Turbulent Mixing in Shock-Driven Variable-Density Flow—from Supernova Explosion to Fusion System

Dr. Devesh Ranjan

Eugene C. Gwaltney, Jr. School Chair and Professor 

George W. Woodruff School of Mechanical Engineering 

Georgia Institute of Technology 

771 Ferst Dr., Atlanta, GA 30332-0405 

Devesh.ranjan@me.gatech.edu  

About Dr. Devesh Ranjun

Devesh Ranjan is the Eugene C. Gwaltney Jr. School Chair in the Woodruff School of Mechanical Engineering at Georgia Institute of Technology. He also holds a courtesy appointment in the Daniel Guggenheim School of Aerospace Engineering and serves as co-director of the $100M Department of Defense-funded University Consortium for Applied Hypersonics (UCAH). Ranjan joined the faculty at Georgia Tech in 2014. Ranjan served as Interim Vice-President for Interdisciplinary Research (Feb 2021-June 2021) at Georgia Tech. Before coming to Georgia Tech, he was a director's research fellow at Los Alamos National Laboratory (2008) and Morris E Foster Assistant Professor in the Mechanical Engineering department at Texas A&M University (2009-2014). He earned a bachelor's degree from the NIT-Trichy (India) in 2003, and master's and Ph.D. degrees from the UW-Madison in 2005 and 2007 respectively, all in mechanical engineering.

Ranjan’s research focuses on the interdisciplinary area of power conversion, complex fluid flows involving shock and hydrodynamic instabilities, and the turbulent mixing of materials in extreme conditions, such as supersonic and hypersonic flows. Ranjan is a Fellow of the American Society of Mechanical Engineers (ASME), and has received numerous awards for his scientific contributions, including the DOE-Early Career Award (first GT recipient), the NSF CAREER Award, and the US AFOSR Young Investigator award. He was invited to participate in the National Academy of Engineering’s 2016 US Frontiers in Engineering Symposium. At Georgia Tech, Ranjan served as a Provost’s Teaching and Learning Fellow (PTLF) from 2018-2020, and was named 2021 Governor’s Teaching Fellow. He was also named Diversity, Equity and Inclusion (DEI) Fellow for 2020-21.

 

Abstract

Mixing is central to several important phenomena in nature and engineering. Rayleigh-Taylor (RT) and Richtmyer-Meshkov (RM) driven wrinkles at the interface of materials lie at the heart of an overarching science for material mixing that stretches from oil trapping salt domes, that develop over tens of millions of years, to degradation of Inertial Confinement Fusion (ICF) capsule performance in 10 -12 ns. RT and RM are insidious instabilities that start with exponential growth (power-law function of time for RM) of small-scale perturbations, and end in a fully turbulent mixing process. Shock tube experiments allow us to explore the effects of Mach number and initial conditions on unsteady variable-density mixing. I will describe here the results from recent experiments which quantifies the effect of initial conditions on the transition to turbulence in RMI driven flows The evolving density and velocity fields are measured simultaneously using high spatial resolution planar laser-induced fluorescence (PLIF) and particle image velocimetry (PIV) techniques. For the first time, we have acquired simultaneous PIV-PLIF measurements at 60KHz in such a transient flow system.  Density, velocity, and density–velocity cross-statistics are calculated using ensemble averaging to investigate the effects of additional modes on the mixing and turbulence quantities. The density and velocity data show that a distinct memory of the initial conditions is maintained in the flow before interaction with reshock.