Numerical Simulations of Magnetized Astrophysical Jets and Comparison with Laboratory Laser Experiments

被引：23

作者：

Belyaev, V. S. ^{[1
]}

Bisnovatyi-Kogan, G. S. ^{[2
,3
]}

Gromov, A. I. ^{[4
]}

Zagreev, B. V. ^{[1
]}

Lobanov, A. V. ^{[1
]}

Matafonov, A. P. ^{[1
]}

Moiseenko, S. G. ^{[2
]}

Toropina, O. D. ^{[2
]}

机构：

[1] Cent Res Inst Machine Bldg TsNIIMash, Korolev 141070, Moscow Region, Russia

[2] Russian Acad Sci, Space Res Inst, Moscow 117997, Russia

[3] Moscow Engn Phys Inst, Natl Nucl Res Inst, Moscow 115409, Russia

[4] Lebedev Phys Inst, Moscow 119991, Russia

来源：

ASTRONOMY REPORTS | 2018年 / 62卷 / 03期

基金：

俄罗斯基础研究基金会;

关键词：

SCALING LAWS; GENERATION; ACCRETION; ABLATION; EMISSION; DYNAMICS; FIELDS; FLOW;

D O I：

10.1134/S1063772918030034

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The results of MHD numerical simulations of the formation and development of magnetized jets are presented. Similarity criteria for comparisons of the results of laboratory laser experiments and numerical simulations of astrophysical jets are discussed. The results of laboratory simulations of jets generated in experiments at the Neodim laser installation are presented.

引用

页码：162 / 182

页数：21

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