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AdV-COM (AdV commissioning (1st part) )
mantovani, fiori - 12:03 Friday 12 May 2017 (37581) Print this report
SPRB link scattered ligth projections on B4 DC and on MICH

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).

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fiori, mantovani, paoletti, chiummo - 17:38 Monday 22 May 2017 (37681) Print this report

We checked if our SPRB LINK injection was really "local", that is how far from the shaker we could sense the injected vibrations. We verified that indeed the shaking was quiet local: injected vibrations were sensed mostly in SPRB_LINK accelerometer and a bit also on the PR tower flange accelerometer (at PR flange facing IB) but not significantly farther away than this. This is a good thing, it means that the induced scattering phenomena indicated by projections is occurring in the link close surroudings.

Figure 1 shows the TF between the injected noise (Volts to the shaker) and all CEB accelerometers, colored lines correspond to >= 0.7 coherence. See only SPRB_LINK and PR accelerometers are coherent.

Figure 2 shows the same TF but during the less intense injection (Volts to shaker was one third). Indeed only the SPRB_LINK was excited.

Figures 3,4, and 5 show the measured TF between DARM (MICH and B4_DC resp.) signal and the SPRB_LINK accelerometer (converted in meters). We show and compare the TF measured with both louder and less louder injections, see that the TF is essentially the same.

One word about the structures in TF (Figure 1):  one clear structure is present at 55Hz, plus additional ones at high frequencies. We suspect this 55hz to be a mech. resonance of the link pipe (the response of the shaker should be flat in acceleration at these frequencies).

Figure 6 compares the quiet time signal of SPRB_LINK accelerometer and accelerometers on the BS-PR link, the PR flange, and the Guralp on CEB floor (all sensors are aligned along the beam, which here W-arm direction). We notice on SPRB_LINK a structure around 55Hz which is not present on ground and on PR tower, and is less intense on BS-PR link. It is interesting to check if this 55 Hz could actually be a radial resonance of the SPRB link pipe: to this end we will put a tri-axia accelerometer on the link.

A bit strange thing we notice:  the big peak present on floor (guralp) slightly above 100Hz seems not at all  present on the other accelerometers... to be further investigated.

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mwas - 8:53 Tuesday 23 May 2017 (37688) Print this report
During the work of putting SPRB under vacuum #37361 a strip of scattered light along the SPRB link was noticed (see last figure in that entry). Given that there is a clear coupling to MICH and then DARM, it would worth exploring if that clipping on the SPRB link is the culprit. I can see two experiment to try:

* do very local injections of vibration on the SPRB link. For example scratching lightly the link on the side with visible clipping, and on the other side of the tube while listening to MICH. And see if the coupling is clearer on the side with clipping.

* create some slow drift control of SPRB using the B4 quadrant DC signals (similar to what is done on SDB1), and then move the POP slightly left and right horizontally. If the drift control work it should allow the bench to rotate and compensate for the miscentering of the beam on the telescope. In one direction the coupling should get worse (more clipping) and in the other better (less clipping). I am not sure that the drift control is really necessary, as shifting the beam by a mm or two shouldn't be enough to remove the beam from the PDs. Or it could just be done by hand using spot position on the camera as a sensor, the bench local control set points as an actuator and a human as the control loop.
fiori, travasso, paoletti - 22:12 Thursday 25 May 2017 (37735) Print this report

In order to check the truthfulness of the large peak slightly above 100Hz in the CEB guralp horizontal spectra today we checked the frequency response of the guralp Warm-oriented component. We laid one meggit accelerometer horizontally fixed to a rigid support attached to the floor nearby the guralp (see Figure 1 for a picture of the setup) and measured the TF between the two (the meggit accelerometer was  temporarely attached to the ENV_BS_ACC_Z readout channel).

This is similar to what we did when we checked  the frequency response of the Guralp vertical channel and found it consistent with specs.

Figure 2 shows the measured TF, coherence and compares the two spectra (the guralp spectrum is converted into m/s2 using dataDisplay). The TF shows the presence of a double peak structure that is exactly in correspondence of the spectral peak. This might be a mechanical mode intrinsic to the sensor. Indeed this frequency is beyond the certified operational range of the sensor that is 50Hz (-3dB deviation from flat response). In conclusion the ~100Hz peak is NOT a real vibration of CEB floor.

Side observation: the guralp' cable looks a bit damaged (picture in Figure 3).

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