DVA-1 Project Overview Gordon Lacy April 2014.

Slides:



Advertisements
Similar presentations
Antennas for MeerKAT March TDP AWG, 13-14/3/08, San Francisco MeerKAT Semantics K.A.T. = Karoo Array Telescope –KAT is Afrikaans for cat –MeerKAT:
Advertisements

FDWAVE : USING THE FD TELESCOPES TO DETECT THE MICRO WAVE RADIATION PRODUCED BY ATMOSPHERIC SHOWERS Simulation C. Di Giulio, for FDWAVE Chicago, October.
DVA1 Project Gary Hovey and Gordon Lacy Herzberg Jamboree 23 October 2014 NRC-Herzberg Astronomy Technology Program - Penticton.
SIW 2003 The antenna element Ravi ATNF, Narrabri 1.The role of the antenna in a Fourier synthesis radio telescope 2.The Compact array antenna.
DVA1 Project Overview and Status Gary Hovey and Gordon Lacy SKA Project Office Visit DRAO 29 March 2014 NRC-Herzberg Astronomy Technology Program - Penticton.
SKA Specifications and Reflector Antennas P. Dewdney Mar 31, 2008.
Progress Report TDP-CART 15m Offset Antenna Collaboration National Research Council Herzberg Institute of Astrophysics Dominion Radio Astrophysical Observatory.
Goals of DVA-1 Meeting Overall goal: build an SKA antenna with SKA feeds/receivers, verify performance and fabrication/costs for the next stages of the.
Manufacturing with Composite
ALTERNATIVE MECHANICALS DVA1 Meeting at NSF Arlington VA April 15-16, 2010 Matt Fleming Contributions from Jack Welch Roger Schultz Gordon Lacy.
SHIP STRUCTURES Unique Structures (6.1) What are they optimized for?
High Performance Low-Cost Composite Antenna Reflectors for the SKA DOMINION RADIO ASTROPHYSICAL OBSERVATORY Herzberg Institute of Astrophysics Penticton.
ATA Antennas Feeds and Systems NSF Review 8/05/08 Jack Welch.
Dominion Radio Astrophysical Observatory DVA-1 Reflector Development Timeline Gary Hovey NRC-HIA Dominion Radio Astrophysical Observaotry.
CURRENT SKA TDP ANTENNA DESIGN 10 DVA1 Meeting at NSF Arlington VA April 15-16, 2010 Matt Fleming Contributions from Jack Welch Roger Schultz Gordon Lacy.
Antenna, Feed, and LNA Integration S. Weinreb, May 7, 2009, LAX Antenna Working Group Meeting 1.Issues 2.Feed Summary 3.LNA Summary 4.Differential LNA’s.
SKA TDP & CART 15m (DVA-1) ANTENNA DESIGN 11 US SKA Consortium Meeting at Arlington VA June 3-4, 2010 Matt Fleming Contributions from Jack Welch Roger.
National Astronomy and Ionosphere Center © Germán Cortés M 2008 SKA TDP Antenna Optics By Germán Cortés M. Cornell University Ithaca NY 14853, USA National.
E. Szpindor, J. Ruff Advisory Committee Briefing June 10-11, Antennas and Feeds.
Name1 title 4 th SKADS Workshop, Lisbon, 2-3 October 2008 Progress in Active Antenna Design and Developement - FIDA3 Timothy Finn FG-IGN
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.
Space Frame Structures for SNAP Bruce C. Bigelow University of Michigan Department of Physics 11/04/04.
BUILDING CONSTRUCTION V ARCHITECTURAL FINISHING SYSTEMS
Concepts for Combining Different Sensors for CLIC Final Focus Stabilisation David Urner Armin Reichold.
Antennas The primary elements of a synthesis array M. Kesteven ATNF 25/September/2001.
Determinate Space Frame Telescope Structures for SNAP Bruce C. Bigelow University of Michigan Department of Physics 7/28/04.
Developing a low cost dish for MeerKAT Willem Esterhuyse Subsystem manager: Antenna Structures
Tenth Summer Synthesis Imaging Workshop University of New Mexico, June 13-20, 2006 Antennas in Radio Astronomy Peter Napier.
P.Napier, Synthesis Summer School, 18 June Antennas in Radio Astronomy Peter Napier Interferometer block diagram Antenna fundamentals Types of antennas.
