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AdV-INJ (ITF Mode Matching Telescope)
derossi, spinicelli - 17:50 Tuesday 14 May 2024 (64256) Print this report
ITF mode matching measurement

- measurement of the mismatch with the hot ITF, opening the dampers, putting in down and giving a kick on the end mirrors z corr (starting from 14:09:25 UTC): we found 1,5% for the west and 3,8 % for the north (but with more uncertainty), see plots 1 and 2

- scan on the green, starting from 14:21:42 UTC: 1,7% for the west and 3,2% for the north (see plot 2). For the scan around the 02 mode we were on the edge of the ramp and for the next time we should change the offset of the ramp.

Images attached to this report
Optical characterization (Optical characterization)
nardecchia, bersanetti, derossi, gosselin, gouaty, melo, magazzu - 19:43 Tuesday 07 May 2024 (64205) Print this report
ITF WP characterization

The goal of the shift was to characterize the ITF working point with the following RH powers:

RH powers 

NE

WE

Current settings

6.9 W

[V=16.04 V]

8.4 W

[V=17.67 V]

The actions performed during the shift are listed below:

13.08 UTC: ITF relocked in LN3

14.18 UTC: ITF manually unlocked to perform input beam mode matching measurement with the free swinging technique and green laser scan (performed by Suzanne, Camilla and Matthieu).

                    See detailes in 64204

15.03 UTC: ITF relocked in CARM NULL 1F

16.08 UTC: OMC scan started (performed by Romain and Andrea)

16.30 UTC: OMC scan ended 

16.52 UTC: ITF relocked in LN2

After 1.5 hr in LN2, at 18.20 UTC, Andrea will proceed with the lock acquisition.

The main ITF signals during this afternoon are shown in figure 1.

Images attached to this report
AdV-INJ (ITF Mode Matching Telescope)
melo, derossi, gosselin - 18:24 Tuesday 07 May 2024 (64204) Print this report
Mismatch measurements

This afternoon we performed some measurements to verify the mismatch towards the arms. The last measurement done is reported in #63374.

First, we performed the free swinging method, giving a kick on the end mirrors (with the dampers opened). The GPS of the kick (we gave the kick simultaneously for the West and North arms) is 14:17:00 UTC.

However, when analysing the data we could not find reasonable values of mismatch. We need to verify if there is any problem with the Matlab code to debug, or there was something wrong with the measurements. In Fig. 1 we can see the time window of the free swinging mirrors. To be noted that the west arm starts swinging after roughly 15 seconds with respect to the North Arm. On Fig.2 we can see the surposed flashs of B7 and B8.

Then, we perform the measurements with the Green Scan. The GPS in this case 14:30:43 UTC (Fig 3). Figs 4 and 5 show the scans of the TEM 00 mode and TEM 02 mode respectively. In this case, for the north arm we found 3.3% and 1.4% for the west arm, as shown in Fig. 6.

Images attached to this report
Comments to this report:
melo, derossi, ruggi - 18:26 Wednesday 08 May 2024 (64213) Print this report

We did not manage to analyze the results of the free swinging mirrors with the kick measurement made yesterday (probably because they were not excited enough).

For this reason this afternoon we performed again this measurement, but we first opened the dampers, we manually put in down the ITF and then we applied the corrections (more than once, to keep the mirror excited).

The first kick was done at 15:51:36 UTC, and the data were analyzed 3 minutes later taking the peaks during 220s (so it cannot be defined "hot" itf measurement).

