1 / 14

Phased-Array Feed Measurements at Green Bank

Phased-Array Feed Measurements at Green Bank. Karl Warnick , Brian Jeffs Jonathan Landon, Mike Elmer Roger Norrod , Rick Fisher. R&D Challenges. Technical Mutual coupling Receiver/element noise Calibration Total bandwidth Cost Drivers Receiver system complexity Signal processing.

badu
Download Presentation

Phased-Array Feed Measurements at Green Bank

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. Phased-Array Feed Measurements at Green Bank Karl Warnick, Brian Jeffs Jonathan Landon, Mike Elmer Roger Norrod, Rick Fisher

  2. R&D Challenges • Technical • Mutual coupling • Receiver/element noise • Calibration • Total bandwidth • Cost Drivers • Receiver system complexity • Signal processing

  3. 20-Meter Experiments • October 2007 • Tsys ~150K • July-August 2008 • LNA Ta = 30K, Tsys ~65K • Sky noise measurements • Direct Control of 20-m • ~1600 MHz, 0.5 MHz BW • 19 A/D samplers to disk • Software beam-forming

  4. Matching network G0 Mutual Coupling Effects • Changes element impedances • Beam-dependent • Couples amplifier noise • Changes element patterns • All frequency dependent

  5. Noise Budget MeasuredModel LNA Tmin33 K 33 K Noise coupling 20 K 23 K Spillover 5 K 5 K Sky 3 K 3 K Loss 4 K -- Tsys: 65 K 64 K Noise matching efficiency 60% Noise Matching Efficiency = 60% ---------- ----------

  6. Calibration • Optimize Ta/Tsys at each beam position in the FOV • Use strong radio source • R = cross-correlation matrix of all elements on and off source • w = beam-forming complex weights • λmax = highest eigenvalue corresponding to the dominant eigenvector of Roffw • Experience thus far is that calibration is stable for hours and possibly days in the experimental setup. • Calibration method does not distinguish between various noise and efficiency factors.

  7. Cygnus-X Region Mosaic Canadian Galactic Plane Survey Convolved to 20-m Beam

  8. RFI Cancellation with Array Processing

  9. Steps Toward a Cooled PFA

  10. Cool the Element Antennas? Polystyrene cover – low loss, low k, and strong enough, but outgassed heavily. Machined PTFE cover – low loss, moderate k, strong.

  11. Cool the Antenna Elements? So, PTFE vacuum cover is probably workable but concerns remain: Radiation loading, scattering, loss, robustness, interface with ground plane. Stress analysis Too thin cover after ~1mo under vacuum. PTFE creep.

  12. Noise Budget ~20cm

  13. Warm Antenna Elements?

  14. Test Facility Summer ‘08 New absorber in retractable roof, surveyed local obstacles and ground shield EM models for spillover estimation.

More Related