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Reports until 14:27, Thursday 05 September 2024
X1 SUS (SUS)
rahul.kumar@LIGO.ORG - posted 14:27, Thursday 05 September 2024 - last comment - 14:27, Thursday 05 September 2024(79923)
O5-HRTS status report.

Ryan C, Rahul

We have finished the assembly of the 10th Ham Relay Triple Suspension (HRTS) for O5, which is being assembled and characterized in the stagings clean room lab upstairs. In June we reported the assembly and testing of first five Freestanding HRTS suspension (see LHO alog 78574 and 78711), since then we have built an additional five of them, thus bringing the total count to ten for both the sites (with two more to go, total twelve required between LHO & LLO which includes one spare at each site).

I have attached several pictures (attachment01, attachment02, attachment03, attachment04) below which shows the assembled & locked HRTS stored in the lab on the flow bench in the clean room. Picture01 shows an HRTS with BOSEMs and cables attached, ready to be characterized on test stand (reference pic is shown here).

In this round of HRTS assembly work we have assembled three Freestanding configuration, one Suspended version (shown in the attachment05 below) and one OM0 (attachment06). The Suspended version of HRTS will be attached to the new BBSS (beam splitter) in O5 and Om0 will have bottom mass (optic) actuation using AOSEMS.The top mass will be controlled by 6 BOSEMs which is common for all types of HRTS.

After finishing the assembly work, we balanced all three stages of the suspensions for all six degrees of freedom. This involved lowering and matching  blade tip height and angle on the top stage (2 blade springs) and on the top mass (4 blade springs). In all the cases, optic's lowest edge was lowered to a height of 40.5mm (+-0.5mm) from the bottom of the cage. The PUM and Top Mass height was adjusted based on the scribe lines on the structure.

Given blow are the details (OLV, offsets and Gain) of the six BOSEMs attached the HRTS.

1. Structure no. 07, Configuration: Suspended

Suspended masses: Top Mass = 755gm, Penultimate mass = 802gm, Dummy optic = 300gm

BOSEMs s/n D060108-E. S1900741, S1900749, S1900622, S1900662, S1900637, S1900613.

OLV OFFSETS GAIN
30830 -15415 0.973078
27619 -13809.5 1.086209
25585 -12792.5 1.172562
24300 -12150 1.234568
26400 -13200 1.136364
26872 -13436 1.116404

2. Structure no. 06, Configuration: OM0

Suspended masses: Top Mass = 755gm, Penultimate mass = 802gm, Dummy optic = 301gm

BOSEMs s/n D060108-E. S1900726, S1900723, S1900746, S1900732, S1900742, S1900747

OLV OFFSETS GAIN
31111 -15555.5 0.964289
30571 -15285.5 0.981322
32384 -16192 0.926383
24964 -12482 1.20173
26685 -13342.5 1.124227
26905 -13452.5 1.115034

 

3. Structure no. 04, Configuration: Freestanding

Suspended masses: Top Mass = 758gm, Penultimate mass = 802gm, Dummy optic = 301gm

BOSEMs s/n D060108-E. S1900749, S1900722, S1900724, S1900735, S1900740, S1900744

OLV OFFSETS GAIN
30687 15343.5 0.977613
27768 13884 1.08038
28421 14210.5 1.055558
26807 13403.5 1.119111
26432 13216 1.134988
30319 15159.5 0.989479

4. Structure no. 05, Configuration: Freestanding

Suspended masses: Top Mass = 755gm, Penultimate mass = 803gm, Dummy optic = 300gm

BOSEMs s/n D060108-E. S1900730, S1900727, S1900750, S1900738, S1900743, S1900734

OLV OFFSETS GAIN
30534 -15267 0.982511
29900 -14950 1.003344
26531 -13265.5 1.130753
26624 -13312 1.126803
24670 -12335 1.216052
29626 -14813 1.012624

5. Structure no. 09, Configuration: Freestanding

Suspended masses: Top Mass = 758gm, Penultimate mass = 800gm, Dummy optic = 300gm

BOSEMs s/n D060108-E. S19007309 S1900725, S1900733, S1900736, S1900803, S1900728

OLV OFFSETS GAIN
31068 -15534 0.965624
30716 -15358 0.97669
27512 -13756 1.090433
25864 -12932 1.159913
26362 -13181 1.138002
32378 -16189 0.926555

********************************************

Note- The test results of the suspension will be posted below as comments.

