Zobrazeno 1 - 9
of 9
pro vyhledávání: '"Shimou Wang"'
Publikováno v:
Magnetochemistry, Vol 10, Iss 11, p 89 (2024)
We report the Magnetospheric Multiscale (MMS) observation of a bifurcated reconnecting current sheet in Earth’s dayside magnetosheath. Typical signatures of the ion diffusion region, including sub-Alfvénic demagnetized ion outflow, super-Alfvénic
Externí odkaz:
https://doaj.org/article/c2b6f95d899c4afe9a05d8d8d541af7e
Publikováno v:
Geophysical Research Letters, Vol 51, Iss 12, Pp n/a-n/a (2024)
Abstract We report in situ observation of magnetic reconnection between magnetic flux rope (MFR) and magnetic hole (MH) in the magnetosheath by the Magnetospheric Multiscale mission. The MFR was rooted in the magnetopause and could be generated by ma
Externí odkaz:
https://doaj.org/article/d5d3a5bbff724f9cab0c4644571f6510
Autor:
Shimou Wang, Rongsheng Wang, Quanming Lu, J. L. Burch, Ian J. Cohen, A. N. Jaynes, R. E. Ergun
Publikováno v:
Geophysical Research Letters, Vol 50, Iss 11, Pp n/a-n/a (2023)
Abstract Two types of filamentary currents (FCs) were observed inside a magnetic flux rope at the magnetopause by the Magnetospheric Multiscale mission. The first FC is identified as an electron vortex, while the other is a reconnecting current sheet
Externí odkaz:
https://doaj.org/article/f9f6fe373e6c41589e0a8a66be25c276
Autor:
Yi Xie, Rongsheng Wang, Xinmin Li, Shimou Wang, Keming Fan, Quanming Lu, Xinliang Gao, San Lu
Publikováno v:
The Astrophysical Journal, Vol 968, Iss 2, p 82 (2024)
Magnetic holes, characterized as magnetic field depressions, have been widely observed in space plasma. Two large-scale magnetic holes, MH1 and MH2, were reported in this paper and the energetic electrons up to 100 keV were detected for the first tim
Externí odkaz:
https://doaj.org/article/b63f5322bee54e62aa436d98830153fb
Publikováno v:
Nature Communications, Vol 11, Iss 1, Pp 1-8 (2020)
Magnetic reconnection is a fundamental plasma process of magnetic energy conversion to kinetic energy. Here, the authors show direct evidence of secondary reconnection in the filamentary currents within the flux ropes indicating a significant contrib
Externí odkaz:
https://doaj.org/article/697cfdadb07b4de1877899028d0bc964
Publikováno v:
The Astrophysical Journal, Vol 955, Iss 1, p 14 (2023)
Recent spacecraft observations have shown that magnetic reconnection occurs commonly in turbulent environments at shocks. At quasi-perpendicular shocks, magnetic field lines are bent by the back-streaming reflected ions, which form a current sheet in
Externí odkaz:
https://doaj.org/article/0faa1009afc843bb88880c236ac7df5b
Publikováno v:
Nature Astronomy. 7:18-28
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::e9f18811686ef4fd33bd86721c1520df
https://doi.org/10.1038/s41550-022-01818-5
https://doi.org/10.1038/s41550-022-01818-5
Turbulent magnetic reconnection was observed in the magnetotail and the magnetopause. In turbulent magnetic reconnection, the diffusion region is filled with a number of filamentary currents primarily carried by the electrons and some flux ropes. The
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::f0db28407f2036732c6afad46b76a45e
https://doi.org/10.5194/egusphere-egu23-2060
https://doi.org/10.5194/egusphere-egu23-2060
Autor:
Shimou Wang1,2,3, Rongsheng Wang1,2,3 rswan@ustc.edu.cn, Quanming Lu1,2,3 qmlu@ustc.edu.cn, Burch, J. L.4, Shui Wang1,2,3
Publikováno v:
Journal of Geophysical Research. Space Physics. Apr2021, Vol. 126 Issue 4, p1-13. 13p.