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Quantifying density fluctuations in compressible turbulence

ORAL

Abstract

Numerical simulations show compressible shock-like structures at turbulent Mach numbers as low as 0.1. Quantifying the conditions that generate these structures is key to understanding how they behave in nature and engineered settings. Our goal is to quantify the density gradient field and to visualize shocks. We examine a turbulent jet inside a pressurized vessel with the ability to adjust the speed of sound using different gases including SF6, reaching up to Reλ~1000 and Mat~0.15. We perform Schlieren imaging and use the Gladstone-Dale relation to infer the density field from the image intensities. We visualize the turbulent jet flow and identify areas associated with large changes in density. These regions are then used to report spatial density gradient distributions and time-varying density fluctuations. With this information, we determine the frequency of highly compressive structures and validate published computer simulations.

Presenters

  • Hazel T Rivera-Rosario

    Cornell University

Authors

  • Hazel T Rivera-Rosario

    Cornell University

  • Naoki N Manzano-Miura

    Cornell University

  • Gregory P Bewley

    Cornell University, Cornell