Search Results - "Amano, Takanobu"
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A SECOND-ORDER DIVERGENCE-CONSTRAINED MULTIDIMENSIONAL NUMERICAL SCHEME FOR RELATIVISTIC TWO-FLUID ELECTRODYNAMICS
Published in The Astrophysical journal (01-11-2016)“…ABSTRACT A new multidimensional simulation code for relativistic two-fluid electrodynamics (RTFED) is described. The basic equations consist of the full set of…”
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Theory of Stochastic Shock Drift Acceleration for Electrons in the Shock Transition Region
Published in The Astrophysical journal (01-04-2019)“…We propose a novel electron acceleration mechanism, which we call stochastic shock drift acceleration (SSDA), that extends the standard shock drift…”
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Theory of Electron Injection at Oblique Shock of Finite Thickness
Published in The Astrophysical journal (01-03-2022)“…Abstract A theory of electron injection into diffusive shock acceleration (DSA) for the generation of cosmic-ray electrons at collisionless shocks is…”
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Persistence of Precursor Waves in Two-dimensional Relativistic Shocks
Published in The Astrophysical journal (01-05-2017)“…We investigated the efficiency of coherent upstream large-amplitude electromagnetic wave emission via synchrotron maser instability in relativistic magnetized…”
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Enhanced Magnetic Field Amplification by Ion-beam Weibel Instability in Weakly Magnetized Astrophysical Shocks
Published in The Astrophysical journal (01-02-2024)“…Abstract We examine the evolution of ion-beam Weibel instability at strong collisionless shocks in weakly magnetized media. We find that a finite background…”
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Precursor Wave Emission Enhanced by Weibel Instability in Relativistic Shocks
Published in The Astrophysical journal (10-05-2018)“…We investigated the precursor wave emission efficiency in magnetized purely perpendicular relativistic shocks in pair plasmas. We extended our previous study…”
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Kinetic Simulations of Nonrelativistic Perpendicular Shocks of Young Supernova Remnants. III. Magnetic Reconnection
Published in The Astrophysical journal (10-04-2020)“…Fully kinetic two-dimensional particle-in-cell simulations are used to study electron acceleration at high-Mach-number nonrelativistic perpendicular shocks…”
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Electron Acceleration at Rippled Low-mach-number Shocks in High-beta Collisionless Cosmic Plasmas
Published in The Astrophysical journal (01-10-2021)“…Abstract Using large-scale fully kinetic two-dimensional particle-in-cell simulations, we investigate the effects of shock rippling on electron acceleration at…”
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Kinetic Simulations of Nonrelativistic Perpendicular Shocks of Young Supernova Remnants. I. Electron Shock-surfing Acceleration
Published in The Astrophysical journal (10-06-2019)“…Electron injection at high Mach number nonrelativistic perpendicular shocks is studied here for parameters that are applicable to young SNR shocks. Using…”
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Kinetic Simulations of Nonrelativistic Perpendicular Shocks of Young Supernova Remnants. II. Influence of Shock-surfing Acceleration on Downstream Electron Spectra
Published in The Astrophysical journal (01-11-2019)“…We explore electron preacceleration at high-Mach-number nonrelativistic perpendicular shocks at, e.g., young supernova remnants, which are a prerequisite of…”
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Particle Acceleration by Pickup Process Upstream of Relativistic Shocks
Published in The Astrophysical journal (01-01-2022)“…Abstract Particle acceleration at magnetized purely perpendicular relativistic shocks in electron–ion plasmas is studied by means of two-dimensional…”
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Magnetic Storm‐Time Red Aurora as Seen From Hokkaido, Japan on 1 December 2023 Associated With High‐Density Solar Wind
Published in Geophysical research letters (28-06-2024)“…We report a citizen science‐motivated study on the cause of an unusually bright red aurora as witnessed from Hokkaido, Japan during a magnetic storm on 1…”
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Mildly relativistic magnetized shocks in electron–ion plasmas – II. Particle acceleration and heating
Published in Monthly notices of the Royal Astronomical Society (01-04-2021)“…ABSTRACT Particle acceleration and heating at mildly relativistic magnetized shocks in electron–ion plasma are investigated with unprecedentedly…”
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Electron–Ion Temperature Ratio in Astrophysical Shocks
Published in The Astrophysical journal (01-06-2023)“…Abstract Collisionless shock waves in supernova remnants and the solar wind heat electrons less effectively than they heat ions, as is predicted by kinetic…”
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Kinetic Simulation of Nonrelativistic Perpendicular Shocks of Young Supernova Remnants. IV. Electron Heating
Published in The Astrophysical journal (01-11-2020)“…High-Mach-number collisionless shocks are found in planetary systems and supernova remnants (SNRs). Electrons are heated at these shocks to temperatures well…”
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A critical Mach number for electron injection in collisionless shocks
Published in Physical review letters (07-05-2010)“…Electron acceleration in collisionless shocks with arbitrary magnetic field orientations is discussed. It is shown that the injection of thermal electrons into…”
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THE ROLE OF SUPERLUMINAL ELECTROMAGNETIC WAVES IN PULSAR WIND TERMINATION SHOCKS
Published in The Astrophysical journal (10-06-2013)“…The dynamics of a standing shock front in a Poynting-flux-dominated relativistic flow is investigated by using a one-dimensional, relativistic, two-fluid…”
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Mildly relativistic magnetized shocks in electron–ion plasmas – I. Electromagnetic shock structure
Published in Monthly notices of the Royal Astronomical Society (01-03-2021)“…ABSTRACT Mildly relativistic shocks in magnetized electron–ion plasmas are investigated with 2D kinetic particle-in-cell simulations of unprecedentedly high…”
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A finite volume formulation of the multi-moment advection scheme for Vlasov simulations of magnetized plasma
Published in Computer physics communications (01-02-2015)“…We present a finite volume version of the multi-moment advection scheme (Minoshima et al., 2011, 2013). The scheme advances zeroth to second order piecewise…”
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STABILITY OF COSMIC-RAY MODIFIED SHOCKS: TWO-FLUID APPROACH
Published in The Astrophysical journal (01-10-2013)“…The stability of cosmic-ray modified shocks (CRMSs) is studied by means of numerical simulations. Owing to the nonlinear feedback of cosmic-ray (CR)…”
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