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Collisionless shock and supernova remnant simulations on VULCAN

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Kirk,  J. G.
Division Prof. Dr. Werner Hofmann, MPI for Nuclear Physics, Max Planck Society;

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Citation

Woolsey, N. C., Ali, Y. A., Evans, R. G., Grundy, R. A. D., Pestehe, S. J., Carolan, P. G., et al. (2001). Collisionless shock and supernova remnant simulations on VULCAN. Physics of Plasmas, 8(5), 2439-2449.


Cite as: http://hdl.handle.net/11858/00-001M-0000-0011-85AB-7
Abstract
The VULCAN [C. N. Danson , Opt. Commun. 103, 392 (1993)] laser at the UK Central Laser Facility is being used for laboratory-based simulations of collisionless shocks. By ensuring that key dimensionless parameters in the experiments have values similar to those of supernova remnants (SNRs), the hydrodynamics and magnetic field of the experiment are scaled to those of a SNR. This makes it possible to investigate experimentally the physics of collisionless magnetized shocks in such objects. The experiments are providing data against which to test current theory. Collisionless shock formation and the interaction of two counterpropagating colliding plasmas permeated by a strong magnetic field are discussed. (C) 2001 American Institute of Physics. [References: 24]