Zobrazeno 1 - 10
of 47
pro vyhledávání: '"LiCan Shan"'
Autor:
Yang Wang, Jun Zhong, James Slavin, Hui Zhang, Lou‐Chuang Lee, Lican Shan, Zhaojin Rong, Yong Wei, Yongxin Pan
Publikováno v:
Geophysical Research Letters, Vol 50, Iss 10, Pp n/a-n/a (2023)
Abstract This paper reports on the standing whistler waves upstream of Mercury's quasi‐perpendicular bow shock. Using MESSENGER's magnetometer data, 36 wave events were identified during interplanetary coronal mass ejections (ICMEs). These elliptic
Externí odkaz:
https://doaj.org/article/6521eac7f07d47c4af0c61669c36da15
Autor:
Di Liu, ZhongHua Yao, Yong Wei, ZhaoJin Rong, LiCan Shan, Stiepen Arnaud, Espley Jared, HanYing Wei, WeiXing Wan
Publikováno v:
Earth and Planetary Physics, Vol 4, Iss 1, Pp 51-61 (2020)
Proton cyclotron waves (PCWs) can be generated by ion pickup of Martian exospheric particles in the solar wind. The solar wind ion pickup process is highly dependent on the “IMF cone angle” — the angle between the solar wind velocity and the in
Externí odkaz:
https://doaj.org/article/c276f09dcaaa4927b62137b7b99f0908
Publikováno v:
Earth and Planetary Physics, Vol 4, Iss 1, Pp 45-50 (2020)
Foreshock ultralow frequency (ULF) waves constitute a significant physical phenomenon in the plasma environment of terrestrial planets. The occurrence of these waves, associated with backstreaming particles reflected and accelerated at the bow shock,
Externí odkaz:
https://doaj.org/article/fd842e8d3c6744d5b5e42655d3f1d003
Autor:
Rajkumar Hajra, Bruce T. Tsurutani, Quanming Lu, Lican Shan, Aimin Du, Rongsheng Wang, San Lu, Xinliang Gao
Publikováno v:
The Astrophysical Journal, Vol 955, Iss 2, p 120 (2023)
From the Ulysses observation of the solar wind between the heliocentric distance r _h of ∼1.0 and ∼5.4 au during 1990–2009, we identified 53 intervals when the solar wind exhibited extreme rarefaction, ∼2 orders of magnitude decreases in the
Externí odkaz:
https://doaj.org/article/fc43bd9064c847ebb09c1157a78546e7
Publikováno v:
The Astrophysical Journal, Vol 954, Iss 1, p 18 (2023)
In this paper, we use a 1D particle-in-cell simulation code to study particle preaccelerations at a high Mach number perpendicular shock. Our simulation results show that almost all of the injected particles can be reflected at the shock front, and t
Externí odkaz:
https://doaj.org/article/6a961fc532184bf19c2c2702f5f03625
Autor:
Guo Chen, Can Huang, Ying Zhang, Yasong Ge, Aimin Du, Rongsheng Wang, Lei Wang, Lican Shan, Christian Mazelle, Hao Luo
Publikováno v:
The Astrophysical Journal, Vol 952, Iss 1, p 37 (2023)
Magnetic reconnection between neighboring magnetic field loops, the so-called interloop reconnection, is a common process to drive flares in the solar atmosphere. However, there is no direct evidence that a similar but less explosive process can take
Externí odkaz:
https://doaj.org/article/9cdef15a1fc7406eba404897270c310f
Publikováno v:
The Astrophysical Journal, Vol 951, Iss 1, p 75 (2023)
The Helios 1 (H1) and Helios 2 (H2) spacecraft measured the solar winds at a distance between ∼0.3 and 1.0 au from the Sun. With increasing heliocentric distance ( r _h ), the plasma speed is found to increase at ∼34–40 km s ^−1 au ^−1 and
Externí odkaz:
https://doaj.org/article/55cda9be3ba44cfcaee2d65b453cb0fe
Autor:
Yang Wang, Jun Zhong, James A. Slavin, Hui Zhang, Lou-Chuang Lee, Lican Shan, Yong Wei, Yongxin Pan
This paper reports on the standing whistler waves upstream of Mercury’s quasi-perpendicular bow shock. Using MESSENGER’s magnetometer data, 36 wave events were identified during interplanetary coronal mass ejections (ICMEs). These elliptic or cir
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::0f61562bdecd65fc5fc164d5bcca6ccb
https://doi.org/10.22541/essoar.167126052.21274720/v1
https://doi.org/10.22541/essoar.167126052.21274720/v1
Autor:
Espley Jared, Zhaojin Rong, Yong Wei, Stiepen Arnaud, Weixing Wan, Lican Shan, Zhonghua Yao, Di Liu, Hanying Wei
Publikováno v:
Earth and Planetary Physics. 4:1-11
Proton cyclotron waves (PCWs) can be generated by ion pickup of Martian exospheric particles in the solar wind. The solar wind ion pickup process is highly dependent on the “IMF cone angle” — the angle between the solar wind velocity and the in
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::875b4ba08145b465c533435d5b7cdf01
https://doi.org/10.26464/epp2020002
https://doi.org/10.26464/epp2020002
Autor:
Bruce T. Tsurutani, Pierre Henri, Lican Shan, Quanming Lu, Can Huang, Karl-Heinz Glassmeier, Aimin Du, Christian Mazelle, Yasong Ge
Publikováno v:
22nd EGU General Assembly
22nd EGU General Assembly, 2020, Online, France. ⟨10.5194/egusphere-egu2020-1508⟩
22nd EGU General Assembly, 2020, Online, France. ⟨10.5194/egusphere-egu2020-1508⟩
Collisionless plasma shocks (CPSs), forming when supersonic plasma streams encounter a magnetized obstacle, are invoked to explain the acceleration of ubiquitously energetic cosmic rays. It has long been theorized from magnetohydrodynamics, but not d
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8ae18d77405945ed1964d11a86473a38
https://doi.org/10.5194/egusphere-egu2020-1508
https://doi.org/10.5194/egusphere-egu2020-1508