<RESEARCH REPORT>Relativistic Shock Wave
スポンサーリンク
概要
- 論文の詳細を見る
Perpendicular shock waves in rather strong magnetic fields (ω_<ce>≳ω_<pe>) are studied by a 1-2/2 dimension, fully relativitic, fully electromagnetic particle simulation with full ion and electron dynamics. In that parameter regime relativistic effects become important in fast magnetosonic shock waves, even if the thermal speeds of ions and electrons in the upstream region are much smaller than the speed of light; a shock wave can trap some ions and promptly accelerate them to relativistic energies. Furthermore, with the mechanism different from that of ions, some electrons also gain relativistic energies through interactions with strong electric fields in the shock region. By showing various simulation results, we discuss the acceleration processes in detail.
- 核融合科学研究所の論文
著者
関連論文
- Particle Simulation Studies on Behaviour of Rapidly-Expanding High-Beta Plasma Column in a Uniform Magnetic Field
- Particle Simulation Studies on Behavior of Laser-Produced High-β Plasma in a Magnetic Field
- Magnetic Field Generation Due to Resonance Absorption
- Propagation of Nonlinear Ion Acoustic Wave with Generation of Long-Wavelength Waves
- Monte Carlo Simulation of Plasma Confinement in Mirror and Cusp Fields
- COMPUTER SIMULATIONS ON THE NONLINEAR FREQUENCY SHIFT AND NONLINEAR MODULATION OF ION-ACOUSTIC WAVES
- PROMPT SIMULTANEOUS ACCELERATION OF PROTONS AND ELECTRONS TO RELATIVISTIC ENERGIES BY SHOCK WAVES IN SOLAR FLARES
- Relativistic Shock Wave
- Strong Ion Accelerating by Collisionless Magnetosonic shock Wave Propagating Perpendicular to a Magnetic Field
- A Solitary Wave of a Relativistic Magnetosonic Wave Propagating Perpendicularly to a Magnetic Field
- Production of Highly Relativistic Ions and Electrons by Quasi-Perpendicular Magnetosonic Shock Waves
- ACCELERATION OF ENERGETIC IONS BY A NEARLY PERPENDICULAR INTERPLANETARY SHOCK