STATE of H1: Observing at 156Mpc
CURRENT ENVIRONMENT:
SEI_ENV state: CALM
Wind: 9mph Gusts, 7mph 5min avg
Primary useism: 0.03 μm/s
Secondary useism: 0.41 μm/s
QUICK SUMMARY:
20:04:31 UTC super event candidate S231113bw
An hour later at 21:09 UTC H1 had an Accidental Drop Out of Observing due to some changes made to the HEPI filters.
The button push then reverted the changes.
21:19 UTC H1 was back in Observing
H1 has now been locked for 61 hours and 29 minutes and is expected to stay locked until Tuesday maintenance commences.
Summary of the report:
Mon Nov 13 10:09:37 2023 INFO: Fill completed in 9min 33secs
FAMIS 20002
No major events of note this week; the FSS TPD has been dropping slowly over the past week or so but is still at ~0.84V.
In October I found a 13 Hz peak in the CER microphone channel whose frequency was similar to a comb of broad 13 Hz harmonics in DARM (broadened due to intermodulation). We found that we could eliminate the peaks in DARM by shutting down AC1 (73430 ). The acoustic peak from AC1 was not very large, so I looked into the high coupling this trip. I first injected globally with the big speaker, and then narrowed the coupling location down with more localized shaker injections, until I could produce it with small shaker injections at the input mode cleaner tube. AC-1 increased the vibration level seen by the MC-tube accelerometer by about a factor of 3 and shaking the tube by a similar factor produced a similar comb in DARM.
The 6 CER ACs all produce peaks near 13 Hz with similar amplitudes, but only AC-1 matched the frequency of the MC-tube coupling resonance, explaining why it alone produced the peaks in DARM. I think these peaks drift some so another AC may couple in the future and AC-1 may not be a problem if we turn it back on.
The coupling site may be the MC baffles, possibly MCA2
There is not a lot in the MC-tube other than the MC baffles. The last time I measured the lowest resonance of MCA2 (the eye baffle) it was 12.37 Hz (35735), but we have damped it since then. MCA1 (swiss cheese) moved from 12.1 to 12.4 Hz when it was damped (36979 ) , so I would expect the resonance of the eye baffle to be close to 13 Hz. The MC tube walls may have resonances in this band, but no peak was evident at the resonance frequency in ambient signals from the accelerometer mounted on these walls. However, I can not yet eliminate the possibility that the resonance may be something in HAM2 or 3, though the frequency is a little low for most other things. So I will test the coupling site identfication when I return, using the beating shaker technique.
The main HVAC may also couple at this site
A recent HVAC turbine shutdown at the corner station increased the range by about 4Mpc (74108). The coupling mechanism is uncertain and produces noise in the 20-200 Hz band. The HVAC turbines only increase the vibration background at the MC tube by factors of about 1.5 between 7 and 27 Hz, but I shook the tube to increase the level by a factor of about 2 and found that the injection produced strong features in DARM (see Figure 1). Thus the HVAC produces at least part, if not all, of the noise it produces in DARM at this site. Note that this also likely means that other ambient sources are producing noise in DARM at this site even when the HVAC is off.
MCA2 could probably be improved in-situ with viton washers and new panels with larger bolt holes
The eye baffle (MCA2) has been damped with Viton corks and pieces ( 38757 ). I noted at the time that there were fairly high-Q panel resonances in the tens of Hz. The next step would be to put viton washers between the panels and all bolts. I think this could be done in-situ. Also, I noted that bulges in the panels defeated the angling of the baffle and produced reflections in beam-spot photos (see figure photos in 38757 ). These bulges could be eliminated with new panels with larger bolt holes to allow for the slight mismatches of the holes.
The SR tube MC baffles also seem to couple, but not as strongly
I also injected at the SR tube, where there are two more MC baffles. I could produce noise in DARM when shaking at 10 and 14.1 Hz, similar to the 13 and 15.2 Hz resonances for the input MC tube. But the velocity from ambient noise does not appear to be high enough to make noise at harmonics in DARM.
