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GEO – VIRGO joint noise hunting project

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Presentation on theme: "GEO – VIRGO joint noise hunting project"— Presentation transcript:

1 GEO – VIRGO joint noise hunting project
G. Vajente and J. Smith ILIAS WG1 Meeting Cascina, November 13th 2006

2 Summary Progress in Virgo Noise Hunting
Automatic longitudinal noise budget Laser intensity noise investigations Frequency noise investigations Control noise investigations Plans and ideas for noise reduction

3 Automatic longitudinal noise budget
Automatic script Measure TFs with noise injections in the error points of the loops Compute projections and coherences Noise budget for WSR5 MICH = short michelson differential length PRCL = Power Recycling Cavity length Pr_B1_ACp = dark fringe signal

4 Laser intensity noise investigations /1
Power stabilization topology Uses one diode after IMC Bs_IMC_D1T_DCHF

5 Laser intensity noise investigations /2
PSTAB OFF PSTAB ON DARK NOISE Pstab error signal reduced below dark noise (ADC) Other diodes limited by dark (ADC) noise above ~50 Hz Improved after diodes tuning and emphasis / de-emphasis filters implentation

6 Laser intensity noise investigations /3
NORTH ARM TRANSM. DARK FRINGE BS PICK-OFF WEST ARM TRANSM. PR REFLECTION Coherences of dark fringe signal with ITF powers High with DC power in the dark fringe itself

7 A possible mechanism MICH control loop generate dark fringe power noise due to an offset This power noise couples to ACp signal due to RMS fluctuation of dark fringe Normal condition MICH noise injected

8 Suspects of MICH longitudinal offset /1
DARK FRINGE BS PICK-OFF SIDEBANDS IN PR CAV. ITF powers versus Michelson error signal Powers should be maximum/minimum around the correct operating point NORTH TRANSMISSION

9 A first experiment about MICH offset
DARK FRINGE BS PICK-OFF DF / (BS PICK-OFF) B5_ACq is MICH error signal Added an artificial offset (uncalibrated) Dependence of ITF powers on the offset Need for an full exploration of two-dimens. MICH-PRCL space SIDEBANDS IN PRC PR REFLECTION NORTH TRANSM.

10 Frequency Noise investigations
WSR2 data Frequency noise is limiting high frequency part of the spectrum Coupling changes a lot in time

11 Fluctuation of freq. Noise coupling
Coherence and TF from frequency servo correction to dark fringe signal, computed while injecting noise, short periods, two different times

12 Coupling measurement with calibration line
Coupling coefficient measured with calibration lines Lots of structures Almost everywhere good coherence with RMS of high frequency noise

13 Origin of coupling fluctuation?
Coherences with mirrors positions read by local control systems PR BS A good candidate is alignment… NE WE

14 Alpha technique impact
MICH correction is sent to end mirrors with opposite phases to reduce dark fringe contamination


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