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Reports until 11:59, Wednesday 28 May 2025
H1 SUS (ISC)
jeffrey.kissel@LIGO.ORG - posted 11:59, Wednesday 28 May 2025 (84631)
More PRMI Glitches, This Time More Obviously Optical Lever Glitches
J. Kissel, S. Dwyer

As opposed to the ''glitch'' I reported this morning (LHO:84622) which was while the IFO was configured in PRX and ISC loops created a large pitch excursion with M1 drive of the H1SUSBS. We're now seeing stuff that is much more "classic optical lever glitching" with the IFO configured in PRMI, with MICH ASC engaged. See attached. This is after Sheila/Camilla increased the current in the BS oplev laser this morning (LHO:84616)

As a reminder, Beam Splitter optical lever loops are only used in PRMI / DRMI until MICH ASC is turned on. The transition happens in the ISC_DRMI guardian, in the "ENGAGE_DRMI_ASC" (index 80) state; the gain in the ASC-MICH banks are ramped ON in 2 seconds, and the gain in SUS-BS_M2_OLDAMP banks are ramped off with a 20 sec ramp (i.e. it's not that the inputs or outputs are switched on or off).

So, beam splitter optical lever glitching had been particularly painful in the past few days when working in PRMI and/or DRMI without the corner ASC loops on. But, now that we've found a good alignment, and fixed the REFLAIR phase (LHO:84630) we're able to quickly transition to using DRMI ASC, and become insensitive to the optical lever performance -- which continues to glitch.
Images attached to this report
H1 ISC
sheila.dwyer@LIGO.ORG - posted 11:48, Wednesday 28 May 2025 (84630)
phasing REFLAIR 45 changes PRCL loop gain in PRMI

Following up on Jennie's PRCL OLG measurements yesterday, 84604, I checked the phasing of REFLAIR 45 (the MICH sensor) while PRMI was locked. I used a template in userapps/lsc/h1/templates/phase_REFLAIR.xml, but had to turn the PRM excitation down to 300 counts. 

THe first attachment shows that improving this phase improved the shape of the PRCL loop.  This has probably been not phased well for a while, not as a result of the vent. 

I also adjusted the phase of REFLAIR 9, SDFs attached.

 

Images attached to this report
LHO VE
david.barker@LIGO.ORG - posted 11:16, Wednesday 28 May 2025 - last comment - 11:25, Wednesday 28 May 2025(84625)
Wed CP1 Fill

Wed May 28 10:15:55 2025 INFO: Fill completed in 15min 51secs

 

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david.barker@LIGO.ORG - 11:25, Wednesday 28 May 2025 (84626)

Yesterday the TCs were staying cold mid-afternoon. I found an ice ball had built up around the discharge line exit. I broke it off and pulled the tumble weed it was attached to out of the way.

Images attached to this comment
H1 ISC
elenna.capote@LIGO.ORG - posted 10:51, Wednesday 28 May 2025 (84623)
DC centering on REFL loop changes

Oli, Elenna

The DC1 and DC2 centering loops have seemed to be way too slow, so Oli and I took some transfer functions of the centering loops. We started with DC2 Y, and the loop didn't even seem to have a UGF. By looking at the phase, Oli and I determined that we could raise the loop gain to get a UGF of about 0.5 Hz with a phase margin of 38 degrees. This involved raising the gain from -0.1 to -8.

The DC1 and 2 yaw loops have the same design and feedback to the same suspensions, so we copied over the gain change and ran a quick OLG to confirm the result is the same.

DC1 and DC2 pitch also have the same design. The low pass filter in use in pitch cuts off at 0.7 Hz instead of 1.5 Hz like the yaw loops, so there was much less phase margin. Oli and I copied over the butterworth low pass at 1.5 Hz in the yaw loops to the pitch loops and found that raising the gain from -0.1 to -7 gave the desired 0.5 Hz UGF.

All four loops have been measured using the templates in [userapps]/asc/h1/templates/DC_centering and saved. I have attached screenshots of DC2 Y and DC1 P. We SDFed these changes.

We copied over the DC1/2 design to DC6 yesterday, so Oli and I also updated the low pass filter in DC6 P to match and SDFed. The gain of DC6 P and Y still needs to be checked.

As a final note, we lowered the bandwidth of these loops just before O4 to avoid noise reinjection into CHARD, so we should check how this higher bandwidth impacts the noise in CHARD at a later date.

