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Chalmers University of Technology Development of a Coolable Decade Bandwidth Eleven Feed System for SKA & VLBI 2010 Radio Telescopes Per-Simon Kildal Chalmers.

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Presentation on theme: "Chalmers University of Technology Development of a Coolable Decade Bandwidth Eleven Feed System for SKA & VLBI 2010 Radio Telescopes Per-Simon Kildal Chalmers."— Presentation transcript:

1 Chalmers University of Technology Development of a Coolable Decade Bandwidth Eleven Feed System for SKA & VLBI 2010 Radio Telescopes Per-Simon Kildal Chalmers University of Technology Gothenburg, SWEDEN 15 cm diameter for 2-13 GHz

2 Chalmers University of Technology Start in 2003: ATA array, forrunner of US SKA (500 MHz – 10 GHz)

3 Chalmers University of Technology Size and complexity for f min = 500 MHz ATA feed: Too large & Problem with phase center variations Eleven feed: Eleven times smaller & No problem with phase center variations

4 Chalmers University of Technology Size and complexity for f min = 500 MHz ATA feed: Too large & Problem with phase center variations Eleven feed: Eleven times smaller & No problem with phase center variations

5 Chalmers University of Technology Idea behind Chalmers feed Two parallel dipoles over ground –from book about Radio Telescopes by Christiansen and Högbom –equal E- and H-plane patterns –phase center is locked to the ground plane –low far-out sidelobes and backlobes. Bandwidth by –Logperiodic –Folded dipoles ”Eleven” name inspired by –Basic dual-dipole geometry –Directivity dBi and S11 <-10 dB –Over more than decade bandwidth (>11) –And size eleven times smaller than classical log-periodic feeds

6 Chalmers University of Technology Interdisciplinary team developing coolable VLBI2010 hardware from Sept 2008 Interdisciplinary research at Chalmers –Department of Signals and Systems, Chalmers –Department of Radio and Space Sciences, Chalmers –Department of Microtechnology and Nanoscience –Chalmers Industriteknik (CIT) for helping to commercialize: No dedicated SKA funding since (US SKA project) Hardware orders from VLBI 2010 partners: –Vertex (BKG) in Germany –Statkart in Norway –Haystack radio telescope in USA

7 Chalmers University of Technology Main contributions Dr Jian Yang: “Electrical design” Dr Miroslav Pantaleev and Leif Helldner: “Mechanical and cryogenic design” Benjamin Klein, South Africa “Noise modeling” Drawing, assembled feed, cooled feed

8 Chalmers University of Technology Assembled 2-13 GHz hardware and drawing

9 Chalmers University of Technology The following choices were made during the project All materials MUST stand cryogenic temp 4 separate panels (petals) with log-per. dipoles PCB technology for antenna petals Minimize thickness of dielectric in center 2x4 ports with no crossing lines in center puck Differential feed line impedance 200 Ohms Experimental model has 2x4 coaxial ports, transf to 50 Ohms We work also with 4 differential 200 Ohms LNAs, 2 per polarization

10 Chalmers University of Technology Front and back sides of Eleven feed with 8 single-ended ports

11 Chalmers University of Technology Integration with differential 200 ohm LNAs from Caltech Four cryogenic differential 200 ohm LNAs from Caltech mounted on the back side of the ground plane Requires in addition two power combiners to get two polarizations out from the cryostat Expected delivery of LNAs: June 2010

12 Chalmers University of Technology Early computed still valid efficiency vs. subtended half angle Optimum subtended angle >50 deg

13 Chalmers University of Technology Early computed figure of Merit versus F/D optimum F/D = 0.4 (i.e. 64 deg) Useful range 0.33 < F/D < 0.50, i.e. 75 deg <    55 deg

14 Chalmers University of Technology Simulations and Measurements at Chalmers of input reflection coefficient (4 ports excited) (power dividers and cables were calibrated away)

