cosmic ray generation;
electron acceleration;
relativistic proton beams;
D O I:
10.1109/TPS.2005.845012
中图分类号:
O35 [流体力学];
O53 [等离子体物理学];
学科分类号:
070204 ;
080103 ;
080704 ;
摘要:
We examine electron acceleration in magnetized plasma by electrostatic waves that move orthogonally across a magnetic field with a phase speed that is comparable to the light speed. We evolve the plasma phase space distribution with a particle-in-cell code. We distribute the computational electrons over an array and we volume-render this phase space density. We show key images of an animation by which we follow the electron phase space distribution throughout the simulation and which shows that the electron transport across the magnetic field, the collapse of the electrostatic wave and the resulting turbulent wave fields can accelerate electrons to gigaelectronvolt energies for wave speeds that we may find in some astrophysical environments.
机构:
RAS, Inst Space Res, Moscow 117997, RussiaRAS, Inst Space Res, Moscow 117997, Russia
Artemyev, A. V.
Neishtadt, A. I.
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h-index: 0
机构:
RAS, Inst Space Res, Moscow 117997, Russia
Univ Loughborough, Dept Math Sci, Loughborough LE11 3TU, Leics, EnglandRAS, Inst Space Res, Moscow 117997, Russia
Neishtadt, A. I.
Vasiliev, A. A.
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h-index: 0
机构:
RAS, Inst Space Res, Moscow 117997, RussiaRAS, Inst Space Res, Moscow 117997, Russia
Vasiliev, A. A.
Zelenyi, L. M.
论文数: 0引用数: 0
h-index: 0
机构:
RAS, Inst Space Res, Moscow 117997, RussiaRAS, Inst Space Res, Moscow 117997, Russia