Localization of the magnetic field in a plasma flow in laboratory simulations of astrophysical jets at the KPF-4-PHOENIX installation


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The results of experiments aimed at investigating axial plasma flows forming during the compression of a current–plasma sheath are presented. These experiments were carried out at the KPF-4-PHOENIX plasma-focus installation, as part of a program of laboratory simulations of astrophysical jets. The plasma flows were generated in a discharge when the chamber was filled with the working gas (argon) at initial pressures of 0.5–2 Torr. Experimental data obtained using a magnetic probe and optical diagnostics are compared. The data obtained can be used to determine the location of trapped magnetic field relative to regions of intense optical glow in the plasma flow.

作者简介

K. Mitrofanov

SRC RF Troitsk Institute for Innovation and Fusion Reseach

编辑信件的主要联系方式.
Email: mitrofan@triniti.ru
俄罗斯联邦, Troitsk, Moscow, 142190

S. Anan’ev

NRC “Kurchatov Institute”

Email: krauz_vi@nrcki.ru
俄罗斯联邦, Moscow, 123182

D. Voitenko

SUE Sukhum Physical Technical Institute

Email: krauz_vi@nrcki.ru
格鲁吉亚, Sukhum, Abkhazia

V. Krauz

NRC “Kurchatov Institute”

编辑信件的主要联系方式.
Email: krauz_vi@nrcki.ru
俄罗斯联邦, Moscow, 123182

G. Astapenko

SUE Sukhum Physical Technical Institute

Email: krauz_vi@nrcki.ru
格鲁吉亚, Sukhum, Abkhazia

A. Markoliya

SUE Sukhum Physical Technical Institute

Email: krauz_vi@nrcki.ru
格鲁吉亚, Sukhum, Abkhazia

V. Myalton

NRC “Kurchatov Institute”

Email: krauz_vi@nrcki.ru
俄罗斯联邦, Moscow, 123182

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