Paper
23 April 2001 Supernova remnant simulation experiments on VULCAN
N. C. Woolsey, Y. Abou Ali, R. Evans, R. A. D. Grundy, S. J. Peschte, P. Carolan, N. Conway, R. O. Dendy, P. Helander, K. G. McClements, J. G. Kirk, Peter A. Norreys, M. M. Notley, S. J. Rose
Author Affiliations +
Proceedings Volume 4424, ECLIM 2000: 26th European Conference on Laser Interaction with Matter; (2001) https://doi.org/10.1117/12.425539
Event: 26th European Conference on Laser Interaction with Matter (ECLIM 2000), 2000, Prague, Czech Republic
Abstract
The VULCAN laser at the Central Laser Facility has been used for laboratory simulations of collision-less astrophysical shocks. By ensuring that the experiment exhibit similar values of key dimension-less parameters to those in supernova remnants the hydrodynamics and magnetic field of the experiment are scaled to those of SNR. This enables some of the most challenging aspects of shock behavior to be tested directly against experiment. The experiments provide dat against which to test current theory. Collision-less shock formation, and plasma interaction of two counter- propagating colliding foils permeated by a strong magnetic field are discussed.
© (2001) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
N. C. Woolsey, Y. Abou Ali, R. Evans, R. A. D. Grundy, S. J. Peschte, P. Carolan, N. Conway, R. O. Dendy, P. Helander, K. G. McClements, J. G. Kirk, Peter A. Norreys, M. M. Notley, and S. J. Rose "Supernova remnant simulation experiments on VULCAN", Proc. SPIE 4424, ECLIM 2000: 26th European Conference on Laser Interaction with Matter, (23 April 2001); https://doi.org/10.1117/12.425539
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KEYWORDS
Plasma

Magnetism

Signal to noise ratio

Chemical oxygen iodine lasers

Explosives

Picosecond phenomena

Pulsed laser operation

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