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AdV-INJ (Input Power Control (IPC) system)
pillant, mantovani, casanueva - 15:40 Tuesday 21 November 2017 (40110) Print this report
Additional optical density on IMC_TRA

Due to the increase of the power sent to the ITF, the photodiode used for FmodErr, IMC_TRA and ITF_INPUT was saturated (up to 9V).

In order to back to a linear range, I added a measured optical density OD = 0.23 @ 1064nm in front of the photodiode and modified the calibration factor in the ADC.

Now the optical power on this photodiode is equivalent to the working point INJ_IMC_TRA = 16W.

The input power on the ITF is 26.5W instead of 24.5W previously announced.

Comments to this report:
mantovani, casanueva - 8:35 Wednesday 22 November 2017 (40116) Print this report

The saturation was leading a worsening on the signal visible in the calibration.

The figure 1 shows the calibration before the attenuator installation which gives a slope of 4.24e-8 V/um while figure 2 shows the calibration after the attenuator installation which gives a calibration of 8.85e-8 V/um

the improvement in the signal is ~ 4 considering the fact that with the attenuator the power inpinging on the diode corresponds to a pick off of 16W instead of 29.9W.

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casanueva, mantovani - 14:32 Thursday 23 November 2017 (40132) Print this report

The trigger of this search was the pathological behaviour of the fmoderr loop. During the night of the 20 to the 21 we have observed that the offset after the initial fmoderr tuning was increasing, increasing significantly as well, the offset of the error signal that is used for this purpose in Dark Fringe. Knowing that this final loop has a very low control bandwidth, arriving in DF with a big offset means that we can not recover nominal conditions.

Figure 1 shows the initial offset after the Fmoderr tuning was done at the beginning of each lock trial during the night of 20 to 21 (max and min values). It can be seen that there is a trend behaviour towards higher values during the night. There are also four points that show the four succesfull locks, and the initial offset of the fmoderr signal used in Dark Fringe. It can be seen that by the end of the night these offsets become too big to be recovered.

Apart from the fixing of the saturation problem, we have adjusted the tolerance values of the initial fmoderr (reducing them of a factor 10), to try to reduce the offset in Dark Fringe to more reasonable values.

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