Images attached to this report
H1 SUS
jeffrey.kissel@LIGO.ORG - posted 10:49, Wednesday 28 May 2025 - last comment - 11:05, Wednesday 28 May 2025(84622)
This Morning's Beam Splitter Excursion; Glitches and ISC Excursion
J. Kissel, S. Dwyer, others

Just so others can see what we're seeing, here's the glitch at 2025-05-28 15:36 UTC that drove us to swap the F1/F2/F3/LF Triple Top coil driver on the H1SUSBS. 

Everything's wrapped in loops, so it's difficult to point fingers at any one component.
ISI is in FULLY_ISOLATED_NO_ST2_BOOST per normal for MICH lock acquisition
SUS has 
    - M1 OSEM PD to M1 OSEM Coil damping loops ON (L, T, V, R, P, Y)
    - M3 Oplev QPD to M2 OSEM Coil damping loops ON (P and Y)
The IFO was attempting to lock PRX.
This is unexpected, but apparently there's also some slow ISC loop that is really causing the majority of the alignment excursion.

Will keep investigating other times to see if this is a consistent issue. 
We've looked at a few other times where we suspect optical lever glitching, but the same ISC loops were not on.
Difficult to trend the configuration of the ISC loops at the moment, 'cause folks are trying lots of different configurations to get DRMI relocked.

We'll post if we find an answer.

We swapped the coil driver because the "glitch" showed up "most" in the F1 sensor, and we feared it was something like we've seen in the past -- SR3 top mass coil driver failures that took us a long time to find (see LHO:62038 and LHO:62123).
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filiberto.clara@LIGO.ORG - 11:05, Wednesday 28 May 2025 (84624)

Chassis Removed: S1100194
Chassis Installed: S1001086

X1 DTS
joshua.freed@LIGO.ORG - posted 10:43, Wednesday 28 May 2025 - last comment - 14:17, Thursday 29 May 2025(84621)
Double Mixer Amplifier Choise

J. Freed

The reason we picked the ZFL-500HLN amp for SPI's Double Mixer was that it was an amp that met requirements from minicircuts

-frequency range contains 80MHz (our operating frequency)

-Operates at voltage supplied by Low Noise Power(15V, 17V, 24V etc.)

-Has a P1dB well above our output power of 10dBm (to remove non-linearity)

-No heat sinks (to fit in a 1U chassis.) (This requirement actually doesnt matter, the ones discussed here are still the best even compaired to amps with heat sinks)

-sma connections

-Low noise

-Low gain (we only need ~8dB of amplification)

The ZFL-500HLN was chosen because it fit all those requirements, with the cavieat of having to attuniate before amplification (adding noise). Though if I am correct and the Low noise power board 5V Vcc port is capable of supporting a 63mA load, another option would be the ZX60-P105LN+ instead due to the lower gain and lower noise. This would remove the need for an attinuator before amplification but its low input return loss means alot of power is reflected back towards our mixers (Also causeing noise). So it becomes a pick your poison of adding noise by attinuating before amplification vs by reflections back into our mixers. In practice, I believe both would operate about the same. Will add a comment if something changes

Double-MixerAmpComparison.png shows a quick comparison of the 2 amps

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joshua.freed@LIGO.ORG - 14:17, Thursday 29 May 2025 (84656)

Acording to this term definitions manual I found on minicircuts: 

"Directivity (active) is defined as the difference between isolation and forward gain in dB. It is an indication of the isolation of the source from the load, or how much the load impedance affects the input impedance and the source impedance affects the output impedance. The higher the active directivity (in dB), the better the isolation."

So directivity is just a measure of Isolation - Gain. Which isolation is just a measure of how much power is sent through the amp to the input port with power applied on the output. This would really only affect the amp when there is a large impedance mismatch on the output (load). If there is little to none, directivity doesnt really matter. But if it did come up, the ZFL-500HLN would do much better. The greater concern I believe for the ZX60-P105LN+ is the large input return loss, which is the power of the reflections off of the ports back the way it came. This would cause a standing wave on our input. To reduce it, we would have to add an attinuator on the input anyway. Probably less than the 10 dB attinuator which we currently have, but still something to consider. 

P.S. VSWR and Return Loss(RL) are the same thing with different units, the conversion between them is VSWRvsRL.png. A VSWR closer to 1 is better, while a higher return loss is better. Converting the  ZFL-500HLN aproximate 1.04:1 VSWR to Return loss gives 34.15dB. This means the reflections power are about 20dB greater on the ZX60-P105LN+. Really not sure if it is worth it excpecilly since mixers are sensitive to these reflections.

