LIGO-G06xxxx-00-M Technical Progress Planned/Needed in FY07 Advanced LIGO Program Advisory Panel meeting, 30 November – 1 December 2006, MIT Dennis Coyne,

Slides:



Advertisements
Similar presentations
LIGO-G M May 17, 2006 Installation (INS) Requirements and Design Breakout Presentation NSF Review of Advanced LIGO Project Dennis Coyne, Caltech.
Advertisements

G v1System Integration Status and Challenges1 System Integration Status and Challenges, Post Project Commissioning Plans to Meet Science Goals May.
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.
Thermal Compensation System – TCS Technical Presentation aLIGO NSF Review LIGO Livingston Observatory April LIGO-G v5.
G R LIGO Laboratory1 Advanced LIGO Research and Development David Shoemaker LHO LSC 11 November 2003.
LIGO-G W Status of LIGO Installation and Commissioning Frederick J. Raab, LIGO Hanford Observatory.
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.
E2E school at LLO1  Han2k »Model of the LHO 2k IFO »Designed for lock acquisition study  SimLIGO1 »Model of all LIGO 1 IFOs »Designed for –noise hunting.
G M Advanced R&D1 Seismic Isolation Retrofit Plan for the LIGO Livingston Observatory Dennis Coyne 29 Nov 2001.
Thermal Compensation NSF David Ottaway LIGO Laboratory MIT.
LIGO-G M LIGO Laboratory1 Adv. LIGO Seismic Isolation (SEI) Plans, Schedule, Costs, Team Schedule »through R&D, including near-term plans »project.
LIGO-G M Advanced LIGO Cost, Schedule and Management Gary H Sanders NSF Review of Advanced LIGO Caltech, June 11, 2003.
G R LIGO Laboratory1 Advanced LIGO Research and Development Update Dennis Coyne LSC Meeting at LLO 16 March 2004.
LIGO-G M 1 Advanced LIGO Status LIGO Scientific Collaboration Meeting August 15, Dennis Coyne LIGO Laboratory, Caltech.
LIGO-G D partial ADVANCED LIGO1 Development Plan R&D including Design through Final Design Review »for all long lead or high risk subsystems »LIGO.
20 Nov 2008G v21 Optical & Vacuum Equipment Layouts Dennis Coyne Mike Smith Luke Williams 20 Nov 2008 Adv. LIGO Team Meeting, Caltech, Pasadena,
Thermal Compensation Review David Ottaway LIGO Laboratory MIT.
LIGO-G M April 5, 2006 Interferometer Sensing and Control (ISC) Cost and Schedule Breakout Presentation NSF Review of Advanced LIGO Project Richard.
Advanced LIGO Commissioning Overview Stanford LVC Meeting, August 27, 2014 Peter Fritschel.
G R Advanced LIGO Seismic Isolation R&D Dennis Coyne 8 Oct 2002.
Overview of Research in the Optics Working Group Gregory Harry, on behalf of the OWG Massachusetts Institute of Technology July 25, 2007 LSC Meeting –
4/25/11 G v3 1 Facility Modifications and Preparations (FMP) Technical Status Annual NSF Review of Advanced LIGO Project April , 2011 John.
LIGO-G D 1 Advanced LIGO Optical & Mechanical Layout Status Dennis Coyne, LIGO Caltech LSC Meeting, 21 Mar 2006 Version -01: with a couple of.
Optical Configuration Advanced Virgo Review Andreas Freise for the OSD subsystem.
LIGO-G M May 31-June 2, 2006 Input Optics (IO) Cost and Schedule Breakout Presentation NSF Review of Advanced LIGO Project David Reitze UF.
1 1.ISC scope and activities 2.Initial Virgo status 3.Design requirements 4.Reference solution and design status 5.Plans toward completion 6.Technical.
LIGO-G M 1 Conceptual Design Review: Initial LIGO Seismic Isolation System Upgrade Development, Implementation Plan & Schedule Dennis Coyne April.
G M 1 Advanced LIGO Update David Shoemaker LSC/Virgo MIT July 2007.
LIGO-G Advanced LIGO Detector upgrade is planned for »Factor of 10 increase in distance probed (‘reach’) »Factor of 1000 increase in event.
Advanced VIRGO WG1: Status VIRGO, Cascina Andreas Freise University of Birmingham.
