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Reports until 13:17, Monday 27 October 2025
H1 General
ryan.short@LIGO.ORG - posted 13:17, Monday 27 October 2025 (87771)
Ops Day Mid-Shift Report

H1 returned to observing at 19:54 UTC after a fairly strightforward relocking process. DRMI took a while to catch, but once it did, we paused to take a few OLG measurements (alog87768).

The 1 HZ ASC ringup started right around reaching low noise. Elenna tried a couple things to mitigate it, but we eventually just transitioned to high-gain ASC to finally subdue it.

I had one SDF to accept (see screenshot) which appears to be from Tony's SQZ troubleshooting overnight (alog87760).

Images attached to this report
H1 PSL
ryan.short@LIGO.ORG - posted 12:35, Monday 27 October 2025 (87770)
PSL 10-Day Trends

FAMIS 31109

PMC TRANS is having a bit of increase again, but otherwise no major events this week. I adjusted the ISS RefSignal this morning to bring the diffracted power back to our target of 4%; something I've been meaning to do for a while.

Images attached to this report
H1 ISC
elenna.capote@LIGO.ORG - posted 12:25, Monday 27 October 2025 - last comment - 15:02, Friday 21 November 2025(87768)
DRMI Inventory log

Some DRMI locking info

MICH, PRCL, SRCL filter banks during the "acquire DRMI 1f" state before the lock is grabbed.

OLGs for MICH, PRCL, SRCL after 1F acquisition, DRMI ASC engaged.

 

Images attached to this report
Comments related to this report
elenna.capote@LIGO.ORG - 14:51, Tuesday 28 October 2025 (87807)

MICH, PRCL, SRCL filter banks when DRMI 1F is locked, settings for the measurement time above.

Images attached to this comment
elenna.capote@LIGO.ORG - 15:02, Friday 21 November 2025 (88199)

PRMI OLGs

Images attached to this comment
LHO VE
david.barker@LIGO.ORG - posted 10:59, Monday 27 October 2025 (87769)
Mon CP1 Fill

Mon Oct 27 10:10:35 2025 INFO: Fill completed in 10min 32secs

 

Images attached to this report
H1 ISC
jennifer.wright@LIGO.ORG - posted 10:58, Monday 27 October 2025 (87766)
Change of reflected power from OMC during DARM offset step

I made plots of anti-symmetric power P_AS vs. power at reflected port of OMC P_OMC_REFL during the DARM offset step measurement on September 4th, (see LHO alog #86785 and 87629).

I had to use the Beckhoff reported power for this (H1:OMC-REFL_A_DC_POWER) as the front-end channel is calibrated wrongly (see LHO alog #87648).

I also plotted the P_OMC_REFL vs.  P_DCPD, ie. reflected vs. transmitted power for the OMC.

The plots for our two measurements taken at different times during IFO thermalisation are below, both were taken when OM2 was hot.

Non-image files attached to this report
X1 SUS
ibrahim.abouelfettouh@LIGO.ORG - posted 10:50, Monday 27 October 2025 (87767)
LHO Dummy Prism Position Measurement (glass test build vs. metal)

Ibrahim, TJ O'Hanlon

There was question about where the prism position was with respect to the nominal position (known to be 2.6775mm from the cetner line as figure 1 shows).

As it turns out, measuring from the scribe line of the center of the dummy test mass, yields an "dummy mass upside down" answer that has confused us (LLO Measurement). However, using the scribe on the glued tooling that we used to determine the secondary prism location resulted in the correct value ~2.73mm. While all these are rough measurements, I wanted to check if LLO's upside-down metal-prism version is equivalent to LHO's scribe-on-prism tooling glued-on version. For the LLO comparison, I used the metal prism build dimensions from D1900580. According to a scale-comparison (using line lengths ratios), they are at least comparable (Figure 2).

TJ agrees that the the scribe line I'm using, which was on D2400027 (also screenshotted below) and says "our prisms are in the same place but you are measuring off of the scribe line off the D24000247 while I am looking at the center round mass. The center round mass scribleline would match with d24000247 if it wasn't flipped".

Meaning LHO and LLO prisms are in the same spots but that the dummy scribe line is not to be trusted. That spot also matches (with at least +-1 mm error until measured more accurately) the 2.67mm nominal value.

I've attached some pictures of the measurement.

