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Interferometer_sensitivity_studies (General)
swinkels, marque - 19:05 Thursday 12 August 2010 (27328) Print this report
Noise-bumps with etalon-like modulation
During the last few weeks, we usually see a modulation of some noise bumps around 50 and 100 Hz during the beginning of a lock (see e.g. fig 1 of air-co switch-off test), which is also visible in the horizon, see fig 1. The temporal behavior of these bumps resembles a sine of an exponential, as we have seen for the etalon of the input mirrors after TCS experiments.

Doing a similar fit to the BRMS around 50 Hz yields a time constant of around 1 hour, see fig 2. Assuming that this is some thermal effect driven by the beam-power, we can set t=0 at the moment the dark-fringe is reached and obtain an amplitude of around 7 fringes. If this would be caused by some sort of etalon, it would correspond to a change of optical path length of 3.5 micron.

We suspected that the noise is is caused by some object on the detection bench, whose amount of scattered light might be modulated by a spurious etalon. For an etalon of a piece of glass, the change in optical path-length is given by DeltaOPD = L * dn/dT * DeltaT = n_fringes * lambda / 2. Using a typical dn/dT of 1e-5, we are thus searching for an object for which L * DeltaT ~= 0.4 during a typical lock. This would require 4 degrees for an object of 10 cm (this excludes the main mirrors, which also have a much longer time constants) or 40 degrees for an object of 1 cm (excluding e.g. the prisms of the OMC). The only objects that might be heated enough are some components in the injection system, but it is hard to explain how they introduce the noise. An alternative explanation might be the interference between two pieces of optics separated by some long piece of aluminum, like the suspended bench itself that might be heated by scattered light. Other ideas welcome ...
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swinkels - 14:20 Wednesday 18 August 2010 (27402) Print this report
We are now reasonbly sure that these fringes are caused by diffused light in the detection tower: The bumps disappear when we align the detection bench and the frequencies of the bumps are predicted very accurately by Irene's noise projection based on the accelerometer attached to the flange of the detection tower.

Apart from reducing the light on the dark fringe and aligning the bench as good as possible (which does not kill the bumps totally), the problem might be solved by reducing the amount of seismic noise. The 100 Hz line might be hard to remove (unless it is a power-supply attached directly to the tower, to be checked). We should spend some time to find the source of the 130 Hz line and try to cure it.
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fiori - 16:20 Thursday 19 August 2010 (27422) Print this report
A test done during VSR2 (switch off test of DE and SR turbo pump fans) let me suspect that the cooling fans contribute to shaking the DETection tower at 100Hz.
It is possible that we can reduce this vibration by detaching the fans from the pump body, similarly to what done for other pumps, but NOT yet done for the detection pump. This isolation operation should be not difficult, to check if it can be managed during next Tuesday mantenance break.
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