After the recent Free Space implementation, today we tested new control filters for CARM and DARM while locked on the beating signals. The idea was to make more robust the lock on the green by increasing the bandwidth of the loops.
In fig.1 is reported the comparison of the OLTF of DARM (for reference) with the older controllers (blue), the extracted model (red) and the new open loop TF with the new controller. We were able to increase the accuracy pushing up the badwidth to ~25 Hz (G.M. of a factor 2), by adjusting the roll-off in order to not renintroduce too much correction noise. To be noted that there's still margin to increase the bandwidth without occurring towards corr saturations, in case it is needed (see fig.3).

In fig.2 is reported the plant measurements. Both in DARM and CARM a notch strutcture at around 70 Hz was present. After some digging in Acl we found that in CEB_ALS process, filters for CARM and DARM (double structure at 68 and 72 Hz) are implemented in order to compensate some INJ structure (?). During the controller design we compensated this structure with a resonant gain at the same frequencies and Qs, so to gain more phase at that region.

In fig.3 are reported the first comparison of DARM and CARM signals and corrections spectra before and after the implementation of the new control filters. In order to reduce the bump visible at ~50 Hz and to reach the declared factor 2 of gain margin, in the second round we reduced the loop gains of a factor 1.3.

N.B.

modification performed (automation side) are the following:

• DARM/CARM control filter: ALS_Arm_control4 -> ALS_Arm_control5;
• carm_gain_boost_final: 0.006 -> 0.0138;
• darm_gain_boost_final: 0.018 -> 0.0138;
• darm_line_ampl: 0.07 -> 0.03;

I noticed that the pixel size of the camera SDB2_B1s2_Cam set in the configuration of DET_Img_CEB is wrong. It is currently defined as 5.2 um (the pixel size of the Smartek CMOS  GC1281XM-S90-NoCG). However this camera is not a CMOS one. Instead this camera is a Smarteck CCD GC1392M-A90-NoCG, for which the pixel size is 6.45 um.

The consequence of this mistake is that the beam size extracted from the camera images is underestimated by a factor 5.2/6.45 = 0.806 (almost 20%).

This mistake is probably present since 09/07/2019 when the B1s2 camera was replaced ( https://logbook.virgo-gw.eu/virgo/?r=46309 ).

We will fix this mistake next week when we will have the opportunity to restart the process DET_Img_CEB.

This morning around 10 UTC I put two dumpers in front of the output windows of the EQB1 bench. This will prevent any beam to reach SQB1.

There was the following DBoxes with the timing_error not at zero , this appeared around 08h50m-UTC for most of them:

• EDB_DBOX_OMC (SN075) and EDB_DBOX_SQZ(SN120) managed by the EDB_QD_dbox_rack server
  • Related to EDB_DBOX_SQZ(SN120), the demodulation board SN38 (mezzanine3) appeared as not available for the DaqBox server, but was weel reachable from the DBox ARM CPU
    • from the DBox ARM CPU; the command /home/daqbox/virgo/App/DaqBox/v8r3/scripts/daqbox_main_fpga_reset.sh  was executed and after the the faultymezzanine was recovered
  • The reconfiguration of these DBoxes allowed to recover the synchronization with the Timing system
• SQB1_DBOX_Up (SN103) and SQB1_DBOX_Up(SN104)  managed by the SQB1_dbox_bench server
  • the LC and SBE SQB1 controls were openned 
  • The reconfiguration of these DBoxes alloweed to recover the synchronization with the Timing system
  • the LC and SBE SQB1 controls were successfully closed after these operations
• EQB1_DBOX_03 (SN091) managed by the SQB1_dbox_rack server and the SQZ_DBOX_O2 managed by the  SQZ_DBOX_DET_EERoom server
  • The reconfiguration of these DBoxes allowed to recover the synchronization with the Timing system

After these operations, all the faulty DBOxes are synchronized  as well the FAST_DAC mezzanines . The attached plot show the trend of the issues 

Today, we verified the OLTF of the RFC, which was 200 Hz and 0.5 rad of phase margin (See Fig. 1). However, this loop should have a unit gain at 180 Hz ideally. So we changed the RFC gain on the DSP card from -0.25 to -0.22. The new OLTF is shown in Fig. 2:  the unit gain is now at 178 Hz and the phase margin is now at 0.62 rad. The gain margin is now 0.5 and it was 0.6 before.

