Simulation of Nonrelativistic Jet Ejections During the Laboratory Studies


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Abstract

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.

About the authors

V. S. Beskin

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

Author for correspondence.
Email: beskin@lpi.ru
Russian Federation, Moscow; Dolgoprudny

Ya. N. Istomin

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

Email: beskin@lpi.ru
Russian Federation, Moscow; Dolgoprudny

A. M. Kiselev

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

Email: beskin@lpi.ru
Russian Federation, Moscow; Dolgoprudny

V. I. Krauz

Research Center “Kurchatov Institute”

Email: beskin@lpi.ru
Russian Federation, Moscow

K. N. Mitrofanov

Troitsk Institute of Innovative and Thermonuclear Research

Email: beskin@lpi.ru
Russian Federation, Troitsk

V. V. Myalton

Research Center “Kurchatov Institute”

Email: beskin@lpi.ru
Russian Federation, Moscow

E. E. Nokhrina

Moscow Institute of Physics and Technology

Email: beskin@lpi.ru
Russian Federation, Dolgoprudny

D. N. Sob’yanin

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

Email: beskin@lpi.ru
Russian Federation, Moscow

A. M. Kharrasov

Research Center “Kurchatov Institute”

Email: beskin@lpi.ru
Russian Federation, Moscow

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