Images attached to this report
Comments related to this report
rahul.kumar@LIGO.ORG - 13:57, Thursday 05 September 2024 (79931)

Test results for structure no. 07, Configuration:- Suspended

Attachment01 shows the transfer function results along with individual osem results, compared against the model

Attachment02 shows the top to top transfer function measurement results for all 6 dof and attachment03 is the zoomed in version of the same. The plots shows three measurements (taken on Aug 12, Aug 19 and Aug 21) after making mechanical changes to the suspension, which includes replacing the bottom wire loop to remove heaving pitch on the optic (caused due to faulty springs in the wire pulling jig). There is some low frequency (0.8Hz approx.) cross coupling in T dof from Yaw. V dof still has R coupling into it. The magnitude for R dof is slightly low when compared against the model. 
We have tried to fine tune the suspension to remove cross coupling and improve the TF magnitude, how it looks like we still need to do so some work over here to further refine the results.This work is still ongoing.

Non-image files attached to this comment
rahul.kumar@LIGO.ORG - 14:03, Thursday 05 September 2024 (79932)

Test results for structure no. 06, Configuration:- OM0

Attachment01 shows the transfer function results along with individual osem results, compared against the model

Attachment02 shows the top to top transfer function measurement results for all 6 dof and attachment03 is the zoomed in version of the same.

L, P, T and Y dof looks fine, although there is a slight frequency shift at Yaw. However the magnitude for R dof is slightly lower than the model and V dof has cross coupling from R which needs further work.

Non-image files attached to this comment
rahul.kumar@LIGO.ORG - 14:09, Thursday 05 September 2024 (79933)

Test results for structure no. 04, Configuration:- Freestanding

Attachment01 shows the transfer function results along with individual osem results, compared against the model.

Attachment02 shows the top to top transfer function measurement results for all 6 dof. Overall the suspension looks healthy. V and Rdof in this case has given us a lot of trouble and after a lot of fine tuning (of the suspended chain, bosems, flags etc) we have been able to bring the results as close as possible to the model. The black trace on V dof was measured with flags at an angle with respect to the PD/LED of the bosem, once corrected the magnitude improve as seen in pin and orange trace.

Non-image files attached to this comment
rahul.kumar@LIGO.ORG - 14:13, Thursday 05 September 2024 (79935)

Test results for structure no. 05, Configuration:- Freestanding

Attachment01 shows the transfer function results along with individual osem results, compared against the model

Attachment02 shows the top to top transfer function measurement results for all 6 dof and attachment03 is the zoomed in version of the same.

V and R dof needs some improvement which is currently ongoing. The rest of them looks healthy.

Non-image files attached to this comment
rahul.kumar@LIGO.ORG - 14:16, Thursday 05 September 2024 (79937)

Test results for structure no. 09, Configuration:- Freestanding

Attachment01 shows the transfer function results along with individual osem results, compared against the model

Attachment02 shows the top to top transfer function measurement results for all 6 dof and attachment03 is the zoomed in version of the same.

The suspension looks healthy and I am happy with the transfer function results. The cross coupling at Vdof (which is common to all the HRTS) needs some attention, which is currently ongoing.

Non-image files attached to this comment
H1 SUS
jim.warner@LIGO.ORG - posted 14:01, Thursday 05 September 2024 (79930)
B&K measurements of BBSS in staging

Betsy asked me to take a look at doing B&K measurements of the BBSS being assembled in the staging building, so I reminded myself how to use the B&K and took measurements this morning. I'll attach a photo shortly, but I put the accel on the very bottom of the cage, with +X axis aligned with optic longitudinal, Z aligned with is optic vertical, Y is optic transverse. Plots are titled with the accel axis that I hit on the suspension cage, while the legends are labeled with the accel axis response, so "BBSS X Meas" shows the X,Y,Z tf from hitting the cage along the accel X axis. These measurements are a kind of a mid point of the assembly, looks like most of the parts were there, but the bottom stage osems didn't have flags, I didn't see any vibration absorbers.

