LIGO-G000339-00-M Overview of the LIGO Continuing Operations (FY2002 - FY2006) Proposal Gary Sanders LIGO PAC9 Meeting December 2000.

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Presentation transcript:

LIGO-G M Overview of the LIGO Continuing Operations (FY FY2006) Proposal Gary Sanders LIGO PAC9 Meeting December 2000

LIGO-G M

LIGO Laboratory Funding To Date MRE

LIGO-G M Construction Project Status

LIGO-G M LHO 2 km Interferometer Strain Sensitivity in Recombined Mode

LIGO-G M Results/Accomplishments Construction as planned nearly complete Installation/Commissioning well underway LSC formed and functioning LSC participating in first Engineering Runs Science working groups formed Observatory operations established at both sites LSC vision for future detectors is leading a vigorous development program International partnership/networking forming LIGO is source of industrial/community/education outreach

LIGO-G M LIGO Facilities Support Detector Upgrades

LIGO-G M Program and Mission of the LIGO Laboratory l observe gravitational wave sources; l develop advanced detectors that approach and exploit the facility limits on interferometer performance; l operate the LIGO facilities to support the national and international scientific community; l and support scientific education and public outreach related to gravitational wave astronomy.

LIGO-G M LIGO Proposes To: l Complete commissioning of the initial LIGO interferometers; l operate the LIGO interferometers for the initial LIGO Science Run; l process and analyze the Science Run data and publish the results of the first scientific searches for gravitational wave sources; l characterize and improve the sensitivity and availability of the operating interferometers; l define interferometer upgrades and carry out a research and development program to underpin future upgrade proposals; l support the development and research of the LIGO Scientific Collaboration; l support the development of the international network of gravitational wave detectors; l interpret the LIGO program to the public; l leverage LIGO in educational settings; l and address new industrial technologies and applications stimulated by the requirements of gravitational wave observation.

LIGO-G M LIGO Funding Evolution and Proposal Request

LIGO-G M Proposal Request

LIGO-G M Increased Operations Tasks at the Observatories

LIGO-G M Increased Hardware Costs

LIGO-G M R&D Most work supports Advanced LIGO realization Some far reaching research All work highly collaborative Lab coordinates program through LSC »full cost/schedule planning in use »monthly telecons with each working group Engineering and some senior effort supported from Lab Operations Big ticket equipment items for LSC program in Lab proposal

LIGO-G M Increased Staffing to Support R&D and Modeling

LIGO-G M R&D Effort

LIGO-G M R&D Equipment in Support of LSC Research Program Equipment costs for the development of advanced seismic isolation prototypes. Equipment costs for the development of multiple pendulum, fused silica fiber suspension prototypes. Materials and manufacturing subcontracts to support the development of sapphire test masses and high Q test mass materials and coatings research. Investment and non-recurring engineering costs for a large coating chamber and its commissioning.

LIGO-G M Isolation Research (STO, SUS, TNI, SEI) FY02 N.B.: Does not include LSC research staff.

LIGO-G M Lasers & Optics Research (LAS, OPT, IOS, AOS) FY02 N.B.: Does not include LSC research staff.

LIGO-G M Advanced Interferometer Systems, Sensing & Control (ISC, 40m, SID, SYS) FY02

LIGO-G M Total LIGO Laboratory R&D FY02