Reports of 61820
AdV-DAQ (Calibration)
verkindt - 23:46 Thursday 28 August 2025 (67590) Print this report
Restart of Hrec using new bias file

Today, around 19:13 UTC, I have restarted Hrec to use the new bias file /virgoData/Hrec/Hrec_bias_202508_with50.txt which is based on checkhrec measurements done between July 14th and Aug 25th. This update of the bias file is a follow-up of the observation that, since start of July, the hrec/hinj bias was impacted by the changes that occured on the ITF.

Plot1 shows the residual bias before the restart of Hrec.
Plot2 shows the residual bias after the restart of Hrec.

Images attached to this report
Virgo Runs (O4c)
direnzo - 23:07 Thursday 28 August 2025 (67587) Print this report
Operator Report - Afternoon shift

At the start of the shift, the interferometer just recovered from an unlock likely due to intense wind, and was in Science mode for about 30 minutes. Another unlock occurred at 13:41:19 UTC, GPS 1440423697. After a series of unlocks for the strong wind (50+ km/h) before reaching LOW_NOISE_3 state, at 14:35 UTC the interferometer has been set to Commissioning mode, moving up the scheduled activities. LOW_NOISE_3 recovered at 18:57 UTC, after the calibration activities.

Below, the list of performed activities:

  • 14:35 UTC - INJ, realignment of the input beam (De Rossi, Casanueva): #67588. Interferometer set to LOCKED_ARMS_IR. Process concluded at 15:30 UTC
  • 15:30 - Napoli team to NEB for microphone and tiltmeter calibration. Operation concluded at 17:00 UTC
  • 15:30 - Started the calibration measurements with ITF unlocked:
    • 15:35 - Started Measurement of the TF between CAL and Sc channels, and of PCal sensing delays. Concluded at 15:48 UTC

    • 16:20 - Measurement of actuators response for PR and BS mirrors. Issue with DET_MAIN shutter closed when setting CALIBRATED_PRWI. Restored by putting DET_MAIN back to INIT, and restarting the calibration procedure. Concluded at 17:17 UTC

    • 17:20 - Measurement of actuators response for NI,WI mirrors. Concluded at 18:40 UTC

  • 15:48 - TCS, Cifaldi check of the powers. Operation competed at 16:18 UTC

  • 19:13 - CALI, Verkindt: Hrec bias updated. 

  • The interfermeter unlocked again at 19:30:51 UTC, GPS 1440444669, when a hailstorm hit the site, and, given that we were already 30 miutes past the end of the Commissioning slot, we decided to postpone the Scattered Light calibration activity by van Haevermaet. The interferometer was set beck to PREPARE_ASCIENCE mode (and AUTOSCIENCE_ON)

Other events to report:

  • Sudden data loss at 16:00:09 UTC. See attached figure
  • At 19:59 UTC, after various failed locking attempts and ITF mode set to BAD_WEATHER. The strong wind even tore down the Belgian flag!
  • At 20:24, ITF reached again LOW_NOISE_3 and set back to AUTO_SCIENCE

Guard tours (time in UTC)

  • 18:03 - 18:39
  • 21:00 - ...
Images attached to this report
AdV-INJ (Beam Pointing Control)
derossi, casanueva - 17:28 Thursday 28 August 2025 (67588) Print this report
beam recentering on the ITMs

Since the input beam was quite decentered on the ITMs, we translated the PR both horizontally and vertically to better recenter it (monitoring at the same time its position on the BPC quadrants).

 

Images attached to this report
Virgo Runs (O4c)
gherardini - 14:58 Thursday 28 August 2025 (67584) Print this report
Operator Report - Morning shift
After the recovery of the WI F7 control loop the ITF locked at the first attempt, science mode started at 5:52UTC; it unlocked at 11:32UTC because of a suddenly increase of the wind over the site; relocked at the second attempt and science mode started at 12:33UTC.
Images attached to this report
Detector Characterisation (Glitches)
dattilo - 12:51 Thursday 28 August 2025 (67586) Print this report
Comment to New type of glitches around 33Hz (67574)
A detail about the power supply that was malfunctioning: the problem was related to its cooling fan, which was no longer working. This was causing the driver to overheat, so after about 130 seconds the protection thermostat would intervene, blocking the power delivery. At that point, the driver would cool down, and after about 5 minutes, it would start supplying power again. Then the cycle would start again.
Detector Characterisation (Glitches)
salvador - 9:39 Thursday 28 August 2025 (67585) Print this report
Comment to New type of glitches around 33Hz (67574)
Virgo Runs (O4c)
amagazzu - 7:51 Thursday 28 August 2025 (67583) Print this report
Operator Report - Night shift

ITF found in LOW_NOISE_3 and in Science Mode. It unlocked at 3:57 UTC, but the ITF kept systematically unlocking at LOCKING_CARM_MC_IR. An issue highlighted by the DMS was a strong oscillation on the WI F7: while investigating we found that the data were abnormal (see attached plot).
With the support of Gherardini we opened the F7 loops and reload the DSP, which seems to have fixed the issue. Relock in progress.