I think the most concerning thing I see is this 65-ish hz X mode on the first plot. It's the biggest peak and is in a band that could potentially really limit some of the ISI loop gains, if it's not well damped on the table.

A while ago I made a script to plot these measurements, but didn't explicitly say how to run it. Script is quick_plot.py is userapps/sys/h1/scripts/bruel_and_kjaer:

jim.warner@cdsws22:~ 0$ userapps
jim.warner@cdsws22:release 0$ cd sys/h1/scripts/bruel_and_kjaer/
jim.warner@cdsws22:bruel_and_kjaer 148$ ./quick_plot.py -t "BBSS Z Meas" -f "/path/to/data/BBSS_Z_meas.csv"
 

 

Images attached to this report
H1 SQZ
naoki.aritomi@LIGO.ORG - posted 13:12, Thursday 05 September 2024 - last comment - 11:45, Friday 20 September 2024(79929)
SRCL offset change from -175 to -290 and FC detuning improvement

Vicky, Sheila, Naoki

First we tried SRCL offset of -400, which looked good in yesterday's FIS SRCL offset measurement 79903. We took the calibration measurement with SRCL offset of -400 in 79911, but Louis reported in the mattermost that there is a large optical spring in the sensing function. Also, FDS with SRCL offset of -400 is worse than nominal. Vicky will add more plots for this.

Then we decided to change the SRCL offset to -290 and optimized FC detuning. This improved the sensitivity below 100 Hz as shown in the first attachment and improved the range by ~5Mpc. The optimal FC detuning changed from -34 Hz to -28 Hz and this could be because of SRCL offset change and arm power change.

After FC detuning improvement, we took the calibration measurement with SRCL offset of -290 in 79922, but the measurement did not make sense according to Louis so we took an another calibration measurement with SRCL offset of -290 in 79928

Images attached to this report
Comments related to this report
victoriaa.xu@LIGO.ORG - 16:03, Thursday 05 September 2024 (79934)

Following up with some FIS SRCL measurements from today as we were navigating how to best optimize SRCL offset for squeezing, which gives best sensitivity around 100 Hz.

Blue & purple traces - When first looking at SQZ after re-calibrating at -400 counts srcl offset, SQZ looked kinda v-shaped, like as if the SRCL detuning is big. We first tried optimizing the sqz angle for the bucket (blue, CLF RF6 demod phase @ 222 deg), then tried to optimize high-freq sqz (purple, CLF RF6 @ 215deg). For this SRCL offset at -400 counts, with about (222-215=) 7 degrees difference on the CLF RF6 demod phase (bad estimate is ~3.5deg diff on sqz angle), this changed the kHz squeezing level by about 1.9dB. See the trends on this screenshot.

Yellow trace - We then tried to see if FIS + SRCL @ -400 counts was the same as yesterday lho79903 and yes it was same. But zooming into yesterday's plots, it looks like this -400 SRCL offset setting (yesterday's blue trace) was actually not a great spot (already well passed zero detuning), as there is a little bit of ballooning between 100-200Hz that we did not notice yesterday.

Given that squeezing, and also calibration, saw that this SRCL offset @ -400 cts had a bad spring effect, we backed it off to -290 counts and took another cal meausrement. We chose -290 to be ~halfway between the -475 ct (pink) and -100 ct (black) settings  tried yesterday (see dtt). For -475 ct and -100 ct, we realized today that DARM between 250-500 Hz had about the same level of anti-sqz coupled in by the SRCL detuning. Unsure if this means they have the same physical detuning, this is something we will try out in quantum noise models to understand better.

Green trace - shows FIS + SRCL @ -290 counts. It is where we expected from yesterday. Leaving it here.

