TITLE: 10/17 Day Shift: 1430-2330 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Observing at 148Mpc
INCOMING OPERATOR: Corey
SHIFT SUMMARY:
Lockloss from SQZrs PSAM activity.
https://ldas-jobs.ligo-wa.caltech.edu/~lockloss/index.cgi?event=1413215714
Relocking notes:
I had IMC Locking issues before entering into Initial_Alignment.
And then I had IMC Locking Issues in SR2 Alignment as well making Initial_Alignment incredibly difficult to Get into and Complete.
Sheila asked me to just take the IMC to Offline and wait until the PSL glitches.
Reached Nominal Low Noise at 18:51 UTC
Commissioning activities started with:
More Issues with IMC Locking and Staying Locked.
LOG:
Start Time | System | Name | Location | Lazer_Haz | Task | Time End |
---|---|---|---|---|---|---|
16:36 | SAFE | HAZARD | LVEA | YES | !!!!!LVEA IS LASER HAZARD!!!! | 03:16 |
15:20 | FAC | Kim | Mid X | N | Technical Cleaning | 16:43 |
16:36 | EE | Ferando | CER | N | Getting a USB Back up to a Beckhoff machine | 17:02 |
17:24 | SQZ | Vicki | CtrlRm | N | Removing typo from SQZ_MAN | 17:54 |
19:48 | PSL | Jason | Optics lab | Yes | Working on new NPRO Laser | 23:41 |
20:53 | Health | Camilla & Jeff | Yarm | N | Jogging Y arm | 21:23 |
21:55 | Health | Landry & Rick | Y-arm | N | Walk down the Arms. | 22:25 |
TITLE: 10/17 Eve Shift: 2330-0500 UTC (1630-2200 PST), all times posted in UTC
STATE of H1: Lock Acquisition
OUTGOING OPERATOR: Tony
CURRENT ENVIRONMENT:
SEI_ENV state: CALM
Wind: 14mph Gusts, 7mph 3min avg
Primary useism: 0.03 μm/s
Secondary useism: 0.22 μm/s
QUICK SUMMARY:
Tony was addressing remaining items to allow H1 to get to OBSERVING at the beginning of my shift. Environmentally, it's been windy the last 7hrs and has been slowly getting less windy; microseism is between the 50th & 95th percentile. Jason is working on the spare NPRO in the Optics Lab.
Violin modes are about 2-orders of magnitude quieter than yesterday.
Sheila and I have been investigating the source of the PRCL/DARM coupling that we observe. As a part of this investigation, Sheila has already run two sets of projections that investigate the PRCL coupling to DARM through the other LSC degrees of freedom, and through CHARD P and Y. Those can be found here: alog 80212 and alog 78969.
Today, I took the frequency noise injection from the noise budget, and added that projection to the total. To the point: PRCL coupling to DARM through frequency noise is smaller than PRCL coupling through the other LSC degrees of freedom, therefore it is not a significant source of coupling of PRCL to DARM. Figure 1 shows the projection of PRCL noise to DARM directly, as well as the projection through other degrees of freedom. Figure 2 shows all DOFs projected to DARM.
Some details:
The PRCL and frequency noise injections were rerun as a part of noise budget injections in 80596. The PRCL injection was run while CARM was only on REFL B, to better estimate the PRCL coupling through frequency noise.
The frequency noise injection is run by using REFL A as an out-of-loop sensor with CARM only on REFL B, therefore the frequency noise projection on one sensor will be higher by sqrt(2) in regions where CARM is limited by shot noise. In the past, we've estimated this to be below 4kHz, although we haven't checked recently. The frequency noise projection to DARM in these plots is divided by sqrt(2).
The notebook used to make these plots is located in /ligo/gitcommon/NoiseBudget/simplepyNB/PRCL_frequency_projections.ipynb
TITLE: 10/17 Day Shift: 1430-2330 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Commissioning
CURRENT ENVIRONMENT:
SEI_ENV state: CALM
Wind: 20mph Gusts, 13mph 3min avg
Primary useism: 0.05 μm/s
Secondary useism: 0.23 μm/s
QUICK SUMMARY:
Lockloss from SQZrs PSAM activity.
https://ldas-jobs.ligo-wa.caltech.edu/~lockloss/index.cgi?event=1413215714
Relocking notes:
I had IMC Locking issues before entering into Initial_Alignment.
And then I had IMC Locking Issues in SR2 Alignment as well making Initial_Alignment incredibly difficult to Get into and Complete.
