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

Slides:



Advertisements
Similar presentations
A Crash Course in Radio Astronomy and Interferometry: 2
Advertisements

BEAM FORMING NETWORKS ( BFN’s ) EE 525 Antenna Engineering.
Antarctic Ice Shelf 3D Cross-sectional Imaging using MIMO Radar A. Hari Narayanan UCL Electronic and Electrical Engineering, UK P. Brennan UCL Electronic.
Schediwy: Advantages and Disadvantages of Sparse Aperture Arrays Fermilab: October 2009.
1 EMLAB Antennas. 2 EMLAB Hertzian dipole antenna Heinrich Hertz ( )
Sparse Array Geometry Mr. Ahmed El-makadema Professor A.K Brown.
The Effect of the Apparent Baseline on Fringe Amplitude and Period By Dana Dawson Rhonda Tully July 2004 MST 562.
Millimeter Wave Sensor: An Overview
Probing the field of Radio Astronomy with the SKA and the Hartebeesthoek Radio Observatory: An Engineer’s perspective Sunelle Otto Hartebeesthoek Radio.
Radio `source’ Goals of telescope: maximize collection of energy (sensitivity or gain) isolate source emission from other sources… (directional gain… dynamic.
Radio Telescopes Large metal dish acts as a mirror for radio waves. Radio receiver at prime focus. Surface accuracy not so important, so easy to make.
BDT Radio – 1b – CMV 2009/09/04 Basic Detection Techniques 1b (2009/09/04): Single pixel feeds Theory: Brightness function Beam properties Sensitivity,
ANTENNA ARRAYS A Short Review. Array Factor (1) Uniform, Linear Array Equally spaced elements along the z-axis Equally spaced elements along the z-axis.
BDT Radio – 2b – CMV 2009/10/09 Basic Detection Techniques 2b (2009/10/09): Focal Plane Arrays Case study: WSRT System overview Receiver and.
Radio Interferometry Jeff Kenney. Outline of talk Differences between optical & radio interferometry Basics of radio interferometry Connected interferometers.
Sascha D-PAD Sparse Aperture Array.
Prototype SKA Technologies at Molonglo: 3. Beamformer and Correlator J.D. Bunton Telecommunications and Industrial Physics, CSIRO. Australia. Correlator.
Performance of station array configurations Sparse vs. Dense, Regular vs Random Jaap D. Bregman AAVP Workshop,Cambridge,
Keith Grainge Calibration requirementsAAVP 2010 Calibration and Imaging Requirements Keith Grainge (plus teams at ASTRON, Oxford, Cambridge)
AA-mid demonstrator Dion Kant AAVP – 10 December 2010, Cambridge, UK.
LOFAR Antenna Systems Dion Kant, Wim van Cappellen AAVP – 10 December 2010, Cambridge, UK.
Central Development Laboratory (Adapted from John Webber’s Viewgraphs, April 2002 Presented tonight by Skip Thacker) IEEE Tour April 2003.
Sarah Middleton Supervised by: Anton van Wyk, Jacques Cilliers, Pascale Jardin and Florence Nadal 3 December 2010.
Assessment of RFI measurements for LOFAR Mark Bentum, Albert-Jan Boonstra, Rob Millenaar ASTRON, The Netherlands Telecommunication Engineering, University.
14 Sep 1998R D Ekers - Synth Image Workshop: INTRODUCTION 1 Synthesis Imaging Workshop Introduction R. D. Ekers 14 Sep 1998.
Meteor Receiver Olajide Durosinmi Hugh Kinsel Kenny Mills Austin Pierce Nick Stelmashenko October 21, 2009.
Backend electronics for radioastronomy G. Comoretto.
SKA AA-Low Station Configurations and Trade-off Analysis Nima Razavi-Ghods, Ahmed El-Makadema AAVP 2011, ASTRON, Dwingeloo Dec
BDT Radio – 1a – CMV 2009/09/01 Basic Detection Techniques Radio Detection Techniques Marco de Vos, ASTRON / Literature: Selected.
ECE 8443 – Pattern Recognition ECE 8423 – Adaptive Signal Processing Objectives: Introduction SNR Gain Patterns Beam Steering Shading Resources: Wiki:
Namaste Project 3.4 GHz Interference Study Preliminary document - Work in Progress updated The intent of this study is to collect data which may.
Solar observation modes: Commissioning and operational C. Vocks and G. Mann 1. Spectrometer and imaging modes 2. Commissioning proposals 3. Operational.
Phased Array Feeds John O’Sullivan SKANZ 2012 CSIRO Astronomy and Space Science,
ANTENNA ARRAYS.
RN /08/05 National Aeronautics and Space Administration Jet Propulsion Laboratory California Institute of Technology Implementation of an Antenna.
