Laboratory modeling of jets from young stars using plasma focus facilities

V.S. Beskin^†^a, b, V.I. Krauz^c, S.A. Lamzin^d
^aLebedev Physical Institute, Russian Academy of Sciences, Leninsky prosp. 53, Moscow, 119991, Russian Federation
^bMoscow Institute of Physics and Technology (National Research University), Institutskii per. 9, Dolgoprudny, Moscow Region, 141701, Russian Federation
^cNational Research Centre ‘Kurchatov Institute’, pl. akad. Kurchatova 1, Moscow, 123182, Russian Federation
^dLomonosov Moscow State University, Shternberg State Astronomical Institute, Universitetskii prosp. 13, Moscow, 119889, Russian Federation

Jets from young stars are used as an example to review how laboratory modeling enables advancement in understanding the main physical processes responsible for the formation and stability of these amazing objects. The discussion focuses on the options for modeling jet emissions in a laboratory experiment at the PF-3 facility at the National Research Center Kurchatov Institute. Many properties of the flows obtained using this experimental setup are consistent with the main features of jets from young stars.

Keywords: jets from young stars, laboratory simulation, plasma focus
PACS: 52.58.Lq, 97.21.+a, 98.38.Fs (all)
DOI: 10.3367/UFNe.2021.12.039130
URL: https://ufn.ru/en/articles/2023/4/a/
Web of Science

001099929700001
Scopus

2-s2.0-85175976900
ADS NASA

2023PhyU...66..327B
Citation: Beskin V S, Krauz V I, Lamzin S A "Laboratory modeling of jets from young stars using plasma focus facilities" Phys. Usp. 66 327–359 (2023)

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Received: 16th, August 2021, revised: 14th, December 2021, accepted: 20th, December 2021

Оригинал: Бескин В С, Крауз В И, Ламзин С А «Лабораторное моделирование струйных выбросов из молодых звёзд на установках с плазменным фокусом» УФН 193 345–381 (2023); DOI: 10.3367/UFNr.2021.12.039130

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