26 April 2013 Immanuel Gfall (HEPHY Vienna) Belle II SVD Overview.
DVA1 Project Status Gary Hovey and Gordon Lacy SKA Visit, Sept NRC-Herzberg Astronomy Technology Program - Penticton.
SKA Dishes, SEEG Meeting Cape Town September 2013 SKA Dish Verification Antenna #1 – Test Plan Gary Hovey, DVA-1 Project Manger Astronomy Technology.
US SKA TDP DVA-1 June 28-29, 2012Dish Verification Antenna No. 1 Critical Design Review, Penticton, BC Overview Of DVA-1 Optics Lynn Baker Bill Imbriale.
Proposed Versatile 1.2 to 14 GHz Radio Telescope Receiver S. Weinreb, JPL/Caltech, Draft July 5, 2005 Contents 1.Introduction and intended applications.
Departement Elektriese en Elektroniese Ingenieurswese  Department of Electrical and Electronic Engineering Ultra Wideband Reflector Antenna Feeds Dirk.
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.
DVA1 Project Status Gary Hovey and Gordon Lacy ngVLA Workshop, April NRC-Herzberg Astronomy Technology Program - Penticton.
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.
4/20/2004s.e.mathews1 Steward Observatory Technical Division Mechanical Engineering Seminar Series Seminar #1 April 20, 2004.
Thoughts on the Design of a WVR for Alan Roy (MPIfR) the Twin Telescope at Wettzell.
Steerable antennas Meeting July 2005
An alternative spectrograph mount Bruce C. Bigelow University of Michigan Department of Physics 5/14/04.
Institute for Astronomy Herson Bagay Mentor : Garry Nitta Advisor : Jeff Kuhn.
April 8/9, 2003 Green Bank GBT PTCS Conceptual Design Review Out of Focus (OOF) Holography for the GBT Claire Chandler.
June 3,4 2010Lynn Baker USSKA Consortia Washington, DC1 TDP / AWG Update Lynn Baker USSKA Consortia Meeting Washington DC June 3,4, 2010.
Dish Verification Antenna – 1 Project NRC - Herzberg Gary Hovey 18 November 2013.
The Allen Telescope Array Douglas Bock Radio Astronomy Laboratory University of California, Berkeley Socorro, August 23, 2001.
IRMOS Diffraction Grating Integral Tab Design  Performance of an optical system is highly sensitive to the surface distortion of the optics in the system.
US SKA TDP Antenna Design Progress US SKA AWG Meeting May 6, 2009, Los Angeles. California Matt Fleming Contributions from Jack Welch Roger Schultz Sandy.
Lightweight mirror technology using a thin facesheet with active rigid support J. H. Burge, J. R. P. Angel, B. Cuerden, H. Martin, S. Miller University.
SSR1 Cryomodule Development for PXIE - Alignment T. Nicol Decenber 6, 2011.
MAGNESIUM THIXOMOLDING
SKA – MID Sensitivity Mike Jones Jamie Leech Angela Taylor University of Oxford with data from Miroslav Pantaleev (Chalmers) Isak Theron (EMSS) Yang.
Building Construction
6 May 2009Lynn Baker AWG Meeting LA1 TDP Antenna and Feed Plan Lynn Baker Antenna Working Group Meeting Los Angeles, CA May 6, 2009.
DVAC PROGRESS OFFSET GREGORIAN DISH (DVAC-1) 郑元鹏 (Yuanpeng Zheng ) Joint Lab. for Radio Astronomy and Technology MAY 29, 2012.
April 17, Dejan TrbojevicFFAG07 -Non-Scaling FFAG gantries1 Non-Scaling FFAG Gantries Introduction: Motives: The most challenging problem in the carbon/proton.
Single Cryocooler 1.2 to 116 GHz Receiver for ngVLA S. Weinreb, A. Soliman, and H. Mani July 30, Rationale 2.Synergistic Reflector Design 3.Dewar.
Earthquake competition
Antennas in Radio Astronomy
Task detailed definition Pierfrancesco Lombardo
Composite Mirror Applications, Inc
The Parabolic Antenna.
NGVLA Science Workshop, Socorro NM June 26, 2017
Reflector & Single Pixel Feed Panel Discussion
DVA-1 Baseline Optical Design
CH-6 CABLE TV.
Agenda, Day 1, Tuesday, June 19
Iross™ Fluxmanager® Stress relieving System
Presentation transcript:

DVA-1 Project Overview Gordon Lacy April 2014

The Dish Verification Antenna, DVA-1 Built on composite knowledge from 2 previous 10m composite dishes Combined composite expertise with US TDP group (ATA design) Key Features: A 15m aperture, feed-high offset Gregorian with shaped optics Rim supported composite shell primary and secondary Composite tubes supporting feed platform and secondary Deep tubular truss backing structure

DVA-1: Designed for High Dynamic Range Capability High Thermal Performance Rim supported monocoque design along with very low CTE materials keeps all thermal movement both small and very uniform to minimize effect on beam pattern High Performance in Wind and Gravity Central compliant connector allows some structural sag without inducing unwanted distortion at center of dish Rim supported design keeps dish deflections to absolute minimum and concentrates any deflections at rim where effect on performance is small. Extremely deep truss back structure keeps dish shape as close to rigid as is possible. High Overall Optics Stability Secondary and feed platform support optimized to maximize stiffness using shape optimization software. Secondary and feed support tubes use zero and matched CTE carbon tubes for extremely high thermal stability.

DVA-1: Shaped Offset Optics Advantage Clear optical path, no blockage or scattering Combined with shaped optics, leads to very low spillover (~ -50db wide angle) Very low spillover yields very low antenna noise temperature (<6 K ground) Very low spillover results in high rejection of RFI and strong sources Shaped optics yield high efficiencies, total result is a high Aeff / Tsys

DVA-1

DVA-1: Composites for Performance Structural Test Composite Design Consideration Metallic Design Consideration Creep high static load Static Strength Material properties Fatigue Life High cyclic load Glass Transition Temp. Choose resin with sufficiently high value. NA Impact Resistance Engineering requirement Galvanic Corrosion Encapsulate reflective layer Paint and primer UV, Moisture, Humidity Paint (no primer required) and resin properties Paint and Primer Reflectivity Degradation Paint (no primer required) Fungus growth Paint

Recovery from Disaster

Crack Repair

DVA-1 Reflector Repairs

DVA-1 Reflector Accuracy After Repairs Primary reflector RMS after repairs and without antenna weighting, 1.0mm RMS with repair areas removed, 0.7mm without antenna weighting

DVA-1 Secondary Reflector Accuracy Secondary Part RMS without antenna weighting 0.2mm With antenna weighting 0.11mm

GDSatcom Secondary Reflector We have now built two sub reflectors for the GDSatcom Meerkat project RMS of reflector 0.090mm Mold RMS 0.058mm

DVA-1 Prototype Target: To meet all of the SKA performance goals, as of Q4 2012. 2014 Target To meet the SKA 2012 performance goals To investigate the SKA 2014 low frequency requirements To investigate the SKA 2014 high frequency requirements

Questions?

End Gordon Lacy, P.Eng. Tel: 250-497-2340 Gordon.lacy@nrc-cnrc.gc.ca www.nrc-cnrc.gc.ca 15