here the BruCo using as target LSC_PRCL: https://scientists.virgo-gw.eu/DataAnalysis/DetCharDev/users/fiori/bruco/LSC_PRCL_1475998223/bruco.html
here the BruCo using as target LSC_PRCL: https://scientists.virgo-gw.eu/DataAnalysis/DetCharDev/users/fiori/bruco/LSC_PRCL_1475998223/bruco.html
ITF found in UPGRADING mode and DOWN state.
All times are UTC.
07:40 Permit to work inside SR tower open (Galimberti, #69937). Flange open shortly after (VAC, #69938).
08:35 SR diaphragm installation begin (Majorana, Pinto). Still ongoing at 14:35.
ITF left in UPGRADING mode and LOCKED_ARMS_IR_ALS requested by ARMS_LOCK metatron node.
We run a BruCo, coherences are computed up to 1kHz:
https://scientists.virgo-gw.eu/DataAnalysis/DetCharDev/users/fiori/bruco/Hrec_hoft_1475998223/bruco.html
The pole at 500Hz noise that appeared on Oct 7 around 19:00 UTC is also visible in other channels earlier in the INJ chain.
Figure 1 and 2 compare the time before the issue started (purple) with a time after (blue) respectively on Oct 8 and Oct 14. All the times are with the interferometer in LN2 or LN3. The additional noise is visible clearly also on the Audio band monitoring of the EOM transmission, on the EOM correction, and much less clearly on the PMC transmission.
If the extra noise is visible on the EOM transmission (INJ_EAB_EOM_TRA_AUDIO) both with the IMC locked and unlocked, then it should make it easier to find. As the IMC can be excluded from the investigation, but most likely the problem becomes invisible in that case, as the laser amplitude noise will dominate everything with the PSTAB loop open.
We restarted the recovery of the system.
The CC PLL was already locked, the first things was checked was the relock of the squeezer. The level of the green was too low and the contrast of the MZ interferometer was too low. As first thing Fiodor realigned the MZ and we managed to relock it with offset of +0.03V
After that we managed to lock the OPA.
Jean Pierre and Marco recovered the other two PLLs in DETeroom. Note that for the third time we found the SC laser off it switched off by itself without any clear reason.
Finally we restarted to recover the alignment of the squeezer:
1) We locked the CC and we closed the AA. The magnitude was too low
2) We checked SQB1 HWP2 (looking the level of the 4 MHz mag in ASQZ) and HWP1 (minimizing the stay light bump on HD DIFF Audio
3) We checked the alignment of EQB1 PDs
4) We realized that we were clipping on the retroreflector Y because in february we moved downwards the vertical position of SQB1 bench.
After the realignment we managed to measure:
we run a phase scan @14:28 UTC but for some reason we found lower level of SQZ and ASQZ. We wanted to redo it but there were some unknow noise probably due to the venting and we could not repeated it.
We decided to move to the delay line. We did not find any light so we asked Fiodor to check in DET lab. And we realized that for safety reason, this summer we closed the GR shutter and we never noticed that when it was closed it clips the beam into the delay line
Once recovered the delay line and aligned with EQB1 Thorlabs picomotors we obtained:
The results of the two fits is in the attached figure.
Losses with delay line 9% and phase noise 60mrad. Phase noise better than in february, losses sligthly higher. The additional HWP in the HD path is still rotated for RR so this can cause additional losses
At the end of the shift we lef the RR on, HWP2 of SQB1 rotated toward HD detector, SC, LO shutter closed and MCIR unlocked
ITF found DOWN in COMMISSIONING mode with SR, SDB2, SDB1 loops opened.
UPGRADING mode set.
- INJ_MAIN, ARMS_LOCK, DRMI_LOCK, OMC_LOCK Metatron nodes set in manual.
- DRMI_LOCK, SUS_PR, SUS_SR Metatron node set in pause. ITF_LOCK, DET_MAIN already in pause.
