Zobrazeno 1 - 10
of 331
pro vyhledávání: '"B. B. Tang"'
Autor:
W. Y. Li, D. B. Graham, Yu. V. Khotyaintsev, A. Vaivads, M. André, K. Min, K. Liu, B. B. Tang, C. Wang, K. Fujimoto, C. Norgren, S. Toledo-Redondo, P.-A. Lindqvist, R. E. Ergun, R. B. Torbert, A. C. Rager, J. C. Dorelli, D. J. Gershman, B. L. Giles, B. Lavraud, F. Plaschke, W. Magnes, O. Le Contel, C. T. Russell, J. L. Burch
Publikováno v:
Nature Communications, Vol 11, Iss 1, Pp 1-10 (2020)
Various types of plasma waves are generated around electron diffusion regions (EDRs). Here the authors show electron Bernstein waves (EBWs), at the electron-scale boundary of the Hall current reversal near EDR, are sufficiently strong to diffuse elec
Externí odkaz:
https://doaj.org/article/e3975f2c57c342b79a8fb72f9c6fd91f
Autor:
B. B. Tang, W. Y. Li, C. Wang, Yu. V. Khotyaintsev, D. B. Graham, Q. H. Zhang, T. R. Sun, H. Li, X. Y. Wang, K. J. Trattner, B. L. Giles, P. A. Lindqvist, R. E. Ergun, J. L. Burch
Publikováno v:
Frontiers in Astronomy and Space Sciences, Vol 8 (2021)
We report local secondary magnetic reconnection at Earth’s flank magnetopause by using the Magnetospheric Multiscale observations. This reconnection is found at the magnetopause boundary with a large magnetic shear between closed magnetospheric fie
Externí odkaz:
https://doaj.org/article/8e5cdfc527ea47028953af4cd42a7388
Publikováno v:
Annales Geophysicae, Vol 31, Pp 489-501 (2013)
We employ a global magnetohydrodynamics (MHD) model, namely the PPMLR-MHD model, to investigate the effect of the solar wind conditions, such as the interplanetary magnetic field (IMF) clock angle, southward IMF magnitude and solar wind speed, on
Externí odkaz:
https://doaj.org/article/f0cec0765ff544cdafbdc851d455af5a
Autor:
H.‐W. Wang, B.‐B. Tang, W. Y. Li, Y.‐C. Zhang, D. B. Graham, Y. V. Khotyaintsev, C.‐H. Gao, X.‐C. Guo, C. Wang
Publikováno v:
Geophysical Research Letters, Vol 50, Iss 10, Pp n/a-n/a (2023)
Abstract In this study, we investigate detailed electron dynamics in strong guide‐field reconnection (the normalized guide field is ∼1.5). This reconnection event is observed by the Magnetospheric Multiscale (MMS) spacecraft at the center of a fl
Externí odkaz:
https://doaj.org/article/b2ecab0f443d4051a93b61d4c05a9c40
Autor:
C.‐H. Gao, B.‐B. Tang, X.‐C. Guo, W. Y. Li, Y. V. Khotyaintsev, D. B. Graham, D. L. Turner, Z. W. Yang, C. Wang
Publikováno v:
Geophysical Research Letters, Vol 50, Iss 4, Pp n/a-n/a (2023)
Abstract Agyrotropic electron distributions are frequently taken as an indicator of electron diffusion regions of magnetic reconnection. However, they have also been found at electron‐scale boundaries of the non‐reconnecting magnetopause and are
Externí odkaz:
https://doaj.org/article/54303b0ba02f44e28a63db63b6c30b8a
Autor:
W.‐Y. Li, Yu V. Khotyaintsev, B.‐B. Tang, D. B. Graham, C. Norgren, A. Vaivads, M. André, A. Le, J. Egedal, K. Dokgo, K. Fujimoto, J.‐S. He, J. L. Burch, P.‐A. Lindqvist, R. E. Ergun, R. B. Torbert, O. Le Contel, D. J. Gershman, B. L. Giles, B. Lavraud, S. Fuselier, F. Plaschke, C. T. Russell, X.‐C. Guo, Q.‐M. Lu, C. Wang
Publikováno v:
Geophysical Research Letters, Vol 48, Iss 16, Pp n/a-n/a (2021)
Abstract Magnetic reconnection is a fundamental process in collisionless space plasma environment, and plasma waves relevant to the kinetic interactions can have a significant impact on the multiscale behavior of reconnection. Here, we present Magnet
Externí odkaz:
https://doaj.org/article/e8f4972c5c134bedad1b188c3eb7b21e
Akademický článek
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Akademický článek
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Autor:
B.‐B. Tang, W. Y. Li, Yu. V. Khotyaintsev, D. B. Graham, C. H. Gao, Z. Z. Chen, H. S. Fu, Q. M. Lu, C. Wang, J. L. Burch
Publikováno v:
Geophysical Research Letters. 49
Autor:
L, Cai, H J, Zhang, F L, He, Y Y, Feng, S X, Hu, J, Wang, F Q, Liu, Y L, Jiang, X L, Tan, H M, Pan, B B, Tang, H, Yang, H Y, Long, Z F, Zhan, L D, Gao
Publikováno v:
Zhonghua liu xing bing xue za zhi = Zhonghua liuxingbingxue zazhi. 41(12)