Statistical properties of kinetic-scale magnetic holes in terrestrial space

Statistical properties of kinetic-scale magnetic holes in terrestrial space

Kinetic-scale magnetic holes (KSMHs) are structures characterized by a significant magnetic depression with a length scale on the order of the proton gyroradius. These structures have been investigated in recent studies in near-Earth space, and found to be closely related to energy conversion and pa...

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Bibliographic Details
Main Authors: ShuTao Yao, ZongShun Yue, QuanQi Shi, Alexander William Degeling, HuiShan Fu, AnMin Tian, Hui Zhang, Andrew Vu, RuiLong Guo, ZhongHua Yao, Ji Liu, Qiu-Gang Zong, XuZhi Zhou, JingHuan Li, WenYa Li, HongQiao Hu, YangYang Liu, WeiJie Sun
Format: Article
Language:English
Published: Science Press 2021-01-01
Series:Earth and Planetary Physics
Subjects:
kinetic scale
magnetic hole
magnetic dip
electron vortex
turbulence
Online Access:http://www.eppcgs.org/article/doi/10.26464/epp2021011?pageType=en

Internet

http://www.eppcgs.org/article/doi/10.26464/epp2021011?pageType=en

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