- SR venting in progress
- planned activity: Squeezing beam blocked towards SDB1 (Sorrentino)
SBE
18:20 UTC - SPRB vertical position recovered via stepping motors.
Today around 16:10 UTC I put three beam dumps on EQB1 in front of the windows towards SQB1 for laser safety in view of SR tower access.
Figure 1. Comparing the spectrum of yesterday to the beginning of the year, the noise level of SRCL, PRCL, MICH is a factor few higher than before. Especially on PRCL. This is also the case of noise on the SSFS quadrature.
The question is what it is and where it comes from. The noise is likely to be present on the laser frequency, and then polluting all LSC channels. It may be related to the higher noise level of the LNFS.
Figure 2 The more structured noise that is visible in SRCL between 300Hz and 3kHz is very coherent with the excess noise in the LNFS. So that part is clearly due to the more noisy LNFS. For the excess noise in PRCL, and the excess noise in SRCL below 300Hz it is less plausiable. As there is no coherence with the LNFS phase noise, and the LNFS broaband noise below 300Hz is the same as it was at the beginning of the year.
Figure 3 shows yesterday in purple, Friday last week in red, and the beginning of the year in blue. Some version of the pole at 500Hz noise is back, it is clearly visible on SIB2 RFC 8MHz I, the level doesn't appear to be stable as it is different on Friday last week and yesterday, and the changes in noise level of PRCL and SSFS quadrature are correlated with those pole at 500Hz noise changes visible on RFC 8MHz I.
Figure 4 Looking at data of various nights with arms locked, the pole at 500Hz noise seems to have appeared on October 7. It would be important to look at that more precisely to see at what time the extra noise appeared. One hardware activity on that day was the realignment of the phase camera, and maybe a change in the splitters for the local oscillator of the phase camera https://logbook.virgo-gw.eu/virgo/?r=69877
Figure 5. Searching more precisely it looks like the problem started around 19:00 UTC, there was an interferometer unlock from LN2 at that time.
The pole at 500Hz noise that appeared on Oct 7 around 19:00 UTC is also visible in other channels earlier in the INJ chain.
Figure 1 and 2 compare the time before the issue started (purple) with a time after (blue) respectively on Oct 8 and Oct 14. All the times are with the interferometer in LN2 or LN3. The additional noise is visible clearly also on the Audio band monitoring of the EOM transmission, on the EOM correction, and much less clearly on the PMC transmission.
If the extra noise is visible on the EOM transmission (INJ_EAB_EOM_TRA_AUDIO) both with the IMC locked and unlocked, then it should make it easier to find. As the IMC can be excluded from the investigation, but most likely the problem becomes invisible in that case, as the laser amplitude noise will dominate everything with the PSTAB loop open.
We run a BruCo, coherences are computed up to 1kHz:
https://scientists.virgo-gw.eu/DataAnalysis/DetCharDev/users/fiori/bruco/Hrec_hoft_1475998223/bruco.html
here the BruCo using as target LSC_PRCL: https://scientists.virgo-gw.eu/DataAnalysis/DetCharDev/users/fiori/bruco/LSC_PRCL_1475998223/bruco.html
WIth the SR tower under venting, we setup the automation in the following way:
ITF found in locked arms ir.
At 7:00 UTC started the planned SR venitng; operations performed:
In parallel other two activities were carried out:
HVAC
Under request of Davide:
A line around 54.7 Hz is visible in the accelerometers installed in the NEB experimental hall, including those along the tower and on the flange, as well as in the acoustic sensors, some of the NN array geophones, and all its microphones, including those located in the technical area behind the building.
The line is not visible in the velocimeter (Guralp) installed beneath the stairs.
This frequency appears to be close to the 9th harmonic of the belt frequency associated with the AHU fan-motor system (~6.15 Hz). The line is also clearly visible in the accelerometer installed on the AHU box (*UTA_BOX_ACC).
It is worth mentioning this observation, although the frequency correspondence could simply be a coincidence.