Ps. to be noted that if the DPS card is reloaded the RFC gain will be reverted to -0.25 again.

Today I measured the OLTF of the IMC. Currently, we have 110 kHz of bandwidth and 20 degrees of phase margin.

ITF founf in LOCKED_ARMS_IR in COMMISSIONING mode.

planned activities

- Improve CARM/DARM handoff to IR (TBC)
- Implement new filters for ALS (TBC)
- Block SQZ beams towards SQB1 (Sorrentino, TBC)

During the shift P. Ruggi noticed a strange behavior of NI Etalon (plot1). After a check, Dattilo and Cavalieri decided to replace (at 08:45 UTC) the old KERT with a new one.
ITF unlocked due to an earthquake in Colombia (fig attached).  SIB2, SNEB, SWEB, SDB2, SPRB SBE loops opened. Loops closed. Relocking in progress...

TCS
14:00 UTC - Post heating loop switched ON, on AUX cooling system (Dattilo, Cavalieri).

This afternoon also the TCS WI AUX laser has been turned on again, and left as the other ones ON for monitoring and thermalization.

The CO2 laser status is as follows:

• NI bench:  
  • AUX LASER:  ON
  • MAIN LASER  ON
• WI bench:
  • AUX LASER:  ON
  • MAIN LASER: ON

All laser beams are blocked inside the benches.
Do not open the acoustic enclosures.
If access is required, please contact Marco and Ilaria.

Another quick look to the acoustic noise peak around 490Hz:

this one is not associated to the INJ HVAC, but switching it off (tests of July 28) caused the frequency of the peak to drift up: see Figure 1

the LB and EIB benches detect a correlated vibration, which is louder in the EIB (vertical accelerometer) than in the LB (horizontal acc.): Figure 2

Browsing back the VIM, the peak seems present since long time, but recently it has changed frequency and became more intense:

• it was around 550Hz and fainter up to Feb 28: Figure 3
• after the March black-out it moved to 400Hz and became more intense: Figure 4
• on May 4 it drifted up to 500 Hz: Figure 5

   Hints may suggest for something located inside the INJ lab, probably on EIB, which is getting more noisy... maybe because of ageing?

ITF found in LOCKED_ARMS_IR in COMMISSIONING mode.

planned activities communicated to the ctrl room and performed:
- Camera installation on MC building (Fabozzi, external company) concluded at 10:20 UTC.
- OMC lock in NI single bounce (Gouaty, Romero) concluded at 10:00 UTC.
- DRMI recovery (w/o TCS) concluded.
- TCS - CO2 WI laser recovery (Nardecchia, Cavalieri, Gherardini) concluded at 10:00 UTC. TCS in standard state!
- CARM/DARM noise injections while on ALS (Bersanetti, Pinto) concluded at 13:30 UTC.

The activity on  OMC lock in NI single bounce started at 07:12 UTC. Gouaty asked me to set ITF in SINGLE_BOUNCE_NI and misalign PR about 20 urad ty-. PR realigned upon concluded the activity.

ITF left in LOCKED_ARMS_IR.

We profited of some machine time to make noise injections on CARM and DARM, to be used to develop new control filters after the free space implementation.

