Experimental Observations of Laser-Driven Tin Ejecta Microjet Interactions

The study of high-velocity particle-laden flow interactions is of importance for the understanding of a wide range of natural phenomena, ranging from planetary formation to cloud interactions. Experimental observations of particle dynamics are sparse given the difficulty of generating high-velocity...

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Veröffentlicht in:Physical review letters 2021-10, Vol.127 (15), p.1-155002, Article 155002
Hauptverfasser: Saunders, A. M., Stan, C. V., Mackay, K. K., Morgan, B., Horwitz, J. A. K., Ali, S. J., Rinderknecht, H. G., Haxhimali, T., Ping, Y., Najjar, F., Eggert, J., Park, H.-S.
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Sprache:eng
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Zusammenfassung:The study of high-velocity particle-laden flow interactions is of importance for the understanding of a wide range of natural phenomena, ranging from planetary formation to cloud interactions. Experimental observations of particle dynamics are sparse given the difficulty of generating high-velocity flows of many particles. Ejecta microjets are micron-scale jets formed by strong shocks interacting with imprinted surfaces to generate particle plumes traveling at several kilometers per second. As such, the interaction of two ejecta microjets provides a novel experimental methodology to study interacting particle streams. In this Letter, we report the first time sequences of x-ray radiography images of two interacting tin ejecta microjets taken on a platform designed for the OMEGA Extended Performance (OMEGA EP) laser. We observe that the microjets pass through each other unattenuated for the case of 11.7 ± 3.2 GPa shock pressures and jet velocities of 2.2 ± 0.5 km / s but show strong interaction dynamics for 116.0 ± 6.1 GPa shock pressures and jet velocities of 6.5 ± 0.5 km / s . We find that radiation-hydrodynamic simulations of the experiments are able to capture many aspects of the collisional behavior, such as the attenuation of jet velocity in the direction of propagation, but are unable to match the full spread of the strongly interacting cloud.
ISSN:0031-9007
1079-7114
DOI:10.1103/PhysRevLett.127.155002