Yasuhiro Kaminou
University of Tokyo
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Featured researches published by Yasuhiro Kaminou.
The Astrophysical Journal | 2012
Naoto Nishizuka; Yoshinori Hayashi; Hiroshi Tanabe; Akihiro Kuwahata; Yasuhiro Kaminou; Yasushi Ono; Michiaki Inomoto; Toshifumi Shimizu
Hinode observations have revealed intermittent recurrent plasma ejections/jets in the chromosphere. These are interpreted as a result of non-perfectly anti-parallel magnetic reconnection, i.e. component reconnection, between a twisted magnetic flux tube and the pre-existing coronal/chromospheric magnetic field, though the fundamental physics of component reconnection is unrevealed. In this paper, we experimentally reproduced the magnetic configuration and investigated the dynamics of plasma ejections, heating and wave generation triggered by component reconnection in the chromosphere. We set plasma parameters as in the chromosphere (density 10^14 cm^-3, temperature 5-10 eV, i.e. (5-10)x10^4 K, and reconnection magnetic field 200 G) using argon plasma. Our experiment shows bi-directional outflows with the speed of 5 km/s at maximum, ion heating in the downstream area over 30 eV and magnetic fluctuations mainly at 5-10 us period. We succeeded in qualitatively reproducing chromospheric jets, but quantitatively we still have some differences between observations and experiments such as jet velocity, total energy and wave frequency. Some of them can be explained by the scale gap between solar and laboratory plasma, while the others probably by the difference of microscopy and macroscopy, collisionality and the degree of ionization, which have not been achieved in our experiment.
Nuclear Fusion | 2013
Michiaki Inomoto; Keii Gi; Toshiyuki Umezawa; Taichi Ito; Kazutake Kadowaki; Yasuhiro Kaminou; Yasushi Ono
A low-energy, high-current neutral beam injection (NBI) was applied to an oblate field-reversed configuration (FRC) for the first time. The NB fast ions reduce growth rates of low-n modes dangerous for the oblate FRC, extending the FRC lifetime by a factor of 1.2. The reduced loss power of 5 MW is much higher than the NBI power of 0.5 MW, indicating that the NBI not only heats the FRC plasma but also improves its stability and transport properties. The NBI also maintains higher pressure and current density profiles of the FRC, improving its flux and energy decay times by a factor of 2.
Physics of Plasmas | 2017
Xuehan Guo; Ritoku Horiuchi; Chio Cheng; Yasuhiro Kaminou; Yasushi Ono
The energy conversion mechanism for electron perpendicular energy, both the thermal and the kinetic energies, is investigated by means of two-dimensional, full-particle simulations in an open system. It is shown that electron perpendicular heating is mainly due to the breaking of magnetic moment conservation in separatrix region because the charge separation generates intense variation of electric field within the several electron Larmor radii. Meanwhile, electron perpendicular acceleration takes place mainly due to the polarization drift term as well as the curvature drift term of E · u ⊥ in the downstream near the X-point. The enhanced electric field due to the charge separation there results in a significant effect of the polarization drift term on the dissipation of magnetic energy within the ion inertia length in the downstream.
Physics of Plasmas | 2017
Yasuhiro Kaminou; Xuehan Guo; Michiaki Inomoto; Yasushi Ono; Ritoku Horiuchi
Hall effects on counter-helicity spheromak merging were investigated by two-dimensional MHD and Hall-MHD simulations of merging two axisymmetric toroidal flux tubes. In Hall-MHD cases, the structure of the reconnection current sheet and reconnection outflow are modified from the MHD case due to the Hall effect. We compared two cases (called “case-O” and “case-I”) of counter-helicity merging, which are distinguished by the polarity of toroidal magnetic fluxes. Radial motion of the reconnection X-point is controlled by poloidal electron flow accompanying the toroidal flux of the merging two spheromaks, and this creates a large difference in the current sheet and flow structure between the two cases of the Hall-MHD regime. The radial shift of the reconnection X-point depending on the polarity of toroidal magnetic flux of the spheromaks breaks the symmetry between the two cases. It was also found that there widely exists separation of ion and electron flow which are affected by the modification of the current...
Plasma and Fusion Research | 2016
Yasuhiro Kaminou; Michiaki Inomoto; Yasushi Ono
Plasma and Fusion Research | 2013
Hiroshi Tanabe; Hirotaka Oka; Masanobu Annoura; Akihiro Kuwahata; Kazutake Kadowaki; Yasuhiro Kaminou; Setthivoine You; Alexander A. Balandin; Michiaki Inomoto; Yasushi Ono
Ieej Transactions on Fundamentals and Materials | 2013
Yasuhiro Kaminou; Shizuo Inoue; Michiaki Inomoto; Yasushi Ono
Ieej Transactions on Fundamentals and Materials | 2014
Yasuhiro Kaminou; Shizuo Inoue; Michiaki Inomoto; Yasushi Ono
Plasma and Fusion Research | 2018
Takahiro Edo; Tomohiko Asai; Fumiyuki Tanaka; Shodai Yamada; A. Hosozawa; Yasuhiro Kaminou; H. Gota; T. Roche; I. Allfrey; Dmitry Osin; Roger Smith; Michl Binderbauer; T. Matsumoto; T. Tajima
The transactions of the Institute of Electrical Engineers of Japan.A | 2016
Akihiro Kuwahata; Yasuhiro Kaminou; Ryoma Yanai; Michiaki Inomoto; Yasushi Ono