We obtained 2% mismatch for the north and 1,6% for the west (see plots)

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AdV-SBE (Minitowers)
bulten, was, bertolini, bersanetti, gouaty, arnaud - 10:47 Tuesday 30 April 2024 (64138) Print this report
DMS flags added to horizontal positions SBE benches
When the horizontal microsprings are adjusted, or maybe when other horizontal actions on the minitower benches are performed, the DMS system does not give a warning if the position is still far off the setpoint. This happened April 16, see logbook entry 64002 from Nicolas Arnaud. After discussions, we decided to add flags to the monitoring system; we had flags for the vertical position (-30that for the relative speeds for SNEB and SWEB with respect to the superattenuators, but this requires further study to see if there are cases that the relative speed between benches is high, but none of the flags (RMS actuator voltage, bench error signal) is already triggering.
Detector Characterisation (Spectral lines)
Tringali, Spinicelli, Fiori - 18:11 Thursday 18 April 2024 (64018) Print this report
Comment to Sideband structure around the 50 Hz mains line (64000)

As Piernicola confirmed, the sidebands at 46.7 Hz and 53.3 Hz are the beating between 50 Hz and DIFFp_TX line at 3.3 Hz (purple curve).
Indeed, when the DIFFp_TX line was set to 4.8 Hz, there were two sidebands at 45.2 Hz and 54.8 Hz, respectively (blue curve).

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AdV-COM (AdV commissioning (1st part) )
casanueva, derossi, gosselin - 21:15 Wednesday 17 April 2024 (64007) Print this report
Noise injections and DIFFp phase tuning

After the earthquake in Japan, we relocked at the first trial and after we arrived LN3_SQZ we started to tune the noise injections for the PSTAB loop (both at LF and HF). After the amplitude of the noise was tuned, we added the corresponding functions into the "injection_SSFS.py" script.

We then proceeded to repeat by hand the two last injections of the SSFS loop, that last shift made the ITF unlock. We decreased slightly their amplitude, while checking that the coherence with Hrec was still high. Now the script launches: CLEAN SSFS_UGF PSTAB_LF PSTAB_HF and then the 4 other SSFS injections at lower frequencies (down to 100 Hz). The operator launched the script and it worked without any problem. Figure 1 shows the injection corresponding to SSFS_UGF, and I think the current UGF is safe enough (I wouldn't push much higher, to ensure robustness, unless the noise injections suggest that it is limiting).

At this point we passed to the DIFFp topic. We started by opening the DIFFp_TX servo loop (which zeros the offset!), and then we started to put back the offset. However this didn't zeroed the new signals and so we continued to increase the offset. During this scan we tried to tune the phase, slightly, even if it was already quite good. Then we repeated the same operation with the TY loop. Figure 2 shows the two scans that we did. For the TY the phases were not clear so we left the deafult ones.

The phases we put are:DIFFp_TX_DCP_HF_mag_B1_phi0 = 0.5;       DIFFp_TX_DCP_mag_B1_phi0 =0.5

 

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AdV-SBE (EIB-SAS commissioning)
bulten - 11:56 Friday 12 April 2024 (63942) Print this report
Comment to EIB ground noise correction, and backscattered light towards SIB1 (63763)
This previous report was not reported at the date I wrote it, I found it in my drafts. Sorry for that.

I compared the EIB SAS movement in z (south) direction with the Sa_IB_F0_x (north) direction on April 2, 13:00 UTC with Jan 18, 13:30 UTC;
both days had high wind speed in PISA and extra microseismic activity. In the plots, EIB_ground_z is derived from the geophone on the
ground below the EIB bench. It is this geophone on which a different filter is applied, to match better Sa_IB_F0_x, which id the LVDT
signal from the injection bench superattenuator. So assuming that between 0.1 and 2 Hz the F0_x should be opposite to ground_z, you expect
a transfer function of 1. Before March 27, when the new calibration was applied, we had a large phase difference in the filtered geophone response
and the superattenuator around 0.3 Hz, where the maximum of the microseismic noise appears. After March 27 this phase difference is smaller, albeit
below 100 mHz I now have less reduction of the geophone DC drift (cutting off the part below 100 mHz gave too large phase shifts and too large
reduction in the range 100mHz- 1 Hz).

EIB_LVDT_z is the LVDT reading of the EIB; it should be minus SA_F0_x (since the EIB z-axis points towards the -x direction in IB). Thus optimally,
the transfer function EIB_LVDT_z/Sa_IB_x should be 1 with a phase of -pi. Same for EIB_ground_z/Sa_IB_F0_x. The EIB_LVDT_zb channel is the sum
of EIB_LVDT_z and EIB_ground_z; this is the channel that we try to control to 0 in the closing of the loop. Thus this channel gives an indication of the
residual motion.

