Focal Plane Array Related Activities at CSIRO
|
|
- Sheryl Banks
- 5 years ago
- Views:
Transcription
1 ICT Centre /antennas Focal Plane Array Related Activities at CSIRO Trevor S. Bird (1), Douglas Hayman (1), Suzy Jackson (2) & Dick Ferris (2) (1) CSIRO ICT Centre (2) CSIRO Australia Telescope National Facility PO Box 76, Epping NSW 1710 Australia
2 Outline of Presentation Past experience with focal plane arrays CSIRO and other activities related to FPAs Antennas SKA proposals FPAs Line feeds Integrated receiver systems High-speed digital correlators What CSIRO brings to collaboration with Europe Design Measurement
3 Parkes Multibeam Receiver System Multibeam receiver system sits in the telescope s focus cabin and receives signals from space Telescope sees 13 patches of sky simultaneously Radio signals from galaxies in space hit surface of telescope and are reflected to focus cabin Telescope detects faint galaxies (Data for the Southern sky)
4 Arecibo Multibeam Feed System Successfully installed in April 2004 Feed array ( GHz) under test at CSIRO Arecibo radio telescope
5 Arecibo Multibeam Feed Array Sample Results Element 3 : Array reference 45, OMT horizontal plane at GHz & distance 3.7m 3 Theory Theory
6 Current Australian Radio Astronomy Projects with FPAs FARADAY and PHAROS MUDDA multi-use dense digital array Australian SKA Concept Demonstration Projects MMIC development Signal processing Australia Telescope Compact Array Broadband Backend (CABB) Bandwidth increased from 128MHz to 2GHz SKAMP SKA Molonglo prototype NTD new technology demonstrator Remote and radio-quiet site Luneburg lens development Techniques for RFI mitigation
7 Antennas
8 SKA Configurations Technical and cost assessments Luneburg lens Cylindrical reflector Wide-field of view (WFOV) reflector Luneburg lens Cylindrical reflector WFOV reflector
9 Prototype Luneburg Lens Construction
10 Measurement of Prototype Luneburg Lens Aperture field Far field Measured results in S-band
11 Luneburg Lens with Egg-crate FPA The ASTRON FARADAY FPA we had on site was used as an illuminator for the Konkur lens.
12 Cylindrical Reflector Offset-fed options Improved cost model Wideband line-feed development (with Sydney Uni.)
13 WFOV Reflector FOV ~10º x 10º ~14m diameter reflector Large array in focal region Array is extendable Technology is well developed and cost known Three CSIRO MultiBeam antennas at SES-ASTRA, Luxembourg. Each antenna covers a ~40º x 1º FOV.
14 Focal-plane Arrays All SKA are expected to use focal-plane arrays Focal-plane arrays: Allow formation of multiple beams Correct for errors in reflectors or lenses Allow electronic beam scanning Prototype focal plane array of Vivaldi elements
15 Approach to Focal Plane Feeds Compact feed elements Close packing (max. spacing < 0.9λ) Wideband Dual polarization Rigorous analysis including mutual coupling Excitation chosen to maximize secondary antenna A eff /T (G/T)
16 Focal Plane Feed Options Single feed per beam Array cluster per beam
17 Cluster Feed Approach Choose array excitation to maximize G/T A Overlap sub-arrays trade-off between number of elements and efficiency Combine signals at: RF IF M x N processor
18 Overlapping Sub-arrays Example: 3 overlapping hexagonal arrays Efficiency improvement is terraced, for example: Beam efficiency % No. of Elements
19 Array Excitation for Maximum G/T A Antenna gain Q(θ,φ) * Q(θ,φ) (cx) (c x) G(θ,φ) = G o = G o P f x x c = correlation coefficients between the focal field and co-polar modes in the apertures x = normalized array excitation coefficient vector Note: Gain is maximum when x = c. Zero cross-polarization in beam direction when x = c d c dd d where d is similar to c except for cross-polar modes Antenna temperature T A = 1 x G(θ,φ)T(θ,φ) 4π B x dω=g o Ω x x For a given beam direction (θ,φ), G/T A is maximum when x = B 1 c Mutual coupling between feed elements is included.
20 Potential Elements for Close Packed Arrays Coaxial waveguide (b/a>0.4) Dielectric rod Microstrip patch b a Helical (Qassim & McEwan) Travelling-wave slot antennas Vivaldi ~0.25λ top patch driven patch x choke ring y Balanced Anti-podal input probe ground plane ~0.8λ (after Kiskh & Shafai) y y=±aexp(rx) A x truncation limits - A
21 Arrays of Coaxial Horns X -20 Mode matching method for coaxial horns Accurate mutual coupling analysis (Bird, Trans. IEEE, Mar. 2004, pp ) In compact arrays 1 a < π(1 + (b/a)) < λ s 2 Y E 2 E Validation of analysis Low-loss polystyrene foam spacers Coupling coefficient db S12 (theory) S13 (theory) S12 (expt) S13 (expt) Frequency GHz X where s is the element spacing in wavelengths < 0.9 Example: s < λ/2, b/a > Y Irises All dimensions in mm Feed element for Jodrell Bank Lovell radio telescope
22 Balanced Anti-podal Vivaldi Antenna E-plane H-plane With dielectric Without dielectric Computations by S. Hanham, CSIRO With CST Microwave Studio Cross-polarization is high
23 Surface Currents on Vivaldi Elements Conventional balanced Vivaldi Crossed balanced Vivaldi
24 Integrated Receiver Systems
25 MUDDA Overview Frontend Oversampled Focal Plane Array of 8x8 (nominal) tapered slot antennas for use on Parkes and other large unshaped dishes. RF frequency range MHz (nom). T sys < 50K (uncooled). Instantaneous IF bandwidth 500 MHz. ~40dB (6 8 bits) dynamic range. Dimensions 1.5m x 1.5m.
