in the ambient solar wind;(3)switchbacks are more likely to rotate clockwise than counterclockwise,and the number of switchbacks with clockwise rotation is 1.48 and 2.65 times those with counterclockwise rotation during the first and second encounters,respectively;(4)the diameter of switchbacks is about 10;km on average and across five orders of magnitude(10^(3)–10^(7)km).

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