As can be seen in plots of Jan 18 and April 2, the LVDTs for EIB_z and Sa_IB_x broadly overlap, but the EIB has extra motion that peaks around 0.8 Hz.
This is about a factor of 5 above the natural resonance of the IP legs of EIB and close to the Ty resonance; this extra motion is due to un-optimal
control in the PID loops, maybe also due to blending the geophones on the springbox with the LVDT. At 0.8 Hz, the EIB motion of the bench is
basically equal to the motion of the ground (EIB_LVDT_z ~ 2*Sa_IB_F0_x and EIB_LVDT_zb, EIB_ground_z ~ 1* SA_IB_F0_x).
You can also see that the ground noise before march 28 was underestimated by about 20% around 0.5 Hz and that the phase difference reaches 90 deg. around 0.2 Hz.
After modifying the filter for EIB_ground_z (which is in the control loop, so it also modifies the bench response in closed loop), on April 2, we see that the
ground motion compared much better with the IB motion; the amplitude of the transfer function is about 1.05 and the phase is much flatter; also the transfer function between EIB_LVDT_z and Sa_IB_F0_z improved. Now the maximal deviation around 0.8 Hz reached about 1.5; giving twice better subtraction of
ground noise. You can also see that EIB_LVDT_zbench is smaller; this is our best measurement of the residual motion of the EIB bench.

In the third figure, I plotted the results for the first 2 figures on top of each other (the reference plot is the April 2 data and the blue line the Jan 18 data)
to compare the change in transfer functions. You can see that the 30 minutes of data of Jan 18 contained a bit more seismic noise than on April 2.
Nevertheless, also the April-2 data contains so much excess microseismic noise that the quality of subtraction can be judged; at april 2 we do better than
at Jan 18. Further improvements could be made, if required, by changing the PID loops, but the EIB is a highly coupled system with tilt stabilization; z and Tx,
x and Tz, and indirectly Tx,Tz and Ty are strongly coupled. It is a priori not clear that we can improve much in the loops and it requires careful study of the
blending of the geophones on the spring box, the loop gains for the vertical and horizontal d.o.f.s etc.



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AdV-SBE (EIB-SAS commissioning)
bulten - 11:08 Friday 12 April 2024 (63763) Print this report
EIB ground noise correction, and backscattered light towards SIB1
During the afternoon shift we had time to commission EIB better. This is a follow-up on entry 63491, backscattered light noise hunting.
Originally, I wanted to track SIB1 just like SNEB, SWEB, SPRB and SDB2 are tracking the superattenuators, but unfortunately SIB1
operates at a setpoint in x of 991 micrometer, and I cannot blend that easily with the LVDTs of EIB.
EIB measures he ground displacement via geophones on the floor below the EIB bench. The phase between the geophone signal and the IB filter0 LVDTs
had a slope and the filtered ground signal for EIB was a bit too small. Therefore, I applied a filter that corrected the phase shift, and another high-pass filter,
to get a better match between the ground noise and the LVDT readings in SIB1.
Figure 1 gives the transfer function between ground-z and Sa_F0_X and also between ground_x and SA_F0_Z.
The reference plot is with the old filter, the blue line with the new filter, which is the old filter times (s(s+1))/(s^2+0.7s+0.08).
Clearly, the phase and the gain are much better. For ground_x, the gain of the subtraction has a slope and we under-subtract ground noise at 1 Hz, but
ground_z is the relevant correction, since that is the distance between EIB and the input mode cleaner (the south direction).
There is some further room for improvement but that requires a new time to try out the filter.