Images attached to this report
H1 ISC
elenna.capote@LIGO.ORG - posted 10:13, Monday 27 October 2025 (87762)
LSC OLGs

I don't have a sense of what exactly the problem is yet, but last week's adventure taught us that this 1 Hz instability is related to the gain of SRCL just as much as it is related to the DHARD, CHARD and CSOFT gains. I checked the SRCL UGF today when we reached NLN and it was at 10.5 Hz, which seems low even by these standards.

I have increased the SRCL gain by 3 dB (-7.5 to -10.5) which brings the UGF to 15 Hz.

I remeasured the MICH OLG, and it's still around 5.5 Hz, which is as Evan designed.

PRCL UGF is back to 50 Hz; we made this change in June.

Guardian and SDF updated.

Images attached to this report
H1 TCS
thomas.shaffer@LIGO.ORG - posted 10:11, Monday 27 October 2025 (87763)
TCS pipe expansion joint leak barrier added

This is a late alog, but I wanted to put it in to document. In July, Randy installed an acrylic barrier on the pipe bridge that would block any spray from a failed cooling line expansion joint from spraying onto squeezer electronics racks or optics tables. Associated FRS30283 

Images attached to this report
LHO General (Lockloss)
ryan.short@LIGO.ORG - posted 07:42, Monday 27 October 2025 - last comment - 10:16, Monday 27 October 2025(87761)
Ops Day Shift Start

TITLE: 10/27 Day Shift: 1430-2330 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Earthquake
OUTGOING OPERATOR: Tony
CURRENT ENVIRONMENT:
    SEI_ENV state: EARTHQUAKE
    Wind: 10mph Gusts, 7mph 3min avg
    Primary useism: 0.19 μm/s
    Secondary useism: 0.26 μm/s 
QUICK SUMMARY: H1 lost lock at 12:48 UTC after spedning almost 16 hours locked from a M6.5 EQ out of the Caribbean. Still in EQ mode, so will start relocking once ground motion calms down.

Comments related to this report
ryan.short@LIGO.ORG - 10:16, Monday 27 October 2025 (87764)Lockloss

H1 back to NLN at 16:57 UTC.

Ran in initial alignment then set to relocking automatically. Paused in a couple of places on the way up for Elenna to make some ASC measurements, now starting some commissioning activities which are slated to be wrapped up by 18:30 UTC.

And of course as soon as I'm about to post this, lockloss @ 17:14 UTC from what looks like an ETM glitch.

H1 SQZ (SQZ)
anthony.sanchez@LIGO.ORG - posted 04:03, Monday 27 October 2025 - last comment - 10:30, Monday 27 October 2025(87760)
Incoherent Ramblings from the AM

At [?] in the morning H1 was Found Locked but SQZ_Man was upset.
SQZ_Man stuck in loop from Beam Div_Open_FRS ->FC_WAIT _FS. 

SHG H1:SQZ-SHG_TEC_SETTEMP was adjusted down to maximixe H1:SQZ-SHG_GR_DC_POWERMON

still stuck in loop

Ran the noconda python switch_nom_sqz_states.py without script
....UH.... Broke all the SQZr Gaurdians.... Ooops
Ran the noconda python switch_nom_sqz_states.py with script
Taking SQZ_man to no_squeezing
Ran the noconda python switch_nom_sqz_states.py without script.... again
Nothing broke !!! But Still cannot get to observing.
Had to manually take SQZ_ SHG to Down. 
Back to Observing. Range only at 133 Mpc

 

Comments related to this report
sheila.dwyer@LIGO.ORG - 10:30, Monday 27 October 2025 (87765)

The problem was that the OPO pump ISS was running out of range, as the OPO reflected power has slowly been increasing since our last crystal move.  I've adjusted the wave plate on SQZT0 to allow more green power to be launched, this now gives a control mon of about 5 when the OPO transmission is 80 uW.  

