Abstract:I• is well known that to obtain very s•nall side lobe radiation the amplitude distribution across a radiating surface should be such that the maximum mnplitude is at the center and the minimum at the edges. The Gaussian distribution gives no side lobes, but requires an infinitely large radiator. This paper gives the analysis of the clampededge disk, vibrating in its first normal mode. It shows that the dynamic curve approximates the Gaussian form and that the sound pressure distribution has very small side lob… Show more
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