26 MUDDA Overview - Backend FPGA filterbank on each element. Beamformer for at least four independent beams. Located remotely from feeds RFI issues. Use technology developed for CABB
27 Possible Block Diagram
28 Radio on a Chip Takes advantage of low cost, low power RF- CMOS processes developed for wireless networking Will integrate Mixer, IF filter, and Sampler, as well as LO distribution. Possibly integrating LNA, RF filter. Design with Cadence toolset (Macquarie Uni.) Integrations issues CMOS inductor Q < 10 bulk substrate FET NFMIN ~40K for 0.25µ, ~20K for 0.18µ (2GHz) comparable with GaAs Broadband LNA noise match. Gilbert cell mixers. Active IF filter.
29 High-speed Digital Correlators
30 2 GHz Bandwidth Correlator with Polyphase Filterbank 2GHz 2GHz 4k channels Basic Configuration 2GHz 4k channels 4k channels 4k channels Multiple Zoom (>2 possible) Simple Zoom 2GHz xn x 0 (m) x 1 (m) xρ(m) x M-1 (m) po(m) p1(m) pρ(m) pm-1(m) X0(m) 0 X1(m) 1 M-Point ρ M-Point DFT DFT Via via FFT M-1 Xk(m) (m) XM-1 DMUX FIR FFT FIR FFT Filterbank Fringe Rotators Correlators FPGA hardware may be completely reprogrammed to produce many different filterbank configurations, as different observations may require. 4k channels 4k channels Compound Zoom A 2GHz bandwidth polyphase digital filterbank with 4096 channels will fit into four XC2V6000 FPGAs
31 Wideband Correlation Build wider bandwidths by paralleling 2GHz slices 8 GHz (per polarisation) high resolution spectrometer for MOPRA 2GHz bandwidth per IF, four IFs per antenna
32 Baseband Receiver / PoC Spectrometer 1024 Channel Spectrum, DC-256MHz
33 Molonglo Observatory Synthesis Telescope Material supplied by Anne Green, University of Sydney Photo: G. Warr
34 SKAMP - the Molonglo SKA Demonstrator Two substantial demonstrator projects have been funded for installation on the Molonglo Telescope: A 96-station, wideband FX correlator A broad-band line feed system for a cylindrical paraboloid. These two projects constitute the SKA Molonglo Prototype SKAMP. They will result in a significant trial of key SKA engineering elements and enhance the scientific value of the Molonglo Telescope Joint venture between University of Sydney and CSIRO
35 SKAMP Science Goals Low-frequency radio spectrometry ( MHz) Selection of objects via their radio spectral shape, e.g. candidate high redshift (z>3) galaxies with ultra-steep radio spectra, study the formation of galaxies and massive black holes. Redshifted HI ( MHz) HI in absorption against bright continuum sources over a wide redshift range (z=0 to 3). HI in emission - evolution of the HI mass function from z=0 to 0.5. Low-frequency Galactic recombination lines Recombination lines of carbon and hydrogen can be used to probe the partially-ionized ISM. Gamma Ray Bursters Electronic beam steering gives a 5% chance of capturing a random event. Concurrent SETI search, and Pulsars and Source Flux Monitoring 18 to 400 deg 2 accessible around main beam. Real time de-dispersion
36 The SKA Molonglo Prototype (SKAMP) Collecting area = 1% of SKA (i.e. equivalent to 1 SKA station) Multibeaming Wide instantaneous field of view Digital beamforming Wide-band FX correlator (2048 channels) Frequency and pointing agility Line feed GHz >100 MHz instant BW Cylindrical antenna prototype RFI mitigation strategies - adaptive noise cancellation
37 Progress in Upgrade of Signal Path Feed Development modelling feed synthesis scan performance Data Acquisition & Beamforming Customised A/D converters delay & phase tracking data acquisition & beamforming hardware installed in 2004 Correlator Development Ball grid FGPAs Testing in progress Signal Processing correlator control computer (CCUBED) with external data interface has been setup
38 Petal Line Feed Element 0-5 Measured Azimuth Patterns for Antenna Prototype, F=1539MHz Co-polar X-po la r B ) (d d e p l itu m A Element pattern θ (degrees )
39 SKA New Technology Demonstrator (NTD) Aims: Antenna, receiver and backend technology for support wide FOV, wideband astronomy Operational facility at a radio-quiet site Demonstrate radio science opportunities in extremely low RFI environment Data transport/processing over long distances Continent-wide, international connectivity Remote energy provision Environmental conditioning on a semi-arid remote site
40 Concluding Remarks Overview of projects in progress Antennas Integrated receivers High-speed digital correlators Demonstrators in progress Keen to continue collaboration with Europe through PHAROS etc
Smart Antennas in Radio Astronomy
Smart Antennas in Radio Astronomy Wim van Cappellen cappellen@astron.nl Netherlands Institute for Radio Astronomy Our mission is to make radio-astronomical discoveries happen ASTRON is an institute for
More informationThe Australian SKA Pathfinder Project. ASKAP Digital Signal Processing Systems System Description & Overview of Industry Opportunities
The Australian SKA Pathfinder Project ASKAP Digital Signal Processing Systems System Description & Overview of Industry Opportunities This paper describes the delivery of the digital signal processing
