Startup process in the Richtmyer-Meshkov instability
- Creators
- Lombardini, M.
-
Pullin, D. I.
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.Attached Files
Published - Lombardini2009p4555Phys_Fluids.pdf
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Additional details
- Eprint ID
- 15180
- Resolver ID
- CaltechAUTHORS:20090820-090629481
- Department of Energy
- B341492
- Department of Energy
- W-7405-ENG-48
- Created
-
2009-08-20Created from EPrint's datestamp field
- Updated
-
2021-11-08Created from EPrint's last_modified field
- Caltech groups
- GALCIT