Abstract
We present a three-dimensional Direct Numerical Simulation (DNS) study of Rayleigh-Taylor Instability (RTI) using an all-speed, fully implicit, nondissipative and discrete kinetic energy conserving algorithm. In order to perform this study, an in-house, fully parallel, finite-volume, DNS solver, iDNS, which solves the set of time-dependent, compressible Navier-Stokes equations with gravity was developed based on the present algorithm and the PETSc parallel library. It is shown that the algorithm is able to capture the correct physics of the baroclinic instability and turbulent mixing. Compressibility (i.e., high Mach number) has been found more effective on the development of the flow after the diffusive growth phase passed. An increase in bubble growth rate together with a decrease in turbulent mixing was also observed at Mach number 1.1.
Original language | English |
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Article number | 1550018 |
Journal | International Journal of Computational Methods |
Volume | 12 |
Issue number | 3 |
DOIs | |
Publication status | Published - 16 Jun 2015 |
Bibliographical note
Publisher Copyright:© 2015 World Scientific Publishing Company.
Funding
Computing resources used in this work were provided by the National Center for High Performance Computing of Turkey (UYBHM) under Grant Number 1001212011 and TUBITAK-ULAKBIM, High Performance and Grid Computing Center (TRUBA Resources).
Funders | Funder number |
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National Center for High Performance Computing of Turkey | |
TUBITAK-ULAKBIM | |
UYBHM | 1001212011 |
Keywords
- all-speed
- DNS
- implicit
- parallel
- Rayleigh-Taylor instability