Timestamps:

• 12:33:00 UTC: clean, 180 s;
• 12:40:00 UTC: DARM noise injection, DARM_noise shape, amplitude 1e5, 180 s;
• 12:58:00 UTC: CARM noise injection, DARM_noise shape, amplitude 1e5, 180 s;

This morning, Fabio and Roberto performed additional checks on the electronics of the WI main CO2 laser. They found that the laser sync was intermittent: touching the sync board caused the signal to fluctuate. The board was therefore replaced with the spare one.

After the replacement, the WI main CO2 laser was switched on again at 09:49 UTC. The restart was successful: the laser reached its nominal output power and has remained stable since then (at least up to the time of writing), as shown in Fig. 1.

In the afternoon, Nicola reopened the cooling valve of the WI auxiliary laser, which was then switched on at 12:15 UTC.

The TCS is now back in its standard operating configuration: all CO2 lasers are on with all beams blocked on their respective benches.

Finally, together with Nicola and Diego, we updated the DMS. If any flip mirror on either CO2 bench is opened, allowing a laser beam to propagate toward the interferometer, the corresponding DMS status flag automatically turns red. 

The CO2 laser status is as follows:

• NI bench:  
  • AUX LASER:  ON
  • MAIN LASER  ON
• WI bench:
  • AUX LASER:  OFF
  • MAIN LASER: ON

All laser beams are blocked inside the benches.
Do not open the acoustic enclosures.
If access is required, please contact Marco and me.

This morning we performed some preparatory actions before the intervention on SDB1/SDB2 scheduled in 2 weeks. One of the goal was to test the DET python scripts (used for OMC lock and picomotor actuation on SDB1) to make sure they were still operational. We also took this opportunity to take an alignment reference in NI single bounce with the OMC locked, we adjusted the demodulation phase of the B1_PD3 photodiode, and we optimized the OMC alignment with 0 offsets on B5_QD2. 

07h15 utc : Thanks to Nicola, the NI single bounce is set. SDB1 bench is in drift control.

At 07h07m10 utc, we open the OMC shutter.

Noticing that the correction in TX applied to the marionetta was around -5V, we acted on the motorized weight of SDB1 (BENCH_TX) by -25000 steps, to lower the correction up to 0.4 V.

At 7h48m25 utc we remove the offsets of the B5_QD2 quadrants (the ones used for ITF lock). This gives us an alignment reference for the single bounce (with B5 QD2 offsets at 0), while B1p is well centered on the camera (within +/-50 um from the center).

We observe that the initial OMC temperature was 22.55 deg.

Between 7h50 and 8h40 we tried several time to lock the OMC but we faced the following problems:

• Initially the B1_PD3 shutter was closed (although the state of the shutter indicated in VPM was open).
• While we were switching off/on the Vbias and closing/opening the shutter of B1_PD3, this triggered the closing of the OMC shutter.
• Then around 8h24 utc we made another attempt of OMC by the lock was not triggered when passing around the resonance. We realized that DET_MAIN probably reseted LSC_DARM to 0 when the OMC shutter automatically closed. So we reset LSC_DARM to 1.
• We also observed that the demodulation phase of B1_PD3 was mistuned. We adjusted it by -1.55 urad at 7h59m09 utc. The new demodulation phase entered in the configuration is 1.85 rad. We also changed the B1 demodulation phase by -1.6 (new value in the configuration file is -0.6 rad) although we did not test the B1 phase.

OMC was locked at 08h42m50 utc (See attached figure). Power on B1_PD3 is initially equal to 12 uW.

We adjusted the OMC alignment by acting on the picomotors, and reached a power on B1_PD3 equal to ~15.7 uW.

At 9h11 utc we start an OMC scan to check the quality of the alignment.

Order 1 = 0.4 uW > This gives an alignment defect of 2.5%

Order 2 = 0.3 uW > This gives a mode mismatch of ~2%

We restored the dark fringe offset for B5_QD2, closed the OMC shutter and concluded our activity.