Furthermore, the geophones on the bench seemed completely mis-calibrated. I tried to get a better calibration by injecting Ty noise and changing the filters
a bit. The problem with the geophones on the bench is that at low frequency, the signal is coming from the tilt Tx,Tz of the bench, not from the acceleration.
Therefore it was difficult to do a good calibration. We should do the transfer function between the geophones on the bench and the ground with the bench
blocked, but that requires another 2 shifts (one to measure and implement it with blocked bench and another with floating bench and noise injection, to
see if everything is still OK in the presence of Tx and Tz tilts) so for the moment I think we should leave that.
I did a rough job getting a better calibration with the injected Ty but it is in no way perfect; the bench positions below 1Hz come from the LVDTs and the ground noise and they can be trusted. Above 1Hz, the spring box is used in the controls and the bench geophones are tilt-corrected and used as monitor signal in EIB_x,EIB_ty, EIB_z. Above 1 Hz, these signals are not accurate (but should be better than with the previous geophone filters) but they are not used in
the PID control, so I think that that is OK.







Images attached to this report
Comments to this report:
bulten - 11:56 Friday 12 April 2024 (63942) Print this report
This previous report was not reported at the date I wrote it, I found it in my drafts. Sorry for that.

I compared the EIB SAS movement in z (south) direction with the Sa_IB_F0_x (north) direction on April 2, 13:00 UTC with Jan 18, 13:30 UTC;
both days had high wind speed in PISA and extra microseismic activity. In the plots, EIB_ground_z is derived from the geophone on the
ground below the EIB bench. It is this geophone on which a different filter is applied, to match better Sa_IB_F0_x, which id the LVDT
signal from the injection bench superattenuator. So assuming that between 0.1 and 2 Hz the F0_x should be opposite to ground_z, you expect
a transfer function of 1. Before March 27, when the new calibration was applied, we had a large phase difference in the filtered geophone response
and the superattenuator around 0.3 Hz, where the maximum of the microseismic noise appears. After March 27 this phase difference is smaller, albeit
below 100 mHz I now have less reduction of the geophone DC drift (cutting off the part below 100 mHz gave too large phase shifts and too large
reduction in the range 100mHz- 1 Hz).

EIB_LVDT_z is the LVDT reading of the EIB; it should be minus SA_F0_x (since the EIB z-axis points towards the -x direction in IB). Thus optimally,
the transfer function EIB_LVDT_z/Sa_IB_x should be 1 with a phase of -pi. Same for EIB_ground_z/Sa_IB_F0_x. The EIB_LVDT_zb channel is the sum
of EIB_LVDT_z and EIB_ground_z; this is the channel that we try to control to 0 in the closing of the loop. Thus this channel gives an indication of the
residual motion.

As can be seen in plots of Jan 18 and April 2, the LVDTs for EIB_z and Sa_IB_x broadly overlap, but the EIB has extra motion that peaks around 0.8 Hz.
This is about a factor of 5 above the natural resonance of the IP legs of EIB and close to the Ty resonance; this extra motion is due to un-optimal
control in the PID loops, maybe also due to blending the geophones on the springbox with the LVDT. At 0.8 Hz, the EIB motion of the bench is
basically equal to the motion of the ground (EIB_LVDT_z ~ 2*Sa_IB_F0_x and EIB_LVDT_zb, EIB_ground_z ~ 1* SA_IB_F0_x).
You can also see that the ground noise before march 28 was underestimated by about 20% around 0.5 Hz and that the phase difference reaches 90 deg. around 0.2 Hz.
After modifying the filter for EIB_ground_z (which is in the control loop, so it also modifies the bench response in closed loop), on April 2, we see that the
ground motion compared much better with the IB motion; the amplitude of the transfer function is about 1.05 and the phase is much flatter; also the transfer function between EIB_LVDT_z and Sa_IB_F0_z improved. Now the maximal deviation around 0.8 Hz reached about 1.5; giving twice better subtraction of
ground noise. You can also see that EIB_LVDT_zbench is smaller; this is our best measurement of the residual motion of the EIB bench.