More informationA Multi-Fielding SKA Covering the Range 100 MHz 22 GHz. Peter Hall and Aaron Chippendale, CSIRO ATNF 24 November 2003
A Multi-Fielding SKA Covering the Range 100 MHz 22 GHz Peter Hall and Aaron Chippendale, CSIRO ATNF 24 November 2003 1. Background Various analyses, including the recent IEMT report [1], have noted that
More informationPractical Aspects of Focal Plane Array Testing
Practical Aspects of Focal Plane Array Testing Lessons from an FPA Test-bed at CSIRO, Marsfield Douglas B. Hayman1-3, Trevor S. Bird2,3, Karu P. Esselle3 and Peter J. Hall4 1 2 3 CSIRO Astronomy and Space
More informationPhased Array Feed Design. Stuart Hay 23 October 2009
Phased Array Feed Design Stuart Hay 23 October 29 Outline Why phased array feeds (PAFs) for radioastronomy? General features and issues of PAF approach Connected-array PAF approach in ASKAP Why PAFs? High
More informationMulti-octave radio frequency systems: Developments of antenna technology in radio astronomy and imaging systems
Multi-octave radio frequency systems: Developments of antenna technology in radio astronomy and imaging systems Professor Tony Brown School of Electrical and Electronic Engineering University of Manchester
More informationMarch Phased Array Technology. Andrew Faulkner
Aperture Arrays Michael Kramer Sparse Type of AA selection 1000 Sparse AA-low Sky Brightness Temperature (K) 100 10 T sky A eff Fully sampled AA-mid Becoming sparse Aeff / T sys (m 2 / K) Dense A eff /T
More informationIntegrated receivers for mid-band SKA. Suzy Jackson Engineer, Australia Telescope National Facility
Integrated receivers for mid-band SKA Suzy Jackson Engineer, Australia Telescope National Facility ASKAP/SKA Special Technical Brief 23 rd October, 2009 Talk overview Mid band SKA receiver challenges ASKAP
More informationPhased Array Feeds for the SKA. WP2.2.3 PAFSKA Consortium CSIRO ASTRON DRAO NRAO BYU OdP Nancay Cornell U Manchester
Phased Array Feeds for the SKA WP2.2.3 PAFSKA Consortium CSIRO ASTRON DRAO NRAO BYU OdP Nancay Cornell U Manchester Dish Array Hierarchy Dish Array L5 Elements PAF Dish Single Pixel Feeds L4 Sub systems
More informationPhased Array Feeds & Primary Beams
Phased Array Feeds & Primary Beams Aidan Hotan ASKAP Deputy Project Scientist 3 rd October 2014 CSIRO ASTRONOMY AND SPACE SCIENCE Outline Review of parabolic (dish) antennas. Focal plane response to a
More informationInstrument Requirements and Options for Meeting the Science Opportunities MHz P. Dewdney A. Gray, B. Veidt
Instrument Requirements and Options for Meeting the Science Opportunities 300-3000 MHz P. Dewdney A. Gray, B. Veidt Dominion Radio Astrophysical Observatory Herzberg Institute of Astrophysics National
More informationNumerical Approach for the Analysis and Optimization of Phased Array Feed Systems
Numerical Approach for the Analysis and Optimization of Phased Array Feed Systems The Netherlands Institute for Radio Astronomy (ASTRON) Supported by part: - The Netherlands Organization for Scientific
More informationTowards SKA Multi-beam concepts and technology
Towards SKA Multi-beam concepts and technology SKA meeting Meudon Observatory, 16 June 2009 Philippe Picard Station de Radioastronomie de Nançay philippe.picard@obs-nancay.fr 1 Square Kilometre Array:
More informationTechnologies for Radio Astronomy Mark Bowen Acting Theme Leader Technologies for Radio Astronomy October 2012 CSIRO ASTRONOMY AND SPACE SCIENCE
Technologies for Radio Astronomy Mark Bowen Acting Theme Leader Technologies for Radio Astronomy October 2012 CSIRO ASTRONOMY AND SPACE SCIENCE Outline Current Projects CABB ATCA C/X Upgrade FAST Parkes
More informationIntegrated receivers for mid-band SKA. Suzy Jackson Engineer, Australia Telescope National Facility
Integrated receivers for mid-band SKA Suzy Jackson Engineer, Australia Telescope National Facility SKADS FP6 Meeting Chateau de Limelette 4-6 November, 2009 Talk overview Mid band SKA receiver challenges
More informationActive Impedance Matched Dual-Polarization Phased Array Feed for the GBT
Active Impedance Matched Dual-Polarization Phased Array Feed for the GBT Karl F. Warnick, David Carter, Taylor Webb, Brian D. Jeffs Department of Electrical and Computer Engineering Brigham Young University,
More informationProgress Towards Coherent Multibeam Arrays
Progress Towards Coherent Multibeam Arrays Doug Henke NRC Herzberg Astronomy and Astrophysics, Victoria, Canada August 2016 ALMA Band 3 Receiver (84 116 GHz) Dual linear, 2SB Feed horn OMT (two linear
More informationNovember SKA Low Frequency Aperture Array. Andrew Faulkner
SKA Phase 1 Implementation Southern Africa Australia SKA 1 -mid 250 15m dia. Dishes 0.4-3GHz SKA 1 -low 256,000 antennas Aperture Array Stations 50 350/650MHz SKA 1 -survey 90 15m dia. Dishes 0.7-1.7GHz
More informationPhased Array Feeds A new technology for multi-beam radio astronomy
Phased Array Feeds A new technology for multi-beam radio astronomy Aidan Hotan ASKAP Deputy Project Scientist 2 nd October 2015 CSIRO ASTRONOMY AND SPACE SCIENCE Outline Review of radio astronomy concepts.