After commissioning the west-arm instrumented baffle, we locked the cavities, kept the input mirrors centred, and performed a very slow-moving snail scan simultaneously with both end mirrors for more than half an hour, starting at approximately 12:45 CEST, Aug 6th.

The objective was to collect data from all the baffle sensors for the relevant studies of the baffle’s performance. The snail scan was perfect for this purpose, as it allowed the laser beam to pass successfully over all the sensors.

In order to evaluate the eventual improvement of the angular control due to the intervention on sensing and driving, one can compare data regarding the lock of the arms before and after the activity. The first data collected in the evening were clearly affected by a new kind of instability, characterized by short spikes. Apparently the reason was a drift of PR from the correct parking position, pruducing resonaces of the arms with a sporious reflected beam. A few hours later an additional misalignment has been applied to PR and the effect has been removed, as shown by the trend of B7_DC_max and B8_DC_max.

The new system is now working steadily, at around 1.8 (NI) - 2 (WI) liters per minute.

Before shutting the old system off, issues and anomalies with the flows (both NI and WI) were observed.

This phenomenon can be a consequence of the following issues:
Clogging in the piping
Clogging in the fittings
Clogging in the utilities
Old or damaged flowmeters
Presence of air
Insufficient circulators
Losses in the circuit

The new cooling system was designed specifically to comply to the correct water treatment and choice of materials to avoid future corrosion, deposition, erosion, pitting or biologic contamination and the flowmeters already in place were replaced. Air was completely removed and the circulator's power was doubled (from a single one for two branches to two separate ones).

Still, the measured flow of the new system was the same or lower than the old one, even when switching back to the old flowmeters, that show the same measurements as the new ones.

First thing that needs to be taken into account is that during the installation the system remained filled with still water for more than a month, so if any debris were present they might have deposited.
This is why Nicola, Piernicola and I carried out a thorough cleaning of every piece of piping and every fitting, laser area included, with air, mechanical friction, alcaline soap and both alcohol and ultrapure water ultrasound bath.
We inverted the laser's inlet and outlet from the circulators onwards and closed the system on itself at every level. The results are the following:
 

The flow up to the split among the utilities, under the bench, is 10 l/min.
After the splitting into 8 utilities, it decreases to 2 l/min (acceptable according to the laser manufacturer)
We tested every utility and found some beam dump to be completely clogged so that not even air could go through. The laser, nevertheless, after being cleaned with dust-free cloths and distilled watere, showed no working issues. 

While dismantling and cleaning the old system, debris were collected and biological contamination was observed. They will be sent to an external laboratory to be analized.
Water pH was between 6 and 6.5.

TDS document addressing pollution in cooling systems coming soon

From a quick look:

The excess noise above 2kHz engaged as well on May 7th: as shown by VIM in Figure 1

This noise seems associated to the INJ HVAC: as it went off and on at the time of its switching off/on on July 28th : Figure 2.

This morning, according to the planned schedule, we attempted to switch on the NI and WI main CO₂ lasers.

After Nicola and Cecilia successfully restored the chillers and the Guardian system, the NI and WI main lasers were switched on at 08:17 UTC and 08:18 UTC, respectively.

Unfortunately, after about 1 minute and 40 seconds of operation, the WI main laser unexpectedly switched off (fig.1). Several attempts were then made to restart it, but without success.

At that point, Roberto and Flavio joined the investigation, and a series of checks was performed to determine whether the problem was related to the laser itself or to the driving electronics.

1. The  electronics in TCS room  were swapped between the NI and WI systems. The NI laser switched on correctly using the WI electronics, while the WI laser still failed to switch on. This excluded the RF driver and the 5 V TTL signal generated in the TCS room as the source of the problem.
2. We then proceeded with additional checks underneath the WI bench, where the laser electronic is installed. With all lasers switched off, Roberto verified that the RF signal was correctly reaching the RF driver.

A visual inspection of the bench, including the BNC connections and the laser itself, did not reveal any obvious anomaly. The laser status LED was correctly lit in red, and all RF driver dongles were green, as expected.