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H1 SUS (ISC)
jeffrey.kissel@LIGO.ORG - posted 09:51, Wednesday 28 May 2025 - last comment - 11:41, Wednesday 28 May 2025(84620)
H1 SUS BS M3 to M2 Oplev Damping Loops' Impulse Response
J. Kissel

As we begin to investigate transient issues with the Beam Splitter where its sensors are reporting intermittent glitching that is spoiling DRMI locking, the optical lever damping loops are always an open question for me. 

Here's the impulse response of the filters, shown both as a normal time-series, which shows that most of the action happens within the first 0.2 seconds. I also show a semilogx plot of the time series to show the early magnitude of the response.

Finally, I attach a screenshot of which filters are on.
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jeffrey.kissel@LIGO.ORG - 11:41, Wednesday 28 May 2025 (84628)
Here's the frequency response of the filters via Bode Plot.
Again the EPICs gain applied to these filters is 300x and 650x for pitch and yaw, respectively.
Images attached to this comment
H1 SUS (ISC)
camilla.compton@LIGO.ORG - posted 08:54, Wednesday 28 May 2025 - last comment - 09:32, Wednesday 28 May 2025(84616)
BS Oplev Laser Current Increased

Sheila, Camilla

As we've had trouble catching PRMI, and there is some signs of the BS oplev laser glitching, see attached. We turned up the laser current so that the Oplev NSUM counts increased from 16,000 to 20,000. BS Oplev laser is in the cooler behind the HWS table / TCSX rack.

Images attached to this report
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camilla.compton@LIGO.ORG - 09:32, Wednesday 28 May 2025 (84619)

Attached is a plot where we believe we see a glitch in the top mass osems (largest in F1) and a different type of glitch in the Oplev NSUM (after current increased).

Images attached to this comment
H1 General
anthony.sanchez@LIGO.ORG - posted 07:58, Wednesday 28 May 2025 (84615)
Wednesday ops day shifty start

TITLE: 05/28 Day Shift: 1430-2330 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Planned Engineering
CURRENT ENVIRONMENT:
    SEI_ENV state: CALM
    Wind: 5mph Gusts, 0mph 3min avg
    Primary useism: 0.13 μm/s
    Secondary useism: 0.10 μm/s
QUICK SUMMARY:

H1 currently in ready state.
Seimic system back to calm after a few earthquake.
I got ALS Locked after touching up Y arm.
I'm going to Try to get DRMI locked for the Comissioners, before they arrive. Im going to try once with out a Full Initial Alignment first and then run an initial alignment since the alog 84610 has it in bold, perhaps I should try it.
 

LHO General (OpsInfo)
ryan.short@LIGO.ORG - posted 22:53, Tuesday 27 May 2025 (84613)
Ops Eve Shift Summary

TITLE: 05/28 Eve Shift: 2330-0500 UTC (1630-2200 PST), all times posted in UTC
STATE of H1: Planned Engineering
INCOMING OPERATOR: None
SHIFT SUMMARY: More progress this evening with H1 locking! We've been able to reach 'RESONANCE' and set the green references there, but DRMI/PRMI locking has continued to be a struggle where flashes will look good, but it will not lock for a long time for some reason. See other logs, mainly alog84610, for details.

As Elenna mentions in her log, first thing in the morning a FULL initial alignment should be run! [Tagging OpsInfo]

LOG:

Start Time System Name Location Lazer_Haz Task Time End
15:30 LASER LASER HAZARD LVEA LASER HAZARD LVEA IS LASER HAZARD (\u2310\u25a0_\u25a0) 07:26
22:51 SQZ Camilla, Georgia, Kevin LVEA Yes SQZT7 work 00:03
23:08 VAC Gerardo LVEA Yes Annulus work 23:54
H1 ISC
elenna.capote@LIGO.ORG - posted 22:32, Tuesday 27 May 2025 - last comment - 14:10, Wednesday 28 May 2025(84610)
CARM on Resonance, green camera refs set

Ryan S., Sheila, Elenna

First thing Wednesday morning: run full initial alignment with green cameras

Ryan and I were able to lock the IFO on DRMI after many hours struggling down rabbit holes. In short: we were able to finally lock DRMI after reverting the ITMX and ITMY alignment to the alignment on Friday, and running manual initial alignment.

Sheila came online while we were in DRMI checking various things, and together we made it to CARM on Resonance. The alignment was very good (mostly hand tuned except for MICH ASC and DHARD). Sheila and I did our usual check of the PRG following alog 62110 and confirmed that everything looks great.