Guard Tour (UTC)
22:28 - 22:52
1:02 - 1:24
3:27 - 4:00

DAQ
From around 14:00 UTC the signals related to INJ and DET ACS weren't avaiable anymore from DMS. After restarting the process BACnetServer at 21:01 UTC they were acquired correctly again.

Images attached to this report
Virgo Runs (O4c)
zaza - 22:59 Wednesday 27 August 2025 (67579) Print this report
Operator Report - Afternoon shift

13:00 UTC ITF found in SCIENCE
14:56 UTC
ITF in ADJUSTING - WI Etalon Servo Disabled/re-enabled to perform WI power supply swap (#67582 Dattilo, Zaza)
15:25 UTC ITF DOWN
16:15 UTC
ITF in SCIENCE

Guard Tours (UTC)
18:02 - 18:50
20:28 - 22:50

Images attached to this report
Detector Characterisation (Glitches)
dattilo, zaza - 17:56 Wednesday 27 August 2025 (67582) Print this report
Comment to New type of glitches around 33Hz (67574)
As a follow up of the recent investigations on this new type of glitches, we made a check of the WI heating belt power supply.
At around 14:57 UTC, with ITF mode set to Adjusting, we went in TCS room where the power supply is located, and also looking at its analog display, we saw that it was delivering intermittently, as indicated by the LSC_WI_HB_moni signal.
We replaced the power supply with a spare one of the same kind (Kert 420). During the intervention the operator temporarily opened the WI etalon loop. It was turned back on at 15:25 UTC.
Now the loop seems working regularly (attached fig).
Unfortunately, during the intervention the ITF unlocked, just a few seconds after the etalon loop was turned back on.
Images attached to this comment
Detector Characterisation (Glitches)
fiori, paoletti, dattilo - 15:44 Wednesday 27 August 2025 (67581) Print this report
Comment to New type of glitches around 33Hz (67574)

The time pattern and magnetic witness point to a noise from the power supply of the heating belts, as evidenced by Bas in O3:  https://logbook.virgo-gw.eu/virgo/?r=48521

sorry I missed the previous post, pointing to the same problem. The time pattern is clear.

However, consulting with Federico and Vincenzo: the cause is likely the power supply, whose fans are old and do not cool down enough, the power supply goes in protection ad switches on/off.

The suggestion is  first inspect and then replace.

Images attached to this comment
Detector Characterisation (Glitches)
direnzo - 15:18 Wednesday 27 August 2025 (67580) Print this report
Comment to New type of glitches around 33Hz (67574)

These glitches look similar to something we’ve already seen in April 2024: #64114.

Virgo Runs (O4c)
direnzo - 15:05 Wednesday 27 August 2025 (67573) Print this report
Operator Report - Morning shift

At the beginning of the shift, the interferometer has been found relocking, with AUTOSCIENCE_ON. Succesfully back to LOW_NOISE_3 state at 5:29:12, and SCIENCE mode at 5:32:12 UTC. Operational status maintained throughout the entire shift. 

Images attached to this report
Detector Characterisation (Glitches)
salvador - 15:03 Wednesday 27 August 2025 (67578) Print this report
Comment to New type of glitches around 33Hz (67574)

Their frequency distribution seems to go from around 15 Hz up to almost 60 Hz.

First glitch is most likely a 25-min glitch. (Picture shows the whitened spectrogram of Hrec_hoft_20000Hz)

Images attached to this comment
Detector Characterisation (Glitches)
fiori - 14:59 Wednesday 27 August 2025 (67577) Print this report
Comment to New type of glitches around 33Hz (67574)

These glitches (I guess these are the same... and 33 Hz or so might be the energy baricenter?) seems to have a precise periodic pattern, see the attached.

Images attached to this comment
Detector Characterisation (Glitches)
narnaud - 14:46 Wednesday 27 August 2025 (67576) Print this report
Comment to New type of glitches around 33Hz (67574)
Environmental Monitoring (Environmental Monitoring)
fiori - 14:42 Wednesday 27 August 2025 (67575) Print this report
Comment to WE scatter light investigation (64481)
Environmental Monitoring (Environmental Monitoring)
fiori, tringali, loche - 14:34 Wednesday 27 August 2025 (67570) Print this report
Comment to WE scatter light investigation (64481)

With a deeper examination of the Hrec data during the WE tapping sequence we notice a characteristic pattern that got excited when tapping from some of the locations.

