Laboratory experiments to simulate the hydrodynamics of supernova remnants and supernovae

Details Laboratory experiments to simulate the hydrodynamics of supernova remnants and supernovae Laboratory experiments to simulate the hydrodynamics of supernova remnants and supernovae

Jul 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999jgr...10414505d&link_type=abstract

Journal of Geophysical Research, Volume 104, Issue A7, p. 14505-14516

Astronomy and Astrophysics

Astrophysics

17

Magnetospheric Physics, Solar Physics, Astrophysics, And Astronomy

Scientific paper

Recent years have seen the emergence of a new approach to the laboratory simulation of astrophysical phenomena. Current experiments are designed to address, with good dimensionless scaling, specific physical issues that matter to the astrophysics. These include experiments to address the hydrodynamic evolution and instabilities in supernova remnants, experiments to address hydrodynamic instabilities in core-collapse supernova explosions, and experiments to address the structure of thermonuclear supernova explosions. They are contrasted with somewhat older experiments that made first attempts in this direction, examining high-velocity spherical expansions into unmagnetized plasma, and the deceleration of spherical expansions by a magnetic field.

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