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Initial Integration of Noise Prediction Tools for Acoustic Scattering EffectsThis effort provides an initial glimpse at NASA capabilities available in predicting the scattering of fan noise from a non-conventional aircraft configuration. The Aircraft NOise Prediction Program, Fast Scattering Code, and the Rotorcraft Noise Model were coupled to provide increased fidelity models of scattering effects on engine fan noise sources. The integration of these codes led to the identification of several keys issues entailed in applying such multi-fidelity approaches. In particular, for prediction at noise certification points, the inclusion of distributed sources leads to complications with the source semi-sphere approach. Computational resource requirements limit the use of the higher fidelity scattering code to predict radiated sound pressure levels for full scale configurations at relevant frequencies. And, the ability to more accurately represent complex shielding surfaces in current lower fidelity models is necessary for general application to scattering predictions. This initial step in determining the potential benefits/costs of these new methods over the existing capabilities illustrates a number of the issues that must be addressed in the development of next generation aircraft system noise prediction tools.
Document ID
20080018651
Acquisition Source
Langley Research Center
Document Type
Conference Paper
Authors
Nark, Douglas M.
(NASA Langley Research Center Hampton, VA, United States)
Burley, Casey L.
(NASA Langley Research Center Hampton, VA, United States)
Tinetti, Ana
(NCI Information Systems, Inc. United States)
Rawls, John W.
(Lockheed Martin Corp. United States)
Date Acquired
August 24, 2013
Publication Date
May 5, 2008
Subject Category
Acoustics
Meeting Information
Meeting: 14th AIAA/CEAS Aeroacoustics Conference
Location: Vancouver
Country: Canada
Start Date: May 5, 2008
End Date: May 7, 2008
Sponsors: American Inst. of Aeronautics and Astronautics, Confederation of European Aerospace Societies
Funding Number(s)
WBS: WBS 561581.02.08.07.18.03
Distribution Limits
Public
Copyright
Public Use Permitted.
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