Analysis of Low Frequency Phased Array Stations Dr. Nima Razavi-Ghods Dr. Eloy de Lera Acedo Cambridge AAVP 2010, 09/12/10 1.

Slides:



Advertisements
Similar presentations
Beamforming Issues in Modern MIMO Radars with Doppler
Advertisements

Antarctic Ice Shelf 3D Cross-sectional Imaging using MIMO Radar A. Hari Narayanan UCL Electronic and Electrical Engineering, UK P. Brennan UCL Electronic.
Update on Measurements and Simulations at Cambridge: SKALA element + LNA Eloy de Lera Acedo Nima Razavi Ghods Cavendish Laboratory University of Cambridge.
Lorentz force detuning measurements on the CEA cavity
2010 SKA Africa Bursary Conference Chalmers University of Technology Jian Yang, Associate Professor Chalmers University of Technology Sweden.
Chapter 4. Antenna Synthesis
Sparse Array Geometry Mr. Ahmed El-makadema Professor A.K Brown.
SKADS: Array Configuration Studies Implementation of Figures-of-Merit on Spatial-Dynamic-Range Progress made & Current status Dharam V. Lal & Andrei P.
BYU Auxiliary Antenna Assisted Interference Cancellation for Radio Astronomy Imaging Arrays Brian Jeffs and Karl Warnick August 21, 2002.
Volkan Cevher, Marco F. Duarte, and Richard G. Baraniuk European Signal Processing Conference 2008.
Netherlands Institute for Radio Astronomy 1 ASTRON is part of the Netherlands Organisation for Scientific Research (NWO) From LOFAR design to SKA1 System.
SMART ANTENNAS. Smart Antennas The presentation is divided into the following: Why? What? How?
Sascha D-PAD Sparse Aperture Array.
Performance of Adaptive Array Antennas in Mobile Fading Environment by: Amin Al-Ka’bi, M. Bialkowski and John Homer School of Information Technology &
Marco de Vos Summary, Conclusions & ActionsAAVP 2010 Summary, Conclusions and Actions Marco de Vos
SKA AA-low: LPD antenna (SKALA) & path towards AAVS0 at Cambridge Eloy de Lera Acedo University of Cambridge 1 AAVP 2011: Taking the AA programme into.
Performance of station array configurations Sparse vs. Dense, Regular vs Random Jaap D. Bregman AAVP Workshop,Cambridge,
Dec 2010 AAVP Cambridge workshop AAVP AAVS1/2-low demonstrators Jan Geralt Bij de Vaate.
Keith Grainge Calibration requirementsAAVP 2010 Calibration and Imaging Requirements Keith Grainge (plus teams at ASTRON, Oxford, Cambridge)
Applicability and limitations of redundancy cal. in phased array stations Parisa Noorishad, Stefan Wijnholds, Arnold van Ardenne & Thijs van der Hulst.
Array Antenna Designs for the SKA-AAlo Eloy de Lera Acedo 1 AAVP 2010, Cambridge, UK. 10/12/10.
Multi-beam Patch Antenna Design Mustafa Konca Supervisor: Prof. Dr. Sener Uysal.
LOFAR Antenna Systems Dion Kant, Wim van Cappellen AAVP – 10 December 2010, Cambridge, UK.
AAVP meeting Cambridge December 2010 Technology Trade –offs: Mid band Array and Elements Prof. A. K. Brown 1 1 School of Electrical and Electronic Engineering.
John Thornton, Yuriy Zakharov, David Grace
Effect of Mutual Coupling on the Performance of Uniformly and Non-
AA-Low Technical Progress Meeting, October 2012, Medicina, Italy AAVS0 & AAVS0.5: System Design and Test Plan Nima Razavi-Ghods Eloy de Lera Acedo.
SKA AA-Low Station Configurations and Trade-off Analysis Nima Razavi-Ghods, Ahmed El-Makadema AAVP 2011, ASTRON, Dwingeloo Dec
Efficient design of a C-band aperture-coupled stacked microstrip array using Nexxim and Designer Alberto Di Maria German Aerospace Centre (DLR) – Microwaves.
Capacity Variation of Indoor Radio MIMO Systems Using a Deterministic Model A. GrennanDIT C. DowningDIT B. FoleyTCD.
ANTENNA ARRAYS.
Joint PHY-MAC Designs and Smart Antennas for Wireless Ad-Hoc Networks CS Mobile and Wireless Networking (Fall 2006)
by P. Sriploy, M. Uthansakul and R. Wongsan
Distributed Adaptive Control and Metrology for Large Radar Apertures Principal Investigator: James Lux, P.E. (337) Dr. Elaine Chapin (334), Samuel Li (337),
