Published April 2009 | Version Published
Journal Article Open

Startup process in the Richtmyer-Meshkov instability

  • 1. ROR icon California Institute of Technology

Abstract

An analytical model for the initial growth period of the planar Richtmyer–Meshkov instability is presented for the case of a reflected shock, which corresponds in general to light-to-heavy interactions. The model captures the main features of the interfacial perturbation growth before the regime with linear growth in time is attained. The analysis provides a characteristic time scale τ for the startup phase of the instability, expressed explicitly as a function of the perturbation wavenumber k, the algebraic transmitted and reflected shock speeds U_(S1) < 0 and U_(S2) > 0 (defined in the frame of the accelerated interface), and the postshock Atwood number A^+: τ=[(1-A^+)/U_(S2)+(1+A^+)/(-U_(s1))]/(2k). Results are compared with computations obtained from two-dimensional highly resolved numerical simulations over a wide range of incident shock strengths S and preshock Atwood ratios A. An interesting observation shows that, within this model, the amplitude of small perturbations across a light-to-heavy interface evolves quadratically in time (and not linearly) in the limit A→1^−.

Additional Information

© 2009 American Institute of Physics. Received 2 October 2008; accepted 4 November 2008; published 14 April 2009. This work was supported by the Advanced Simulation and Computing ASC Program under Subcontract No. B341492 of DOE Contract No. W-7405-ENG-48. M.L. and D.I.P. would like to thank Dr. David J. Hill for numerous discussions and comments on the manuscript.

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Identifiers

Eprint ID
15180
Resolver ID
CaltechAUTHORS:20090820-090629481

Funding

Department of Energy
B341492
Department of Energy
W-7405-ENG-48

Dates

Created
2009-08-20
Created from EPrint's datestamp field
Updated
2021-11-08
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