In the third figure, I plotted the results for the first 2 figures on top of each other (the reference plot is the April 2 data and the blue line the Jan 18 data)
to compare the change in transfer functions. You can see that the 30 minutes of data of Jan 18 contained a bit more seismic noise than on April 2.
Nevertheless, also the April-2 data contains so much excess microseismic noise that the quality of subtraction can be judged; at april 2 we do better than
at Jan 18. Further improvements could be made, if required, by changing the PID loops, but the EIB is a highly coupled system with tilt stabilization; z and Tx,
x and Tz, and indirectly Tx,Tz and Ty are strongly coupled. It is a priori not clear that we can improve much in the loops and it requires careful study of the
blending of the geophones on the spring box, the loop gains for the vertical and horizontal d.o.f.s etc.



Images attached to this comment
AdV-ISC (Commissioning up to first full interferometer lock)
boldrini, masserot, spinicelli, pinto - 16:33 Wednesday 10 April 2024 (63918) Print this report
DIFFp_TX_SET servo adjustment

After the intervention of last Monday, the DIFFp_TX_SET servo was trying to build a signal with a line that did not exist anymore.

We changed the frequency of the demodulation to 3.3 Hz in ASC_pre and the frequency of the high-pass cut-off in DIFFp_alignment to 3.3 Hz as well. We also tuned the demodulation phase of DIFFp_TX_B1p to -1.8.

After that the offset manually added during debugging (63916) was removed and the servo changed it back to a value that minimizes B1p, as it is supposed to.

We reloaded the filters in ASC_pre to make this solution permanent. The new value of the demodulation phase is saved in ASC_pre but the config file has not been reloaded to avoid the risk of an unlock. Since Metatron does not change it, the value we set online should remain until there is a chance of reloading ASC_pre safely.

It should work as intended now (the servo brings the setpoint to a value that corresponds to the minimum of the "ball" that appear on the istogram with SDB2_B1p_DC and ASC_DIFFp_TX_INPUT, Figs.1,2), but we will keep monitoring it over the next few days.

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AdV-ISC (Automatic Alignment)
boldrini, pinto, spinicelli - 12:29 Wednesday 10 April 2024 (63916) Print this report
Comment to Is DIFFp TX set point loop active? (63908)

The DIFFp_TX_SET servo is indeed not working.

For the moment, we disengaged the servo and set a better sepoint by hand, since the servo was slowly but constantly drifting away from the minimum of the fringe.

The state of the ITF was changed to ADJUSTING for this intervention and it's now back to SCIENCE.

AdV-ISC (Commissioning up to first full interferometer lock)
boldrini, spinicelli, pinto, mwas - 18:23 Monday 08 April 2024 (63885) Print this report
DIFFp_TX line adjustment

During the recovery of last Saturday, one of the unlocks was caused by DIFFp_TX's gain becoming too low overtime. The coherence of the UGF monitor line was too low and the servo was not functional. As a patch, the ISC crew increased considerably the lines' amplitude.

As a result, the lines became dominating on B1_PD1/2_Audio rms (63876) and caused them to occasionally saturate introducing loud glitches in the sensitivity. The issue concerns DIFFp_TX line.

Today we tried to find an amplitude that allowed the UGF servo to work while avoiding the saturation on B1 audio channels, but we observed that there was no possible amplitude that satified both conditions.

Instead, we elected to move the line at lower frequency (4.8 -> 3.3 Hz) and recalibrate the target UGF (2.7 -> 3.6). The result is positive: audio channels remain within \pm0.025 mW instead of \pm0.04 mW and the line coherence is good (Fig.1).

Moving the UGF servo line allowed Michal to lower SDB1's dithering line as well, since it is no longer "competing" with DIFFp's line.

During our tests, we noticed that the noise floor on the audio channels spike when the filters of MICH and SRCL are swapped between LN2 and LN3. We tested a lock acquisition without this filter swap (we changed the UGF servos' target as well to remain consistent with the control filters), and then introduced the new filters manually one at a time. The noise level on B1 audio channels did not increase as a result, what we observed must have been due to something else.

After this test, we leave the ITF in the final state.

