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BDT Radio – 2a – CMV 2009/10/06 Basic Detection Techniques 2a (2009/10/06): Array antennas Theory: interferometry & synthesis arrays Introduction Optical.

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Presentation on theme: "BDT Radio – 2a – CMV 2009/10/06 Basic Detection Techniques 2a (2009/10/06): Array antennas Theory: interferometry & synthesis arrays Introduction Optical."— Presentation transcript:

1 BDT Radio – 2a – CMV 2009/10/06 Basic Detection Techniques 2a (2009/10/06): Array antennas Theory: interferometry & synthesis arrays Introduction Optical interferometry, coding of phase Radio interferometry, aperture synthesis Briefly: calibration Theory: aperture arrays & phased array feeds Beamforming Basics Sparse & dense arrays

2 BDT Radio – 2a – CMV 2009/10/06

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6 MIDI

7 BDT Radio – 2a – CMV 2009/10/06

8 1971

9 BDT Radio – 2a – CMV 2009/10/06 Correlatie functies

10 BDT Radio – 2a – CMV 2009/10/06 Spectra

11 BDT Radio – 2a – CMV 2009/10/06 Aperture synthesis (4 hours, 45 deg dec)

12 BDT Radio – 2a – CMV 2009/10/06 Less sample points

13 BDT Radio – 2a – CMV 2009/10/06 Splitting the dots

14 BDT Radio – 2a – CMV 2009/10/06 Dynamic Modelling

15 BDT Radio – 2a – CMV 2009/10/06 Ongecalibreerd beeld

16 BDT Radio – 2a – CMV 2009/10/06 Gecalibreerd beeld

17 BDT Radio – 2a – CMV 2009/10/06 Redundancy XX YY Amplitude on 2 identical baselines of about 400m at 60 MHz Fringes CasA stopped, CygA shows as oscillation

18 BDT Radio – 2a – CMV 2009/10/06 Dynamic Modelling Global Sky Model Environment Model Instrument Model Sensor Data “Predict” (simulated data) “Solve”

19 BDT Radio – 2a – CMV 2009/10/06

20 Connecting Europe …

21 BDT Radio – 2a – CMV 2009/10/06

22 Aperture arrays

23 BDT Radio – 2a – CMV 2009/10/06 System level Overview

24 BDT Radio – 2a – CMV 2009/10/06 Sparse & dense Definition: Dense array: element spacing < λ/2 Sparse array: element spacing > λ/2

25 BDT Radio – 2a – CMV 2009/10/06 Grating lobes

26 BDT Radio – 2a – CMV 2009/10/06 Element spacinig Criterion for maximum element spacing grating lobes at the horizon Example: an array scanning up to θ = 30° requires d < 0.53 λ to avoid grating lobes

27 BDT Radio – 2a – CMV 2009/10/06 Element configuration

28 BDT Radio – 2a – CMV 2009/10/06 Array patterns LOFAR Station beams

29 BDT Radio – 2a – CMV 2009/10/06 Effective area

30 BDT Radio – 2a – CMV 2009/10/06 Beamforming Ideally, time delays are required For practical reasons, phase shifters are used For a single frequency: same effect Offset frequencies result in beam squint (similar to scanning)

31 BDT Radio – 2a – CMV 2009/10/06 Effect of beamsquint

32 BDT Radio – 2a – CMV 2009/10/06 True time delay beamformer (photonic)

33 BDT Radio – 2a – CMV 2009/10/06 Polyphase Filter Digital Controls Buffer amplifiersSwitches for combining Output amplifier Pads for probing


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