Simulation of Nonrelativistic Jet Ejections During the Laboratory Studies


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We discuss a possibility of simulating nonrelativistic jet ejections during the laboratory experiment using the PF-3 facility. It is shown that many properties of the flows obtained with the help of the experimental facility agree with the basic characteristics of the jet ejections which are observed in the neighborhood of young stars. The future experiments, which can allow one to understand the nature of the stable plasma ejections observed in many astrophysical sources, are discussed.

作者简介

V. Beskin

P. N. Lebedev Physical Institute of the Russian Academy of Sciences; Moscow Institute of Physics and Technology

编辑信件的主要联系方式.
Email: beskin@lpi.ru
俄罗斯联邦, Moscow; Dolgoprudny

Ya. Istomin

P. N. Lebedev Physical Institute of the Russian Academy of Sciences; Moscow Institute of Physics and Technology

Email: beskin@lpi.ru
俄罗斯联邦, Moscow; Dolgoprudny

A. Kiselev

P. N. Lebedev Physical Institute of the Russian Academy of Sciences; Moscow Institute of Physics and Technology

Email: beskin@lpi.ru
俄罗斯联邦, Moscow; Dolgoprudny

V. Krauz

Research Center “Kurchatov Institute”

Email: beskin@lpi.ru
俄罗斯联邦, Moscow

K. Mitrofanov

Troitsk Institute of Innovative and Thermonuclear Research

Email: beskin@lpi.ru
俄罗斯联邦, Troitsk

V. Myalton

Research Center “Kurchatov Institute”

Email: beskin@lpi.ru
俄罗斯联邦, Moscow

E. Nokhrina

Moscow Institute of Physics and Technology

Email: beskin@lpi.ru
俄罗斯联邦, Dolgoprudny

D. Sob’yanin

P. N. Lebedev Physical Institute of the Russian Academy of Sciences

Email: beskin@lpi.ru
俄罗斯联邦, Moscow

A. Kharrasov

Research Center “Kurchatov Institute”

Email: beskin@lpi.ru
俄罗斯联邦, Moscow

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