Thanks to the measurements performed in 37461, we have projected the stray ligth noise in the B4 DC and on MICH. We used the daya of May 10.
In order to do this, we have measured the TF between the Meggit accelerometer ENV_SPRB_LINK_ACC_Z (placed on the link) and the B4 DC and MICH signals as coupling targets.
As displacement noise input has been used the quiet data merging the GURALP data at low frequency (below 10Hz) and the Megitt above (the ENV_SPRB_LINK_ACC_Z). We used the 95th percentile of both seismic sensors computed over that day.
The attenuation factor between the bounches has been chosen (more or less arbitrarely to be 10).
The outcomes of the simulations are shown in Figure 1 for B4 and Figure 2 for MICH. It is clear that the contribution of stray ligth noise is not negligible below a few hundred hertz.
Moreover some structure are well reconstructed by the projected noise (such as ~19Hz, 25Hz, 90Hz, ...)
More investigations are needed and a test of reducing the coupling by moving the beam in the link should be performed (even if there is really a poor margin of beam displacement)
Moreover a test to mitigate the link vibration can be performed such as applying weigths on the link itslef (such as the sand bags used in Virgo for the brewster window).