LIGO Status and Plans Barry Barish / Gary Sanders 13-May-02.
LIGO-G030286-00-M LIGO Laboratory1 Adv. LIGO Seismic Isolation (SEI) Plans, Schedule, Costs, Team...
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Transcript of LIGO-G030286-00-M LIGO Laboratory1 Adv. LIGO Seismic Isolation (SEI) Plans, Schedule, Costs, Team...
LIGO Laboratory 1LIGO-G030286-00-M
Adv. LIGO Seismic Isolation (SEI)Plans, Schedule, Costs, Team
Schedule» through R&D, including near-term plans
» project phase
Costs for project phase (proposed) Team -- list of people and places
LIGO Laboratory 2LIGO-G030286-00-M
Adv. LIGO Seismic Isolation (SEI)Schedule: R&D/Design Phase
Technology Demonstrator and Controls Development Testbed» Approx. full scale, HAM-like unit installed in the Stanford University
Engineering Test Facility (ETF) vacuum system
» Verify kinematics & dynamics of design ( completed)
» Further the servo-control development begun on the proof-of-concept, two-stage system (currently in process)
» Expect initial phase of servo-controls development in support of the LASTI prototypes by 4thQ 2004
LIGO Laboratory 3LIGO-G030286-00-M
Adv. LIGO Seismic Isolation (SEI)Schedule: R&D/Design Phase
“Pathfinder” Prototypes part of Preliminary Design
» Full scale, HAM and BSC units (1 each) for the LASTI integrated test system
» External Pre-Isolation (EPI) stages– Already in place at LASTI on a HAM and a BSC chamber – One unit must be reworked once a technology decision is
made (electro-magnetic vs hydraulic actuation); decision Jun2003
» RFP (“tender”) for 2 phase structural design issued Apr2003
– Proposals are being evaluated now – Source selection for phase 1 (value engineering) in Jun2003
– likely 3 awards– Source selection for phase 2 (design & fabrication) in
Sep2003 -- likely 2 awards– Hiatus during LASTI SEI subsystem testing before
production phase (phase 3)
LIGO Laboratory 4LIGO-G030286-00-M
Adv. LIGO Seismic Isolation (SEI)Schedule: R&D/Design Phase
Preliminary Design Review (PDR) held Apr 2005» After assembly and installation experience at LASTI
» Follows 5 months of “Pathfinder” stand-alone prototype testing at LASTI
Production and procurement of long lead items initiated after PDR
Final Design Review (FDR) held Nov 2005» After integrated SUS/SEI testing (test for coupled
dynamics/interaction)
LIGO Laboratory 5LIGO-G030286-00-M
Adv. LIGO Seismic Isolation (SEI)Schedule: Project Phase
WBS 4.02.4 SEI Fabrication» 4.02.4.1 Fabrication/Procurement» 4.02.4.2 Assembly» 4.02.4.3 Alignment, Calibration and Test» Total duration is 42 months for 30 units
WBS 4.02.4.1 Fabrication/Procurement» Scope includes:
– procurement of commercial off the shelf components, e.g. sensors, processors, racks, crates, etc.
– contract fabrication of custom equipment, e.g. UHV actuators, structure, etc.– In-house fabrication of custom conditioning electronics– Assembly
» Start of Jun2005 enabled by completion of LASTI HAM & BSC SEI prototype test completion, plus test and design review
» Estimated total duration is 29 months, of which structural fabrication is 24 months» Recent structural fabrication incumbent bidder estimated 23 months total required for
the production phase» First interferometer set of hardware ready for assembly 13 months after start, or
Jul2006
LIGO Laboratory 6LIGO-G030286-00-M
Adv. LIGO Seismic Isolation (SEI)Schedule: Project Phase
WBS 4.02.4.2 Assembly WBS 4.02.4.3 Alignment, Calibration and Test
» Scope includes:– Receipt/acceptance of materials/components and sub-assembliees
(assembled structure, sensor/actuator pod structures, sensors, actuators, in-vacuum cabling, etc.)
– Clean room assembly of SEI systems (HAM and BSC chamber versions) by LIGO Lab at LLO
– Alignment of sensors, actuators, flexures; balancing & calibration of actuation & sensing
– Functional testing
» Starts Jul2006, when first sets of hardware are received» First interferometer set (5 BSC units and 5 HAM units) completed
by Jul2007 (12 months)» Next 2 interferometer sets (10 BSC units and 10 HAM units)
completed Feb2009 (20 months)
LIGO Laboratory 7LIGO-G030286-00-M
Adv. LIGO Seismic Isolation (SEI)Schedule
ETC.
LIGO Laboratory 8LIGO-G030286-00-M
Adv. LIGO Seismic Isolation (SEI)Summary Schedule
N.B:Primavera detailed schedule is summarized in top, gray barsSystems group proposed revision (M020121-E2) is lower, blue bars
LIGO Laboratory 9LIGO-G030286-00-M
Adv. LIGO Seismic Isolation (SEI)Costs
All costs are in base year dollars (un-escalated) Production cost = $37,952K including 26% contingency Proposed construction cost = $37,952K – 1.7 x $667K direct labor incl.
