This paper brings new insights on an experiment, measuring the Kelvin–Helmholtz (KH) instability evolution, performed on the OMEGA-60 laser facility. Experimental radiographs show that the initial seed perturbations in the experiment are of multimode spectrum with a dominant single-mode of 16 μm wavelength. In single-mode-dominated KH instability flows, the mixing zone (MZ) width saturates to a constant value comparable to the wavelength. However, the experimental MZ width at late times has exceeded 100 μm, an order of magnitude larger. In this work, we use numerical simulations and a statistical model in order to investigate the vortex dynamics of the KH instability for the experimental initial spectrum. We conclude that the KH instability evolution in the experiment is dominated by multimode, vortex-merger dynamics, overcoming the dominant initial mode.
Skip Nav Destination
Article navigation
July 2016
Research-Article
The Effect of a Dominant Initial Single Mode on the Kelvin–Helmholtz Instability Evolution: New Insights on Previous Experimental Results
Assaf Shimony,
Assaf Shimony
Department of Physics,
NRCN,
Beer-Sheva 84190, Israel;
NRCN,
Beer-Sheva 84190, Israel;
Search for other works by this author on:
Dov Shvarts,
Dov Shvarts
Department of Physics,
NRCN,
Beer-Sheva 84190, Israel;
NRCN,
Beer-Sheva 84190, Israel;
Department of Atmospheric,
Oceanic, and Space Sciences,
University of Michigan,
Ann Arbor, MI 48109
Oceanic, and Space Sciences,
University of Michigan,
Ann Arbor, MI 48109
Search for other works by this author on:
Guy Malamud,
Guy Malamud
Department of Physics,
NRCN,
Beer-Sheva 84190, Israel;
NRCN,
Beer-Sheva 84190, Israel;
Department of Atmospheric,
Oceanic, and Space Sciences,
University of Michigan,
Ann Arbor, MI 48109
Oceanic, and Space Sciences,
University of Michigan,
Ann Arbor, MI 48109
Search for other works by this author on:
Carlos A. Di Stefano,
Carlos A. Di Stefano
Department of Atmospheric,
Oceanic, and Space Sciences,
University of Michigan,
Ann Arbor, MI 48109;
Oceanic, and Space Sciences,
University of Michigan,
Ann Arbor, MI 48109;
Los Alamos National Laboratory,
Los Alamos, NM 87507
Los Alamos, NM 87507
Search for other works by this author on:
Carolyn C. Kuranz,
Carolyn C. Kuranz
Department of Atmospheric,
Oceanic, and Space Sciences,
University of Michigan,
Ann Arbor, MI 48109
Oceanic, and Space Sciences,
University of Michigan,
Ann Arbor, MI 48109
Search for other works by this author on:
R. P. Drake
R. P. Drake
Department of Atmospheric,
Oceanic, and Space Sciences,
University of Michigan,
Ann Arbor, MI 48109
Oceanic, and Space Sciences,
University of Michigan,
Ann Arbor, MI 48109
Search for other works by this author on:
Assaf Shimony
Department of Physics,
NRCN,
Beer-Sheva 84190, Israel;
NRCN,
Beer-Sheva 84190, Israel;
Dov Shvarts
Department of Physics,
NRCN,
Beer-Sheva 84190, Israel;
NRCN,
Beer-Sheva 84190, Israel;
Department of Atmospheric,
Oceanic, and Space Sciences,
University of Michigan,
Ann Arbor, MI 48109
Oceanic, and Space Sciences,
University of Michigan,
Ann Arbor, MI 48109
Guy Malamud
Department of Physics,
NRCN,
Beer-Sheva 84190, Israel;
NRCN,
Beer-Sheva 84190, Israel;
Department of Atmospheric,
Oceanic, and Space Sciences,
University of Michigan,
Ann Arbor, MI 48109
Oceanic, and Space Sciences,
University of Michigan,
Ann Arbor, MI 48109
Carlos A. Di Stefano
Department of Atmospheric,
Oceanic, and Space Sciences,
University of Michigan,
Ann Arbor, MI 48109;
Oceanic, and Space Sciences,
University of Michigan,
Ann Arbor, MI 48109;
Los Alamos National Laboratory,
Los Alamos, NM 87507
Los Alamos, NM 87507
Carolyn C. Kuranz
Department of Atmospheric,
Oceanic, and Space Sciences,
University of Michigan,
Ann Arbor, MI 48109
Oceanic, and Space Sciences,
University of Michigan,
Ann Arbor, MI 48109
R. P. Drake
Department of Atmospheric,
Oceanic, and Space Sciences,
University of Michigan,
Ann Arbor, MI 48109
Oceanic, and Space Sciences,
University of Michigan,
Ann Arbor, MI 48109
1Corresponding author.
Contributed by the Fluids Engineering Division of ASME for publication in the JOURNAL OF FLUIDS ENGINEERING. Manuscript received January 31, 2015; final manuscript received August 15, 2015; published online April 12, 2016. Assoc. Editor: Praveen Ramaprabhu.
J. Fluids Eng. Jul 2016, 138(7): 070902 (7 pages)
Published Online: April 12, 2016
Article history
Received:
January 31, 2015
Revised:
August 15, 2015
Citation
Shimony, A., Shvarts, D., Malamud, G., Di Stefano, C. A., Kuranz, C. C., and Drake, R. P. (April 12, 2016). "The Effect of a Dominant Initial Single Mode on the Kelvin–Helmholtz Instability Evolution: New Insights on Previous Experimental Results." ASME. J. Fluids Eng. July 2016; 138(7): 070902. https://doi.org/10.1115/1.4032530
Download citation file:
Get Email Alerts
Cited By
Related Articles
A Numerical Model for the Analysis of the Locomotion of a Cownose Ray
J. Fluids Eng (March,2022)
Effect of Process Parameters on Wavy Interfacial Morphology During Magnetic Pulse Welding
J. Manuf. Sci. Eng (January,2021)
Related Proceedings Papers
Related Chapters
Thermal Interface Resistance
Thermal Management of Microelectronic Equipment
Cavitating Structures at Inception in Turbulent Shear Flow
Proceedings of the 10th International Symposium on Cavitation (CAV2018)
Experimental and Numerical Investigation of Vortex Dynamics in Ventilated Cavitating Flows Around a Bluff Body
Proceedings of the 10th International Symposium on Cavitation (CAV2018)