Large Scale Simulations of Jets in Dense and Magnetised Environments

Martin Krause () and Max Camenzind
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Martin Krause: Landessternwarte Königstuhl
Max Camenzind: Landessternwarte Königstuhl

A chapter in High Performance Computing in Science and Engineering ’03, 2003, pp 95-106 from Springer

Abstract: Abstract We have used the vectorised and parallelised MHD code NIRVANA on the NEC SX-5 in parallel mode to simulate the interaction of jets with a dense environment on a scale of more than 200 jet radii. A maximum performance of 0.75 GFLOP per processor could be reached.

Keywords: Galaxy Cluster; Radio Galaxy; Contact Discontinuity; Host Galaxy; Large Scale Simulation (search for similar items in EconPapers)
Date: 2003
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Persistent link: https://EconPapers.repec.org/RePEc:spr:sprchp:978-3-642-55876-4_7

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DOI: 10.1007/978-3-642-55876-4_7

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