Main beam representation in non-regular arrays
Survey Quality Jim Condon NRAO, Charlottesville. Survey Qualities Leiden 2011 Feb 25 Point-source detection limit S lim Resolution Ω s Brightness sensitivity.
EFFECTS OF MUTUAL COUPLING AND DIRECTIVITY ON DOA ESTIMATION USING MUSIC LOPAMUDRA KUNDU & ZHE ZHANG.
School of something FACULTY OF OTHER School of Physics & Astronomy FACULTY OF MATHEMATICS & PHYSICAL SCIENCES The Cornish Survey Workshop.
Controlling Field-of-View of Radio Arrays using Weighting Functions MIT Haystack FOV Group: Lynn D. Matthews,Colin Lonsdale, Roger Cappallo, Sheperd Doeleman,
1 The OSKAR Simulator (Version 2!) AAVP Workshop, ASTRON, 15 th December 2011 Fred Dulwich, Ben Mort, Stef Salvini.
Widefield Astronomy and Technologies for the SKA November 2009 at Limelette, Belgium The SKA AA-lo array; E.M. simulation and design Eloy de Lera.
Rosie Bolton1 SKADS Costing work 4 th SKADS Workshop, Lisbon, 2-3 October 2008 SKADS Costing work: Spreadsheets to scalable designs Rosie Bolton Dominic.
NSF SURE Program, Summer 2002 / Clemson University, Clemson, SC 1 Broadband Arrays and Switching Antennas Dan Palecek, SD School of Mines and Technology,
Fundamental limits of radio interferometers: Source parameter estimation Cathryn Trott Randall Wayth Steven Tingay Curtin University International Centre.
Modeling GPS Adaptive Nulling Receivers
Adaptive Filters for RFI Mitigation in Radioastronomy
The Very Small Array Angela Taylor & Anze Slosar Cavendish Astrophysics University of Cambridge.
NASSP Masters 5003F - Computational Astronomy Lecture 14 Reprise: dirty beam, dirty image. Sensitivity Wide-band imaging Weighting –Uniform vs Natural.
Power Quality: A Nonlinear Adaptive Filter for Improved Power System Operation and Protection Research Overview: Focuses on the application of a new algorithm.
Performance of Adaptive Beam Nulling in Multihop Ad Hoc Networks Under Jamming Suman Bhunia, Vahid Behzadan, Paulo Alexandre Regis, Shamik Sengupta.
The Allen Telescope Array Douglas Bock Radio Astronomy Laboratory University of California, Berkeley Socorro, August 23, 2001.
AAVP Workshop December 2010 TITLEAAVP Workshop December 2010 Aeff/Tsys evaluation for AAlo sensors Cambridge 8th-10th December 2010 Federico Perini 1,
Philippe Picard1EMBRACE station processing SKADS Conference, Limelette, 4-6 November 2009 EMBRACE station processing P. Picard Station de Radioastronomie.
SKA: Configurations and Simulations Ramesh Bhat Colin Lonsdale Roger Cappallo Shep Doeleman Divya Oberoi Joanne Attridge MIT Haystack Observatory.
A System View on SKA Bandwidth Usage G.W. (Dion) Kant AAVP Dwingeloo, 14 December 2011.
Keith Grainge Calibration issuesAA-low Technical Progress meeting Calibration Issues Keith Grainge.
RADAR ANTENNA. Functions of Radar Antenna Transducer. Concentrates the radiated energy in one direction (Gain). Collects echo energy scattered back to.
Antenna Arrays and Automotive Applications
Hanyang University 1/21 Antennas & RF Devices Lab. antenna arrays and automotive applications Kim Tae Won.
Nicolas Fagnoni – Cosmology on Safari – 14th February 2017
A.Zanichelli, B.Garilli, M.Scodeggio, D.Rizzo
AAVS1 Calibration Aperture Array Design & Construction Consortium
Nortel Corporate Presentation
Data Reduction and Analysis Techniques
OSKAR station simulator
MadMax Experiment: Algorithm to Place Discs MadMax Mini Workshop MPP
Nithyanandan Thyagarajan (Arizona State University) HERA+, MWA+
Analysis of Adaptive Array Algorithm Performance for Satellite Interference Cancellation in Radio Astronomy Lisha Li, Brian D. Jeffs, Andrew Poulsen, and.
Aperture Array Simulations
Lessons learned from station calibration
Presentation transcript:

