CNR IEIIT – Applied Electromagnetics Group AAVP, Dwingeloo, December 12-16 2011 AAVS0 Results, Dual-Polarized Vivaldi Antenna G. Virone, R. Tascone, A.

Slides:



Advertisements
Similar presentations
Johanson Technology Inc Calle Tecate Camarillo, CA 93012
Advertisements

P. M. Livingston (Presentation from a few years back) An 80 meter Aerostat-borne Phased Array for Field-Day.
Practical Radio design
6935 Oakland Mills Road, Suite G
Yoshiyuki FUJINO National Institute of Information and Communications Technology, Japan Wireless Power Transmission Activity in NICT.
SKAMP Square Kilometre Array Molonglo Prototype. Supporting Institutions  University of Sydney  Argus Technologies  ATNF  ICT Centre.
Jan Geralt Bij de Vaate DS4-T4 Wideband Integrated Antennas DS4-T4 Jan Geralt Bij de Vaate ASTRON.
Update on Measurements and Simulations at Cambridge: SKALA element + LNA Eloy de Lera Acedo Nima Razavi Ghods Cavendish Laboratory University of Cambridge.
2010 SKA Africa Bursary Conference Chalmers University of Technology Jian Yang, Associate Professor Chalmers University of Technology Sweden.
Outline We will see main families of antenna used to create a radiated radio wave: wire antennas (dipole, monopole Yagi) slot antennas (half or quarter.
APRS ANTENNAS by ED LAWRENCE WA5SWD SIMPLIFIED & TRANSMISSION LINES.
Rome – June, 19th 2012 Measurements of the RF Antenna pattern using a Unmanned Aerial Vehicle (UAV): test and results POLITECNICO DI TORINO DIPARTIMENTO.
ASTRON / Photonics p1. Photonics and AA station design Peter Maat – ASTRON Photonics and AA station design Peter Maat – ASTRON.
AAVS receiver Federico Perini AAVP December, ASTRON, Dwingeloo.
Microstrip Reflectarrays Myths and Realities JINA Conference David M
National Institute of Science & Technology Technical Seminar Presentation-2004 Presented By: Danish Kumar Hotta [EC ] Compact Microstrip Antenna.
A NEW PRINTED QUASI-LANDSTORFER ANTENNA
By: Deepika Thakur. Conceptual design of the Communication Subsystem.
A Parametric Study on the Platform Tolerance of RFID Antennas and their Performance Enhancement with Artificial Magnetic Conductors A. S. Hoenshel and.
OEIC LAB National Cheng Kung University 1 Ching-Ting Lee Institute of Microelectronics, Department of Electrical Engineering, National Cheng Kung University.
Faisal Abedin Advisor: Dr. Mohammod Ali
Phased-Array Feed Measurements at Green Bank Karl Warnick, Brian Jeffs Jonathan Landon, Mike Elmer Roger Norrod, Rick Fisher.
BDT Radio – 2b – CMV 2009/10/09 Basic Detection Techniques 2b (2009/10/09): Focal Plane Arrays Case study: WSRT System overview Receiver and.
Aperture-coupled Stacked Coplanar Patch Antenna Presented by: Mohamed Morsy Date: October 19,2006.
Prototype SKA Technologies at Molonglo: 2. Antenna and Front End G.B. Warr 1,2, J.D. Bunton 3, D. Campbell-Wilson 1, R.G. Davison 1, R.W. Hunstead 1, D.A.
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.
Dec 2010 AAVP Cambridge workshop AAVP AAVS1/2-low demonstrators Jan Geralt Bij de Vaate.
National Astronomy and Ionosphere Center © Germán Cortés M 2008 SKA TDP Antenna Optics By Germán Cortés M. Cornell University Ithaca NY 14853, USA National.
9. Radiation & Antennas Applied EM by Ulaby, Michielssen and Ravaioli.
Array Antenna Designs for the SKA-AAlo Eloy de Lera Acedo 1 AAVP 2010, Cambridge, UK. 10/12/10.
July 2015 doc.: IEEE /XXXXr0 July 2015
ESTeem Training Class Antenna Fundamentals. Decibels (dB) Used for all mathematical calculations in the radio world. – dB is a logarithmic number dB =10.
LOFAR Antenna Systems Dion Kant, Wim van Cappellen AAVP – 10 December 2010, Cambridge, UK.