In summary, today we tried a few methods of "optimizing srcl detuning," to get it closer to 0, but also realized we need to think more carefully with quantum noise models like, what is the easiest / most sensitive metric for squeezing to see the srcl detuning.

  1. looked at mid-squeezing, where the high freq squeezing angle matches no squeezing. the hope was that at this angle, we are mostly seeing phase variations across the band, using no-sqz as the reference. -400 ct was noticeably less flat compared to no-sqz than -290 ct.
  2. while always maximizing 1 kHz squeezing, try to see if we can "flatten" darm in the 100s Hz band.  This was a kinda confusing to evaluate because QN in the bucket is a very marginal/small effect you have to squint closely to see. We tried to do this yesterday and only in hindsight noticed that -400 counts was not good in yesterday's plots. From models, we can look for what do we even want / expect for 0 detuning.
  3. while maximizing bucket ~350 Hz squeezing, try to see what is the best we can do for darm noise in the bucket.

We then moved onto FDS + SRCL @ -290 counts, and optimized the filter cavity detuning, as Naoki describes above.

Images attached to this comment
francisco.llamas@LIGO.ORG - 11:45, Friday 20 September 2024 (80210)

Adding plots of the sensing function. From these measurements, we see that the sensing function is also an indicator of bad/good SRCL offset. Additionally, *something* changed from Thursday to Saturday, as seen in the Saturday calibration measurement trace.

Figures (1) and (2) are the different sensing functions where the second figure ranges from 0-40 Hz. The uncertainties of each measutrement are plotted in figures (3) and (4), where figure (4) ranges from 0-40Hz.

Images attached to this comment
H1 ISC
elenna.capote@LIGO.ORG - posted 12:42, Thursday 05 September 2024 (79927)
AS WFS offset test - no appreciable change in sensitivity

This was a fast test right at the end of the commissioning period. I tried changing the offset on the AS WFS to see if that changes the low frequency sensitivity of DARM. Short answer: no change in sensitivity without the offset, and no improvement in sensitivity with a higher offset, which yesterday's tests suggested would help (79904).

I forgot to save the reference for the higher offset test (it was exactly the same as the others), but here is a comparison of the current offset (-0.15) and zero offset. The April 11 reference trace is also shown. We are very close to our best low frequency sensitivity in April (pre-OFI problems).

I think that if it helps the SQZ ASC to have no offset, we should turn this offset off. DHARD Y coherence is now very low even with the offset off.

Images attached to this report
LHO General
corey.gray@LIGO.ORG - posted 12:21, Thursday 05 September 2024 (79926)
Mid-Shift Status (Thurs)

Dropped out of OBSERVING at 1530utc (830amPT), for calibration measurements and then went immediately into Thurs COMMISSIONING time.  Commissioning ended 1917utc (1217pmPT).

H1 CDS
david.barker@LIGO.ORG - posted 12:18, Thursday 05 September 2024 (79925)
Added SENSMON2 CLEAN channel to IFO Range MEDM

Sheila, Dave:

On Sheila's request, I have edited the generate_ifo_range_medm.py script to add a new line for the H1:CDS-SENSMON2_BNS_EFF_RANGE_CLEAN_MPC channel (plus its associated GPS channel).

Images attached to this report
H1 CAL (CAL)
corey.gray@LIGO.ORG - posted 11:58, Thursday 05 September 2024 (79922)
Thurs Late Morning H1 Calibration Measurement Post-Commissioning Changes (broadband headless + simulines)

This icalibration was requested by Sheila after today's Commissioning work.

Measurement NOTES:

Images attached to this report
H1 CDS
david.barker@LIGO.ORG - posted 11:56, Thursday 05 September 2024 (79924)
CDS section on CDS overview using new system widget

I've expanded the use of the new "system" MEDM widget to the CDS section of the oveview. HW_STAT, PICKET_FENCE and CDS_SDF are now color coded blocks, replacing the related-display+LED pairs.

These blocks will turn RED in non-nominal conditions. In addition HW and PKT will turn MAGENTA if their respective servers stop updating.

