Reports 1-1 of 1 Clear search Modify search
VIS (IX)
kouseki.miyo - 7:41 Wednesday 28 April 2021 (16602) Print this report
Comment to Preparation for noise evaluation of ITMX geophones (16559)

Miyo
Summary

  1. We calibrated the Geophone for out-of-loop use, which we named H4.  The method is the same as the one we did yesterday, so please refer to yesterday's log.
  2. The noise levels of H1, 2, and 3 were estimated from the differential signal between each signals. According to the differential signal, ITMX Geophone have 10 times lager noise than LIGO although we know. Calibration of the Out-of-loop Geophone

1. H4 calibration
We did. please see the diaggui file in /users/Miyo/dropbox/LOG/210427/itmx_geohone.xml.

2. Noise level estimation for H1,2,3 Geophones

The noise level was estimated by measuring the differential signal between the each signal of Geophones placed in the same location as we reported in past klog entry. Since these Geophones are placed in the same location with the same orientation, the ground vibration motion is measured as an common signal with good coherence. This means that if we calculate the differential signal between the Geophones, only an uncorrelated signal left in the differential signal. This is the noise we are interested in. The measurements were performed as follows. First, in order to create the difference signal, we temporarily set the ACC2EUL matrix so that the In1 signals of the downstream ACCL, ACCT, and ACCY are H1-H2, H1-H3, and H2-H3, respectively. In this condition, the signals of H1, H2, and H3 and the difference signal were measured.

The results of the measurements and a plot of the LIGO Geophone noise[1] are shown in Fig. 1 for reference. First, comparing the three difference signals obtained from the three seismometers with each other, the overall noise level is almost the same, which is 1e-7 m/sec/rtHz at 0.1Hz. Looking at the details, the H1-H2 signal is smaller around 1 Hz than the other combinations, which probably means that the noise level of H3 is larger than the others. Furthermore, comparing these noise levels with LIGO, we can see that LIGO is one order of magnitude more sensitive at 0.1Hz. therefore, we need to investigate the cause of this, but on 04/26 we amplifired the geophone signal by 12dB with Whitening Filter and briefly checked if the signal was masked by ADC noise, but the coherence around 0.1Hz did not improve, so it is probably limited by the Geophone noise. Incidentally, the noise level found in the difference signal should be the remaining signal component due to the variation of the calibration coefficients (there is indeed a small amount of coherence between the differential signal and the individual signals), but this is only an upper limit of the noise level. In any case, we are able to measure the ground vibration with sufficient S/N above 0.1Hz, so we plan to use them to perform the Inertial Damp next.

[1] https://aip.scitation.org/doi/10.1063/1.5000592

Images attached to this comment
Search Help
×

Warning

×