Simulations of radiative effects on the Rayleigh–Taylor instability using the CRASH code
Future experiments at the National Ignition Facility will be able to generate diagnosable Rayleigh–Taylor instability growth in the presence of locally generated, high radiation fluxes. This interplay of radiative energy transfer and hydrodynamic instability is relevant to many astrophysical systems...
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Published in | High energy density physics Vol. 9; no. 2; pp. 303 - 308 |
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Main Authors | , , , , , , , , |
Format | Journal Article |
Language | English |
Published |
Elsevier B.V
01.06.2013
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Subjects | |
Online Access | Get full text |
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