This entry presents the measurement made in the arm this morning. The aim of the shift is to measure the orientation of astigmatism within the arm cavities. The method is similar to the one attempt in (68385). The NE and WE mirrors are misaligned during the scan, but instead of scanning the full FSR, only the frequency range of the first fundamental mode and first order mode is scanned. After half an hour, the arms are aligned using the automation loop before starting a new scan series.
Below is the list of scans performed during the shift with the associated misalignments
- scan n°1: 10h07 TX+=0.3 urad, TY+=0.0 urad
- scan n°2: 10h07 TX+=0.0 urad, TY+=0.3 urad
- scan n°3: 10h07 TX+=0.29 urad, TY+=0.08 urad
- scan n°4: 10h07 TX+= -0.08 urad, TY+=0.29 urad
The arms have been realigned using the automation loops
-scan n°5: 10h52 TX+=-0.15 urad, TY+=0.26 urad
-scan n°6: 11h01 TX+=-0.26 urad, TY+=0.15 urad
-scan n°7: 11h11 TX+=0.21urad, TY+=0.21 urad
-scan n°8: 11h19 TX=-0.21uradn, TY+=0.21urad
The arms have been realigned using the automation loops
-scan n°9: 11h34 TX=0.15urad, TY+=0.26urad
-scan n°10: 11h44 TX+=-0.26urad, TY+=0.15urad
-scan n°11: 11h54 TX+=0.08urad, TY+=0.29urad
-scan n°12: 12h03 TX+=-0.29, TY+=0.08urad
The arms have been realigned using the automation loops
-scan n°13: 12h18 TX+=0urad TY+=0.3urad
-scan n°14: 12h26 TX+=-0.3urad TY+=0.0urad
Profiting of the scans of yesterday evening on the SRCL set, I ve tried to check which is the best error signal.
the comparison is between the DCP and the DCP phi (ASC_DCP_HF_B1_phi_FS_mean found by Michal already in the past)
the two error signals have been built as:
Err = 0.1892*DCP -85.16;
Err1 = -125.8*DCP_phi +237.1;
in figure 1 the comparison is shown and the last seems a good error signal for the SRCL detuing
This morning around 7:00 UTC I adjusted the alignment of the MZI inside the squeezer box on EQB1. The contrast increased substantially, see first plot.
Witn Marco's support I also checked the OPA alignment, and I found it was already good, see second plot.
Added LSC_WE_CORR_SHAPED and LSC_NE_CORR_SHAPED to the BruCo unsafe-channel list: /data/dev/detchar/online/bruco/share/virgo_excluded_channels_Hrec_hoft.txt. These correspond to the unsafe Sc_{WE,NE}_MIR_Z_CORR channels (see logbook entry #67154), which in recent runs were dominating the observed coherences.
ITF found locked at LN2 in COMMISSIONING mode, with the planning ISC activity (Pinto Mantovani) in progress.
At 19:00 UTC the ISC activity concluded and I.Nardecchia switched off the SR RH at 19:14 UTC.
ITF left locked on LOCKED_ARMS_IR.
The SR RH was switched off at 19:14 UTC.
The morning shift started by relocking the interferometer, which had no issue on that front for the whole shift.
The idea of the shift was to start studying again the SRC longitudinal detuning. Before starting that, and also because we are now working decentering, a very basic set of angular noise injections was done (DIFFp, PR). The log file is in /virgoData/NoiseInjections/ASC/ASC_injection-1476000002.txt
After that, the tests on the SR detuning started; the first few tests were done naively by changing the setpoint of the SRCL_SET loop, which in the past did not give very good results, as the signal was not carrying enough information to drive it properly in the intended way (higher frequency for the optical spring). This happened in LOW_NOISE_3_ALIGNED.
Here the recap of the tests done in this way:
08:14:10 UTC : SRCL_SET_SET = 0.5 -> 5.0 in 300 s, then 480 s of clean data;
08:27:30 UTC : SRCL_SET_SET = 5.0 -> 10.0 in 300 s, then 600 s of clean data.
