LIGO-G020059-00-W Tidal Compensation Update Fred Raab, Hugh Radkins, Daniel Sigg LIGO Hanford Observatory.

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Presentation transcript:

LIGO-G W Tidal Compensation Update Fred Raab, Hugh Radkins, Daniel Sigg LIGO Hanford Observatory

LIGO-G W Tidal Compensation Update In Previous Work… Paladin code by Eric Morganson found to predict tides to within 10-20% (E2) But temperatures drifts from PSL reference cavity were large and poorly characterized Savage and Schwinberg modified temperature monitor & controller to get into ballpark (1 mK = 2 microns in a 4K arm) Radkins got tidal feedforward fine acutation working (thanks to Josh, Richard McCarthy & Dave Barker) In final days before E7, Sigg & Radkins kludged feedback path to fine actuators to remove low- frequency drive to the ETMs

LIGO-G W Tidal Compensation Update Tidal Compensation Using Fine Actuator for E7

LIGO-G W Tidal Compensation Update A Look at Eight Days of E7 Data All plots use same vertical scale (40  m/large division)

LIGO-G W Tidal Compensation Update Preliminary Fit to Feedforward and Feedback Corrections X arm Y arm feedforward feedback feedforward feedback amp period phase amp period phase

LIGO-G W Tidal Compensation Update Preliminary Fit to Tidal Perturbation Phasors at Hanford from E7 Data, Compared to Simple Earth Model Prediction

LIGO-G W Tidal Compensation Update Need Common-Mode Tidal Actuation for 4K IFOs

LIGO-G W Tidal Compensation Update Measured Frequency Response of 2K PSL Tidal Actuator Over Xmas

LIGO-G W Tidal Compensation Update What Works & What Needs Work Tides no longer cause lock to break on 2K IFO The 4K IFOs will hit the +/- 90 micron rails on the fine actuators unless common mode tide is fed forward to the PSL tidal actuator An earlier attempt to use PSL tidal actuator helped a little; frequency response measurements imply we may have used wrong pole in filter for actuator. Should test again with better identification of pole A redesign of PSL tidal actuator would help (SURF project this summer)