Because of their directional properties, ellipsoidal dish-microphones (elliptic mirrors) have proved useful for locating noise sources in aeroacoustic flows. A scan of the source region produces a source map. It is customary to interpret a source map as a slightly blurred but otherwise faithful representation of the underlying source distribution. The spatial distribution of the sound pressure level is assumed to represent the main features of the layout and relative strengths of the sources. In this paper, we discuss a number of factors that introduce distortions or aberrations in the transformation from source strength distribution to source map. When aberrations are operative, a source map can convey misleading information about the source distribution. Some aberrations are related to test setup, and we show that these are fairly simple to avoid or correct for. However, a more fundamental distortion is induced by source spatial correlation or directivity. This is discussed using a discrete model of a source distribution. Finally, it is shown that for uncorrelated source clusters, aggregate source strength may be estimated by direct area-integration of a source map. (Author) Page 1 Downloaded by CORNELL UNIVERSITY on July 30, 2015 | http://arc.aiaa.org |
Abstract
Because of their directional properties, ellipsoidal dish-microphones (elliptic mirrors) have proved useful for locating noise sources in aeroacoustic flows. A scan of the source region produces a source map.It is customary to interpret a source map as a slightly blurred but otherwise faithful representation of the underlying source distribution: the spatial distribution of sound pressure level is assumed to represent the main features of the layout and relative strengths of the sources. In this paper, we discuss a number of factors that introduce distortions or aberrations in the transformation from source strength distribution to source map. When aberrations are operative, a source map can convey misleading information about the source distribution. Some aberrations are related to test setup, and we show that these are fairly simple to avoid or correct for. However, a more fundamental distortion is induced by source spatial correlation or directivity. This is discussed using a discrete model of a source distribution. Finally, it is shown that for uncorrelatedsourceclusters,aggregatesourcestrength may be estimated by direct area-integration of a source map.