Indirect = $36,819 Labor costs are borne by LIGO operations funds Average hardware cost = $36,819/30 units = $1,227K each chamber
LIGO Laboratory 10LIGO-G030286-00-M
Adv. LIGO Seismic Isolation (SEI)Costs
98.6%
LIGO Laboratory 11LIGO-G030286-00-M
Adv. LIGO Seismic Isolation (SEI)Costs
In-chamber mechanical fabrication 50.3% Instruments 19.5% Electronics 14.7% Mechanics 11.8% Assembly, align, calibrate, test 3.1% Controls 1.8%
LIGO Laboratory 12LIGO-G030286-00-M
Adv. LIGO Seismic Isolation (SEI)Costs
3 Interferometers (IFOs) x $6,363K = $19,089K for in-chamber Mechanical Fab Contracts
LIGO Laboratory 13LIGO-G030286-00-M
Adv. LIGO Seismic Isolation (SEI)In-Chamber Mechanical Fab. Costs
In-chamber mechanical fabrication contract unit costs are based on an analysis of the actual ETF technology demonstrator costs (LIGO-M030024-02)
Item Nominal Cost
Min Cost
Max Cost
% Max/Nominal
HPD/Allied Estimate
ETF Design & Fab -- -- -- -- $748K actual
ETF Fab -- -- -- -- $588K actual
ETF production -- -- -- -- $429K estimate
LASTI HAM prototype $744K $639K $886K 20% --
HAM First Article $553K $448K $642K 16% --
HAM Production $436K $331K $522K 20% --
LASTI BSC prototype $887 $700 $1100 24 --
BSC First Article $636K $449K $766K 20% --
BSC Production $581K $423K $715K 23% --
*
* Should have used $436K for HAM production unit cost in the cost bookrather than the estimated ETF production unit cost of $429K
LIGO Laboratory 14LIGO-G030286-00-M
Adv. LIGO Seismic Isolation (SEI)Instrument Costs
Sensing and actuation topology in relation to the two in-chamber, isolation stages
Sensors:» Low noise, capacitive
displacement sensors (6 between stages, 12 total)
» Seismometers, L4-C (6/stage 1)» Broadband Seismometer, STS-2
(3/stage 1)» Seismometer, GS-13 (3/stage 2)
Electro-magnetic Actuators:» “High” force between stages 0
and 1, BEI Kimko LA50-62-004Z» “low” force between stages 0
and 1, BEI Kimko LA18-32-006Z» Need ultra-high vacuum (UHV)
compatible versions – should be covered by 26% contingency
LIGO Laboratory 15LIGO-G030286-00-M
SEI Instrument Costs
LIGO Laboratory 16LIGO-G030286-00-M
SEI Instrument Costs
Interferometer 1 (IFO1 or LLO) will already have an external pre-isolation (EPI or stage 0) system installed» Instrument costs = $2,273K
IFO2 and IFO3 (LHO) also require instrumentation for the EPI systems:» Seismometers, L4-C, 8 total/chamber» Load Cells, 8 total/chamber» Inductive position sensors, Kaman DIT-5200, 8 total/chamber» Instrument costs = $2,558K for each of IFO2 and IFO3
Total instrument costs= $2,273K + 2 x $2,558 = $7,389K
LIGO Laboratory 17LIGO-G030286-00-M
SEI Electronics Costs
Electronics module counts are based on a conceptual system block diagram employing initial LIGO elements and anticipated processing requirements for the digital control
IFO1 will already have installed EPI (stage 0) systems; IFO2 and IFO3 will not (just as in the case of the instrumentation)
Total electronics costs= $1,513K IFO1 + $2,039K IFO2 + $2,021K IFO3= $5,573K
LIGO Laboratory 18LIGO-G030286-00-M
SEI Electronics Costs
LIGO Laboratory 19LIGO-G030286-00-M
SEI Electronics Costs
BOE continues
LIGO Laboratory 20LIGO-G030286-00-M
Adv. LIGO Seismic Isolation (SEI)Team
LIGO Lab manages the effort and carries the financial responsibility for all project phase costs
» Leader: Larry Jones (LIGO Lab, acting)» Cognizant Engineer: Larry Jones (LIGO Lab)» Cognizant Scientist: Joe Giaime (LSU)» Cognizant Scientist for EPI: Brian Lantz (Stanford)
Other Key Participants:» Stanford: Dan DeBra, Amit Ganguli, Corwin Hardham, Wensheng Hua,
Brian Lantz, Joe van Niekerk, Norna Robertson» LSU: Joe Giaime, Shyang Wen, » LIGO Lab: Rich Abbott, Dennis Coyne, Marcel Hammond, Jonathan Kern,
Katie Lilienkamp, Ken Mailand, Ken Mason, Richard Mittleman, Samir Nayfeh, David Ottaway, Kyle Ryan , Lei Zuo