After closing the bench, we performed one final startup attempt. This time the WI laser switched on, but only at approximately half of its nominal power. After another power cycle, the laser briefly reached its nominal output power before dropping again to approximately half power (fig.2).

During the brief period in which the laser reached nominal power, I acquired a thermal camera image of the DAS beam (fig.3). No anomalies were observed.
These observations suggest that the problem is more likely related to the electronics than to the laser itself. To be understood.For safety reasons, we decided to switch off both lasers on the WI bench.

At the time of writing, the laser status is as follows:

• NI bench: both the auxiliary and the main CO₂ lasers are switched on, with all beams blocked on the bench.
• WI bench: both the auxiliary and the main CO₂ lasers are switched off.

The WI main chiller is off. The backup chiller is connected only to the NI.

For the auxiliary chiller, the valve to the WI branch has been closed to avoid circulating cold water through the switched-off WI laser.

================================

As a side note (but an important one), I am experiencing significant difficulties with online monitoring using Data Display, even when using the previous version (Dy/v11r2/Linux-x86_64-AL9). While monitoring the channels, the displayed data frequently disappear for several seconds before reappearing. After some time, the application freezes completely and has to be restarted (see Fig. 4 for an example).

Acoustic noise inside the INJ room has changed significantly between the most recent switch off (July 28, https://logbook.virgo-gw.eu/virgo/?r=69458) and the previous which was in November (Nov. 27 2025: https://logbook.virgo-gw.eu/virgo/?r=68269). The changes are shown in the LAST plot attached comparing mics ASD. We tried to track these changes and found the following:

Reduced 20Hz acoustic bump:

On June 18th the RETURN fan frequency of INJ HVAC was changed from the usual 21 Hz to 14 Hz, and the acoustic bump around 20 Hz reduced significantly: Figure 1 and Figure 2. This is consistent with (but more pronounced then) what observed in our quick slow down in https://logbook.virgo-gw.eu/virgo/?r=67829   (return fan moved only down to 17Hz). We do not know why this reduction to 14 Hz was done, but the HVAC is running in this way since then. Good news is also that the environmental parameters seems not significantly affected (Figure 3).

Acoustic bumps 40-120 Hz changing level:

Examing VIM spectrogram back since Dec 2025, we noticed that in a number of occasions (see Table) some acoustic bumps in the INJ room mics increased or reduced. Bumps are roughly at 40, 60, 80 120 Hz. Figures 4 to 8 show some of these occurrences. The last increase happened on May 7th, and the noise condition is this since then. It looks that these occurences coincide with people entering and then leaving the INJ area (seismic activity).  Examining some occurences, we often find a change in the pressure of the INJ room, yet no change in the fans' frequency: see in Figure 9 and following. 

Excess noise around 490 Hz and above 2kHz: this has to be investigated .... :-)

A list of these occurences:

ITF in COMMISSIONING, DOWN

Activities reported to the control room:

• Instrumented baffle commissioning (Vallejo, Sadiq, Boldrini)
• CO2 DAS lasers were switched on: NI switched on properly, WI did not. Investigation carried out with both lasers switched off (Cavalieri, Menzione, Nardecchia, Zaza). WI DAS left switched off
• CO2 CH cooling system testing (Menzione, Nardecchia, Zaza). Due to WI DAS malfunctioning, WI CH was left switched off too. NI cooling test ongoing.
• Input mirrors local controls checks (Majorana)

The assembly of the new cooling system for the TCS auxiliary lasers is complete.