The pattern, shown in the attached figures, consists of a family of narrow spectral peaks at precise frequencies (Hz) : 

  • 41.4
  • 44.5
  • 52.9
  • 66.1
  • 69.7
  • 88.9
  • 97.2
  • 105.0
  • 120.3

This pattern gets excited when tapping on locations at the tower chamber, not from CT locations. Most peaks are more excitable when tapping on HR side, but the 88 Hz is much louder in hrec when tapping the viewport on the AR side (the 41 Hz has a similar behaviour).  Some coherence with accelerometer is present for all of them, pointing to a mechanical structure attached to the tower that gets excited by the tapping.

Tapping on the AR viewport also excited a clear peak at 167Hz which clearly associates to a corresponding peak in the AR flange accelerometer, as already noted in the previous.

Other notes:

  • the excess noise appearing sometimes below 30 Hz and always lasting exactly 4 minutes, is now understood to be due to a reassessment of the Hrec online computation after a large impuse noise, sometimes due to our action: these are indicated with magenta circles and magenta arrows in Figure 1. Indeed the same noise is not seen in DARM. Thanks to Francesco DiRenzo for explaining this to us.
  • we also notice a faint structure around 180Hz that was present during the first part of the shift apparently not correlated with our actions, in Figure 4.
Images attached to this comment
Detector Characterisation (Glitches)
mwas - 14:32 Wednesday 27 August 2025 (67574) Print this report
New type of glitches around 33Hz

Figure 1. A new family of glitches started on Sunday around 15:30 UTC. These glitches are loud and frequent, and look to be around 33Hz.

Figure 2. These glitches are continuing during last night, so this problem is still present. 

Images attached to this report
Comments to this report:
narnaud - 14:46 Wednesday 27 August 2025 (67576) Print this report
fiori - 14:59 Wednesday 27 August 2025 (67577) Print this report

These glitches (I guess these are the same... and 33 Hz or so might be the energy baricenter?) seems to have a precise periodic pattern, see the attached.

Images attached to this comment
salvador - 15:03 Wednesday 27 August 2025 (67578) Print this report

Their frequency distribution seems to go from around 15 Hz up to almost 60 Hz.

First glitch is most likely a 25-min glitch. (Picture shows the whitened spectrogram of Hrec_hoft_20000Hz)

Images attached to this comment
direnzo - 15:18 Wednesday 27 August 2025 (67580) Print this report

These glitches look similar to something we’ve already seen in April 2024: #64114.

fiori, paoletti, dattilo - 15:44 Wednesday 27 August 2025 (67581) Print this report

The time pattern and magnetic witness point to a noise from the power supply of the heating belts, as evidenced by Bas in O3:  https://logbook.virgo-gw.eu/virgo/?r=48521

sorry I missed the previous post, pointing to the same problem. The time pattern is clear.

However, consulting with Federico and Vincenzo: the cause is likely the power supply, whose fans are old and do not cool down enough, the power supply goes in protection ad switches on/off.

The suggestion is  first inspect and then replace.

Images attached to this comment
dattilo, zaza - 17:56 Wednesday 27 August 2025 (67582) Print this report
As a follow up of the recent investigations on this new type of glitches, we made a check of the WI heating belt power supply.
At around 14:57 UTC, with ITF mode set to Adjusting, we went in TCS room where the power supply is located, and also looking at its analog display, we saw that it was delivering intermittently, as indicated by the LSC_WI_HB_moni signal.
We replaced the power supply with a spare one of the same kind (Kert 420). During the intervention the operator temporarily opened the WI etalon loop. It was turned back on at 15:25 UTC.
Now the loop seems working regularly (attached fig).
Unfortunately, during the intervention the ITF unlocked, just a few seconds after the etalon loop was turned back on.
Images attached to this comment
salvador - 9:39 Thursday 28 August 2025 (67585) Print this report
dattilo - 12:51 Thursday 28 August 2025 (67586) Print this report
A detail about the power supply that was malfunctioning: the problem was related to its cooling fan, which was no longer working. This was causing the driver to overheat, so after about 130 seconds the protection thermostat would intervene, blocking the power delivery. At that point, the driver would cool down, and after about 5 minutes, it would start supplying power again. Then the cycle would start again.
Virgo Runs (O4c)
amagazzu - 7:08 Wednesday 27 August 2025 (67572) Print this report
Operator Report - Night shift

ITF found in LOW_NOISE_3 and in Science Mode. It kept the lock for the whole night but unlocked at 4:43 UTC.
Relock in progress.

