Advanced LIGO Quad Prototype Janeen Romie LSC, March 2004

Slides:



Advertisements
Similar presentations
R. Kumar 1, K. Tokmakov 2, A. V. Cumming 1, G. D. Hammond 1, J. Hough 1, S. Rowan 1 1 SUPA, University of Glasgow, Glasgow, G12 8QQ, UK, 2 SUPA, University.
Advertisements

2 mm diameter region 300 micron thermoelastic noise cancellation section Neck region, for transition from 2 mm stock to 300  m fibre 150  m section for.
G v1 H1 Squeezer Experiment Update L-V Meeting, Caltech, March 18, 2009 ANU, AEI, MIT, CIT and LHO Ping Koy Lam, Nergis Mavalvala, David McClelland,
LIGO-G D Comments: Staged implementation of Advanced LIGO Adv LIGO Systems 17 may02 dhs Nifty idea: a way to soften the shock, spread cost, allow.
QUAD Testing Outline, Phase 2B Fiber Lower “half” Build-up and Testing M. Barton, B. Bland, D. Cook, J. Kissel, N. Robertson, J. Romie, T. Sadecki, for.
G R LIGO Laboratory1 Advanced LIGO Research and Development David Shoemaker LHO LSC 11 November 2003.
LIGO-G D Suspensions Update: the View from Caltech Phil Willems LIGO/Caltech Livingston LSC Meeting March 17-20, 2003.
Overview of ACIGA high performance vibration isolator Jean-Charles Dumas Eu-Jeen Chin Chunnong Zhao Li Ju David Blair.
Seismic attenuation chains concept, design and advancement status Riccardo DeSalvo for the KAGRA Seismic group JGW-G September 10, 20121JGW-G
LIGO-G D partial ADVANCED LIGO1 Optical Layout Cavity Lengths Input Mode Cleaner (IMC) »IMC FSR = ~9 MHz »Length = ~16.6 m = ~HAM1 to HAM3 separation.
G D LIGO Laboratory1 Advanced LIGO Dennis Coyne Hannover LSC 19 August 2003.
Review of HAM Suspension Designs for Advanced LIGO Norna A Robertson HAM Isolation Requirements Review Caltech, July 11th 2005.
G R LIGO Laboratory1 Advanced LIGO Research and Development Update Dennis Coyne LSC Meeting at LLO 16 March 2004.
LIGO-G D Suspensions Design for Advanced LIGO Phil Willems NSF Review, Oct , 2002 MIT.
LSC Meeting August ‘04 1 LIGO ADVANCED SYSTEMS TEST INTERFEROMETER (LASTI) Program Update: LSC Meeting, Hanford Dave Ottaway for the LASTI team August.
LIGO-G D 1 25-May-02 Advanced LIGO Suspension Model in Mathematica Gravitational Wave Advanced Detector Workshop Elba - May 2002 Mark Barton.
September 8, 2015 THE MONOLITHIC SUSPENSION STATUS FOR THE VIRGO INTERFEROMETER THE MONOLITHIC SUSPENSION STATUS FOR THE VIRGO INTERFEROMETER Helios Vocca.
Low noise Fused Silica suspensions: from the GEO600 experience to the 2 nd generation requirements Geppo Cagnoli INFN Sez. Firenze University of Glasgow.
Overview of Research in the Optics Working Group Gregory Harry, on behalf of the OWG Massachusetts Institute of Technology July 25, 2007 LSC Meeting –
LIGO-G v1 Form F v1 HAM Suspensions Update Advanced LIGO Suspensions LIGO-Virgo Meeting March 2009 Derek Bridges representing Advanced LIGO.
SUSPENSION DESIGN FOR ADVANCED LIGO: Update on GEO Activities Norna A Robertson University of Glasgow for the GEO 600 suspension team LSC Meeting, Louisiana,
Conceptual Design for Advanced LIGO Suspensions Norna A Robertson University of Glasgow and Stanford University for the GEO suspension team +contribution.
G M 1 Advanced LIGO Update David Shoemaker LSC/Virgo MIT July 2007.
Update on Advanced LIGO suspension design and technology development towards the quad noise prototype Caroline A. Cantley for Advanced LIGO Suspension.
B. Willke, Mar 01 LIGO-G Z Laser Developement for Advanced LIGO Benno Willke LSC meeting LIGO-Livingston Site, Mar 2001.
Advanced LIGO Suspension Status Caroline A. Cantley Advanced LIGO Suspension Team / University of Glasgow for the GEO600 Group LSC Meeting, LLO March 2004.
LIGO-G D ETM STRUCTURAL DESIGN SUMMARY FEA OF PROPOSED ETM STRUCTURE ANSYS Workbench (ANSYS University Advanced) version 9.0 LIGO-G Z.
LIGO-G M Major International Collaboration in Advanced LIGO R&D Gary Sanders NSF Operations Review Hanford February, 2001.
G Z LIGO R&D1 Input Optics Definition, Function The input optics (IO) conditions light from the pre- stabilized laser (PSL) for injection into.
Cavity Work at LASTI LSC-VIRGO Meeting, Hannover - 24 th October 2007 Lisa Barsotti and Matthew Evans for the LASTI group G D.