More informationTHE KAROO ARRAY TELESCOPE (KAT) & FPA EFFORT IN SOUTH AFRICA
THE KAROO ARRAY TELESCOPE (KAT) & FPA EFFORT IN SOUTH AFRICA Dr. Dirk Baker (KAT FPA Sub-system Manager) Prof. Justin Jonas (SKA SA Project Scientist) Ms. Anita Loots (KAT Project Manager) Mr. David de
More informationMemo 65 SKA Signal processing costs
Memo 65 SKA Signal processing costs John Bunton, CSIRO ICT Centre 12/08/05 www.skatelescope.org/pages/page_memos.htm Introduction The delay in the building of the SKA has a significant impact on the signal
More informationDense Aperture Array for SKA
Dense Aperture Array for SKA Steve Torchinsky EMBRACE Why a Square Kilometre? Detection of HI in emission at cosmological distances R. Ekers, SKA Memo #4, 2001 P. Wilkinson, 1991 J. Heidmann, 1966! SKA
More informationFocal Plane Arrays & SKA
Focal Plane Arrays & SKA Peter Hall SKA International Project Engineer www.skatelescope.org Dwingeloo, June 20 2005 Outline Today: SKA and antennas Phased arrays and SKA Hybrid SKA possibilities» A hybrid
More informationMay AA Communications. Portugal
SKA Top-level description A large radio telescope for transformational science Up to 1 million m 2 collecting area Operating from 70 MHz to 10 GHz (4m-3cm) Two or more detector technologies Connected to
More informationCharacteristics of Smooth-Walled Spline-Profile Horns for Tightly Packed Feed-Array of RATAN-600 Radio Telescope
Characteristics of Smooth-Walled Spline-Profile Horns for Tightly Packed Feed-Array of RATAN-600 Radio Telescope N. POPENKO 1, R. CHERNOBROVKIN 1, I. IVANCHENKO 1, C. GRANET 3, V. KHAIKIN 2 1 Usikov Institute
More informationFundamentals of Radio Astronomy. Lyle Hoffman, Lafayette College ALFALFA Undergraduate Workshop Arecibo Observatory, 2008 Jan. 13
Fundamentals of Radio Astronomy Lyle Hoffman, Lafayette College ALFALFA Undergraduate Workshop Arecibo Observatory, 2008 Jan. 13 Outline Sources in brief Radiotelescope components Radiotelescope characteristics
More informationIntroduction to Radio Astronomy!
Introduction to Radio Astronomy! Sources of radio emission! Radio telescopes - collecting the radiation! Processing the radio signal! Radio telescope characteristics! Observing radio sources Sources of
More informationDetector Systems. Graeme Carrad
Detector Systems Graeme Carrad November 2011 The Basic Structure of a typical Radio Telescope Antenna Receiver Conversion Digitiser Signal Processing / Correlator They are much the same CSIRO. Radiotelescope
More informationArray noise temperature measurements at the Parkes PAF Test-bed Facility
Array noise temperature measurements at the Parkes PAF Test-bed Facility Douglas B. Hayman, Aaron P. Chippendale, Robert D. Shaw and Stuart G. Hay MIDPREP 1 April 2014 COMPUTATIONAL INFORMATICS ASTRONOMY
More information2-PAD: An Introduction. The 2-PAD Team
2-PAD: An Introduction The 2-PAD Team Workshop, Jodrell Bank, 10 Presented th November 2009 by 2-PAD: Dr An Georgina Introduction Harris Georgina Harris for the 2-PAD Team 1 2-PAD Objectives Demonstrate
More informationMultiplying Interferometers
Multiplying Interferometers L1 * L2 T + iv R1 * R2 T - iv L1 * R2 Q + iu R1 * L2 Q - iu Since each antenna can output both L and R polarization, all 4 Stokes parameters are simultaneously measured without
More informationPhased Array Feed (PAF) Design for the LOVELL Antenna based on the Octagonal Ring Antenna (ORA) Array
Phased Array Feed (PAF) Design for the LOVELL Antenna based on the Octagonal Ring Antenna (ORA) Array M. Yang, D. Zhang, L. Danoon and A. K. Brown, School of Electrical and Electronic Engineering The University
More informationAntenna Fundamentals. Microwave Engineering EE 172. Dr. Ray Kwok
Antenna Fundamentals Microwave Engineering EE 172 Dr. Ray Kwok Reference Antenna Theory and Design Warran Stutzman, Gary Thiele, Wiley & Sons (1981) Microstrip Antennas Bahl & Bhartia, Artech House (1980)
More informationMulti-Mode Antennas for Hemispherical Field-of-View Coverage
Multi-Mode Antennas for Hemispherical Field-of-View Coverage D.S. Prinsloo P. Meyer R. Maaskant M.V. Ivashina Dept. of Electrical and Electronic Engineering Dept. of Signals and Systems Stellenbosch, South
More informationSKA The Australian Perspective
SKA The Australian Perspective Peter J Hall CSIRO SKA Program Leader http://www.atnf.csiro.au/ska Presentation Outline Background Australia and the SKA New seed research program» Philosophy, Working Principles,
More informationInterference Mitigation Using a Multiple Feed Array for Radio Astronomy