Stability of Maximum S/N Beams CSIRO ASTRONOMY AND SPACE SCIENCE Aidan Hotan | ASKAP Deputy Project Scientist 4 th March 2014 SKA Workshop on Calibration.
SMART ANTENNA.
Radio Astronomy ASTR 3010 Lecture 25. Intro to Radio Astronomy Concepts - Amplifiers - Mixers (down-conversion) - Principles of Radar - Radio Astronomy.
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.
Mileura Widefield Array – Low Frequency Demonstrator MHz * Currently in “Early Deployment” phase Goal: HI at redshift 6 to 17.
The Role of Interferometers in Future Space Astrophysics Missions Ron Allen Space Telescope Science Institute Synthesis Imaging Scientist Space Interferometry.
AST 443: Submm & Radio Astronomy November 18, 2003.
Electromagnetic Design of Broadband Antenna Feed Systems for the Northern Cross Radio Telescope (Bologna, Italy) Designed Broad Band Antenna Feed Systems.
02/6/ jdr1 Interference in VLBI Observations Jon Romney NRAO, Socorro ===================================== 2002 June 12.
Atacama Large Millimeter/submillimeter Array Expanded Very Large Array Robert C. Byrd Green Bank Telescope Very Long Baseline Array Phased Array Feed Development.
Observing Modes from a Software viewpoint Robert Lucas and Philippe Salomé (SSR)
Distributed Adaptive Control and Metrology for Large Radar Apertures PI: James Lux Co-Is: Adam Freedman, John Huang, Andy Kissil, Kouji Nishimoto, Farinaz.
ASKAP Update David DeBoer ASKAP Project Director 26 May 2010.
WELCOME TO IHEP. RF Phase Control for BEPCII Linac Accelerator Wenchun Gao.
A Sample IHY 2007 Instrumentation Proposal J. Kasper, B. Thompson, N. Fox.
Philippe Picard1EMBRACE station processing SKADS Conference, Limelette, 4-6 November 2009 EMBRACE station processing P. Picard Station de Radioastronomie.
Observed and Simulated Foregrounds for Reionization Studies with the Murchison Widefield Array Nithyanandan Thyagarajan, Daniel Jacobs, Judd Bowman + MWA.
Philippe Picard 2 nd SKADS Workshop October 2007 Station Processing Philippe Picard Observatoire de Paris Meudon, 11th October 2007.
A Survey of Selected Radio Telescope Receiver Types
Term paper on Smart antenna system
Antenna Arrays and Automotive Applications
European Pre-AAVS1 Update AADC all-hands, Bologna, 9-13 May 2016 Nima Razavi-Ghods.
Correlators ( Backend System )
Nithyanandan Thyagarajan1, Aaron R. Parsons2,
Mid Frequency Aperture Arrays
Improved radio data analysis with LOPES Katrin Link, for the LOPES Collaboration #0404, ICRC 2011, Beijing.
Chapter 4 Antenna Arrays
Phased Array Feeds SKANZ 2012 John O’Sullivan
Modern Interferometric Arrays
Telescopes and Images.
Nithyanandan Thyagarajan (Arizona State University) HERA+, MWA+
Observational Astronomy
Observational Astronomy
Technical Foundations & Enabling Technologies – DS4
Lessons learned from station calibration
Presentation transcript:

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

BDT Radio – 2a – CMV 2009/10/06

MIDI

BDT Radio – 2a – CMV 2009/10/06

1971

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

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

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

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

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

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

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

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

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

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

BDT Radio – 2a – CMV 2009/10/06

Connecting Europe …

BDT Radio – 2a – CMV 2009/10/06

Aperture arrays

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

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

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

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

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

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

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

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)

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

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

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