Guard Tour (UTC)
20:59 - 21:36
23:05 - 23:43 
1:07 - 1:42
3:27 - 4:01

Images attached to this report
Virgo Runs (O4c)
zaza - 22:58 Tuesday 26 August 2025 (67564) Print this report
Operator Report - Afternoon shift

13:00 UTC ITF found in LOCKED_ARMS_IR - TROUBLESHOOTING
13:30 UTC NEB green laser recovery following a loss in power (see pic. 1)  (Casanueva, De Rossi)
13:30 UTC CEB Suspension Vertical System Centering (#67568) (Boschi, Razzano) 
14:12 UTC stol02 processes reboot (#67567) (Salconi, Kraja, Masserot)
15:14 UTC NI TCS bench thermalization (Gherardini, Melo)
16:04 UTC NI TCS end of maintenance. As suggested by Nardecchia, we waited one hour (more or less) to allow the system to adjust before trying to lock
16:58 UTC ITF in CARM_NULL_1F. After aligning west arm, PR and SR and reaching the state, SDB2_B1p_DC signal was too high (Bersanetti)
17:38 UTC NI DAS CO2 laser (outer ring) first power adjusting step (Nardecchia)
18:26 UTC second power adjusting step (#67571) (Bersanetti, Nardecchia)
20:36 UTC ITF in LOW_NOISE_3 - SCIENCE

Guard Tours (UTC)
18:04 - 18:37
20:58 - 

Images attached to this report
AdV-TCS (CO2 laser projector)
bersanetti, nardecchia, zaza - 22:56 Tuesday 26 August 2025 (67571) Print this report
Lock acquisition recovery after NI CO2 bench intervention

After the activity on the NI CO2 bench, the ITF successfully relocked at CARM NULL 1F on the first attempt at 16.58 UTC.
However, we observed that the power on B1p was too high (0.03 mW) to proceed with the lock acquisition, so we started tuning the NI DAS to reduce it.

Step 1 (17:38 UTC): Decreased outer ring power

  • NI CO2 PICK OFF: 0.55 W → 0.52 W
    Positive effect on B1p

Step 2 (18:26 UTC): decreased outer ring power

  • NI CO2 PICK OFF: 0.52 W → 0.49
    ​​​​​​Negative effect on B1p

Step 3 (19:04 UTC): Increased outer ring power

  • NI CO2 PICK OFF: 0.49 W → 0.51  

Step 4 (19:20 UTC): Increased inner ring power

NI CO2 PICK OFF: 0.51 W → 0.522
​​
Once the B1p power reached 0.02 mW, we resumed the lock acquisition.
The ITF relocked in LN3 at 20:36 UTC.
Lock acquisition procedure is still to be verified.