G Consideration of HAM SAS for Advanced LIGO David Shoemaker LIGO Excomm 30 April 07.
SUSPENSION DESIGN FOR ADVANCED LIGO: Update on GEO Activities Norna A Robertson University of Glasgow for the GEO 600 suspension team LSC Meeting, Hanford.
G R 1 Advanced LIGO Update David Shoemaker LSC LHO March 2006.
Advanced LIGO UK G K 1 Some recent work on blade performance Caroline Cantley, Justin Greenhalgh, Mike Plissi, Norna Robertson, Calum Torrie,
G R LIGO R&D1 Advanced LIGO Update Dennis Coyne LSC LLO March 2005.
LSC August G Z Gingin High Optical Power Test Facility (AIGO) 1 High Optical Power Test Facility - Status First lock, auto-alignment and.
Update on Suspension Activities for Advanced LIGO Caroline A. Cantley University of Glasgow for the GEO600 Group LSC Meeting, Livingston, March 2003 (Technical.
LSC-March  LIGO End to End simulation  Lock acquisition design »How to increase the threshold velocity under realistic condition »Hanford 2k simulation.
LIGO-G D What can we Expect for the “Upper Limit” Run Stan Whitcomb LSC Meeting 13 August 2001 LIGO Hanford Observatory A Personal Reading of.
Prototype Quadruple Pendulum Update – Part 1 Norna Robertson and Calum Torrie University of Glasgow for the GEO 600 suspension team LSC Meeting, Hanford,
ILIAS - GWA N5 - Strega JRA3 General Meeting Orsay - November 5th-6th, 2004 M1 Activities.
Update on Activities in Suspensions for Advanced LIGO Norna A Robertson University of Glasgow and Stanford University LSC meeting, Hanford, Aug 20 th 2002.
LSC Meeting March ‘05 1 LIGO ADVANCED SYSTEMS TEST INTERFEROMETER (LASTI) Program Update: LSC Meeting, LLO Dave Ottaway for the LASTI team March 2006 LIGO-G Z.
Thermal Noise performance of advanced gravitational wave detector suspensions Alan Cumming, on behalf of the University of Glasgow Suspension Team 5 th.
LIGO- G050xxx -00-D Advanced LIGO SUS Installation into BSC Chambers: Mechanical Fixtures Dennis Coyne (with input from many) G May 4 th 2005.
LSC Meeting at LHO LIGO-G E 1August. 21, 2002 SimLIGO : A New LIGO Simulation Package 1. e2e : overview 2. SimLIGO 3. software, documentations.
LIGO-G M LIGO Status Gary Sanders GWIC Meeting Perth July 2001.
Advanced LIGO UK 1 LIGO-G Z Development issues for the UK Advanced LIGO project Caroline Cantley Glasgow University for the UK Advanced LIGO Team.
LSC Meeting March ‘07 1 LIGO ADVANCED SYSTEMS TEST INTERFEROMETER (LASTI) LASTI Progress and Plans LSC Meeting, LLO Dave Ottaway/Richard Mittleman March.
Lasti ISI Update March 2007 On behalf of the SEI Team LIGO-G Z.
G R LIGO R&D1 Advanced LIGO Update David Shoemaker LSC LHO August 2004.
G R Advanced LIGO1 David Shoemaker LLO LSC 19 Aug 2002.
LIGO-G Z Silicon as a low thermal noise test mass material S. Rowan, R. Route, M.M. Fejer, R.L. Byer Stanford University P. Sneddon, D. Crooks,
Advanced LIGO UK 1 LIGO-G K OSEM Development UK Advanced LIGO project Stuart Aston University of Birmingham for the UK Advanced LIGO Team LSC.
LIGO-G Z LIGO’s Thermal Noise Interferometer Progress and Status Eric D. Black, Kenneth G. Libbrecht, and Shanti Rao (Caltech) Seiji Kawamura.
LSC Meeting Baton Rouge, LA, V.Boschi for the HAM-SAS team Ben Abbott, Valerio Boschi, Dennis Coyne, Michael Forte, Jay Heefner, Yu-mei Huang,
ALIGO Monolithic stage Giles Hammond, University of Glasgow for the Advanced LIGO Suspensions Team aLIGO/aVirgo Workshop Pisa, Italy 23 rd -24 th February.
Overview of monolithic suspension work for Advanced LIGO Mariëlle van Veggel, Mark Barton, Tim Bodiya, Alan Cumming, Liam Cunningham, Giles Hammond, Gregg.
Quadruple Suspension Design for Advanced LIGO
LIGO LAB R&D PROGRAM TECHNICAL REVIEW, OCT 02
LIGO ADVANCED SYSTEMS TEST INTERFEROMETER (LASTI)
HLTS Kickoff Presentation Derek Bridges Bobby Moore July 7, 2011
LV Meeting – 22 September 2009 Brett Shapiro G v1
Update on the Advanced LIGO PSL Program
Lasti Update July 25, 2007 LIGO-G Z
S. Rowan, M. Fejer, E. Gustafson, R. Route, G. Zeltzer
P Fritschel LSC Meeting LLO, 22 March 2005
HAM SAS Test Plan at LASTI
Characterisation of the aLIGO monolithic suspensions
R&D in Glasgow MATERIALS ACTIVITY AIM Silica
Presentation transcript:

Advanced LIGO Quad Prototype Janeen Romie LSC, March 2004 LIGO LAB: CIT: H. Armandula, M. Barton, D. Coyne, J. Heefner, J. Romie, C. Torrie, P. Willems. MIT:P. Fritschel, R. Mittleman, D. Ottaway, D.Shoemaker LHO: B. Bland, D. Cook LLO: J. Hanson, J. Kern, H. Overmier, G. Traylor GEO600: GLASGOW: G. Cagnoli, C. Cantley, D. Crooks, E. Elliffe, A. Grant, A. Heptonstall, J. Hough, R. Jones, M. Perreur-Lloyd, M. Plissi, D. Robertson, S. Rowan, K. Strain, P. Sneddon, H. Ward UNIVERSITAT HANNOVER: S. Gossler, H. Lueck STANFORD UNIVERSITY: N. Robertson (also GEO/Glasgow) RUTHERFORD APPLETON LABORATORY: J. Greenhalgh, I. Wilmut THE UNIVERSITY OF BIRMINGHAM: S. Aston, M. Cruise, D. Hoyland, C. Speake, A. Vecchio STRATHCLYDE UNIVERSITY: N. Lockerbie LIGO II

Quad Prototype SUS Preliminary Design – 2 MCs & 1 Quad The Quad Prototype – one ETM, assembled at CIT, tested at LASTI. Controls Prototypes demonstrate mech. & controls requirements – use metal masses and metal suspension wires. Noise Prototypes set the limits on the thermal and excess noise in Advanced LIGO suspensions - based on GEO 600 triple pendulums. LIGO II

Quad Controls Prototype Quad Prototype Suspension Optic: 314mm diameter x 130mm thick 40 kg Metal for controls prototype same mass and moment of inertia modeled for FS and sapphire designed for sapphire Metal wires Full reaction chain 20kg, 20kg, 40kg, 40kg (masses from top to bottom) ETM > ITM LIGO II

Quad Prototype Requirements 1st mode resonance of support structure 150 Hz or greater – TBD Total mass of 418 kg with non-suspended mass of 170 kg (including contingency) Stay clear zones defined by SEI for support tubes and Stage 0 support LIGO II

Quad Concept Suspension Mass budget Structure = 66 kg + 25% contingency Non-Suspended = 70 kg + 25% contingency @ Top Blades = 24 kg @ Upper Mass = 13 kg + TBD @ Upper Int. Mass = 9 kg @ Penultimate Mass = 7 kg @ Test Mass = 7 kg Suspended = 248 kg 2x (22-22-40-40) kg OVERALL TOTAL = 418 kg REF: LIGO-T030137-04 LIGO II

Quad Progress Single, 40kg mass suspended Initial modeling and layout complete, including reduction in length – T040028 Blade Test Facility designed – parts in workshop Composite test mass designed, metal parts fabricated Layout of eddy current dampers & osems w.r.t. upper mass complete Electrostatic HV amplifiers received from Glasgow Analog electronics received from Glasgow Dspace systems at both sites ready Catcher being updated from GEO 600 RM design to quad-size FEA of structure Approach using 6 hybrid osems and 8 ligo 1 osems is for controls prototype only. MC has analog electronics designed and prototyped by GEO and Digital electronics and dSPACE interface designed and prototyped by LIGO LAB. The other MC prototype stays at CIT for testing. LIGO II

Quad Fabrication Plan Single Pendulum – 40 kg metal test mass Double Pendulum – two 40 kg metal masses Springs [cantilever blades] Upper Masses Upper Section Lower Section All leading to a Quad for Christmas Interface and Ergonomics LIGO II

Quad Fabrication Quad Task List, LIGO-T040016 Overall Assembly Suspensions Structure Jigs (including Catcher) Glass Concept Modeling and Software Springs Installation Tooling Electronics Documents LIGO II

Suspension Milestones MC controls prototype to LASTI June 2004 Installation test, local controls test Working quad prototype at CIT Christmas 2004 Local controls test, global controls functioning, ECDs, electrostatic Quad to LASTI end of January 2005 Installation test LASTI cavity test start June 2005 LIGO II

SUS Interface Every Monday, 8am Pacific – Design Meeting Every Tuesday, 9am Pacific – Technical Meeting http://www.ligo.caltech.edu/SUS.html Web-updated MATLAB and Mathematica modeling tools http://www.ligo.caltech.edu/~mbarton/ PDMWorks secure vault for data management and configuration control, in conjunction with DCC 131.215.115.155 Common design tools for SolidWorks developed by M. Perreur-Lloyd and C. Torrie http://www.ligo.caltech.edu/docs/D/D030382-04/D030382-04.pdf LIGO II

Quad Prototype Short term challenges Meeting our schedule goals. LIGO II