Images attached to this report
AdV-COM (AdV commissioning (1st part) )
casanueva, bersanetti, boldrini, ruggi, spinicelli - 23:32 Saturday 06 April 2024 (63870) Print this report
Turn on DIFFp UGF servos in LN3

After solving the issue of the marionetta of the NI, the ITF started unlocking at acquire LN3. We noticed very fast unlocks, due to the fast shutter closing very soon. No clear loop seemed guilty, but we noticed that the DIFFp TX UGF servo was not working because its line didn't have coherence. However the DIFFp TY gain was increasing quite strongly during the transition. So we increased the gain of the loop to keep the UGF stable, and it seemed to work. We also noticed that the UGF servos were off once in science, even if the lines were ON, so we commented the commands that turn them off.

We left the ITFlocked  in LN3.

AdV-COM (AdV commissioning (1st part) )
ruggi, casanueva, bersanetti, boldrini, spinicelli - 17:36 Saturday 06 April 2024 (63869) Print this report
1.8 Hz oscillation due to NI marionette reallocation

The locking troubles were due to an instability at 1.8 Hz of NI marionette reallocation. The problem appears when the correction on the mirror is moved from NI to NE, and at the same time the splitting filters with higher crossover are engaged. Such a problem has never been observed before, but in principle an instability in that region cannot be excluded. There are resonances of the two suspensions which can have slightly different frequency and can create unstable crossing points. Why this problem should appear now, after years of correct work, I don't know. Some measurement is required in order to see if the problem can be explained by a loop model, and a more robust strategy can be found. For the moment, the gain on the filter on MA branch has been changed from the nominal one (0.416) to 0.38. The instability is no more there, but clearly is not very far. Changing more the gain could create different problems, so let's leave the things like that untill a good model will be available.

AdV-INJ (General opto-mechanical layout, common parts construction, Installation and pre-commissioning)
gosselin - 16:09 Thursday 04 April 2024 (63840) Print this report
Comment to INJ noise hunting shift - RFC alignment and SBE EIB noise injections in LN3 (63830)

To be noted that we managed to improve the alignment only using the PZT mounted on M19.
The PZT mounted on M20 had a strange behavior (red circle on figure attached). We were doing steps of 5V that were slightly changing the transmission and but then this transmission was going back to its original value by its own. Nothing was visible on the QPD.

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Environmental Monitoring (Environmental Monitoring)
derossi, spinicelli, tringali - 13:10 Thursday 04 April 2024 (63838) Print this report
Comment to Shaker installation on laser bench (63577)

On the March 12th, a shaker has been installed on the Laser Bench to perform sismic noise injection. After those studies done on the 14th, the electronics that controls the shaker (deployed on the ground) has been left ON (with 0V of input voltage) to have the possibility to further perform other remote injections. 
However, entering in the laser lab few days later, we noticed a slightly higher acoustic noise than usual. We decided then to switch OFF that electronics, and indeed the noise reduced.

Looking at the environmental sensors present in laser lab, we found this noise visible as both high frequency broad noise (>200Hz)  and with some lines a low frequency (~45Hz and harmonics).
Moreover, we see it on acoustic (see fig. 1-3, 5) and sismic (fig. 4) sensors. While the noise is visible on both benches, the effect (seismic and acoustic) on EIB is really faint (see fig 4-5).

Nevertheless, we didn't find any noticeble effect on Hrec.  

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AdV-INJ (General opto-mechanical layout, common parts construction, Installation and pre-commissioning)
gosselin, derossi - 11:05 Thursday 04 April 2024 (63837) Print this report
Comment to INJ noise hunting shift - RFC alignment and SBE EIB noise injections in LN3 (63830)

We checked some signals of interest after the realignment of the RFC and could not see any clear improvment neither in LN3 (figure1) nor in INJ stand alone (figure 2).

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AdV-INJ (General opto-mechanical layout, common parts construction, Installation and pre-commissioning)
derossi, melo, gosselin - 21:21 Wednesday 03 April 2024 (63830) Print this report
INJ noise hunting shift - RFC alignment and SBE EIB noise injections in LN3

RFC alignment in LN3

We moved the setpoints of the piezo from around 17h45 UTC to 18h10. We improved the alignment as shown in fig.1

(We also updated the thresholds in the DMS).