Interference Mitigation Using a Multiple Feed Array for Radio Astronomy Chad Hansen, Karl F Warnick, and Brian D Jeffs Department of Electrical and Computer Engineering Brigham Young University Provo,
More informationSubmitted to the SKA Engineering and Management Team by
Authors: John D. Bunton Carole A. Jackson Elaine M. Sadler CSIRO Telecommunications and Industrial Physics RSAA, Australian National University School of Physics, University of Sydney Submitted to the
More informationDesign of a Novel Compact Cup Feed for Parabolic Reflector Antennas
Progress In Electromagnetics Research Letters, Vol. 64, 81 86, 2016 Design of a Novel Compact Cup Feed for Parabolic Reflector Antennas Amir Moallemizadeh 1,R.Saraf-Shirazi 2, and Mohammad Bod 2, * Abstract
More informationL-Band and X-Band Antenna Design and Development for NeXtRAD
L-Band and X-Band Antenna Design and Development for NeXtRAD S. T. Paine, P. Cheng, D. W. O Hagan, M. R. Inggs, H. D. Griffiths* Department of Electrical Engineering Radar Remote Sensing Group University
More informationThe SKA New Instrumentation: Aperture Arrays
The SKA New Instrumentation: Aperture Arrays A. van Ardenne, A.J. Faulkner, and J.G. bij de Vaate Abstract The radio frequency window of the Square Kilometre Array is planned to cover the wavelength regime
More informationMore Radio Astronomy
More Radio Astronomy Radio Telescopes - Basic Design A radio telescope is composed of: - a radio reflector (the dish) - an antenna referred to as the feed on to which the radiation is focused - a radio
More informationRecent Developments in Measuring Signal and Noise in Phased Array Feeds at CSIRO
Recent Developments in Measuring Signal and Noise in Phased Array Feeds at CSIRO A. P. Chippendale, D. McConnell, K. Bannister, N. Nikolic, A. W. Hotan, K. W. Smart, R. D. Shaw, D. B. Hayman, S. G. Hay
More informationPhased Array Feeds A new technology for wide-field radio astronomy
Phased Array Feeds A new technology for wide-field radio astronomy Aidan Hotan ASKAP Project Scientist 29 th September 2017 CSIRO ASTRONOMY AND SPACE SCIENCE Outline Review of radio astronomy concepts
More informationTechnologies for Radio Astronomy
Technologies for Radio Astronomy CSIRO Astronomy and Space Science Alex Dunning in lieu of Tasso Tzioumis Facilities Program Director Technologies June 2017 Directions for ATNF Engineering (Update since
More informationOPTICS OF SINGLE BEAM, DUAL BEAM & ARRAY RECEIVERS ON LARGE TELESCOPES J A M E S W L A M B, C A L T E C H
OPTICS OF SINGLE BEAM, DUAL BEAM & ARRAY RECEIVERS ON LARGE TELESCOPES J A M E S W L A M B, C A L T E C H OUTLINE Antenna optics Aberrations Diffraction Single feeds Types of feed Bandwidth Imaging feeds
More informationDesign of Rotman Lens Antenna at Ku-Band Based on Substrate Integrated Technology
Journal of Communication Engineering, Vol. 3, No.1, Jan.- June 2014 33 Design of Rotman Lens Antenna at Ku-Band Based on Substrate Integrated Technology S. A. R. Hosseini, Z. H. Firouzeh and M. Maddahali
More informationNewsletter 3.1. Antenna Magus version 3.1 released! New antennas in the database. Square pin-fed septum horn. July 2011
Newsletter 3.1 July 2011 Antenna Magus version 3.1 released! Antenna Magus 3.0 was such a feature laden release that not all of the new features could be mentioned in the newsletter, so we decided to rather
More informationFocal Plane Array Beamformer for the Expanded GMRT: Initial
Focal Plane Array Beamformer for the Expanded GMRT: Initial Implementation on ROACH Kaushal D. Buch Digital Backend Group, Giant Metrewave Radio Telescope, NCRA-TIFR, Pune, India kdbuch@gmrt.ncra.tifr.res.in
More informationPhased Array Feeds for Parkes. Robert Braun Science with 50 Years Young
Phased Array Feeds for Parkes Robert Braun Science with Parkes @ 50 Years Young Outline PAFs in the SKA context PAFSKA activities Apertif, BYU, NRAO, NAIC, DRAO, ASKAP ASKAP PAF MkI ASKAP PAF MkII Parkes:
More informationENHANCEMENT OF PHASED ARRAY SIZE AND RADIATION PROPERTIES USING STAGGERED ARRAY CONFIGURATIONS
Progress In Electromagnetics Research C, Vol. 39, 49 6, 213 ENHANCEMENT OF PHASED ARRAY SIZE AND RADIATION PROPERTIES USING STAGGERED ARRAY CONFIGURATIONS Abdelnasser A. Eldek * Department of Computer
More informationGreen Bank Instrumentation circa 2030
Green Bank Instrumentation circa 2030 Dan Werthimer and 800 CASPER Collaborators http://casper.berkeley.edu Upcoming Nobel Prizes with Radio Instrumentation Gravitational Wave Detection (pulsar timing)
More informationFinal Feed Selection Study For the Multi Beam Array System
