Bluering Prototype System Results
- G. Hampson, W. Cheng,
- D. Humphrey, J. Bunton,
- P. Roberts, K. Bengston,
- R. Beresford, Y. Chen,
- R. Chekkala
22nd September 2020
RadioNet Workshop: Future Trends in Radio Astronomy Instrumentation
Bluering Prototype System Results G. Hampson, W. Cheng, D. - - PowerPoint PPT Presentation
Bluering Prototype System Results G. Hampson, W. Cheng, D. Humphrey, J. Bunton, P. Roberts, K. Bengston, R. Beresford, Y. Chen, R. Chekkala 22 nd September 2020 RadioNet Workshop: Future Trends in Radio Astronomy Instrumentation Bluering
22nd September 2020
RadioNet Workshop: Future Trends in Radio Astronomy Instrumentation
○ Using “RFSOC” = Radio Frequency System On Chip ○ Tailored RF front end to suit most types of astronomy antenna systems ○ Coax connected to enable high dynamic range RF front ends that can be operated with RFI
DSP FPGA too
○ Can beamform at the antenna (if only limited # of beams) ○ Can calculate correlations, time pulsars, and RFI mitigation
efficient receiver
○ Optical clocks and control ○ Optical data path out
19” Rack
(containing the RFSOC), plus supporting equipment
M&C Server Razorback (RFSOC) Razorback (RFSOC) Optical Circuit AC-to-48V Cooling Irukandji White Rabbit Master WR Slave Link to DSP Backend Coax (2 per antenna) Fibre (WR, 1GbE,
*GbE)
# Remote Systems
○ Synthesizer for ADC sample clock and LO generation ○ DDR4 for transient data capture (raw, filterbank, beam, …) ○ MBO for 10GbE ring/star beamformer data, 1GbE, timing and calibration signals ○ Q/SFP for beam output (short or long distance)
○ Timing, Calibration, 1GbE (M&C) 48/ 12V 48V (Isolated) 32 RF Signals (coax) 32 RF Chains MBO RFSOC DDR4 DC/DC Q/SFP To beamformer/ correlator/ capture Synth
Taipan
Network, Timing, Calibration
Irukandji
RAZORBACK
Optical Beamformer Network
○ 16 RF customisable modules (coax/RFOF, frequency, gain, etc.)
○ 40/100GbE QSFP ○ 10/25GbE SFP ○ 12x10GbE MBO
○ 2560 channel oversampled filterbank ○ 2GSPS results in 781kHz channels (926kSPS)
○ 1GbE M&C (SFP) ○ Reference (125MHz) ○ 1 pulse-per-second ○ Calibration signal
○ Also SDcard and 8GB iNAND
x8x2
and distribution
extend dynamic range - a 12dB improvement
architecture to sample both polarisations in the same ADC
To Dual Pol Antenna (power over coax) LPF C LPF C BPF RFSOC ADC 125MHz Reference PLL PLL 875MHz 2000MHz 12-bits to DSP x16 for RFSOC Taipan RF board
Calibration Signal
RF X 5V-LNA RF Y Cal LO 5V-LO Y-attenuator X-attenuator RF out (to final amplifier and ADC) 5V-RF
Taipan
○ (purple hashed section in drawing)
($1) for first and second stage amplification
final amp and balun
ADC Noise
○ SNR is -150dBFS/Hz or
○ SFDR is 85dB ○
https://www.xilinx.com/support/docu mentation/data_sheets/ds926-zynq- ultrascale-plus-rfsoc.pdf
spurious
○ IM2 just as important as IM3
ADC input level for 300MHz Sky is -33dBm
○ Can still adjust up and down further with attenuator depending on RFI ADC SNR 60dB ADC SFDR 85dB ADC Full Scale +1dBm Sky noise (300MHz BW) ADC Spurious RFI Spurious Sky 1MHz 25dB 32dB RFI IM2 spurious -50dBc RFI IM3 spurious -89dBc Sky (1MHz BW) 32dB 13dB ADC IM2 85dB ADC IM3 78dB RFI Average 17dB
Slope
Cal Signal
○ Seems to be everywhere - even the MWA site has FM at times
Spatial filtering experiment with the Murchison Widefield Array - G.Hellbourg & I. Morrison, URSI GASS 2020
ADC Capture FB Capture 2GS ADC Coarse Filter bank Quantise, Select & Packetise 10/100 GbE 16-RF Beamformer ADC Statistics Spectrum Maxhold IO Processor & AXI IF Irukandji Attenuators 1pps /BAT 1GbE ADC Sync To PLL 128MHz SysMon monitoring Test Signals Test Packets
LMK04610 Clock Jitter Cleaner CVHD-950 Ultra-Low Phase Noise Oscillator 125MHz 125MHz 125MHz 125MHz 125MHz LMX2594 RF Synthesizer LMX2594 RF Synthesizer ECUO Firefly Rx ECUO Firefly Rx 1pps Manchester Encoded ZU29DR Decode Sync Pulse LMK00304 Differential Clock Buffer LMK00304 Differential Clock Buffer SC4PS-33+ RF Splitter ZU29DR ADC Clocks ZU29DR SysRef & Logic Sync Pulse 2GHz ECUO Firefly Rx High Isolation Resistive RF Splitter Calibration Taipan RF Receivers
875 MHz
with 16x2560 FIR taps
○ Using sample clock 2000MHz results in 721kHz channels ○ Can be modified to suit your application
○ LUTs : 122911 (29%) ○ DSPs : 2112 (49%) ○ 36K BRAMs : 568 (53%)
○ Measure slightly less (data dependent)
liquid cooling
leaks - good performance
and >150dB in the double
○ Gets very hard to measure
is filtered many times
configurations - so getting the first ADC samples out is a particularly pleasing moment in time!
is locked to the 125MHz reference clock) is input into the ADC
○ RF in is -20dB and ADC SNR is 60dB, so about 40dB above noise floor ○ But processing gain reduce level of noise by 10log10(16384) = 42dB ○ So peak to noise floor is 40+42=~82dB ○ Measure 155-75=80dB so levels close to right for a first measurement 80dB
○ Wrong values, wrong side, or just missing
○ Originally MBO + QSFP + SFP cages ○ Moving to quad QSFP - similar to Jimble (another CSIRO RFSOC receiver) ○ Enables more data output options ○ QSFP’s are lower cost than MBO now - as it's more of a COTS product
○ Moving away from ganged RF connector to SMA ○ Using a surface mount connector to improve RF over wider frequency range
○ Originally soldered in and potentially difficult to replace ○ Now moving to MMBX solution to enable easy replacement/upgrades
Many thanks to Wan, Keith and David
the Australia Telescope
array arms
at the Australia Telescope
https://i-love-png.com/images/octopus-tentacles-png-photos.png