Images attached to this report
Environmental Monitoring (Environmental Monitoring)
iannotta, de rosa, allocca, paoletti, fiori - 22:24 Tuesday 26 August 2025 (67565) Print this report
Infrasound microphones installed at NEB
This morning three new microphones have been installed at the North End Building. The reasons are several, including the necessity of monitoring the acoustic noise, but, above all, our team idea is to seek for correlations between the tilt signal read by the tiltmeter and the pressure difference between the two opposite sides of the tiltmeter vacuum chamber.
The required instrumentation consisted of four total microphones: an infrasound GRAS 47AC (serial number 468275), an infrasound Bruel&Kjaer 4193 (serial number 2615925) and a standard GRAS 46AZ (serial number 231053) which was then substituted by another infrasound B&K (serial number 3032669) for reasons that will be clear in a moment.
First of all, we executed a cross calibration of the instruments using the HR mic and the B&K 4193 present at the Central Building (ENV_CEB_MIC, ENV_CEB_MIC_HR). Specifically, we placed our GRAS 47AZ and our B&K 4193, adequately protected by windproof balls, in the same direction of the existing mics, as near them as we could, for them to measure (roughly) the same data. This is shown in Figure 1.
The GRAS mic acquisition required a GRAS 12AL CCP supply whilst the B&K needed a NEXUS amplifier.
After an acquisition of roughly 30 minutes, from 11:05 to 11:25 LT, we were able to conclude that our microphones have a similar response to each other both at low and high frequencies and they're quite coherent with the existing mics from 0.1Hz on. For lower frequencies, coherence is lost, as one can see in Figure 2.
Additionally, in Figure 3 we can see the usefulness of the windproof ball, since the coherence between the protected mics and the HR one is higher than the one between the B&K 4193 unprotected one and the HR.
The following step was the installation of the mics at the North End Building. Even though the installation procedure was identical to the one executed at CEB, we had several problems that forced us to substitute one of the GRAS microphones.
We started by positioning the infrasound GRAS and B&K mic, protected by the windproof ball, in line with the tiltmeter present in the building, as one can see in Figure 4. The third microphone, the standard GRAS, was positioned facing the same direction as the exiting one (ENV_NEB_MIC) for similar reasons as before, free of the windproof ball.
While reading the acquisition data, however, we acknowledged that the two GRAS mics were not able to read the same low frequency data of the other B&K microphones. In addition, the frequency spectrum showed an irregular reduction of their response.
Since this problem wasn't faced in the CEB measurements, we reckon that we either had problems with the electronics, or we made mistakes we're currently not aware of.
Nevertheless, since we wanted to measure the difference of pressure between the two faces of the tiltmeter chamber, we decided to substitute the infrasound GRAS with another B&K 4193 (serial number 3032669), connected to the same NEXUS used for the other measurement. This swap should actually improve our measurements, since in the first place the implied microphones were not identical, whereas now they’re both B&K 4193. The other standard GRAS (connected to PCB 482C05, channel 3) remained in its original position but will only be used for acoustic noise monitoring.
After analysing the data coming from this last configuration, shown in Figure 5, we can successfully affirm that the two infrasound B&K placed near the tiltmeter (ENV_NEB_MIC_4193_N and ENV_NEB_MIC_4193_S), are coherent with the already existing B&K mic at the North Building. The standard GRAS response (ENV_NEB_MIC_GRAS_HR) is definitely different and not quite performing at frequencies lower than 1Hz, but it’s not concerning, since that microphone aim is to monitor higher frequencies.
Images attached to this report
AdV-TCS (CO2 laser projector)
gherardini, melo, nardecchia - 18:24 Tuesday 26 August 2025 (67569) Print this report
Damaged mirror replacement on the NI bench / Part 2

This afternoon, Suzanne and Fabio adjusted the M3 mirror to restore the pre-mirror replacement alignment.

The comparison of the DAS before and after the mirror replacement is shown in Fig. 1.

Work on the bench was completed at 15:55 UTC.
The correct powers were recovered, and all flip mirrors were re-opened at 16:04 UTC with standard powers. 

Images attached to this report
Environmental Monitoring (Environmental Monitoring)
fiori, gargiulo, pasqualetti, soldani - 17:06 Tuesday 26 August 2025 (67566) Print this report
measurements of air velocity inside DET

This morning from about 10:45 to 12:00 LT we entered the DET lab to perform measurements of air speed velocity in different locations inside the lab. The used tool is a hot wire anemometer (sauermann KIMO VT110) by Davide. The scope is to get a quantitative idea of how the air moves inside the lab. We took measurements with the air conditioning on in REDUCED mode from 10:45 to 11:15 LT, then with the air conditioner on in NORMAL mode from 11:40 to 12:00 LT. The air conditioner was set in Nominal flux mode from 11:36 to 12:17 LT. 

We took measurements at approx. 20cm from the air inlets in the ceiling, the two air outlets in the walls, around the covered EDB and in a pair of positions in the EDB room at beam height. When in REDUCED mode we measured air speeds in the range  0.05 to 0.35 m/s close to the inlets, 0.05 m/s and 0.02 m/s close to the two outlets (respectively the one close to the entrance door and the one in the SW corner),  from 0.02 to 0.15 m/s around the EDB, 0.02 m/s in the room close to SDB2 chamber doors. When in NOMINAL mode air speed values close to the inlets and around the EDB roughly doubled, but also were significantly oscillating (by a factor 3 or so) on the time scale of 10 seconds or so. At the two outlets the air speed increase was more substantial and stable (no oscillation observed), reaching 0.3 m/s near both.

Additionally, when HVAC in NOMINAL mode we measured a value of 0 m/s inside the SQZ area (only one position measured). 

The air flow seems to slow down going from the East wall towards the West, the larger air flux is on the lab East side, as it seems reasonable since the 4 air inlets are placed on the ceiling along this wall. 

We shall add a map reporting all measured values.

Figures show values of HVAC fans speed, air fluxes in/out of the DET lab, temperature and microphone RMS, during the measurements time.

Images attached to this report
AdV-SAT (Suspension control upgrade)
piendibene, Razzano, Boschi, Vacatello - 17:03 Tuesday 26 August 2025 (67568) Print this report
Vertical centering of BS and WI

Due to saturation of BS and WI F0 vertical coils we recenter the vertical position of the filters.
Start at 15:40 LT
End at 17:00 LT

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