Exploration of Frequency Interactions and Correlations in High Scatter Events

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Delve into the analysis of high scatter events through spectrograms and waveform comparisons of varying frequencies. Researchers investigate correlations with different signals and accelerometers, seeking to replicate and identify key patterns in the observed noise data. Ongoing efforts include examining motion thresholds, lock losses coinciding with specific events, and historical data analysis for configuration changes impact assessment.


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  1. Daytime Scatter at LLO

  2. Whats going on here?

  3. Spectrogram during high scatter time ???????? = 2?????(?) ? Scatter model using ~0.2 Hz + ~4 Hz velocities

  4. 1 cycle in 5 sec = 0.2 Hz 0.2 Hz Sine wave Abs(0.2 Hz Sine wave) Abs(0.2 Hz Sine wave + 4.45 Hz Sine wave)

  5. But its not as simple when you beat two frequencies against each otherHere we see that the amplitude of the 4.45 Hz is smaller than the 0.2 Hz, so the small peaks correspond to a full cycle instead of a half cycle as we saw with the 0.2 Hz series. ?t = 0.22 sec -> 4.45 Hz

  6. Whats been done: Next steps: Marissa, Sidd, et al looked for correlations with trains during noise sprint in January, but didn t find a clear winner Terra looked for ~4 Hz motion in accelerometers during scatter times, but didn t find a clear winner (alog 44897) Lots of injections at various places show high coupling at End-Y, but haven t been able to fully replicate the noise we see or identify a sensor that sees the same motion as the scattering surface (alogs 41789,44485 + many more) Collect statistics on fast and slow arches as Josh did in alog 44803 Look for correlations with motion of mirrors as Andy did in alog 44561 Look for correlations with control signals: ASC, tidal, etc (can provide a list of channels) Look back through commissioning data to see if the behavior changed with IFO configuration changes Continue to look for correlations with accelerometers (as per Terra s work in 44897)

  7. Other ideas Look for thresholds of motion Is there a threshold of the sum of the microseism BLRMS and anthropogenic BLRMs for scatter in DARM? Look at locklosses coincident with trains April 6 at ~14:00 UTC Range dip April 8 at ~0:00 UTC

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