15 Chalmers University of Technology Co- and crosspolar patterns in 45 deg plane totaland with removed higher order  variations

16 Chalmers University of Technology Co- and crosspolar patterns in 45 deg plane totaland with removed higher order  variations

17 Chalmers University of Technology Co- and crosspolar patterns in 45 deg plane totaland with removed higher order  variations

18 Chalmers University of Technology Co- and crosspolar patterns in 45 deg plane totaland with removed higher order  variations

19 Chalmers University of Technology Co- and crosspolar patterns in 45 deg plane totaland with removed higher order  variations

20 Chalmers University of Technology Co- and crosspolar patterns in 45 deg plane totaland with removed higher order  variations

21 Chalmers University of Technology Co- and crosspolar patterns in 45 deg plane totaland with removed higher order  variations

22 Chalmers University of Technology Co- and crosspolar patterns in 45 deg plane totaland with removed higher order  variations

23 Chalmers University of Technology Co- and crosspolar patterns in 45 deg plane totaland with removed higher order  variations

24 Chalmers University of Technology Co- and crosspolar patterns in 45 deg plane totaland with removed higher order  variations

25 Chalmers University of Technology Co- and crosspolar patterns in 45 deg plane totaland with removed higher order  variations

26 Chalmers University of Technology Co- and crosspolar patterns in 45 deg plane totaland with removed higher order  variations

27 Chalmers University of Technology Sub-efficiencies from measured radiation patterns at TUD Looks good, except for BOR1 efficiency below 2.5 GHz and above 9 GHz. BOR1 efficiency is power lost in sidelobes due to higher order  variations.

28 Chalmers University of Technology After survival test to 14 K Three stages of cryostat (Dewar) can be seen

29 Chalmers University of Technology Deformation simulations and testing at cryogenic temperatures

30 Chalmers University of Technology Integration of Eleven feed in cryostat The MIL infrared filter reduces the temperature to 25K The 70K shield has infrared window of one layer Teflon The temperature on the Feed surface is measured with temperature sensor Lakeshore DT-470 mounted on thin copper support soldered at the edge of the third dipole.

31 Chalmers University of Technology Front and back sides of Eleven feed with 8 single-ended ports

32 Chalmers University of Technology Noise Temperature Measurements

33 Chalmers University of Technology Noise temperatures Ohmic loss LNA Sky and ground Total predicted and measured

34 Chalmers University of Technology Summary of measurement results Hardware: Good. Appears solid and appealing Matching: abs(S11) < -10 dB up to 13 GHz –measured by removing effects of power dividers and cables by calibration Independent gain measurements at Technical University of Denmark –Losses smaller than 0.5 dB (Uncertainty due to multiple reflections between 180 deg hybrid, 3dB power divider and antenna, which were not calibrated out in this case) –Radiation patterns: Good between 2.5 and 9 GHz. Otherwise low BOR1 efficiency –Overall efficiency in reflector better than -2 dB between 2.5 and 9 GHz Promising system noise measurements with T LNA = 5 – 10 K

35 Chalmers University of Technology Integration with differential 200 ohm LNAs from Caltech Four cryogenic differential 200 ohm LNAs from Caltech mounted on the back side of the ground plane Requires in addition two power combiners to get two polarizations out from the cryostat Expected delivery of LNAs: June 2010

36 Chalmers University of Technology Planned work Design and test compact 1-10 GHz SKA model Improve low BOR1 efficiency above 9 GHz More studies of radiation fields and S11 in cryostat Improve noise models Test with 4 differential LNAs Integrate and test with passive balun and 2 single-ended LNAs More optimizatioins and compare with horn solutions (narrow band)

37 Chalmers University of Technology Comparison of figure of merit A/T (predicted) A/T of the Eleven feed system For a reflector of 1 m 2 area with subtended half angle of 60 o, i.e. F/D = Cooled system is with Caltech cryogenic LNA and cryostat is at 30 K. The uncooled system is with Chalmers room temperature LNA at room temperature.


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