LIGO- G D The LIGO Instruments Stan Whitcomb NSB Meeting LIGO Livingston Observatory 4 February 2004.
G Z LIGO R&D1 Input Optics Definition, Function The input optics (IO) conditions light from the pre- stabilized laser (PSL) for injection into.
G Consideration of HAM SAS for Advanced LIGO David Shoemaker LIGO Excomm 30 April 07.
Advanced Virgo Optical Configuration ILIAS-GW, Tübingen Andreas Freise - Conceptual Design -
G R 1 Advanced LIGO Update David Shoemaker LSC LHO March 2006.
LIGO-G D LIGO R&D1 Advanced LIGO R&D Review The PSL Peter King & Rich Abbott October 8, 2002.
G R LIGO R&D1 Advanced LIGO Update Dennis Coyne LSC LLO March 2005.
LIGO LaboratoryLIGO-G R Coatings and Their Influence on Thermal Lensing and Compensation in LIGO Phil Willems Coating Workshop, March 21, 2008,
Nov 3, 2008 Detection System for AdV 1/8 Detection (DET) Subsystem for AdV  Main tasks and requirements for the subsystem  DC readout  Design for: the.
Advanced LIGO Simulation, 6/1/06 Elba G E 1 ✦ LIGO I experience ✦ FP cavity : LIGO I vs AdvLIGO ✦ Simulation tools ✦ Time domain model Advanced.
LIGO-G D 1 Status of Detector Commissioning LSC Meeting, March 2001 Nergis Mavalvala California Institute of Technology.
G R Proposed Adv. R&D FY R&D for Advanced LIGO David Shoemaker & Dennis Coyne 29 January 2001.
LIGO-G M Advanced LIGO Cost, Schedule and Management Gary H Sanders NSF Review of Advanced LIGO Caltech, June 11, 2003.
LSC Meeting at LHO LIGO-G E 1August. 21, 2002 SimLIGO : A New LIGO Simulation Package 1. e2e : overview 2. SimLIGO 3. software, documentations.
Advanced LIGO Status Report
LIGO-G M LIGO Status Gary Sanders GWIC Meeting Perth July 2001.
LIGO-G M Overview of LIGO R&D and Planning for Advanced LIGO Detectors Gary Sanders NSF R&D Review Caltech, January 29, 2001.
Cascina, Nov. 4 th, 2008 AdV review 1 AdV Injection system E. Genin European Gravitational Observatory.
LSC Meeting March ‘07 1 LIGO ADVANCED SYSTEMS TEST INTERFEROMETER (LASTI) LASTI Progress and Plans LSC Meeting, LLO Dave Ottaway/Richard Mittleman March.
LIGO-G D Commissioning at Hanford Stan Whitcomb Program Advisory Committee 12 December 2000 LIGO Livingston Observatory.
G R Interferometer Sensing & Control P Fritschel 8 Oct 02.
LIGO-G M Overview of the LIGO Continuing Operations (FY FY2006) Proposal Gary Sanders LIGO PAC9 Meeting December 2000.
G R LIGO R&D1 Advanced LIGO Update David Shoemaker LSC LHO August 2004.
Advanced Towards Advanced Virgo Giovanni Losurdo – INFN Firenze Advanced Virgo Coordinator on behalf of the Virgo Collaboration.
G I Enhanced LIGO Update Rana Adhikari July ’07 LSC Meeting.
LIGO-G M State of the LIGO Laboratory Gary Sanders LIGO/Caltech LSC Meeting, LLO March 16, 2004 State of LIGO.
LIGO- G M LIGO Status Stan Whitcomb Oversight Committee 20 October 2004.
LIGO-G D Advanced LIGO Systems & Interferometer Sensing & Control (ISC) Peter Fritschel, LIGO MIT PAC 12 Meeting, 27 June 2002.
G R 2004 Plan Update LIGO Systems meeting 22 Jan 04 dhs.
LIGO-G d April 24, 2007 Auxiliary Optics System (AOS) Technical Breakout Presentation NSF Review of Advanced LIGO Project Mike Smith, Phil Willems.
Thermal Compensation NSF
Next Generation Low Frequency Control Systems
Reaching the Advanced LIGO Detector Design Sensitivity
First Lessons from the Advanced LIGO Integration Testing
Update on the Advanced LIGO PSL Program
R&D Highlights Seismic Isolation Suspensions ISC/40m
Stan Whitcomb LSC meeting Livingston 21 March 2005
Improving LIGO’s stability and sensitivity: commissioning examples
Auxiliary Optics System (AOS)
Advanced LIGO R&D Review Input Optics
Presentation transcript:

LIGO-G06xxxx-00-M Technical Progress Planned/Needed in FY07 Advanced LIGO Program Advisory Panel meeting, 30 November – 1 December 2006, MIT Dennis Coyne, Caltech

LIGO-G06xxxx-00-M 2 Technical Progress: Planned/Needed in FY07 state of development -- advise on triage or prioritization to ensure readiness Systems (SYS) Interferometer Sensing & Controls (ISC) Control & Data Systems (CDS) incl. Data Acquisition, Diagnostics & Control (DAQ) Data and Computing Systems (DCS) Seismic Isolation (SEI) Suspensions (SUS) Core Optics Components (COC) Input Optics (IO) Auxiliary Optics System (AOS) Thermal Compensation System (TCS) Pre-Stabilized Laser (PSL) system Facility Modifications & Preparations (FMP) Installation (INS) LIGO Advanced System Test Interferometer (LASTI) 40 m Lab Experiment (40m) Subsystems without significant start-of-project, readiness concerns: » PSL – 35W front-end MOPA for enhanced LIGO will be installed 2007 » IO – high power component technology & subsystem design well developed; components to be tested in Enhanced LIGO » AOS –low-risk engineering, with the exception of AOS/Thermal Compensation System (TCS) » Data and Computing Systems (DCS) – design based on off-the-shelf hardware (in the future) » FMP/INS – minimal preparation for contracted items; mostly not schedule critical » 40m – responsive to ISC needs

LIGO-G06xxxx-00-M 3 Systems: Planned/Needed FY07 Progress Conduct a Systems Preliminary Design Review (1 st Qtr 2007) » Effort lags plan –Risk of improper requirements flowdown – Systems Scientist & Engineer involved in most subsystem meetings & decisions –Distraction of key staff -- hiring & setting priorities » Decision: Stable vs Nearly-Unstable Signal &/or Power Recycling Cavities » Modulation scheme & frequencies chosen (ISC) » Definitive optical layout for the Core Optics » Preliminary (but complete) opto-mechanical layout for all LVEA systems » Finalize all generic design & fabrication guidance (EMI/EMC, UHV, QA/QC, etc.) » Interface Control Documents established for all subsystems » Contamination Control Plan/Design (with COC) » Simulation –Demonstrate angular stability at high power –Sensitivity of optical design to optical figure, thermal lensing Likely defer till Final Design Phase (FY08): » Suspension Point Interferometer (SPI) » Simulation –Determine if parametric instability (coupled acoustic & optical modes) are to be mitigated by COC design (ITM transmission, coating aperture) –Improved lock acquisition approaches

LIGO-G06xxxx-00-M 4 Interferometer Sensing & Control (ISC): Planned/Needed FY07 Progress Hold a Design Requirements Review (1 st Qtr 2007) Preliminary Design progress through 2007 (review late 07 or early 08) » In-vacuum, suspended Output Mode Cleaner (OMC) and photodection to be demonstrated –LASTI testing starts May 2007; currently in preliminary design » DC read-out and OMC performance in an interferometer –40m Lab experiment: non-suspended prototype under test –Enhanced LIGO: to be installed Nov 2007 » Length, Alignment and modulation scheme chosen –Required to definitize the optics layout & COC parameters (COC polishing starts CY08) –Modeling underway » Lock acquisition scheme –demonstrated in End-to-End (E2E) simulation (possibly) –Demonstrated in 40m experiment

LIGO-G06xxxx-00-M 5 Control & Data Systems (CDS): Planned/Needed FY07 Progress Conduct a Data Acquisition, Networking & Supervisory Control (DAQ) Requirements Review (early 2007) Preliminary Design progress through 2007 (review late 07 or early 08) » Install & Test at LASTI (PCIX & EPICS architecture): –FrameBuilder, RealTime Network (Myranet) & Quad Suspension controls (PCI-X) have been installed & are under test –Install/test of HAM-SAS prototype controls has begun (to be completed Jan) –BSC-ISI prototype controls –OMC Length & Alignment Controls, OMC SUS Controls & antisymmetric optical port Read-out electronics –DC Power distribution system » EMI/EMC and thermal management approach to be defined Install & Test at 40m Lab: » OMC Length & Alignment Controls & Read-out electronics & software are nearing completion (based on new architecture) Concerns: » QA & QC (including proper & timely definition of requirements) » Thermal management for front-end systems – liquid cooled?

