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The maximum noise radiation angle from supersonic jet turbulence is controlled by Mach wave radiation. We explore different definitions of the turbulence convective Mach number, using far-field noise from the T-7A and other jet data. A simpler, data-driven definition of convective Mach number predicts the T-7A noise radiation angles over a range of thrust conditions as well as the analytical expression for Kelvin-Helmholtz instability waves.

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This page is a summary of: Convective Mach Number and Full-Scale Supersonic Jet Noise Directivity, AIAA Journal, December 2024, American Institute of Aeronautics and Astronautics (AIAA),
DOI: 10.2514/1.j064208.
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