 

LHO General
corey.gray@LIGO.ORG - posted 22:00, Sunday 26 October 2025 (87759)
Sun EVE Ops Summary

TITLE: 10/26 Eve Shift: 2330-0500 UTC (1630-2200 PST), all times posted in UTC
STATE of H1: Observing at 150Mpc
INCOMING OPERATOR: Tony
SHIFT SUMMARY:

H1's been locked 8+hrs & microseism continues to fall (almost touching 50th percentile line) and winds are calm.
LOG:  n/a

H1 AOS (DetChar)
robert.schofield@LIGO.ORG - posted 17:31, Sunday 26 October 2025 (87758)
Update on the search for the site of non-linear vibration coupling in the LVEA

Summary

I found vibration coupling associated with motion of the HAM4 ISI (at a few times background),  BSC2 ST2 motion (at about 10 times background), and, likely, on the chamber walls of the ITMs (accounting for much of DARM in the 20 Hz region). The coupling associated with HAM4 may be due to reflection of the 45 degree annular beams from the BS and its cage, and may be mitigated by BBS installation and table baffles at HAM4. The coupling at the chamber walls of the ITMs may be due to the 20 degree annular beam from the ITM bevels, which would be mitigated by installation of cage baffles on the ITMs. However,  I would like some more commissionsing time to be more sure of this.

Recently, broad-band non-linear vibration coupling in the corner station was revealed by investigations of the coupling of HVAC components to DARM (86412). This is an update on searches for the site of that coupling. 

We check for sites on the internal tables (ISIs) by shaking individual ISIs or HPIs. Discriminating between sites on the vacuum enclosure is more difficult because shaking at one location tends to shake many vacuum chambers about the same amount. To identify an enclosure site, we use frequency dependance and  propagation delays (velocities on these steel membranes are only 100s of m/s). The basic idea is that if a patch of chamber wall is producing noise by reflecting scattered light back into the interferometer, then an accelerometer that is placed on the outside of that patch will, comapared to other accelerometers, produce a signal that is  precisely correlated with the signal in DARM.

Internal tables

I eliminated most of the tables in the LVEA either by injecting into the ISI control loops or by monitoring their motion during external injections. However, I did find coupling at the HAM4 ISI and the BS ISI.

Coupling at HAM4 ISI

Figure 1 shows that we found coupling at the HAM4 ISI. An increase in Y-axis motion of about 30 produced a feature in DARM that was several times background. This coupling appeared mainly linear and so was not the coupling we were looking for. A potential source of this coupling is reflection of the 45 degree annular beam from the beamsplitter that illuminates this table (83050). The BBS, its less reflective cage and planned table baffling may mitigate this coupling.

Coupling with motion of ST2 of the BS ISI

Figure 2 shows that I produced noise in DARM by shaking the BS ISI.  I did a series of injections that suggest that noise in DARM is produced by motion of BS ISI ST2 (where the cage is attached), but not motion of ST0  (where the eliptical baffles are attached) or of the BS itself.  This noise may be associated with the 45 degree annular beam from the BS (83050) and may be reduced with the new BBS cage, which is less reflective.

Vacuum enclosure

I have been using three techniques to find coupling sites on the inside walls of the vacuum enclosure. These tests, while ongoing, have narrowed down the non-linear coupling to the enclosure walls in the vertex.

1) Shaker and speaker sweeps from multiple locations

Shaker sweeps are used in two ways. First, frequency consistency - if an accelerometer is mounted at the coupling site, and shows a resonance at some frequency, then there should be an indication of greater motion in DARM at that frequency also. Second, consistency for vibration injections from multiple locations. Thus if the accelerometer is mounted at the coupling site, and it moves less for injections onto the mode cleaner tube than onto BSC8, then DARM should also be less affected by the SR tube injection. Figure 3 illustrates this for one of the sweep pairs.

The most consistent accelerometer locations in frequency:  ITMX, ITMY and BS chamber walls

The most consistent accelerometer locations in response to different shaker locations: ITMX, ITMY and BS chamber walls

2) Beating shakers technique

The Beating Shaker technique (52184) uses differences in propagation time from different shaker locations to locate the coupling site. When two shakers inject at two slightly different frequencies (e.g. 35.005 Hz and 35 Hz), the beat envelope will have a different phase at different locations due to propagation delays. If the accelerometer is at the coupling site, its beat enveope will be in phase with DARM’s for any shaking location.

The beat envelope in DARM was not as clear as it has been for past uses of the Beating Shaker technique, because of the side bands. So I fit a simulated beat envelope using a cross correlation technique. This is illustrated in Figure 4.  The best accelerometers for beat consistency were ITMY–Y, ITMY-X and ITMX-Z. I think it might be useful for DetChar or others to search for an ASC motion that could account for the side bands during the injection period shown in Figure 4.