LIGO-G06xxxx-00-M 6 Core Optic Components (COC): Planned/Needed FY07 Progress Preliminary Design efforts through 3Q 2007 ‘Polishing Pathfinder’ RFP » Achieve Advanced LIGO requirements on full scale optics (better figure & tighter Radius Of Curvature tolerance) » Hope to contract 3 polishers soon Coating R&D continues to reduce thermal noise & absorption » coatings good enough, but improvements help performance Prepare production polishing RFP package (ready for FY2008 funds) Concerns: » Understanding & Controlling loss due to point scatter –Currently installed test masses indicate ppm of scatter loss –R&D continues to identify source/cause (substrate, coating) » Polishing Pathfinder is late – COC is a (near) critical path effort » Single Source for Test Mass Coatings (LMA/Lyon)

LIGO-G06xxxx-00-M 7 Thermal Compensation System (TCS): Planned/Needed FY07 Progress Thermal compensation strategy is still evolving (conceptual design last Aug) » Compensation plate dimensions changed to improve radiative coupling to the test mass » Proposed addition of low emissivity coating on the test mass barrel (to mitigate radial gradients) » Considering removal of compensation plate ring heater » … » All of these considerations effect suspension and COC design details Testing » Hartmann sensors at Gin Gin » Initial and Enhanced LIGO (CO2 heating beam) » Ring heater at LASTI (temperature fields only) » Full scale performance via simulation alone Concern is late development compared to need to finalize the COC optics and Suspension design details external heating beam Ring heater mask Compensation plate might be a –dn/dT material

LIGO-G06xxxx-00-M 8 Seismic Isolation (SEI): Planned/Needed FY07 Progress HAM Isolation » ISI (baseline, “stiff”) or SAS (alternate, “soft”) Decision (4/2007) –HAM-ISI (“stiff”) single stage prototype design & revised costing –HAM-SAS (“soft”) prototype test at LASTI » HAM prototype fabrication (Enhanced & Advanced LIGO) –1 st unit ready for install at LLO by Oct –2 nd & 3 rd units ready for install at LHO & LASTI by Dec BSC-ISI prototype » Complete clean assembly & installation » Performance testing: –Stand-alone –With quadruple, ETM suspension (test dynamic coupling, control re-allocation, etc.) System Diagnostics & Control Synthesis Tool Development » Essential for rapid control system tuning after installation » Stanford’s on-going ETF Technology Demonstration effort supports the control synthesis Concerns: » HAM-SEI is critical path and development schedule has risk – contractor hired » LIGO SEI is understaffed – looking for personnel now » Dual HAM-ISI & HAM-SAS effort may have significant payoff but saps critical resources & is divisive – hold to April 2007 decision date

LIGO-G06xxxx-00-M 9 Suspensions (SUS): Planned/Needed FY07 Progress Suspensions – 11 Types: BSC Chamber Suspensions (UK): » Paced by UK Funding » Proceeding ahead of project need dates » Stressing LASTI integrated test plan HAM Chamber Suspensions (US): » Efforts are delayed by lack of personnel – in hiring mode now » US suspension focus is Output Mode Cleaner (OMC) suspension for ISC and Enhanced LIGO » Prototyping for FY07 dependent on LASTI integrated test replan Electrostatic Charging Issues » R&D to understand charge generation, transfer and mitigation has been slow » Testing new earthquake stop design intended for Enhanced LIGO use

LIGO-G06xxxx-00-M 10 LIGO Advanced System Test Interferometer (LASTI): Planned/Needed FY07 Progress LASTI planning has undergone very significant changes over the years to accommodate HEPI development and late R&D schedules for SUS & SEI LASTI oversight committee is charged with advising on a replan » Does the deployment of adv. LIGO elements into Enhanced LIGO obviate the need for LASTI system-level, optical-cavity testing? (HAM-SEI, OMC, PSL)? » Should we consider any system-level testing at LASTI to be risk reduction alone and not tie to development/fabrication schedules? Original two test-cavity layout for LASTI