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


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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 107 cm, the electron spectrum expands; some of the electrons are accelerated to 1.3 of their initial velocity. In addition, a narrow (~105 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 ~107 cm–108 cm; however, the energy density of Langmuir turbulence in this layer is ~(10–6–10–7) of the plasma thermal energy.

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I. Kudryavtsev

Ioffe Institute, Russian Academy of Sciences; The Central Astronomical Observatory at Pulkovo, Russian Academy of Sciences

编辑信件的主要联系方式.
Email: Igor.Koudriavtsev@mail.ioffe.ru
俄罗斯联邦, St. Petersburg, 194021; St. Petersburg, 196140

T. Kaltman

Special Astrophysical Observatory, St. Petersburg Branch, Russian Academy of Sciences

Email: Igor.Koudriavtsev@mail.ioffe.ru
俄罗斯联邦, St. Petersburg, 196140

P. Vatagin

Ioffe Institute, Russian Academy of Sciences

Email: Igor.Koudriavtsev@mail.ioffe.ru
俄罗斯联邦, St. Petersburg, 194021

Yu. Charikov

Ioffe Institute, Russian Academy of Sciences

Email: Igor.Koudriavtsev@mail.ioffe.ru
俄罗斯联邦, St. Petersburg, 194021

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