 

SBE EIB noise injections in LN3 (sine @ 0.5Hz)

DOF gps start UTC duration amplitude pp
tx 18:22:45 3 min 10 urad
ty 18:26:50 3 min 10 urad
tz 18:31:10 3 min 10 urad
x 18:34:40 3 min 10 um
y 18:38:08 3 min 10 um
z 18:41:39 3 min 10 um

Analysis of the noise injections will follow.

 

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Comments to this report:
gosselin, derossi - 11:05 Thursday 04 April 2024 (63837) Print this report

We checked some signals of interest after the realignment of the RFC and could not see any clear improvment neither in LN3 (figure1) nor in INJ stand alone (figure 2).

Images attached to this comment
gosselin - 16:09 Thursday 04 April 2024 (63840) Print this report

To be noted that we managed to improve the alignment only using the PZT mounted on M19.
The PZT mounted on M20 had a strange behavior (red circle on figure attached). We were doing steps of 5V that were slightly changing the transmission and but then this transmission was going back to its original value by its own. Nothing was visible on the QPD.

Images attached to this comment
AdV-ISC (Commissioning up to first full interferometer lock)
casanueva, boldrini, bersanetti, spinicelli, masserot - 18:08 Tuesday 02 April 2024 (63817) Print this report
Evening unlocks

After the maintenance, we have had mainly two types of unlocks: some at CARM_MC_IR, which we didn't pay much attention since the seismic and wind activity are high. However, every time that we rach CARM NULL 1f we would unlock. We could see many "oscillations" on all the longitudinal loops, the PR angular loops and then saturation of B2 photodiode.

It took some time to understand the reason for these unlocks, but since they were all of them at the same moment Diego remembered that it was the moment when we enagge the CARM slow loop. Indeed it looked like it was oscillating at veyr low frequency, so we increased its gain and it worked (1/1 times, we need to see if this works in the long time). Figure 1 shows the clearest example.

WHile debugging I profited to tune the demodulation phase of MICH and SRCL on DRMI 3F, which was off by 0.2 only, then I checked it at STEP 3, and CARM NULL 3f and it looked well tuned. I also fine tuned the DARM phase in STEP3, which ws off by 0.3.

This doesn't explain the unlocks of yesteday on STEP 2 and STEP 3. We keep on investigating.

Images attached to this report
AdV-INJ (Beam Pointing Control)
spinicelli - 16:54 Tuesday 02 April 2024 (63815) Print this report
Recentering of the input beam

After the weekly check of the input beam position, the operator noticed that the we had an important vertical shift of the input beam.

Thus, I moved the PR X and Y by 60um in order to both recover the centered position and lower the BPC correction (see fig. 1).

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AdV-ISC (Commissioning up to first full interferometer lock)
mantovani, spinicelli - 16:32 Friday 29 March 2024 (63788) Print this report
Start of long etalon 2D scan

This afternoon, at 15.24UTC we started the 2D etalon scan which will take 1 week long.

As previously indicated, we had to initially tune the phase for the WI scan.

The final values used are the following:

amplitude 0.4

duration 604800 s

sin phase -pi/4

AdV-DAQ (Data Acquisition and Global Control)
gosselin, masserot - 20:26 Wednesday 27 March 2024 (63767) Print this report
Comment to ITF and FDS Acl servers update with v1r23p17 (63757)

All the INJ_rtpc (rtpc19) Acl servers have been started with the Acl v1r23p17 between 2024-03-27-17h24m10-UTC and 2024-03-27-17h25m06-UTC

Injection system (General activities)
gosselin, derossi - 18:57 Wednesday 27 March 2024 (63765) Print this report
INJ recovery and removed of the set up to inject laser phase noise

Today we blocked the beam on the LB to allow HJ. Bulten to work on the control of EIB (details in another entry)
We took advantage of having INJ in down to remove the set up that we added few weeks ago with Walid to be able to inject laser phase noise. We were indeed suspecting that it could be the responsible for the loss of phase margin of the IMC loop that has been seen these last days.
When HJ finished, we try to relock the injection but it was not relocking. After multiple tests we eventually noticed that the BPC was locked on the reference values which were quite far from the ones it had before putting INJ in down.
The alignment of the whole system had indeed drifted away during the long lock of the night+day.to follow the ITF.