Images attached to this report
H1 ISC
thomas.shaffer@LIGO.ORG - posted 11:41, Thursday 05 September 2024 (79921)
A2l script vs hand tuning continued

Sheila D, Elenna C, TJ S

Yesterday we ran the a2l_min_multi.py script and then Elenna adjusted the ITM yaw gains by hand to see if the script was actually helping our coupling in a way we would like (alog79904). Today, we did a similar exercise but made some adjustments to the script to see if we could tune it a bit better and get it work properly. The short answer is that the script stills seems to want the ITMY Y gain to be ~0.2 different compared to where Elenna found the best CHARD Y coherence. Other quads and dofs seemed to be ok in this instance though.

This morning we were curious if the script agreed with the changes made yesterday, so we quickly ran it at the start of commissioning. Sheila and Elenna noticed that the script didn't actually have a zero crossing for a few of the dofs, ITMY was particularly far off (seen in <a href="https://alog.ligo-wa.caltech.edu/aLOG/uploads/79921_20240905113858_a2l_demod_3_tries.png">attachment 2</a>). When the script doesn't find a zero crossing within its scan range, it would just return the initial gain and stop. So, Sheila and I made some changes by hand using a pen to screen linear fit, then ran the script again. This was better but ITMY Y didn't change because the magnitude of the gain change was greater than the gain change threshold coded in. We bumped this up from 0.2 to 0.5 and tried one more time. This try had only ITMY Y gain appreciably change, and all other dofs looked much better from a perspective of all of their demod signals had zero crossings in the center of their scan range.

At this point, the script wants ITMY Y at -2.46. Elenna then moved ITM Y gains by hand and found that the previous value (from the second running of the script) of -2.2 for ITMY Y looked best. See attachment 1. The -2.46 gain looked worse <20Hz, see the top right plot in the attached. Elenna also checked DHARD and agreed that it looks good.

We aren't really sure why the script disagrees so much with this one dof right now. This script is based on one that LLO uses, and it seems to work for them. More thought needed.

Initial a2l gains before starting this morning:

            'P2L':{'ITMX':-0.98,
                   'ITMY':-0.36,
                   'ETMX':3.08,
                   'ETMY':4.48},
            'Y2L':{'ITMX':2.90,
                   'ITMY':-1.7,
                   'ETMX':4.85,
                   'ETMY':1.13 },

Final a2l gains:
            'P2L':{'ITMX':-1.0,
                   'ITMY':-0.39,
                   'ETMX':2.98,
                   'ETMY':4.72},
            'Y2L':{'ITMX':2.87,
                   'ITMY':-2.25,
                   'ETMX':4.88,
                   'ETMY':1.49 },

Images attached to this report
H1 CDS
david.barker@LIGO.ORG - posted 09:49, Thursday 05 September 2024 (79920)
O4 IPC error summary

Here is a summary of the 4 spontaneous IPC errors we have seen during the O4 run so far.

alog date details
79913 02:08:03 Thu 05sep2024 long-range-dolphin h1susetmx sender @
74665 11:09:47 Thu 07dec2023 CS dolphin h1lsc0 sender *
74365 05:22:13 Tue 21nov2023 CS dolphin h1lsc0 sender *
73584 18:47:05 Wed 18oct2023 long-range-dolphin h1susetmx sender @

Note that both the * and the @ events are identical pairs of events.

The fact that h1susetmx had todays issue back on Oct 2023 rules out the recent addition of the new LIGO-28AO32 DAC card as being a possible problem.

H1 ISC
elenna.capote@LIGO.ORG - posted 09:19, Thursday 05 September 2024 (79918)
SRCL FF works with new SRCL Offset, 100-200 Hz improved

Today after the SRCL offset was changed from -175 to -400, I quickly ran an injection to check the performance of the feedforward. I also had uploaded a new feedforward that would fix the 100-200 Hz bump that is injecting excess noise.

