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Electron accelerations at high Mach number collision-less shocks are investigated by means of two-dimensional electromagnetic Particle-in-Cell simulations with various Alfven Mach numbers, ion-to-electron mass ratios, and the upstream…

高能天体物理现象 · 物理学 2013-11-01 Yosuke Matsumoto , Takanobu Amano , Masahiro Hoshino

A full particle simulation study is carried out on the electron acceleration at a collisionless, relatively low Alfven Mach number (M_A=5), perpendicular shock. Recent self-consistent hybrid shock simulations have demonstrated that the…

天体物理学 · 物理学 2011-02-11 Takayuki Umeda , Masahiro Yamao , Ryo Yamazaki

Electron injection process at high Mach number collisionless quasi-perpendicular shock waves is investigated by means of one-dimensional electromagnetic particle-in-cell simulations. We find that energetic electrons are generated through…

天体物理学 · 物理学 2011-02-11 T. Amano , M. Hoshino

Electron acceleration in high Mach number perpendicular shocks is investigated through two-dimensional electrostatic particle-in-cell (PIC) simulation. We simulate the shock foot region by modeling particles that consist of three components…

天体物理学 · 物理学 2009-11-13 Yutaka Ohira , Fumio Takahara

Energetic electrons are a common feature of interplanetary shocks and planetary bow shocks, and they are invoked as a key component of models of nonthermal radio emission, such as solar radio bursts. A simulation study is carried out of…

天体物理学 · 物理学 2008-11-26 D. Burgess

We study the suprathermal electron acceleration mechanism in a perpendicular magnetosonic shock wave in a high Mach number regime by using a particle-in-cell simulation. We find that shock surfing/surftron acceleration producing the…

天体物理学 · 物理学 2009-11-07 M. Hoshino , N. Shimada

Using large-scale fully-kinetic two-dimensional particle-in-cell simulations, we investigate the effects of shock rippling on electron acceleration at low-Mach-number shocks propagating in high-$\beta$ plasmas, in application to merger…

高能天体物理现象 · 物理学 2021-10-04 Oleh Kobzar , Jacek Niemiec , Takanobu Amano , Masahiro Hoshino , Shuichi Matsukiyo , Yosuke Matsumoto , Martin Pohl

We perform a numerical-simulation study of the acceleration of electrons at shocks that propagate through a prespecified, kinematically defined turbulent magnetic field. The turbulence consists of broadband magnetic fluctuations that are…

高能天体物理现象 · 物理学 2015-06-22 Fan Guo , Joe Giacalone

We study the physics of electron acceleration at collisionless shocks that move through a plasma containing large-scale magnetic fluctuations. We numerically integrate the trajectories of a large number of electrons, which are treated as…

太阳与恒星天体物理 · 物理学 2015-03-13 Fan Guo , Joe Giacalone

How electrons get accelerated to relativistic energies in a high-Mach-number quasi-perpendicular shock is presented by means of ab initio particle-in-cell simulations in three dimensions. We found that coherent electrostatic Buneman waves…

高能天体物理现象 · 物理学 2017-09-13 Yosuke Matsumoto , Takanobu Amano , Tsunehiko N. Kato , Masahiro Hoshino

Electron acceleration to non-thermal energies in low Mach number (M<5) shocks is revealed by radio and X-ray observations of galaxy clusters and solar flares, but the electron acceleration mechanism remains poorly understood. Diffusive…

高能天体物理现象 · 物理学 2014-10-14 Xinyi Guo , Lorenzo Sironi , Ramesh Narayan

Shock accelerated electrons are found in many astrophysical environments, and the mechanisms by which they are accelerated to high energies are still not completely clear. For relatively high Mach numbers, the shock is supercritical, and…

空间物理 · 物理学 2018-10-17 D. Trotta , D. Burgess

A full particle simulation study is carried out on a perpendicular collisionless shock with a relatively low Alfven Mach number (M_A=5). In the present study, we have performed a two-dimensional (2D) electromagnetic full particle simulation…

等离子体物理 · 物理学 2011-04-04 Takayuki Umeda , Masahiro Yamao , Ryo Yamazaki

Electron acceleration to non-thermal energies is known to occur in low Mach number (M<5) shocks in galaxy clusters and solar flares, but the electron acceleration mechanism remains poorly understood. Using two-dimensional (2D)…

高能天体物理现象 · 物理学 2014-11-26 Xinyi Guo , Lorenzo Sironi , Ramesh Narayan

To undergo diffusive shock acceleration, electrons need to be pre-accelerated to increase their energies by several orders of magnitude, else their gyro-radii are smaller than the finite width of the shock. In oblique shocks, where the…

等离子体物理 · 物理学 2022-06-08 Paul J. Morris , Artem Bohdan , Martin S. Weidl , Martin Pohl

We study diffusive shock acceleration (DSA) of electrons in non-relativistic quasi-perpendicular shocks using self-consistent one-dimensional particle-in-cell (PIC) simulations. By exploring the parameter space of sonic and Alfv\'{e}nic…

高能天体物理现象 · 物理学 2020-07-22 Rui Xu , Anatoly Spitkovsky , Damiano Caprioli

Shock drift acceleration plays an important role in generating high-energy electrons at quasi-perpendicular shocks, but its efficiency in low beta plasmas is questionable. In this article, we perform a two-dimensional particle-in-cell…

空间物理 · 物理学 2024-09-06 Ao Guo , Quanming Lu , San Lu , Zhongwei Yang , Xinliang Gao

We investigate shock structure and particle acceleration in relativistic magnetized collisionless electron-ion shocks by means of 2.5D particle-in-cell simulations with ion-to-electron mass ratios (m_i/m_e) ranging from 16 to 1000. We…

高能天体物理现象 · 物理学 2015-05-19 Lorenzo Sironi , Anatoly Spitkovsky

Strong non-relativistic shocks are known to accelerate particles up to relativistic energies. However, for Diffusive Shock Acceleration electrons must have a highly suprathermal energy, implying a need for very efficient pre-acceleration.…

等离子体物理 · 物理学 2023-10-24 Karol Fulat , Artem Bohdan , Gabriel Torralba Paz , Martin Pohl

Electron motion in an oblique shock wave is studied by means of a one-dimensional, relativistic, electromagnetic, particle simulation code with full ion and electron dynamics. It is found that an oblique shock can produce electrons with…

等离子体物理 · 物理学 2009-10-31 Naoki Bessho , Yukiharu Ohsawa
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