1 / 23

The Correlators ( Spectrometers ) Mopra Induction - May 2005

The Correlators ( Spectrometers ) Mopra Induction - May 2005. Frequency Conversion. Mixer. RF. IF. LO. RF. IF. LSB. LO. USB. Frequency. Sampling. Filter. Sampler. Digitiser. IF. N. Sampling Clock. SCLK. BB. LSB. USB. Baseband. Frequency. IF Frequency. 01. 00. 10. 11.

zena-kemp
Download Presentation

The Correlators ( Spectrometers ) Mopra Induction - May 2005

An Image/Link below is provided (as is) to download presentation Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author. Content is provided to you AS IS for your information and personal use only. Download presentation by click this link. While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server. During download, if you can't get a presentation, the file might be deleted by the publisher.

E N D

Presentation Transcript


  1. The Correlators( Spectrometers )Mopra Induction - May 2005

  2. Frequency Conversion Mixer RF IF LO RF IF LSB LO USB Frequency

  3. Sampling Filter Sampler Digitiser IF N Sampling Clock SCLK BB LSB USB Baseband Frequency IF Frequency

  4. 01 00 10 11 Digitisation V=0

  5. Coarse digitisers -> Quantisation noise • S/N compared to ideal: • 1-bit digitiser - 66% • 2-bit 3-level - 82% • 2-bit 4-level - 88%

  6. Digital Spectrometer Types • Autocorrelation spectrometer (correlator) • well established • Polyphase Digital Filter Bank • new development

  7. Autocorrelation spectrometer (Correlator) Power Spectrum -- Autocorrelation Function

  8. C C C C C C C C C C C C C C C C C C C C C C = multiply and accumulate Digital Correlator INPUT 1 INPUT 2 ---- -9 -8 -7 -6 -5 -4 -3 -2 -1 0 +1 +2 +3 +4 +5 +6 +7 +8 +9 ----- Lag (delay) in samples

  9. Synthesis Array Correlators • XF • For each baseline ( ~N2 ) : • Form cross correlation function • FT to form spectrum • FX • For each signal ( ~N ) : • Form spectrum • For each baseline ( ~N2 ) : • Multiply corresponding frequencies

  10. FX correlator has advantages for large N arrays • Preferred scheme for SKA - very large N • Key SKA technology • Demonstrate in upgrade of ATCA - CABB • - increase max. bandwidth from 128MHz to 2GHz • - 2048 channels • Funded under MNRF2001

  11. FX • For each signal ( ~N ) : • Form spectrum • For each baseline ( ~N2 ) : • Multiply corresponding frequencies

  12. x (m) X (m) 0 0 0 x (m) X (m) 1 1 1 M-Point x n DFT X (m) x (m) via ρ k ρ FFT X (m) x (m) M-1 M-1 M-1 Fourier Transform Spectrometer

  13. Polyphase Digital Filterbank

  14. Implemented in FPGAs • Field Programmable Gate Arrays • Large commercially available chips containing many tens of thousands of re-configurable logic cells, plus memory and digital multipliers. • Clock rates of up to 300MHz.

  15. Conventional Channelisation

  16. Filterbank Channelisation

  17. ZOOM • Standard • Zoom • n*Zoom • n*Zoom^m

  18. Autocorrelator : • 2-bit bandwidths 4MHz to 128MHz • At 4MHz BW - up to 16,000 frequency channels • At 128MHz BW - up to 256 frequency channels • 1-bit bandwidth 256MHz - up to 512 channels • Digital Filterbank : • July 2004 - 256MHz BW - 1024 channels • July 2005 - 600MHz BW - 1024 (2048?) channels • Sep 2005(??) - 2GHz BW - 2048 channels • Next season - 8GHz - 8192 channels

  19. 4-12 GHz IF from mm Receiver E/O Vertex Room Control Room IF UNIT SAMPLER SAMPLER SAMPLER SAMPLER DIGITAL FILTER BANK DIGITAL FILTER BANK DIGITAL FILTER BANK DIGITAL FILTER BANK 4 * ( 2GHz BW, 2048 ch. ) Mopra 8GHz DFB Spectrometer

  20. Polyphase Digital Filter Bank Spectrometer- using commercial hardware

  21. ATNF 2 x 2GHz DFB PCB - CABB Prototype PCB: 28,600 Pads 136,000 Track segments 18,800 holes 2,300 components 12 signal layers 9 power layers 17 Xilinx FPGAs Each FPGA: 21,000 Logic Cells 1.6Mbit RAM 88 18x18 multipliers 564 I/O signals 1152 pin BGA 12U

More Related