Name1 SKA(DS) System Design Aspects 4 th SKADS Workshop, Lisbon, 2-3 October 2008 SKA(DS) System Design Aspects: building a system Laurens Bakker.
Electromagnetic Compatibility of a DC Power Distribution System for the ATLAS Liquid Argon Calorimeter G. BLANCHOT CERN, CH-1211 Geneva 23, Switzerland.
1 Platform-Tolerant RFID Tag Antenna Y. C. Or (1), K. W. Leung * (1), R. Mittra (2), and K.V.S. Rao (3) (1). Wireless Communications Research Centre and.
General Licensing Class G9A – G9D Antennas Your organization and dates here.
FAA/NASA Joint University Program for Air Transportation Research Jeff Dickman Chris Bartone June 20, 2003 A New Anechoic Chamber for Nearfield Antenna.
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.
Phased Array Feeds John O’Sullivan SKANZ 2012 CSIRO Astronomy and Space Science,
Distributed Adaptive Control and Metrology for Large Radar Apertures Principal Investigator: James Lux, P.E. (337) Dr. Elaine Chapin (334), Samuel Li (337),
Investigating EMC policies for the SKA Paul van der Merwe Prof. HC Reader Stellenbosch University.
Design and Miniaturization of an RFID Tag Using a Simple Rectangular Patch Antenna for Metallic Object Identification Mun Leng Ng Auto-ID Adelaide.
Designing and Manufacturing Microstrip Antenna for Wireless Communication at 2.4 GHz Monday December 27, 2010 Presented for Undergraduate Thesis ByRachmansyah.
SKA Dishes, CSIRO February 2013 SKA Dish Verification Antenna #1 Gary Hovey Astronomy Technology Program – Penticton 12 February 2013.
Electromagnetic Design of Broadband Antenna Feed Systems for the Northern Cross Radio Telescope (Bologna, Italy) Designed Broad Band Antenna Feed Systems.
DVP Testing Neil Roddis Apr 15, SPDO Why is test and verification so important for SKA dishes? Capital cost: design for low cost of a few thousand.
1 Effects of Quadratic Phase Error 2 Patterns at different range If the antenna is impedance matched, how can we check the Antenna is in radiation? Antenna.
1 Practical considerations on train antenna design CSEM.
O. García-Pérez (FG-IGN) 1FIDA3 Wide Field Astronomy and Technologies for the SKA, Limelette, 4-6 November 2009 FIDA3: A Novel Active Array for the Mid-SKA.
Ph.D. Candidate: Yunlei Li Advisor: Jin Liu 9/10/03
CODALEMA A Cosmic Ray Radio Detection Array ICRC 2007, 3-11 July Merida, Mexico CODALEMA A Cosmic Ray Radio Detection Array Didier Lebrun, LPSC Grenoble.
AAVP Workshop December 2010 TITLEAAVP Workshop December 2010 Aeff/Tsys evaluation for AAlo sensors Cambridge 8th-10th December 2010 Federico Perini 1,
Antenna II LN09_Antenna Measurements 1 /10 Antenna Measurements.
Antenna Basics.
Hanyang University 1/21 Antennas & RF Devices Lab. antenna arrays and automotive applications Kim Tae Won.
DESIGN PARAMETRES AT BASE STATION Prittu Ann Thomas Roll no :14.
Istvan Szini Alexandru Tatomirescu Gert Pedersen Aalborg University
Recent Results with the UAV-based Array Verification and Calibration System Giuseppe Virone POLITECNICO DI TORINO DIATI.
Nicolas Fagnoni – Cosmology on Safari – 14th February 2017
Antenna An antenna is a transducer that converts radio frequency electric current to electromagnetic waves that are then radiated into space. The electric.
Phased Array Feeds SKANZ 2012 John O’Sullivan
Jessore University of Science and Technology,
Phased Array Feeds Wim van Cappellen
Amateur Extra Q & A Study Pool
Slot antenna.
WEEKLY SEMINAR Sunryul Kim
Paper review Yun-tae Park Antennas & RF Devices Lab.
Panel Antenna Simulation Results Design Test Results
Presentation transcript:

CNR IEIIT – Applied Electromagnetics Group AAVP, Dwingeloo, December AAVS0 Results, Dual-Polarized Vivaldi Antenna G. Virone, R. Tascone, A. Olivieri, O.A. Peverini, G. Addamo F. Perini*, M. Schiaffino*, J. Monari*, G. Bianchi *, S. Montebugnoli* *Istituto di Radio Astronomia Istituto Nazionale di Astro Fisica

CNR IEIIT – Applied Electromagnetics Group AAVP, Dwingeloo, December Dual-pol Vivaldi 50 Ohm ver1 Maximum size 1.1 m Metal-only 50 Ohm unbal impedance No additional ground plane Very Low Cross-Pol

CNR IEIIT – Applied Electromagnetics Group AAVP, Dwingeloo, December Feed Configuration and Labeling Front Probe Back Probe Housing for Electronics

CNR IEIIT – Applied Electromagnetics Group AAVP, Dwingeloo, December Manufacturing Laser cutter -First Prototype -Laser cutting machine -Multi-layer alluminum prototype

CNR IEIIT – Applied Electromagnetics Group AAVP, Dwingeloo, December VNA Reflection Measurement

CNR IEIIT – Applied Electromagnetics Group AAVP, Dwingeloo, December Radiation Pattern Measurements Outdoor Elevated Antenna Test Range (Turin, July 2011)

CNR IEIIT – Applied Electromagnetics Group AAVP, Dwingeloo, December From Version 1 to Version 2 Good matching in the MHz band High back lobe Low directivity at 45° in E-plane Acceptable matching in the MHz band Lower back lobe Higher directivity in the ±45° sky coverage

CNR IEIIT – Applied Electromagnetics Group AAVP, Dwingeloo, December Vivaldi A eff /T sys for each polarization Theta=0° Theta=45°

CNR IEIIT – Applied Electromagnetics Group AAVP, Dwingeloo, December Effect of the Soil ICRAR Soil DATA Radiation Efficiency = 0.7 Rad. Eff. = 0.92

CNR IEIIT – Applied Electromagnetics Group AAVP, Dwingeloo, December Computation of Tant Gnd Tant gnd = T 0 (1-η R ) T 0 = 290 K

CNR IEIIT – Applied Electromagnetics Group AAVP, Dwingeloo, December Gain vs Frequency

CNR IEIIT – Applied Electromagnetics Group AAVP, Dwingeloo, December Hexacopter Far-Field Measurements (1) Telemetry and GPS RF TX and additional battery Collaboration with DITAG, Politecnico di Torino Hexacopter Battery Bow-tie antenna Optical Scatterer

CNR IEIIT – Applied Electromagnetics Group AAVP, Dwingeloo, December Hexacopter (2) FF Pattern measurement in the operative condition (ground, small array) Meas. range > 60 m GPS Accuracy : 0.5 m-> 1 cm Total Station Accuracy: 5 mm GPS-sync spectrum analyzer

CNR IEIIT – Applied Electromagnetics Group AAVP, Dwingeloo, December Low-cost Manufacturing Target Cost 200€ x antenna Target Cost 200€ x antenna Mini-production of (48) Vivaldi, with 2cm honeycomb (used for High speed NL trains)

CNR IEIIT – Applied Electromagnetics Group AAVP, Dwingeloo, December Optical Self-Powered Vivaldi BATTERY - Galvanic isolation between FE and DS -more stable amplitude&phase Vs temperature -RFI immunity (self-shielded) -no Gain disequalization -no Power Distribution  no DC power losses -easy-deployable (no buried FO) Front End That area could be sufficient, but we need more investigation and tests on the field. Thin film (amorphous silicon ) We have 0.15 m 2 maximum available area per arm.

CNR IEIIT – Applied Electromagnetics Group AAVP, Dwingeloo, December Conclusion Experimental results confirmed the computed data of the Dual-Pol Vivaldi v1. An improved version (v2) has been designed (AAVS0) and manufactured (4 x 4 array) Simulations of the soil ground effect confirm the performance (without additional mesh) A new measurement setup is being developed Industrialization process is in progress Optical Self-powered element

CNR IEIIT – Applied Electromagnetics Group AAVP, Dwingeloo, December

CNR IEIIT – Applied Electromagnetics Group AAVP, Dwingeloo, December x 3 Regular Array Simulation Element Spacing is 1.5 m

CNR IEIIT – Applied Electromagnetics Group AAVP, Dwingeloo, December VNA Coupling Measurement