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Published byJanel Skinner Modified over 8 years ago
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LIGO-G010310-00-W Status of the LHO PSLs Rick Savage LIGO Hanford Observatory LIGO Scientific Collaboration Meeting August 13-16, 2001
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LIGO-G010310-00-W LSC Meeting - August 2001 2 (Selected) PSL issues Improved optics layout Optical table support legs NPRO frequency glitches Reference cavity tidal correction servo Intensity stabilization
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LIGO-G010310-00-W LSC Meeting - August 2001 3 Revised PSL/IOO optics layout
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LIGO-G010310-00-W LSC Meeting - August 2001 4 Improved frequency noise Number of optical components reduced Path lengths shortened Reference cavity orientation changed
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LIGO-G010310-00-W LSC Meeting - August 2001 5 Frequency noise – table leg resonances Bolts tight Bolts loose Stacis system did not work -electronics noise We will try PEPS system ASAP
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LIGO-G010310-00-W LSC Meeting - August 2001 6 2 sec. 5 MHz NPRO frequency glitches Approximately one per day Alternates between step up and step down T. Kane attributes to mode instability in pump laser diode
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LIGO-G010310-00-W LSC Meeting - August 2001 7 Tidal corection servo Reduce susceptibility to room temperature fluctuations 1 mK >> m common mode arm length
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LIGO-G010310-00-W LSC Meeting - August 2001 8 Tidal servo (cont.)
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LIGO-G010310-00-W LSC Meeting - August 2001 9 Tidal servo sensor noise 25 mK
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LIGO-G010310-00-W LSC Meeting - August 2001 10 Intensity stabilization servo First loop of prototype system operational on 2-km interferometer. (R. Karwoski, P. Russell, D. Ottaway) Inside the loop after PMC Outside the loop after MC
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LIGO-G010310-00-W LSC Meeting - August 2001 11 RIN after modecleaner P/P ~6.8e-8/rtHz Detector noise floor (laser light blocked) Light on PD = 0.5 mW >> 4.6e-8/rtHz shot noise limit Only “inside” loop active
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