Why is it so hard to find low-level coupling from scattering noise?
For finding linear coupling, we can inject louder vibration signals and produce a larger, more obvious peak in DARM. But for scattering noise in the regime where the motion is comparable to the laser wavelength, increasing the vibration injection amplitude tends to produce smaller, not larger peaks. The increased vibration produces more peaks, at harmonics of the fundamental frequency, and so the scattering “shelf” extends to higher frequencies, but, if the total scattered light does not increase, energy conservation requires that the more numerous peaks be lower in amplitude. If DARM is more sensitive in the higher frequency band that the shelf of harmonics reaches during the injection, the scattering noise can become more obvious even though the peaks are smaller. But when the scattering noise peaks are already small in the most sensitive regions of the detector, increasing the vibration amplitude can actually make them harder to find.
To find the subtle noise in DARM without being able to increase its amplitude, I used spectrograms with very small normalized color scale ranges (I start with 1.3 to 1.5 while the typical default covers several orders of magnitude) to observe small changes in DARM as the “shelf” cutoff moved.
FAMIS 26217
Laser Status:
NPRO output power is 1.819W (nominal ~2W)
AMP1 output power is 67.52W (nominal ~70W)
AMP2 output power is 137.1W (nominal 135-140W)
NPRO watchdog is GREEN
AMP1 watchdog is GREEN
AMP2 watchdog is GREEN
PMC:
It has been locked 5 days, 22 hr 30 minutes
Reflected power = 15.92W
Transmitted power = 109.3W
PowerSum = 125.2W
FSS:
It has been locked for 2 days 9 hr and 19 min
TPD[V] = 0.8332V
ISS:
The diffracted power is around 3.0%
Last saturation event was 2 days 9 hours and 19 minutes ago
Possible Issues: None
TITLE: 11/13 Day Shift: 16:00-00:00 UTC (08:00-16:00 PST), all times posted in UTC
STATE of H1: Observing at 156Mpc
OUTGOING OPERATOR: Ryan S
CURRENT ENVIRONMENT:
SEI_ENV state: CALM
Wind: 13mph Gusts, 11mph 5min avg
Primary useism: 0.03 μm/s
Secondary useism: 0.39 μm/s
QUICK SUMMARY:
H1 has been locked for 55 hours and 42 minutes and observing.
Every thing seems to be in working order at first glance.
TITLE: 11/13 Eve Shift: 00:00-08:00 UTC (16:00-00:00 PST), all times posted in UTC
STATE of H1: Observing at 156Mpc
INCOMING OPERATOR: Ryan S
SHIFT SUMMARY:
Quiet night, H1 is going strong (almost 48 hours!) and seismic activity remains low.
LOG:
No log for this shift.
H1 is still chugging along, current lock has just hit 43.5 hours. IFO appears stable and seismic activity is also low.
TITLE: 11/13 Day Shift: 16:00-00:00 UTC (08:00-16:00 PST), all times posted in UTC
STATE of H1: Observing at 156Mpc
INCOMING OPERATOR: Austin
SHIFT SUMMARY:
Literally nothing happened all day.
Locked for close to 40 hours still in observing.
LOG:
TITLE: 11/12 Eve Shift: 00:00-08:00 UTC (16:00-00:00 PST), all times posted in UTC
STATE of H1: Observing at 156Mpc
OUTGOING OPERATOR: Tony
CURRENT ENVIRONMENT:
SEI_ENV state: CALM
Wind: 11mph Gusts, 7mph 5min avg
Primary useism: 0.04 μm/s
Secondary useism: 0.45 μm/s
QUICK SUMMARY:
- H1 has been locked for just under 40 hours
- CDS/SEI/DMs ok
36 hours of Lock reached!
The wind has picked back up to 20mph.
Other than that it's been quiet thus far today.