Sheila asked me to just take the IMC to Offline and wait until the PSL glitches stopped so we waited abotu 20 minutes.
Took ISC_LOCK back to down and started a Manual Initial_Alignment @ SR2 Align.
Reached Nominal Low Noise at 18:51 UTC
Commissioning activities started with:
Thu Oct 17 10:18:47 2024 INFO: Fill completed in 18min 42secs
Jordan confirmed a good fill curbside. TCs are looking nominal again.
Vicky, Camilla
Two things to note form this morning's commissioning time before we cause a lockloss while we turned off the new PSAMS filter limit, sorry :(
TITLE: 10/17 Day Shift: 1430-2330 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Observing at 160Mpc
OUTGOING OPERATOR: TJ
CURRENT ENVIRONMENT:
SEI_ENV state: CALM
Wind: 7mph Gusts, 5mph 3min avg
Primary useism: 0.02 μm/s
Secondary useism: 0.20 μm/s
QUICK SUMMARY:
The super moon setting behind the LIGO water tower was majestic as I pulled in to the parking lot today. I should have snapped a picture.
H1 is Observing again for 6 Hours now.
Looks like it was relocked by H1_MAN last night after an Earthquake caused a Lockloss @ 6:29 UTC.
14:50 UTC - SQZ_MAN just dropped us from Observing for a a moment.
14:53 UTC - We are back to Observing.
TITLE: 10/16 Eve Shift: 2330-0500 UTC (1630-2200 PST), all times posted in UTC
STATE of H1: Earthquake
INCOMING OPERATOR: TJ
SHIFT SUMMARY:
With environmental conditions improved (mainly winds dying down), this made for an easier night for H1 and also allowed for slowly damping down the violins to 3xe-18.
LOG:
Recent report from LLO (LLO alog 73576) showed that the test that was sent from LHO to LLO broke because the hard stop was set to the low position and the bobbin/mirror assembly hit the stop hard.
While we were testing our "dirty spare" unit in the EE shop today, however, we have found that the same bobbin/mirror assy can break even when we're quite sure that it didn't hit the stop.
We set up the testing apparatus using the dirty spare FS, a spare driver D1400078 and FAST Shutter test board D1400208. We set the HV to 250V. We made sure that the hard stop was at its highest position.
The first 4 fast shutting motion was good, Fil and Betsy shot the slow-mo video and we are convinced that the bobbin/mirror assy didn't hit the stop. On 5th attempt, while nobody was shooting video, the mirror and a PEEK plate backing broke off and was shot into the air. On a closer inspection we see partial delamination of the glass and PEEK, but it's not like the delamination is the main reason why the PEEK failed. Also a small chunk of the glass was ripped apart from the mirror and left inside the bobbin where the glass was glued to the bobbin and the coil.
Betsy and Fil will post pictures/video later.
Attached is the video of the dirty unit firing CLOSED but before the episode where the mirror broke off. Also a snapshot capturing the frame when the Bobbin assembly (D1003319) was in the most UP/CLOSED position in it's bounce. It does not look like it rammed into the hard stop viton bars.
H1's had a bit of a rough go the last day(s).
Just had a lockloss at LOWNOISE_ESD_ETMX with ASC signals getting noisy over 2-min prior to the lockloss (see attached for a look at the lead-up to the lockloss, with a burst seen on the Error Signals [mainly MICH P & Y] and then the slow ring-up for several ASC channels [with CHARD & CSOFT pitch signals being noticeable culprits]. Additionally, the PR GAIN channel also rung up with ASC.).
For the next lock, I'll pause at MAX POWER to see if this helps, and then watch ASC when stepping through next steps.
(Additionally--around the lockloss there was an earthquake bump (0.03-0.1Hz) around that time, AND we are also riding through increased winds for the last 3hrs...but they seem to be slowly calming down).
Paused for ~1min for the states around where that last lockloss was. Saw no signals ringing up. Eventually made it to NLN. Violins are high (but atleast they are still on nuc30's DARM plot (at 1e-15) and appear to be slowly coming down on nuc31's DCPD scope.
It also should be mentioned, environmentally, no earthquakes and the winds have drastically calmed down in the last 30min. (But really all the environmental noisiness does not seem too crazy or bad....so perhaps H1, for some reason, is more susceptible/sensitive to seismic noise?)