It is a two-stage system (pic 1 - schematics)
1. Primary stage –. The tank temperature is maintained by one of two chillers, operating in a redundant configuration: one unit designated as the primary chiller (working) and a second unit
as a (non operating until needed) backup, to ensure continuous operation. In case of failure, the operator on shift will only have to switch the piping from one chiller to the other (pic 2: AuxCooling Chiller)
2. Secondary stage – From the tank (pic 3 - AuxCooling Tank), water is distributed through two separate piping and valve systems, one per laser (pic 4 (temporary) - Distribution and post-heating system assembly phase). Each system includes four pipe collar heaters, enabling post-heating control of the oscilations in temperature, to keep them within the 0.1 limit (more details in future entries that will be posted as comments of this one).

New sensors were installed and new channels were created, soon to be implemented on DMS. Together with the old ones, the system can be monitored using (see schematics): 

1. INF_TCS_AuxCooling_Pri_OUT_TE (chiller --> tank)
2. INF_TCS_AuxCooling_Pri_IN_TE (tank --> chiller)
3. INF_TCS_AuxCooling_Pri_FLOW (chiller --> tank) 
4. INF_TCS_AuxCooling_Tank_OUT_TE (tank --> circulators)
5. INF_TCS_AuxCooling_NI_IN_TE (NI utilities --> tank)
6. INF_TCS_AuxCooling_WI_IN_TE (WI utilities --> tank)
7. INF_TCS_AuxCooling_NI_FLOW (NI utilities --> tank)
8. INF_TCS_AuxCooling_WI_FLOW (WI utilities --> tank)
9. HVAC_TCS_NI_TE (placed after the resistors, used for the post-heating control loop)
10. HVAC_TCS_NI_TE_SET (post-heating control loop)
11. HVAC_TCS_NI_ALARM (post-heating control loop)
12. HVAC_TCS_NI_CORR (post-heating control loop)
13. HVAC_TCS_WI_TE (placed after the resistors, used for the post-heating control loop)
14. HVAC_TCS_WI_TE_SET (post-heating control loop)
15. HVAC_TCS_WI_ALARM (post-heating control loop)
16. HVAC_TCS_WI_CORR (post-heating control loop)
17. INF_TCS_AuxCooling_NI_IN (temperature of NI laser, already in use)
18. INF_TCS_AuxCooling_WI_IN (temperature of WI laser, already in use)
19. TCS_NI_CO2_CH_PWRLAS (NI laser power, already in use)
20. TCS_WI_CO2_CH_PWRLAS (WI laser power, already in use)

We commissioned the WI instrumented baffle for the prealignment of the WE, repeating the procedure used yesterday for the NI (69514)

The starting position for the WE is (TX; TY) = (24.5; 136.8) urad

We then swept the NE right by about 100 - 110 urad until we intersected the symmetrical column c5 and repeated the process. Overall, the power detected were:

• column c17 (East - South - East section of the baffle, fig.3), WE_TX/TY = (26.65; 186.0) urad 
  • sensor r0: 16.80 uW
  • sensor r1: 18.47 uW
  • sensor r2: 16.48 uW
• column c5 (West - North - West section of the baffle, fig.4), WE_TX/TY = (25.3; 87.8) urad 
  • sensor r0: 16.94 uW
  • sensor r1: 18.68 uW
  • sensor r2: 16.81 uW

The median point identified by these positions is (<TX>;<TY>) = (24.5; 136.9) urad.

We repeated the process with a vertical scan:

• column c23 (North - North - East section of the baffle, fig.5), WE_TX/TY = (74.8; 133.0) urad 
  • sensor r0: 18.12 uW
  • sensor r1: 19.62 uW
  • sensor r2: 18.17 uW
• column c11 (South - South - West section of the baffle, fig.6), WE_TX/TY = (-24.1; 140.1) urad 
  • sensor r0: 17.32 uW
  • sensor r1: 18.71 uW
  • sensor r2: 17.22 uW

The median point identified by these positions is (<TX>;<TY>) = (25.3; 136.5) urad.

We were able to apply the procedure much faster, as we become more familiar with the behaviour of the baffle, and the obtained accuracy is still within a few urads from the well aligned position of the WE.