The "current" feedforward, which is in FM5, still worked well even with the new -400 offset. The "new" feedforward, in FM8, fixes the excess noise and also still performs well. The "old" feedforward FM4, post vent, is shown for comparison (this is what I was improving against last week).

I have SDFed in observe and changed the guardian to use this new FF.

Images attached to this report
H1 CAL (CAL, ISC)
corey.gray@LIGO.ORG - posted 09:04, Thursday 05 September 2024 (79911)
Thurs Morn H1 Calibration Measurement With New SRCL1 OFFSET (broadband headless + simulines)

This is with a new SRCL1 OFFSET of -400 (for H1:LSC-SRCL1_OFFSET), as requested by Sheila from commissioning work yesterday.

Measurement NOTES:

Now handing over to Commissioners for Thurs Commissioning.

Images attached to this report
H1 ISC (ISC)
corey.gray@LIGO.ORG - posted 08:44, Thursday 05 September 2024 (79916)
H1 SRCL1 Offset Change

Before running this morning's calibration, Sheila asked me to change the offset for LSC's SRCL1 (so change to -400 [from -175] for H1:LSC-SRCL1_OFFSET) was made and the SDF has been ACCEPTED (attached).

Images attached to this report
LHO VE
david.barker@LIGO.ORG - posted 08:37, Thursday 05 September 2024 (79915)
Thu CP1 Fill

Thu Sep 05 08:08:55 2024 INFO: Fill completed in 8min 51secs

Gerardo confirmed a good fill curbside.

Images attached to this report
H1 CDS
david.barker@LIGO.ORG - posted 08:29, Thursday 05 September 2024 - last comment - 08:48, Thursday 05 September 2024(79913)
X-Arm long-range-Dolphin IPC errors from h1susetmx model 02:08 Thursday

At 02:08:03 the h1oaf and h1calcs models reported a single IPC receive error for channels being sent by the h1susetmx model.

Preliminary findings:

For all three channels this was a single IPC error in all receivers (one packet in that second's 16384 packets didn't get received in time)

There was no issue with h1susetmx's CPU usage at the time

There was no issue with h1cdsrfm's EX2CS thread (nor any thread) processing at the time

Images attached to this report
Comments related to this report
david.barker@LIGO.ORG - 08:33, Thursday 05 September 2024 (79914)

The three IPC channels which went into error are the complete set of LRD channels being sent by the h1susetmx model. (grep for RFM0 channels sent by h1sustemx model in the H1.ipc file shown)

05Sep08:17 > grep -B 1 -A 3 RFM0 H1.ipc|grep -B 4 h1susetmx$
[H1:SUS-ETMX_CAL_CS_L1_LINE]
ipcType=RFM0
ipcRate=16384
ipcHost=h1susex
ipcModel=h1susetmx
--
[H1:SUS-ETMX_CAL_CS_L2_LINE]
ipcType=RFM0
ipcRate=16384
ipcHost=h1susex
ipcModel=h1susetmx
--
[H1:SUS-ETMX_CAL_CS_L3_LINE]
ipcType=RFM0
ipcRate=16384
ipcHost=h1susex
ipcModel=h1susetmx
 

david.barker@LIGO.ORG - 08:48, Thursday 05 September 2024 (79917)
H1 CDS
david.barker@LIGO.ORG - posted 09:16, Thursday 19 October 2023 - last comment - 09:40, Thursday 05 September 2024(73584)
Rare IPC receive errors on h1oaf and h1calcs from h1susetmx

Last night at GPS=1381715243 (Wed Oct 18 18:47:05 2023 PDT) h1oaf and h1calcs long-range-dolphin receivers from h1susetmx reported a single receive error (1 errror in the 16384 packets received in that second). This is the first error of this type this year. There was no issue with h1susetmx at the time, its cpu max is 20uS. I'll clear the errors on the next TOO.

With an error rate of 1 per year, (1 in 5.2e+11) we will just continue to monitor this for now.

Images attached to this report
Comments related to this report
david.barker@LIGO.ORG - 09:40, Thursday 05 September 2024 (79919)

Happened again 02:08:03 Thu 05sep2024. FRS32032

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