Around 8:31 UTC we observed some bursts of noise in the MICH loop (and, fainter, in the SRCL one) at around 3.6 Hz. Given that in that state the UGF servo loops are not operational anymore (with the exception of the DARM one), the gains of both of them were raised around 8:35:30 UTC. We unlocked at 8:38:52 UTC.
In the following lock, that started at 09:16:53 UTC:
09:27:42 UTC: SRCL_SET_SET = 0.5 -> 10.0 in 600 s
09:46:39 UTC: unlock
There were a couple of unattended tests during the lunch break, which look very similar and probably do not carry more information.
Later, we verifired offline from the tests that the OS signal moved back to a more manual approach: LOW_NOISE_2 state, SRCL_SET loop technically close but in reality frozen in place (LSC_SRCL_SET_CAL = 0), then LSC_SRCL_SET moved manually as a static offset.
Test #1:
12:29:00 UTC: start of LOW_NOISE_2
12:33:00 UTC: SRCL_SET loop frozen (value of _SET_TOT at the time ~ -8.3)
12:33:52 UTC: SRCL_SET = 0 -> -5 in 300 s
12:41:00 UTC: SRCL_SET = -5 -> -10 in 300 s
Noise injection on DARM (and clean data): logfile in /virgoData/NoiseInjections/LSC/LSC_injection-1476017575.txt
13:01 UTC: SRCL_SET = -10 -> -15 in 300 s
13:20 Noise injection on DARM (and clean data): logfile in /virgoData/NoiseInjections/LSC/LSC_injection-1476019008.txt
13:29:21 UTC: unlock
We continued to change the SRCL set at step LN2 (in order to have all the servo for the gains active) and we took :
- DARM OLTF measurements to fit the OS for different SRCL set
- Angular noise coupling (DIFFp) to see if the coupling could change with the SRCL set
the gps are:
SRCL set @ -10 gpsDARM=utc2gps(2026,10,14,14,32,45); dur DARM=120;
SRCL set @ -20 gpsDARM2=utc2gps(2026,10,14,14,47,50); dur DARM2=120;
gpsDptx=utc2gps(2026,10,14,14,57,00); dur Dptx=120;
gpsDpty=utc2gps(2026,10,14,15,04,10); dur Dpty=120;
It is visible that the -20 configuration shows a lower coupling of DIFFp TX (Figure 1)
After that we tried a SRCL set up to -30 but it failed the LN3 aligned state transition (a 3.5 Hz oscillation on MICH - most probably low gain, which is surprising since we let the servos to adjust the gain in the SRCL set increase and to stabilize).
We have then reached the LN3 aligned configuration and performed a SRCL detune to check the sensitivity (to be able to compare with the one that will be achieved with the diaphragm)
RECAP
the overall changes in the violins notches are the following: 4 notches for the first violins modes in the region 412-415 Hz.
we removed an old second order mode notch at 882.17 Hz, moved down to the 2nd order frequency mode of the new violin: 827.1 Hz, Q ratio=100.
The overall effect on DARM OLTF are negligible for the bandwidth; loss of less than 2 deg at 150 Hz; change of ~12.5 deg at 491 Hz, (already considered during the notch design) compensated by retuning the SR alignment phase. See fig.1 and 2 where the overall phase of the new notches is shown.
Just two possible hints:
The first is an old entry (... too old) dating 2011 which mentions one 54.8 Hz mechanical mode of WI payload: https://logbook.virgo-gw.eu/virgo/?r=30230. Indeed, most of the payload has changed since than, so I guess this must be just an unlucky concidence (!)
The second observation concens the attached plot. I picked some of the signals for which the BruCo found a coherence at the little one at 53.92 Hz. Couriously, these signals, which belonng to the SDB1 (OB) suspension have a peak at 54.7x Hz which appear to match closely to the main Hrec one... but no coherence on this. I do not have an interpretation for this.