From there, Ryan and I ran the green camera offset scripts, watched them converge, and set the camera values. These are all SDFed- Ryan will add screenshots. To reiterate: run full initial alignment!

Sheila will add comments about checking and fixing the REFL phases.

While Sheila was adjusting the REFL phases so we could go to CARM on analog, I tried setting up the POP X centering using PM1 (so we could do DRMI on POP). I confirmed that moving PM1 moves the beam on POPX in reasonable ways. I had to flip the DC centering sign to positive when I engaged the loop, DC6, so the centering would converge. I was trying to check the UGF of the DC6 pitch loop by adding an offset to the loop, and accidentally added a massive offset, which tripped a lockloss since the beam went crazy on POPX and therefore LSC POP and that's a lockloss trigger diode.

I also had to turn on the PM1 signal output from the ASC model, which I then SDFed. After lockloss, the PM1 locking output doesn't get cleared, so Sheila will add that to the list of suspensions to clear after lockloss.

Images attached to this report
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ryan.short@LIGO.ORG - 22:38, Tuesday 27 May 2025 (84611)ISC, OpsInfo

I also made a couple changes in Guardianland to keep ALS locked to set green references (line 6583 in ISC_LOCK.py; change weight from 10 to 1 to keep green locked) and I set the manual_control flag to True to not have DRMI/PRMI automatically jump to PRMI/MICH (line 22 in lscparams.py).

Screenshots of SDF accepting for green references at 'RESONANCE' attached.

Images attached to this comment
sheila.dwyer@LIGO.ORG - 22:47, Tuesday 27 May 2025 (84612)

I saved a template in userapps/lsc/h1/templates/CARM/check_refl_a_9_phase.xml, that puts a 200 Hz excitation (amplitude 3e-4 counts) on LSC-EXTRA_AO_OUT_2, which needs to be plugged into the CM board excitation and enabled to run this.  We ran this while locked on resonance on REFLAIR, to check the phase of REFL 9.  We adjusted the phase by about 20 degrees from what Jennie Wright did this morning based on the table from Daniel, 84581,. for a phase shifter setting of 24 degrees.  This template also indicates that the sign of REFL9 is now oposite of the sign of REFLAIR, which we have to flip at the summing junction. 

I added a line to ISC LOCK to flip this polarity in CARM_TO_ANALOG, but we lost lock before getting to try this, so we will have to watch it in the next locking attempt. 

I also added PM1 to the list of suspensions that get their lock filters cleared in DOWN of ISC LOCK, and added DC6 to the list of ASC loops that get turned off in the DOWN of ISC_DRMI.  These guardian changes have been added but not tested. 

I also went to ISC_GEN_STATES, and added arguments to the WFS centering state to allow one to choose POP centering, or AS_REFL_POP.  We can change the DRMI WFS centering to turn on the POP centering, but I haven't done that yet.

 

Images attached to this comment
elenna.capote@LIGO.ORG - 09:05, Wednesday 28 May 2025 (84617)

I took some open loop gain measurements of MICH and SRCL in DRMI. I had made small changes to the gains but ended up reverting all of them.

I found these templates in userapps lsc, and I saved the old traces as refs and ran new traces to compare.

Images attached to this comment
elenna.capote@LIGO.ORG - 09:10, Wednesday 28 May 2025 (84618)

My mistake last night was because DC6 nominally has an offset of 15000 in the bank because it used to control a PZT for POPX centering. To avoid making this mistake in the future, I have SDFed that offset to 0 (it's already set to be off all the time). Also, when I was setting up the POP centering, I noticed the loop needed positive gain instead of negative gain, so I flipped the sign of the gain in DC6 P and Y. We still need to tune the overall magnitude of the gain in the loop.

Images attached to this comment
daniel.sigg@LIGO.ORG - 14:10, Wednesday 28 May 2025 (84636)

LSC-REFL_B DAQ readbacks were not connected. Now they are. The aanalog whitening filters were also turned on at the demod chassis (no remote control).

LHO FMCS
eric.otterman@LIGO.ORG - posted 10:25, Tuesday 27 May 2025 - last comment - 07:22, Wednesday 28 May 2025(84584)
Mid station chiller plants started
The chiller systems at the mid stations were started this morning for the season. 
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david.barker@LIGO.ORG - 07:22, Wednesday 28 May 2025 (84614)

7 day trend of mid station VEA temps after chillers turned on yesterday is attached

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