Zobrazeno 1 - 3
of 3
pro vyhledávání: '"ZongShun Yue"'
Autor:
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
Publikováno v:
Earth and Planetary Physics, Vol 5, Iss 1, Pp 63-72 (2021)
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
Externí odkaz:
https://doaj.org/article/47e6f28721aa44a58d2c1bf3a403a3b5
Autor:
Alexander W. Degeling, Quanqi Shi, Qiugang Zong, Anmin Tian, Xu-Zhi Zhou, Y. Y. Liu, Ruilong Guo, Zhonghua Yao, Andrew Vu, Jing-Huan Li, Ji Liu, Zongshun Yue, Weijie Sun, Hongqiao Hu, Hui Zhang, Wenya Li, Huishan Fu, Shutao Yao
Publikováno v:
Earth and Planetary Physics. 5:63-72
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
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::662d03707064920419382fca961d9f9f
https://doi.org/10.26464/epp2021011
https://doi.org/10.26464/epp2021011
Kinetic- scale magnetic hole (KSMH) is a kind of structure whose spatial scale is only or smaller than the ion gyroradius and the magnetic field intensity shows rapid decrease in the observation. Recently, with the improvement of high spatio-temporal
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::81832a54cecfaf79bf51299425f96507
https://doi.org/10.5194/egusphere-egu21-14077
https://doi.org/10.5194/egusphere-egu21-14077