National Astronomy and Ionosphere Center Arecibo Observatory Focal Array Memo Series Final Feed Selection Study For the Multi Beam Array System By: Germán Cortés-Medellín CORNELL July/19/2002 U n i v e
More informationCHAPTER 2 MICROSTRIP REFLECTARRAY ANTENNA AND PERFORMANCE EVALUATION
43 CHAPTER 2 MICROSTRIP REFLECTARRAY ANTENNA AND PERFORMANCE EVALUATION 2.1 INTRODUCTION This work begins with design of reflectarrays with conventional patches as unit cells for operation at Ku Band in
More informationField Experiments in RFI Detection using an Array
Field Experiments in RFI Detection using an Array International SKA Meeting Berkeley July 2001 Steve Ellingson ellingson.1@osu.edu http://esl.eng.ohio-state.edu/rfse/argus/rfse-argus.html Introduction
More informationCHAPTER 5 ANALYSIS OF MICROSTRIP PATCH ANTENNA USING STACKED CONFIGURATION
1 CHAPTER 5 ANALYSIS OF MICROSTRIP PATCH ANTENNA USING STACKED CONFIGURATION 5.1 INTRODUCTION Rectangular microstrip patch with U shaped slotted patch is stacked, Hexagonal shaped patch with meander patch
More informationAperture Antennas. Reflectors, horns. High Gain Nearly real input impedance. Huygens Principle
Antennas 97 Aperture Antennas Reflectors, horns. High Gain Nearly real input impedance Huygens Principle Each point of a wave front is a secondary source of spherical waves. 97 Antennas 98 Equivalence
More informationIntroduction to Radio Astronomy. Richard Porcas Max-Planck-Institut fuer Radioastronomie, Bonn
Introduction to Radio Astronomy Richard Porcas Max-Planck-Institut fuer Radioastronomie, Bonn 1 Contents Radio Waves Radio Emission Processes Radio Noise Radio source names and catalogues Radio telescopes
More informationLE/ESSE Payload Design
LE/ESSE4360 - Payload Design 4.3 Communications Satellite Payload - Hardware Elements Earth, Moon, Mars, and Beyond Dr. Jinjun Shan, Professor of Space Engineering Department of Earth and Space Science
More informationTunable Multi Notch Digital Filters A MATLAB demonstration using real data
Tunable Multi Notch Digital Filters A MATLAB demonstration using real data Jon Bell CSIRO ATNF 27 Sep 2 1 Introduction Many people are investigating a wide range of interference suppression techniques.
More informationBRAND EVN EVN) Joint Research Activity in RadioNet4 Gino Tuccari & Walter Alef plus partners
BRAND EVN (BRoad-bAND EVN) Joint Research Activity in RadioNet4 Gino Tuccari & Walter Alef plus partners EVN Observing Bands < 22GHz Today in the EVN separate receivers cover: 18 cm - L band 13 cm - S
More informationNewsletter 4.4. Antenna Magus version 4.4 released! Array synthesis reflective ground plane addition. July 2013
Newsletter 4.4 July 2013 Antenna Magus version 4.4 released! We are pleased to announce the new release of Antenna Magus Version 4.4. This release sees the addition of 5 new antennas: Horn-fed truncated
More informationTechnology Drivers, SKA Pathfinders P. Dewdney
Technology Drivers, SKA Pathfinders P. Dewdney Dominion Radio Astrophysical Observatory Herzberg Institute of Astrophysics National Research Council Canada National Research Council Canada Conseil national
More informationNew Trends on Receivers Development" May 30, 2005, Medicina. RECEIVING SYSTEMs for the ANTENNAS OPERATED by the INSTITUTE of RADIOASTRONOMY in ITALY
New Trends on Receivers Development" May 30, 2005, Medicina RECEIVING SYSTEMs for the ANTENNAS OPERATED by the INSTITUTE of RADIOASTRONOMY in ITALY Alessandro Orfei IRA-INAF, Medicina station (Italy) RADIONET
More informationOverview of the SKA. P. Dewdney International SKA Project Engineer Nov 9, 2009
Overview of the SKA P. Dewdney International SKA Project Engineer Nov 9, 2009 Outline* 1. SKA Science Drivers. 2. The SKA System. 3. SKA technologies. 4. Trade-off space. 5. Scaling. 6. Data Rates & Data
More informationNotes 21 Introduction to Antennas
ECE 3317 Applied Electromagnetic Waves Prof. David R. Jackson Fall 018 Notes 1 Introduction to Antennas 1 Introduction to Antennas Antennas An antenna is a device that is used to transmit and/or receive
More informationEtude d un récepteur SIS hétérodyne multi-pixels double polarisation à 3mm de longueur d onde pour le télescope de Pico Veleta
Etude d un récepteur SIS hétérodyne multi-pixels double polarisation à 3mm de longueur d onde pour le télescope de Pico Veleta Study of a dual polarization SIS heterodyne receiver array for the 3mm band
More informationBroadband Balanced Microstrip Antenna Fed by a Waveguide Coupler
278 Broadband Balanced Microstrip Antenna Fed by a Waveguide Coupler R. Gotfrid*, Z. Luvitzky*, H. Matzner* and E. Levine** * HIT, Holon Institute of Technology Department of Communication Engineering,
