Zobrazeno 1 - 10
of 16
pro vyhledávání: '"T. K. M. Nakamura"'
Autor:
K. A. Blasl, T. K. M. Nakamura, R. Nakamura, A. Settino, H. Hasegawa, Z. Vörös, M. Hosner, D. Schmid, M. Volwerk, Owen W. Roberts, E. Panov, Yi‐Hsin Liu, F. Plaschke, J. E. Stawarz, J. C. Holmes
Publikováno v:
Geophysical Research Letters, Vol 50, Iss 19, Pp n/a-n/a (2023)
Abstract We present Magnetospheric Multiscale observations of an electron‐scale reconnecting current sheet in the mixing region along the trailing edge of a Kelvin‐Helmholtz vortex during southward interplanetary magnetic field conditions. Within
Externí odkaz:
https://doaj.org/article/d972b5028081418c93ef9b5f658be8a2
Publikováno v:
Frontiers in Astronomy and Space Sciences, Vol 8 (2022)
At the Earth’s low-latitude magnetopause, the Kelvin-Helmholtz (KH) waves, which are driven by the super-Alfvénic velocity shear across the magnetopause, have been frequently observed during periods of northward interplanetary-magnetic-field (IMF)
Externí odkaz:
https://doaj.org/article/29fe4baac0774880a4cd5854d0d780a5
Publikováno v:
The Astrophysical Journal, Vol 947, Iss 1, p 4 (2023)
Coalescence of multiple magnetic islands is recognized as an effective process to energize particles during magnetic reconnection, while its energy conversion process still remains unclear. Here, a two-dimensional fully kinetic simulation of multiple
Externí odkaz:
https://doaj.org/article/313bb607da91480b8374b23cd8653f45
Autor:
K-J. Hwang, K. Dokgo, E. Choi, J. L. Burch, D. G. Sibeck, B. L. Giles, C. Norgren, T. K. M. Nakamura, D. B. Graham, Y. Khotyaintsev, Q. Q. Shi, D. J. Gershman, C. J. Pollock, R. E. Ergun, R. B. Torbert, C. T. Russell, R. J. Strangeway
Publikováno v:
Frontiers in Astronomy and Space Sciences, Vol 8 (2021)
On May 5, 2017 MMS observed a bifurcated current sheet at the boundary of Kelvin-Helmholtz vortices (KHVs) developed on the dawnside tailward magnetopause. We use the event to enhance our understanding of the formation and structure of asymmetric cur
Externí odkaz:
https://doaj.org/article/5c38dee24eaf41a4935ec566bbfd45d5
Publikováno v:
Nature Communications, Vol 8, Iss 1, Pp 1-8 (2017)
Vortex-induced reconnection originates from non-linear vortex flows due to Kelvin-Helmholtz instability in the Earth’s magnetosphere. Here, the authors perform a large-scale kinetic simulation to unveil dynamics of the vortex-induced reconnection a
Externí odkaz:
https://doaj.org/article/bdbaf6a282a3497d8466aed40715e134
Dual-spacecraft reconstruction of a three-dimensional magnetic flux rope at the Earth's magnetopause
Publikováno v:
Annales Geophysicae, Vol 33, Pp 169-184 (2015)
We present the first results of a data analysis method, developed by Sonnerup and Hasegawa (2011), for reconstructing three-dimensional (3-D), magnetohydrostatic structures from data taken as two closely spaced satellites traverse the structures.
Externí odkaz:
https://doaj.org/article/e0b6162ecd18421db613b00379bbf74b
Publikováno v:
Journal of Geophysical Research: Space Physics. 128
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::7e10f6fe85aa85c138b750677bc4751b
https://doi.org/10.1029/2022ja031092
https://doi.org/10.1029/2022ja031092
Publikováno v:
Geophysical Research Letters. 49
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::04983d23a5ce4973150eb6a4958d8a1a
https://doi.org/10.1029/2022gl100652
https://doi.org/10.1029/2022gl100652
Autor:
T. K. M. Nakamura, W.-L. Teh, S. Zenitani, T. Umeda, M. Oka, H. Hasegawa, A. M. Veronig, R. Nakamura
Publikováno v:
Physics of Plasmas. 30:022902
Magnetic reconnection is a key fundamental process in collisionless plasmas, which converts magnetic energy to plasma kinetic energy. Past observation and simulation studies suggested that this process causes an efficient energy conversion through th
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::51bf27726794c786d5a769f8287354eb
https://doi.org/10.1063/5.0127107
https://doi.org/10.1063/5.0127107
Autor:
T. K. M. Nakamura, K. A. Blasl, H. Hasegawa, T. Umeda, Y.-H. Liu, S. A. Peery, F. Plaschke, R. Nakamura, J. C. Holmes, J. E. Stawarz, W. D. Nystrom
At the Earth's low-latitude magnetopause, the Kelvin–Helmholtz instability (KHI), driven by the velocity shear between the magnetosheath and magnetosphere, has been frequently observed during northward interplanetary magnetic field (IMF) periods. H
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0b40d263064736189290c2a27c6d2660
http://hdl.handle.net/10044/1/95461
http://hdl.handle.net/10044/1/95461
