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
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
收藏
页码:87 / 94
页数:8
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