Magnetic Field Effects on the Vishniac Overstability in Scaled Radiative Blast Waves

被引：1

作者：

Riley, N. J. ^{[1
,3
]}

Quevedo, H. J. ^{[1
]}

Bengtson, Roger D. ^{[1
]}

Ditmire, T. ^{[1
]}

Kimmel, M. ^{[2
]}

Speas, C. S. ^{[2
]}

Porter, J. L. ^{[2
]}

机构：

[1] Univ Texas Austin, Austin, TX 78712 USA

[2] Sandia Natl Labs, POB 5800, Albuquerque, NM 87185 USA

[3] Lawrence Livermore Natl Lab, Livermore, CA 94550 USA

来源：

ASTROPHYSICAL JOURNAL | 2020年 / 895卷 / 01期

关键词：

Supernova remnants; Supernova dynamics; Laboratory astrophysics; OSCILLATORY INSTABILITY; LINEAR-ANALYSIS; RESOLUTION; STABILITY;

D O I：

10.3847/1538-4357/ab899e

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We report experimental results on the stability of a magnetized laser-launched blast wave scaled to simulate a late-stage supernova remnant. We extend previous results to show the effect of a dynamically significant magnetic field on the spatial mode spectrum of the instability. We find that magnetic fields reduce instability growth, possibly influencing turbulent feedback to the interstellar medium.

引用

页数：6

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