3) Hand held mini-shaker

A small shaker made of a speaker with an attached reaction mass (Figure 5) is used to take advantage of the large amplitude near-field region right at the shaker in an attempt to find a region on the vacuum enclosure where the shaker coupling dramatically increases. This technique eliminated the BSC7 potential sites and I hope to use it to test the 20 degree ITM  beam hypothesis in future commissioning sessions.

 

Since our accelerometer array has low spatial resolution (something to think about for CE) we also mount temporary accelerometers as we narrow in on a site. This is the stage I am at, mounting accelerometers to further narrow the site. However, the results so far are consistent with coupling of the 20 degree beam from the ITM bevels (83050) . These annular beams were elimited by the cage baffles at LLO and we plan on installing them at LHO.

 

Non-image files attached to this report
LHO General
corey.gray@LIGO.ORG - posted 16:59, Sunday 26 October 2025 (87757)
Sun EVE Ops Transition

TITLE: 10/26 Eve Shift: 2330-0500 UTC (1630-2200 PST), all times posted in UTC
STATE of H1: Observing at 151Mpc
OUTGOING OPERATOR: Ryan S
CURRENT ENVIRONMENT:
    SEI_ENV state: CALM
    Wind: 13mph Gusts, 7mph 3min avg
    Primary useism: 0.03 μm/s
    Secondary useism: 0.30 μm/s 
QUICK SUMMARY:

H1's been locked just over 3hrs with range hovering arouind 154Mpc.

In the last 14hrs, microseism has steadily been dropping off the 90th percentile line.  Winds are calm-ish for the last 8-ish hours.

LHO General
ryan.short@LIGO.ORG - posted 16:33, Sunday 26 October 2025 (87756)
Ops Day Shift Summary

TITLE: 10/26 Day Shift: 1430-2330 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Observing at 153Mpc
INCOMING OPERATOR: Corey
SHIFT SUMMARY: Two lock acquisitions today, both of which had locklosses during TRANSITION_FROM_ETMX on the first try. This made the relocking times a bit longer, but generally the process was automatic. H1 has been locked for 2.5 hours.

H1 General (ISC, OpsInfo, SUS)
ryan.short@LIGO.ORG - posted 16:27, Sunday 26 October 2025 (87755)
Summary of H1 Locking Troubles and Changes for the Week of Oct. 20th-25th

Now that we're back to observing with regularity after a week full of intense troubleshooting, I decided it would be nice to have a summary of the events that contributed to IFO locking issues in the past week and what was done along the way to fix them all in one place, so that's what I'll attempt do in this alog. Anyone should be encouraged to add comments with things I missed or additional commentary. Things I believe to be the most significant changes either contributing to or fixing IFO locking issues I've bolded.

H1 General (Lockloss)
ryan.short@LIGO.ORG - posted 12:40, Sunday 26 October 2025 - last comment - 14:40, Sunday 26 October 2025(87753)
Lockloss @ 18:54 UTC

Lockloss @ 18:54 UTC after 1:41 locked - link to lockloss tool

No obvious cause, but I did see a couple glitches in the PRG a few seconds before the lockloss.

Comments related to this report
ryan.short@LIGO.ORG - 14:40, Sunday 26 October 2025 (87754)

Back to observing at 20:59 UTC.

Had another lockloss during TRANSITION_FROM_ETMX so relocking took a bit longer than usual. Fully automatic otherwise, except for some touchup of PRM I did during DRMI acquisition.

H1 PSL
ryan.short@LIGO.ORG - posted 11:44, Sunday 26 October 2025 (87752)
PSL Status Report - Weekly

FAMIS 27400

Laser Status:
    NPRO output power is 1.858W
    AMP1 output power is 70.71W
    AMP2 output power is 140.2W
    NPRO watchdog is GREEN
    AMP1 watchdog is GREEN
    AMP2 watchdog is GREEN
    PDWD watchdog is GREEN

PMC:
    It has been locked 33 days, 0 hr 29 minutes
    Reflected power = 25.05W
    Transmitted power = 106.7W
    PowerSum = 131.8W

FSS:
    It has been locked for 0 days 2 hr and 11 min
    TPD[V] = 0.5278V

ISS:
    The diffracted power is around 3.4%
    Last saturation event was 0 days 3 hours and 41 minutes ago


Possible Issues:
    PMC reflected power is high

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