Laboratory experiments and numerical models of interacting explosions

被引：0

作者：

Velázquez, PF

Sobral, H

Raga, AC

Villagrán-Muniz, M

Navarro-González, R

机构：

[1] Natl Autonomous Univ Mexico, Inst Astron, Mexico City 04510, DF, Mexico

[2] Natl Autonomous Univ Mexico, Ctr Instrumentos, Mexico City 04510, DF, Mexico

[3] Natl Autonomous Univ Mexico, Inst Ciencias Nucl, Lab Quim Plasmas & Estudios Planetarios, Mexico City 04510, DF, Mexico

来源：

REVISTA MEXICANA DE ASTRONOMIA Y ASTROFISICA | 2001年 / 37卷 / 01期

关键词：

hydrodynamics; ISM : supernova remnants; methods : laboratory; methods : numerical; shock waves;

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present laboratory experiments and numerical simulations of the interaction between two explosions. In the laboratory, two expanding shock waves were produced using two Nd: YAG lasers, and the numerical simulations were carried out with the yguazu-a code (Raga et al. 2000). We show that the numerical simulations and laboratory experiments agree in a satisfactory way, and we discuss the general properties of the resulting flows. Finally, we discuss the similarities and differences between the laboratory experiments and some astrophysical objects.

引用

页码：87 / 94

页数：8

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