NASA NTRS · 20120013789
Implementation of a Digital Signal Processing Subsystem for a Long Wavelength Array Station
Abstract
This paper describes the implementation of a Digital Signal Processing (DP) subsystem for a single Long Wavelength Array (LWA) station.12 The LWA is a radio telescope that will consist of many phased array stations. Each LWA station consists of 256 pairs of dipole-like antennas operating over the 10-88 MHz frequency range. The Digital Signal Processing subsystem digitizes up to 260 dual-polarization signals at 196 MHz from the LWA Analog Receiver, adjusts the delay and amplitude of each signal, and forms four independent beams. Coarse delay is implemented using a first-in-first-out buffer and fine delay is implemented using a finite impulse response filter. Amplitude adjustment and polarization corrections are implemented using a 2x2 matrix multiplication
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Soriano, Melissa, Navarro, Robert, D'Addario, Larry, Sigman, Elliott, Wang, Douglas. 2011-03-05. Implementation of a Digital Signal Processing Subsystem for a Long Wavelength Array Station. https://ntrs.nasa.gov/citations/20120013789
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