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FP7 Uniboard project

Digital Receiver G. Comoretto, A. Russo, G. Tuccari, A Baudry, P. Camino, B. Quertier Dwingeloo, February 27, 2009. FP7 Uniboard project. Framework. Wideband radioastronomy receivers Instantaneous BW 4-12 GHz Digitizers: current 1-2 GHz, near future 4-8 GHz

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FP7 Uniboard project

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  1. Digital Receiver G. Comoretto, A. Russo, G. Tuccari, A Baudry, P. Camino, B. Quertier Dwingeloo, February 27, 2009 FP7 Uniboard project

  2. Framework • Wideband radioastronomy receivers • Instantaneous BW 4-12 GHz • Digitizers: current 1-2 GHz, near future 4-8 GHz • Digital hardware: limited by clock, 100-300 MHz bandwidth → Need for frequency multiplexing • Multibeam receivers • Tens → hundreds of pixels 7 feed FP5 Faraday receiver

  3. Existing systems DBBC • DBBC • 4x 1GHz BW, up to 16 Virtex5 cores • EVN standard: 4 cores = VLBI terminal • DBBC3: wider band ADC3 & V.6 core • MPI-Agilent FFT Spectrometer • 1 GHz BW, Virtex4 core • Up to 8 boards on a PCI bus • Casper • Up to 1.5 GHz BW, 1x (IBOB) or 5 x Virtex2 (BEE2) • ROACH: Virtex-5 based Avoid duplications! Keep an open path to future apps & HW ROACH

  4. Specifications • Input: • Bandwidth: 4 GHz (8 GS/s) • Quantization: 6 bit minimum (8 bit possible) • Future development, 2-3 yrs: 8 GHz 4-6 bit • Format: data on several 10G links, one sample per link, time multiplexed • Output: • Bandwidth: up to 64 MHz/channel (128 MS/s), up to 64 channels • Quantization: 1, 2, 4, 8 bit • Format: Standard MK5C format, UDP packets, on 10G links • Each channel position and BW independently selectable (with limitations) • Everything fits in a single board

  5. General structure • Two stage filter • 1st stage: • Polyphase FFT • real input • 32x250MHz complex output, divided into 8 groups • 125 MHz channel spacing • 2nd stage: • Tunable filter: LO/mixer, low-pass FIR, complex-to-real • 4 sets of 16 FIRs • Each set selects input among a 1st stage channel group

  6. High SFDR using polyphase filter • 8 GHz BW likely affected by RFI • RFI mitigation by excision of affected spectral region • Good chan.-to-chan. rejection to avoid contamination • 18 bit multipliers: limit to ~85 dB SFDR • Filter design: 85 dB stopband • 96% useful BW, 0.04 dB ripple • >90 dB with 94% BW channel 1 channel 2 channel 3 Out BW Channels overlapped to avoid holes

  7. How to fit in the Uniboard • Uniboard structure: • 4 input + 4 output FPGAs • Each FPGA has 2x10G in/out • No vertical interconnect • 4x4 fixed interconnect between input and output FPGAs • 2.5 Gbps per link • 250 MS/s @ 8 bit

  8. 2 stage DIT FFT • Decimation in time FFT algorithm: • separate data flow for parallel decimated samples • Limitation in interconnections: only selected channels processed

  9. Channels and groups 32 overlapping channels ½ channel spacing Channels are grouped in groups of 4 Groups 0, 1, 2, 3 Groups 4, 5, 6, 7 Up to 4 groups available at each time: segmented coverage of whole 4 GHz (with edge holes, ~4% lost) or continuous coverage of narrower band

  10. 8 bit between stages enough? • Limited BW between input and output FPGAs: max 256MS @ 8 bit per link • Requantization with 8 bit may degrade SFDR • Tests with Gaussian noise + spectral line in 1 channel • > 80 dB SFDR observed

  11. 2nd stage FIR • Derived from ALMA Tunable Filterbank • Variable Decimation FIR Filter: D=2-256 • Taps: 32*D, tap recirculation, symmetric • 32 (2x16, real-imaginary) multipliers Output conversion to real by ½ band shift Specifications TBD. • Example from ALMA design • 18 bit required for high rejection • Tradeoff between complexity and performances Example: filter performance for 9 bit, 94% BW, 16 multipliers ½ to 1/256 BW

  12. Conclusions • 4 GHz BW, 64 tunable channels system feasible in a single Uniboard • 4x1GHz bypassing 2nd butterfly (but easier w. DBBC!) • 8 GHz BW feasible (Phase 2 of the project) • >80 dB spurious free dynamic range (may improve) • Applications • Front-end for other systems • VLBI channelization system • FFT very wide band spectrometer (e.g. 4GHz 64k pts)

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