After having relocked we blocked the beam again to allow Alain to do the restart of rtpc19.

Then everyting relocked correctly.

We measured the OLTF of the IMC with the attenuation of 20 dB (10+10) we had an UGF of 100 kHz and 14 degrees of phase margin
We added few dB of attenuation 22 (20+2) and we had an UGF of 93 kHz with 16.5 degrees of phase margin (see figure).
It is better than what we had few days ago but still not at the level of what we add when we measured it on the 04/03.

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AdV-DAQ (Data Acquisition and Global Control)
bersanetti, boldrini, casanueva, masserot, spinicelli, vardaro - 11:39 Wednesday 27 March 2024 (63757) Print this report
ITF and FDS Acl servers update with v1r23p17

All the Acl servers  (AclISC, AclLC, AclSBE, AclFCoplev, Acl) are running with the v1r23p17 version  since the 2024-03-26-15h20mn-UTC .

The main new features are

  • for the Cm commands use to set the ACL object parameters, the numeric parameters can be sent  as integer or double .
  • the ACL_SINECOMB_CH keyword to define a comb of lines
  • the possibly to to delay the readout of the AclAdcCh objets.

The first trial was done the 2024-03-25  starting at 14H-LT

  • all the Acl servers were restarting the Acl v1r22p17 : operation complete around 17h-LT
  • upgrade of the INJ Acl server configurations
  • Some tuning were done on the NEB and WEB Als servers to avoid missing ADCs sample by adjusting the timing sequence:  the LOOP_DELAY was increased to 6us for NEB and 7us for WEB
  • after the recovery of Injection system  and the ITF alignment,  we faced some troubles with the lock sequence 
    • some Cm messages sent  by the Automation servers with the "load" or "apply'  commands  related to ACL_MATRIX_CH or ACL_SUM_CH objects were all rejected by the Acl servers
    • To relock the ITF, the LSC_Acl, ASC_Acl, NEB_ALS_BPC, WEB_ALS_BPC and the SDB1_LC servers were restarted with the Acl v1r20p17 version .  The ITF was relocked at LN3 . Unfortunatly , the SDB1_OMC server was not updated  and the OMC lock sequence was not correctly achieved
  • To fix the issue the Acl v1r23p17 was created and deployed on all the Acl servers

 

Comments to this report:
gosselin, masserot - 20:26 Wednesday 27 March 2024 (63767) Print this report

All the INJ_rtpc (rtpc19) Acl servers have been started with the Acl v1r23p17 between 2024-03-27-17h24m10-UTC and 2024-03-27-17h25m06-UTC

Detector Characterisation (Broadband noise)
spinicelli - 15:58 Tuesday 26 March 2024 (63744) Print this report
Comment to noise in tonight lock (63741)

PSTAB0 line (43Hz) has been switched off (amp=0) at 12.52.40UTC.

We could then relock in LN3: the bump at 43 disappeared while the broadband noise was still there.

To be noted that PSTAB1 line (236Hz) is still injected while, as far as I know, not used by any loop.

AdV-ISC (Commissioning up to first full interferometer lock)
derossi, spinicelli - 14:48 Tuesday 26 March 2024 (63742) Print this report
Comment to ISC shift: recovery after INJ reset (63734)

In order to understand why the IMC OLTF has changed since the 4th of march (UGF at 107kHz with a phase margin of 16deg, #63487), this morning we tuned the angular and longitudinal working points of the IMC loop (plot 1).

We remeasured the OLTF but it was the same as yesterday (84kHz UGF and 10deg phase margin, plot 2).

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