TY - GEN
T1 - Design of a LabVIEW-based polyphase filter bank spectrometer for radio astronomy using FlexRIO FPGA technology and CUDA-enabled GPU
AU - Freundt, Rodrigo G.
AU - Heraud, Jorge A.
N1 - Publisher Copyright:
© 2017 URSI.
PY - 2017/11/10
Y1 - 2017/11/10
N2 - The spectrometer is the most important back-end in single antenna radio astronomy observations. The state-of-the-art designs for this type of instruments propose to reduce the effects of spectral leakage by using the Polyphase Filter Bank (PFB) technique and to achieve wideband and high resolution by using digital, reconfigurable, and high-performance computing hardware, such as commercial-available FPGA and GPU. We herein describe the development of a prototype PFB spectrometer using an integrated hardware and software development environment from National Instruments (Nl), along with FlexRIO FPGA technology for acquisition and CUDA-enabled GPU card for intensive processing. The results show that the proposed design, configured as a 4-tap PFB with 222 channels and 200MHz instantaneous bandwidth, is 95 times faster than a CPU implementation. It can be concluded that the hardware and software design approach used to prototype the spectrometer in this paper must be further studied within radio astronomy applications.
AB - The spectrometer is the most important back-end in single antenna radio astronomy observations. The state-of-the-art designs for this type of instruments propose to reduce the effects of spectral leakage by using the Polyphase Filter Bank (PFB) technique and to achieve wideband and high resolution by using digital, reconfigurable, and high-performance computing hardware, such as commercial-available FPGA and GPU. We herein describe the development of a prototype PFB spectrometer using an integrated hardware and software development environment from National Instruments (Nl), along with FlexRIO FPGA technology for acquisition and CUDA-enabled GPU card for intensive processing. The results show that the proposed design, configured as a 4-tap PFB with 222 channels and 200MHz instantaneous bandwidth, is 95 times faster than a CPU implementation. It can be concluded that the hardware and software design approach used to prototype the spectrometer in this paper must be further studied within radio astronomy applications.
UR - http://www.scopus.com/inward/record.url?scp=85046278356&partnerID=8YFLogxK
U2 - 10.23919/URSIGASS.2017.8105039
DO - 10.23919/URSIGASS.2017.8105039
M3 - Conference contribution
AN - SCOPUS:85046278356
T3 - 2017 32nd General Assembly and Scientific Symposium of the International Union of Radio Science, URSI GASS 2017
SP - 1
EP - 4
BT - 2017 32nd General Assembly and Scientific Symposium of the International Union of Radio Science, URSI GASS 2017
PB - Institute of Electrical and Electronics Engineers Inc.
T2 - 32nd General Assembly and Scientific Symposium of the International Union of Radio Science, URSI GASS 2017
Y2 - 19 August 2017 through 26 August 2017
ER -