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Fast Fourier transform of sparse spatial data to sparse Fourier data

机译:将稀疏空间数据快速傅里叶变换为稀疏傅里叶数据

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The nonuniform fast Fourier transform (FFT) on a line has been of interest to a number of scientists for its practical applications. However, not much has been written on Fourier transforming sparse spatial data where the Fourier transform is needed at only sparse data points in the Fourier space in 2D or 3D. It finds applications in remote sensing, inverse problems, and synthetic aperture radar where the scattered field is related to the Fourier transform of the scatterers. We outline an algorithm to perform this transform in NlogN operations, where N is the number of spatial data available, and we assume that the number of Fourier data desired is also of O(N). The algorithm described here is motivated by the multilevel fast multipole algorithm (MLFMA), but is different from that described by Brandt (1991). In MLFMA, an embedded fast Fourier transform algorithm is inherent, where the spatial data is arbitrarily distributed, but the Fourier data is required on the Ewald sphere. In the present algorithm, the restriction of the Fourier data to an Ewald sphere is lifted so that it can be arbitrarily distributed as well. The present algorithm can be easily generalized to 3D.
机译:在线上的非均匀快速傅立叶变换(FFT)已因其实际应用而受到许多科学家的关注。但是,关于傅立叶变换稀疏空间数据的文章很少,其中仅需要在2D或3D傅立叶空间中的稀疏数据点处进行傅立叶变换。它可用于遥感,反问题和合成孔径雷达,其中散射场与散射体的傅立叶变换有关。我们概述了一种在NlogN操作中执行此变换的算法,其中N是可用空间数据的数量,并且我们假设所需的傅立叶数据的数量也为O(N)。此处描述的算法受多级快速多极算法(MLFMA)的启发,但与Brandt(1991)所描述的算法不同。在MLFMA中,固有的是嵌入式快速傅里叶变换算法,其中空间数据是任意分布的,但是在Ewald球体上需要傅里叶数据。在本算法中,将傅里叶数据对Ewald球的限制解除了,因此它也可以任意分布。本算法可以很容易地推广到3D。

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