TITLE: 10/16 Eve Shift: 2330-0500 UTC (1630-2200 PST), all times posted in UTC
STATE of H1: Earthquake
OUTGOING OPERATOR: Tony
CURRENT ENVIRONMENT:
SEI_ENV state: CALM
Wind: 23mph Gusts, 13mph 3min avg
Primary useism: 0.07 μm/s
Secondary useism: 0.21 μm/s
QUICK SUMMARY:
Walked in to Tony locking H1 at PRMI and he just left as it was on its way to MAX POWER. (The DRMI lock & ASC step were a bit odd with POP18+90 making several sharp drops....but it obviously made it through that rollercoaster.)
Several EQs over last 24hrs; useism is squarely between the 50th & 90th percentile lines; winds had been elevated the last 2hrs, but appear to be dropping.
TITLE: 10/16 Day Shift: 1430-2330 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Earthquake
INCOMING OPERATOR: Corey
SHIFT SUMMARY:
Found out why the Violins were being rung up.
Tj was right it was a settings issue, The coil drivers were cranked up to state 3.
After this was resolved:
16:55 UTC OMC_whitening, Can't get to NLN noise, violins too high for Whitening, Damping Violins.
17:43 UTC UTC Nominal_LOW_NOISE was reached! yay!
17:46UTC reached Observing!!!
18:05 UTC lockloss
https://ldas-jobs.ligo-wa.caltech.edu/~lockloss/index.cgi?event=1413137125
NLN reached at 21:17:10 UTC Yay!!!
Lockloss 21:18:19 UTC
https://ldas-jobs.ligo-wa.caltech.edu/~lockloss/index.cgi?event=1413148718
I noticed an IMC Fault.
I Believe this lockloss may have been caused by the FSS glitches.
A lockloss that was caused by a 35+MPH wind gust while we were in LOWNOISE_COILDRIVER[552]
https://ldas-jobs.ligo-wa.caltech.edu/~lockloss/index.cgi?event=1413152106
TLDR: Day full of small Earthquakes, a wind gust and Some PSL FSS glitches meant that I had short locks today. One of which was only 1 minute long.
LOG:
Start Time | System | Name | Location | Lazer_Haz | Task | Time End |
---|---|---|---|---|---|---|
16:36 | SAFE | HAZARD | LVEA | YES | !!!!!LVEA IS LASER HAZARD!!!! | 03:16 |
14:55 | FAC | Karen | Optics lab & Vac | No | technical cleaning | 15:49 |
16:13 | EE | Josh & Marc | Mid Y | N | trading parts | 17:19 |
19:44 | PCAL | Rick | PCAL Lab | yes | Returning parts | 20:40 |
TITLE: 10/16 Day Shift: 1430-2330 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Earthquake
CURRENT ENVIRONMENT:
SEI_ENV state: EARTHQUAKE
Wind: 6mph Gusts, 3mph 3min avg
Primary useism: 0.93 μm/s
Secondary useism: 1.11 μm/s
QUICK SUMMARY:
16:55 UTC OMC_whitening, Can't get to NLN noise, violins too high for Whitening, Damping Violins.
17:43 UTC UTC Nominal_LOW_NOISE
17:46UTC reached Observing!!!
18:05 UTC Earthquake lockloss
https://ldas-jobs.ligo-wa.caltech.edu/~lockloss/index.cgi?event=1413137125
While trying to relock another earthquake struck.
Also Initial Alignment is acting strange in SRC_Align Offloaded, Sheila and I will work on this once the Quake passes.
Holding in IDLE.
Last done in April 2024.
plots for reference, 1412435458.png, HWS_aborbs.png
Using /ligo/gitcommon/labutils/hws_absorption_fit/april2024/fit_absprtion_v2.py with lockloss time 1412435458, edited P_y and P_x values to adjust the fit.
ITMX: 155mW absorbed = 398ppb (155mW / 389kW)
ITMY: 140mW absorbed = 360ppb (140mW / 389kW)
April 2022 (62468, 62782) | Nov 2022 (66036) | April 2023 (71400) | April 2024 | October 2024 | |
ITMX | 430ppb | 490ppb | 475ppb | 430ppb |
398ppb |
ITMY | 370ppb | 385ppb | 375ppb | 330ppb |
360ppb |
Overnight the ITMX coil driver states were wrong, causing the ASC controls to satuate the PUM durring acquisition. (This become aparent when the DHARD gains are increased at the end of DHARD WFS, which happens right before PARK_ALS_VCO 80699)
This used to be reset in ISC_LOCK PREP_FOR_LOCKING state, this has been commented out (line 618), with a note that SDF will take care of this, this has been commented out in the guardian for over a year. Indeed. we found that the coil driver state was incorrectly set to 3
The attached screenshot shows the error was introduced to the safe.snap sometime between 2:30 and 5 pm yesterday, as it was correctly reset in the first two locking attempts of the day, but wasn't correctly reset after the lockloss at 5 local time last night.