Analysis of Low Frequency Phased Array Stations Dr. Nima Razavi-Ghods Dr. Eloy de Lera Acedo Cambridge AAVP 2010, 09/12/10 1

Overview Phased array design parameters AA-lo station configuration studies (regular vs. random) Randomisation of elements Simulations to compute T A and A/T (geometries, weighting, element types) Future work and conclusions 2

Factors Affecting Beam on the Sky Array size (fundamental limit on Aeff/Tsys) Array geometry (main and side-lobe profile) ◦Fully filled grids (regular lattice) ◦Sparse or thinned grids ◦Truly randomised grids Antenna element response (scan/polarisation response, matching, mutual coupling) Operating frequency, processing bandwidth, integration time Weighting schemes (main beam and side-lobe profile) ◦Spatial windows (e.g. Hamming, Gaussian, Kaiser) ◦Side-lobe profile control (e.g. Dolph-Chebyshev/Taylor, Fourier design method) ◦Adaptive nulling Back-end processing ◦Fully digital core (any weighting in single or multiple stages) ◦First level analogue (some limitations in response)

Antenna Array Geometries 4

Random Vs. Regular 5 Sky (Haslam) Lat = 28.59S, Long = E Date: 01/01/2020, Time 19.33h Triangular Lattice Beam 10,000 elements, d = 0.8

Random Vs. Regular 6 Sky (Haslam) Lat = 28.59S, Long = E Date: 01/01/2020, Time 19.33h Random Lattice Beam 10,000 elements

Randomised Array: AA-lo 7 d = /3 : 2

Randomisation algorithm 8 Fixed min. distance Variable min. distance

Simulations to compute T A 9 T A was analysed as the beam tracked 3 cold patches on the sky over four and half hours. Array factor based simulations carried computed using NFFT. AA-lo Station ~10k elements. 6 Geometries: regular, triangular, sparse random, thinned, concentric rings, and fully random. 4 minimum inter-element separations: 0.5, 0.8, 1, 2. 3 Weights: Uniform, Taylor and Dolph-Chebyshev (SLL = 35 dB) 3 Element types.

SKA AA-lo observable Sky 10 Region 1: 09 h 07 m 12 s 0000’46’’, Region 2: 04 h 03 m 36 s -3448’00’’ Region 3: 04 h 45 m 00 s -6100’00’’ R1 R2 R3

Results for T A : Region 1 11

Results for T A : Region 2 12

Results for A/T: Region 1 13

Results for A/T: Region 2 14

Taylor Weighting (SLL = 35 dB) 15

16 AA-lo Observable Sky

Low Gain vs. High Gain Element 17

Xarray Tool: MATLAB GUI 18

Future work and collaborations Main objective: SKA simulator Faster and more accurate simulations of the station beam based on MBF approach (collaboration with UCL). Computation framework for station simulator (collaboration with Oxford). Further analysis of beam synthesis techniques and weight calibration. Design of optimal geometry, e.g. far out versus close in side-lobes. 19

Thank You. 20