Sun Nov 12 10:15:27 2023 INFO: Fill completed in 15min 23secs
TITLE: 11/12 Day Shift: 16:00-00:00 UTC (08:00-16:00 PST), all times posted in UTC
STATE of H1: Observing at 158Mpc
OUTGOING OPERATOR: Ryan S
CURRENT ENVIRONMENT:
SEI_ENV state: CALM
Wind: 7mph Gusts, 5mph 5min avg
Primary useism: 0.04 μm/s
Secondary useism: 0.50 μm/s
QUICK SUMMARY:
H1 is locked and observing for almost 32 hours.
Violins look much better thida morning.
The winds died down around 7 hours ago.
Everything looks good for a quiet shift.
TITLE: 11/12 Eve Shift: 00:00-08:00 UTC (16:00-00:00 PST), all times posted in UTC
STATE of H1: Observing at 158Mpc
INCOMING OPERATOR: Ryan S
SHIFT SUMMARY:
- While L1 was down and running an initial alignment, I took the opportunity to adjust the opo temp and SQZ angle, in doing this I was able to squeeze (ha ha) out ~3-4 Mpc, bringing us to 161 Mpc
- 5:11 - inc 5.9 EQ from Papua New Guinea
- 7:04 - SQZr unlocked, then relocked on its own, back to OBSERVE @ 7:08
LOG:
No log for this shift.
H1 just got back into observing after tuning the opo temperature and sqz angle while L1 was down. IFO seems to be stable, locked for 20 hours, and seismic activity looks to be calming down as well.
TITLE: 11/12 Day Shift: 16:00-00:00 UTC (08:00-16:00 PST), all times posted in UTC
STATE of H1: Observing at 154Mpc
INCOMING OPERATOR: Austin
SHIFT SUMMARY:
So far so good, the wind speed has picked up
The PSL Dust mon just hit 300 again on H1:PEM-CS_DUST_PSL101_300NM_PCF
18:13 UTC Dropped out of Observing due to SQZ_MANAGER changed
2023-11-11_08:11:39.133044Z SQZ_MANAGER REQUEST: SQZ_READY_IFO
2023-11-11_08:11:39.133044Z SQZ_MANAGER calculating path: SQZ_READY_IFO->SQZ_READY_IFO
It seems like the SQZ Manager had some sort of issue with the FC-IR unlocked!
Tagging SQZ
18:15 UTC back to Observing
4 tours rolled through the control room, and out to the overpass.
PSL Dum Mon has been alarming all
LOG:
Start Time | System | Name | Location | Lazer_Haz | Task | Time End |
---|---|---|---|---|---|---|
19:38 | Tour | Corey Janos Mike Cassidy + Tours | Control room | N | Standard tours goin to the overpass. | 22:38 |
TITLE: 11/12 Eve Shift: 00:00-08:00 UTC (16:00-00:00 PST), all times posted in UTC
STATE of H1: Observing at 157Mpc
OUTGOING OPERATOR: Tony
CURRENT ENVIRONMENT:
SEI_ENV state: CALM
Wind: 21mph Gusts, 19mph 5min avg
Primary useism: 0.04 μm/s
Secondary useism: 0.51 μm/s
QUICK SUMMARY:
- H1 currently at a 15:45 hour lock
- Wind has been high all day (gusts of 60+ mph!) but are starting to trend downwards
- CDS/DMs ok
Sat Nov 11 10:11:59 2023 INFO: Fill completed in 11min 55secs
TITLE: 11/11 Day Shift: 16:00-00:00 UTC (08:00-16:00 PST), all times posted in UTC
STATE of H1: Observing at 155Mpc
OUTGOING OPERATOR: Ryan S
CURRENT ENVIRONMENT:
SEI_ENV state: CALM
Wind: 26mph Gusts, 19mph 5min avg
Primary useism: 0.09 μm/s
Secondary useism: 0.47 μm/s
QUICK SUMMARY:
Wind Speeds were gusting at over 50mph and we stayed locked!
Winds are still above 25 mph right now, PSL had a dust alarm on dust mon 101 going up and down in that last several hour with a Peak Value of 450 on channel H1:PEM-CS_DUST_PSL101_300NM_PCF
Violins look elevated but not as high as yesterday above 2.e-16 ish