More informationRecent progress and future development of Nobeyama 45-m Telescope
Recent progress and future development of Nobeyama 45-m Telescope Masao Saito: Director of Nobeyama Radio Observatory Tetsuhiro Minamidani: Nobeyama Radio Observatory Outline Nobeyama 45-m Telescope Recent
More informationBRAND EVN AND EVN) (BRoad-bAND Joint Research Activity in RadioNet4 Gino Tuccari & Walter Alef plus partners
BRAND EVN (BRoad-b AND EVN) (BRoad-bAND Joint Research Activity in RadioNet4 Gino Tuccari & Walter Alef plus partners digital VLBI-receiver: ~1.5-15.5 GHz for the EVN and other telescopes Prototype for
More informationA NOVEL DUAL-BAND PATCH ANTENNA FOR WLAN COMMUNICATION. E. Wang Information Engineering College of NCUT China
Progress In Electromagnetics Research C, Vol. 6, 93 102, 2009 A NOVEL DUAL-BAND PATCH ANTENNA FOR WLAN COMMUNICATION E. Wang Information Engineering College of NCUT China J. Zheng Beijing Electro-mechanical
More information"(c) 2017 IEEE. Personal use of this material is permitted. Permission from IEEE must be obtained for all other users, including reprinting/
"(c) 17 IEEE. Personal use of this material is permitted. Permission from IEEE must be obtained for all other users, including reprinting/ republishing this material for advertising or promotional purposes,
More informationBRAND EVN (BRoad-bAND EVN) Joint Research Activity in RadioNet4 Gino Tuccari & Walter Alef plus partners
BRAND EVN (BRoad-bAND EVN) Joint Research Activity in RadioNet4 Gino Tuccari & Walter Alef plus partners digital VLBI-receiver: ~1.5-15.5 GHz for the EVN and other telescopes Prototype for prime focus
More informationSKA station cost comparison
SKA station cost comparison John D. Bunton, CSIRO Telecommunications and Industrial Physics 4 August 2003 Introduction Current SKA white papers and updates present cost in a variety of ways which makes
More informationCasper Instrumentation at Green Bank
Casper Instrumentation at Green Bank John Ford September 28, 2009 The NRAO is operated for the National Science Foundation (NSF) by Associated Universities, Inc. (AUI), under a cooperative agreement. GBT
More informationPLANAR BEAM-FORMING ARRAY FOR BROADBAND COMMUNICATION IN THE 60 GHZ BAND
PLANAR BEAM-FORMING ARRAY FOR BROADBAND COMMUNICATION IN THE 6 GHZ BAND J.A.G. Akkermans and M.H.A.J. Herben Radiocommunications group, Eindhoven University of Technology, Eindhoven, The Netherlands, e-mail:
More informationThe Importance of Polarization Purity Author: Lars J Foged, Scientific Director at MVG (Microwave Vision Group)
The Importance of Polarization Purity Author: Lars J Foged, Scientific Director at MVG (Microwave Vision Group) The polarization purity of an antenna system is an important characteristic, particularly
More informationWide-Band Imaging. Outline : CASS Radio Astronomy School Sept 2012 Narrabri, NSW, Australia. - What is wideband imaging?
Wide-Band Imaging 24-28 Sept 2012 Narrabri, NSW, Australia Outline : - What is wideband imaging? - Two Algorithms Urvashi Rau - Many Examples National Radio Astronomy Observatory Socorro, NM, USA 1/32
More informationAllen Telescope Array & Radio Frequency Interference. Geoffrey C. Bower UC Berkeley
Allen Telescope Array & Radio Frequency Interference Geoffrey C. Bower UC Berkeley Allen Telescope Array Large N design 350 x 6.1m antennas Sensitivity of the VLA Unprecedented imaging capabilities Continuous
More informationThe Future: Ultra Wide Band Feeds and Focal Plane Arrays
The Future: Ultra Wide Band Feeds and Focal Plane Arrays Germán Cortés-Medellín NAIC Cornell University 1-1 Overview Chalmers Feed Characterization of Chalmers Feed at Arecibo Focal Plane Arrays for Arecibo
More informationIntroduction to Radio Astronomy
Introduction to Radio Astronomy The Visible Sky, Sagittarius Region 2 The Radio Sky 3 4 Optical and Radio can be done from the ground! 5 Outline The Discovery of Radio Waves Maxwell, Hertz and Marconi
More informationCircular Focal Plane Array for Astronomic Applications
International Workshop on Phased Array Antenna Systems for Radio Astronomy Circular Focal Plane Array for Astronomic Applications Rémi Sarkis, Christophe Craeye May 3-5, 21 Provo, Utah, USA 1 Introduction
More informationA 3 20GHz Vivaldi Antenna with Modified Edge
A 3 20GHz Vivaldi Antenna with Modified Edge Bieng-Chearl Ahn* * and Otgonbaatar Gombo Applied Electromagnetics Laboratory, Department of Radio and Communications Engineering Chungbuk National University,
More informationSome Notes on Beamforming.
