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Joshua Smith, Elba, Italy 31.05.06
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Elba, Italy 31.05.06 Joshua Smith for the GEO 600 team Picture of GEO in stormy weather?? Or pics of tractors with trees? Instrumental and environmental noise in GEO600 North building
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Joshua Smith, Elba, Italy 31.05.06 Overview Environmental: oSeismic oDust oMagnetic fields / Mains Instrumental: oNoise Projections oTracking couplings oNoise subtraction oNoise vetoes A selection of recent detector characterization work
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Joshua Smith, Elba, Italy 31.05.06 Seismic / up-conversion H @ 240Hz H @ 290Hz H @ 340Hz Seis @ 49Hz 0 Time [h] 3.5 Amplitude (max)
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Joshua Smith, Elba, Italy 31.05.06 Dust
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Power glitches Detector output Input port power
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Joshua Smith, Elba, Italy 31.05.06 Back-coupling? Strain coupling to DC power Dark port DC Power Strain back-coupling doesn’t explain instrumental channel coincidence
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Joshua Smith, Elba, Italy 31.05.06 Power glitches vs. dust Dark port DC power glitch count Particle count Dark port DC power glitch count Input port DC power glitch count 0 Time [m] 180
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Joshua Smith, Elba, Italy 31.05.06 Particle waves filtered 140 20 45 5 3 0.2 (Particles/cu.ft)/1000 AaAa
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Joshua Smith, Elba, Italy 31.05.06 Dust made loudest glitches Before filterAfter filter Time [h] Det. output BLRMS @~ 170Hz
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Joshua Smith, Elba, Italy 31.05.06 Magnetic fields / Mains
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Joshua Smith, Elba, Italy 31.05.06 Magnetic field glitches B glitches H glitches Linear coupling, coherence
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Joshua Smith, Elba, Italy 31.05.06 Magnetic field “projection” B-field nearly limiting noise around 100Hz? oCoupling not yet understood oChecks: magnetometer measures B-field, IFO back-coupling ruled out
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Joshua Smith, Elba, Italy 31.05.06 Hourly mains glitches Hourly series start: o24 secs after GPS hour o10 secs after UTC hour 24s
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Joshua Smith, Elba, Italy 31.05.06 Mag./mains coinc. with H Frequency [Hz] Magnetometer central building ~ 50coinc./8hrs Time-freq glitch maps Time-shifted coincidence Mains monitor central building ~ 30coinc./8hrs Time [h] 0088 50 0 0 Time shift [s] 1 1 Frequency [Hz]
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Joshua Smith, Elba, Italy 31.05.06 Noise Projections
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Joshua Smith, Elba, Italy 31.05.06 Noise Budget Alignment actuation Scattering, up-conversion, ? Shot, dark, osc. phase
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Joshua Smith, Elba, Italy 31.05.06 Tracking noise transfer func’s Tracked: Signal Recycl. FB Osc. Phase Laser intensity Frequency Amp ratio ~ 1 phase diff ~ 0
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Joshua Smith, Elba, Italy 31.05.06 Transfer func’s: long-term (10d) 10 days, most projections: +/- 10% mag +/- 10 degs phase So, long-term stable Ratio/Diffs drifts Histogram of drifts
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Joshua Smith, Elba, Italy 31.05.06 Noise transfer func’s: short-term +/- 20% mag. variations on second timescales!
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Joshua Smith, Elba, Italy 31.05.06 Noise Subtraction
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Joshua Smith, Elba, Italy 31.05.06 Detector output and noise Detector output Noise chans. Record subset Noise projection Noise budget Improved H
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Joshua Smith, Elba, Italy 31.05.06 Noise subtraction requirements Subtraction factor depends on amplitude ratio and phase difference of filter used and real transfer function response.
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Joshua Smith, Elba, Italy 31.05.06 Noise subtraction results Time domain subtraction, simple IIR filters fit to measured TF response. Ratio H/(H-Projs) But, no reduction of up-conversion
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Joshua Smith, Elba, Italy 31.05.06 Technical noise veto
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Joshua Smith, Elba, Italy 31.05.06 Noise veto: eg. injection H Michelson oscillator phase noise
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Joshua Smith, Elba, Italy 31.05.06 Noise veto performance “Robust vetoes for gravitational-wave burst triggers using known instrumental couplings” P. Ajith, M. Hewitson, J. R. Smith, K. A. Strain, submitted to CQG, http://arxiv.org/abs/gr-qc/0605079 Estimated veto efficiency vs. rejection probability for the chosen thresholds.
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Joshua Smith, Elba, Italy 31.05.06 The end 'falco tinnunculus', better know as 'Turmfalke'
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Joshua Smith, Elba, Italy 31.05.06 Noise subtraction II Used simple IIR filters - good match to simple transfer function
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Joshua Smith, Elba, Italy 31.05.06 Statistical dust veto? MID VIS veto TF map and timeshifted results
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