Erik, EJ, Dave:
We found that h1susitmx's safe.snap file was truncated from 2265 lines to 1336 lines (last 929 lines removed) at 14:47 Tue 15oct2024. This truncated file was loaded into the model at 17:09 Tue. The BIO STATEREQ channels were in the missing block, and so were not restored to val=2 until the safe.snap file was fixed Wed 09:20.
Ibrahim, Oli
Below are updates and promising findings concerning the most recent BBSS LHO Top Mass -4mm BP Adjustments to tackle the F1 Drift issue summarized in alog 80577.
On Friday 10/11, Oli P and I moved the blade positions (mm BP Units) to:
Front Left: Side: 0.02, Top: -4.03 Back Left: Side: -0.03, Top -3.90 Front Right: Side: 0.02, -3.91 Back Right: Side: -0.05, -3.95 Avg: Side: -0.01 Height: -3.95
Find:
The good news is that with these 4.5 days of Data, we see no sign of F1 Drift.
We will post another alog with TF to model comparisons as we find which model d1 parameter fits these -4mm BP positions best.
That's good news! What is the configuration for the addable masses on the top mass for both the bottom and top plate?
The Addable Masses on the top plate were redistributed to the Front (top). 150g and 150g as shown in the attached image. No change to the bottom plate. We did not change the total mass.
Adding this Pitch Plot (which still shows no drift!) to give a measure of how much the diurnal moves day-to-day. Plot attached shows a max of 31.8 cts trough to peak max.
This is such that future drift measurements (e.g. at LLO) can try new configurations quickly and measure the prevailing drift without getting caught in the daily pitch breathing error.
Gerardo, Janos Reacting to the issue in aLog https://alog.ligo-wa.caltech.edu/aLOG/index.php?callRep=80619, the GV10 AIP was swapped, as the pump broke down. The AIP was swapped with a noble diode pump, as a lesson learnt from the latest AIP swap: https://alog.ligo-wa.caltech.edu/aLOG/index.php?callRep=80411. The only difficulty was after swapping the pump and then pumping on the Annulus line, the old Varian controller did not work (the reason for its malfunction is now supposedly diagnosed), and so now the Ion pump runs with an Agilent IPC Mini controller. The downside of this is that the wiring of its data cable is not compatible with the current CDS setup, and therefore on the MEDM screen the AIP still appears as faulty - see picture attached. The controller will be replaced shortly, after the Varian controller is fixed. Until then, the Agilent controller will be periodically checked. Nevertheless, the Noble-diode pump proved to be an excellent choice again, as it pumped the Annulus volume down pretty quickly (in about 7 minutes) below 1E-6 Torr.
Gerardo replaced the IPC Mini controller with a Varian controller back on yesterday, so now the MEDM screen is also clear.
A slow motion video of the fast shutter, firing with the high voltage driver in air, is here: slow motion video
Sheila's original video is ~2sec footage of fast shutter, supposedly at 150 fps according to the file metadata.
Attached is an edited video that shows the 50ms of FS action slowed down by a factor of 10. "SRC TC" is the time elapsed since the start of (Sheila's original) video multiplied by a factor of 10, i.e. 1 sec in SRC TC is actually 100ms. This timestamp is not to be trusted at the lowest digit of sub-second (ms level in reality) because there's some frame interpolation going on due to mismatch between the standard output frame rate of 24FPS VS the source frame rate (150 slowed down to 15 FPS). Anyway, the mirror goes down lower than the closed position right after the initial thrust of the HV fast shutter motion, and even a few bounces after that, before the shutter eventually settles to the permanently closed position.
Also attached is an annotated png file of four frames ("Open", "HV thrust", "Bounce to the bottom" and "Close").
In light of recent failure of the replacement FS at LLO where the mirror broke off due to the hard stops that were set too low, and a comment by Rich (LLO alog 73584) I watched the video of the LHO unit again (see my entry above).
Though LHO video was shot from the side where we cannot see the position of the hard stop, the bobbin might be hitting the stops right after the launch even though the height of the stops looks good to my eyes. See TC~00:00:05:06. And the bobbing oscillates several times though it never hits the stops again.
Does this mean that the magnetic braking is too weak?