The Medicina IRA-SKA Engineering Group Some Notes on Beamforming. S. Montebugnoli, G. Bianchi, A. Cattani, F. Ghelfi, A. Maccaferri, F. Perini. IRA N. 353/04 1) Introduction: consideration on beamforming
More informationA NEW INNOVATIVE ANTENNA CONCEPT FOR BOTH NARROW BAND AND UWB APPLICATIONS. Neuroscience, CIN, University of Tuebingen, Tuebingen, Germany
Progress In Electromagnetics Research, Vol. 139, 121 131, 213 A NEW INNOVATIVE ANTENNA CONCEPT FOR BOTH NARROW BAND AND UWB APPLICATIONS Irena Zivkovic 1, * and Klaus Scheffler 1, 2 1 Max Planck Institute
More informationPRIME FOCUS FEEDS FOR THE COMPACT RANGE
PRIME FOCUS FEEDS FOR THE COMPACT RANGE John R. Jones Prime focus fed paraboloidal reflector compact ranges are used to provide plane wave illumination indoors at small range lengths for antenna and radar
More informationSchool of Electrical Engineering. EI2400 Applied Antenna Theory Lecture 8: Reflector antennas
School of Electrical Engineering EI2400 Applied Antenna Theory Lecture 8: Reflector antennas Reflector antennas Reflectors are widely used in communications, radar and radio astronomy. The largest reflector
More informationA METHOD TO DESIGN DUAL-BAND, HIGH-DIRECTI- VITY EBG RESONATOR ANTENNAS USING SINGLE- RESONANT, SINGLE-LAYER PARTIALLY REFLECTIVE SURFACES
Progress In Electromagnetics Research C, Vol. 13, 245 257, 2010 A METHOD TO DESIGN DUAL-BAND, HIGH-DIRECTI- VITY EBG RESONATOR ANTENNAS USING SINGLE- RESONANT, SINGLE-LAYER PARTIALLY REFLECTIVE SURFACES
More informationAn FPGA-Based Back End for Real Time, Multi-Beam Transient Searches Over a Wide Dispersion Measure Range
An FPGA-Based Back End for Real Time, Multi-Beam Transient Searches Over a Wide Dispersion Measure Range Larry D'Addario 1, Nathan Clarke 2, Robert Navarro 1, and Joseph Trinh 1 1 Jet Propulsion Laboratory,
More informationBroadband Dual Polarized Space-Fed Antenna Arrays with High Isolation
Progress In Electromagnetics Research C, Vol. 55, 105 113, 2014 Broadband Dual Polarized Space-Fed Antenna Arrays with High Isolation Prashant K. Mishra 1, *, Dhananjay R. Jahagirdar 1,andGirishKumar 2
More informationChalmers Publication Library
Chalmers Publication Library Parabolic cylindrical reflector antenna at 6 Hz with line feed in gap waveguide technology This document has been downloaded from Chalmers Publication Library (CPL). It is
More informationDesign and Verification of Cross-Polarization Compensation Feed for Single Reflector Compact Antenna Test Range over a Wide Bandwidth
Design and Verification of Cross-Polarization Compensation Feed for Single Reflector Compact Antenna Test Range over a Wide Bandwidth L. J. Foged, A. Giacomini, A. Riccardi Microwave Vision Italy s.r.l.
More informationA NEW WIDEBAND DUAL LINEAR FEED FOR PRIME FOCUS COMPACT RANGES
A NEW WIDEBAND DUAL LINEAR FEED FOR PRIME FOCUS COMPACT RANGES by Ray Lewis and James H. Cook, Jr. ABSTRACT Performance trade-offs are Investigated between the use of clustered waveguide bandwidth feeds
More informationIntroduction to Radar Systems. Radar Antennas. MIT Lincoln Laboratory. Radar Antennas - 1 PRH 6/18/02
Introduction to Radar Systems Radar Antennas Radar Antennas - 1 Disclaimer of Endorsement and Liability The video courseware and accompanying viewgraphs presented on this server were prepared as an account
More informationThe Shaped Coverage Area Antenna for Indoor WLAN Access Points
The Shaped Coverage Area Antenna for Indoor WLAN Access Points A.BUMRUNGSUK and P. KRACHODNOK School of Telecommunication Engineering, Institute of Engineering Suranaree University of Technology 111 University
More informationA Compact Broadband Printed Circular Slot Antenna with Stair Shaped Ground Plane
Progress In Electromagnetics Research Letters, Vol. 74, 9 16, 2018 A Compact Broadband Printed Circular Slot Antenna with Stair Shaped Ground Plane Baudha Sudeep 1, * and Kumar V. Dinesh 2 Abstract This
More informationChalmers Publication Library
Chalmers Publication Library Analysis of the strut and feed blockage effects in radio telescopes with compact UWB feeds This document has been downloaded from Chalmers Publication Library (CPL). It is
More informationGBT Spectral Baseline Investigation Rick Fisher, Roger Norrod, Dana Balser (G. Watts, M. Stennes)
GBT Spectral Baseline Investigation Rick Fisher, Roger Norrod, Dana Balser (G. Watts, M. Stennes) Points to Note: Wider bandwidths than were used on 140 Foot Cleaner antenna so other effects show up Larger
More informationBroadband and High Efficiency Single-Layer Reflectarray Using Circular Ring Attached Two Sets of Phase-Delay Lines
Progress In Electromagnetics Research M, Vol. 66, 193 202, 2018 Broadband and High Efficiency Single-Layer Reflectarray Using Circular Ring Attached Two Sets of Phase-Delay Lines Fei Xue 1, *, Hongjian
More informationPhotonic Integrated Beamformer for Broadband Radio Astronomy
M. Burla, D. A. I. Marpaung, M. R. H. Khan, C. G. H. Roeloffzen Telecommunication Engineering group University of Twente, Enschede, The Netherlands P. Maat, K. Dijkstra ASTRON, Dwingeloo, The Netherlands
More informationAntenna Theory and Design
Antenna Theory and Design Antenna Theory and Design Associate Professor: WANG Junjun 王珺珺 School of Electronic and Information Engineering, Beihang University F1025, New Main Building wangjunjun@buaa.edu.cn
More information