Dynamics of Fast Electrons in an Inhomogeneous Plasma with Plasma Beam Instability

被引:5
|
作者
Kudryavtsev, I., V [1 ,2 ]
Kaltman, T., I [3 ]
Vatagin, P. V. [1 ]
Charikov, Yu E. [1 ]
机构
[1] Russian Acad Sci, Ioffe Inst, St Petersburg 194021, Russia
[2] Russian Acad Sci, Cent Astron Observ Pulkovo, St Petersburg 196140, Russia
[3] Russian Acad Sci, St Petersburg Branch, Special Astrophys Observ, St Petersburg 196140, Russia
基金
俄罗斯基础研究基金会;
关键词
HARD X-RAY; BRIGHTNESS DISTRIBUTION; SOLAR-FLARES; POLARIZATION; EMISSION;
D O I
10.1134/S001679321907020X
中图分类号
P3 [地球物理学]; P59 [地球化学];
学科分类号
0708 ; 070902 ;
摘要
The results of numerical simulation of the one-dimensional propagation of fast electrons in a plasma with Langmuir turbulence are presented. The resonant interaction of fast electrons with Langmuir waves and Coulomb collisions with particles of the background plasma are taken into account. It is shown that an increase in plasma density along the direction of the propagation of the electron beam leads to the transformation of the Langmuir turbulence spectrum into a region of high phase velocities and "spreading" of the velocity distribution function of accelerated electrons. For a Gaussian electron beam with an energy of 30 keV at its peak and a characteristic scale of an increase in plasma density of 10(7) cm, the electron spectrum expands; some of the electrons are accelerated to 1.3 of their initial velocity. In addition, a narrow (similar to 10(5) cm) layer with an increased turbulence level forms in the plasma. As the electrons move deeper into the plasma, Coulomb collisions restore the inverse over velocity part of the electron distribution function, which leads to the formation of a turbulent layer at a distance from the plasma boundary of similar to 10(7) cm-10(8) cm; however, the energy density of Langmuir turbulence in this layer is similar to(10(-6)-10(-7)) of the plasma thermal energy.
引用
收藏
页码:838 / 842
页数:5
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