Displaying reports 841-860 of 82955.Go to page Start 39 40 41 42 43 44 45 46 47 End
Reports until 14:39, Thursday 22 May 2025
H1 SUS (SUS)
edgard.bonilla@LIGO.ORG - posted 14:39, Thursday 22 May 2025 - last comment - 14:52, Thursday 22 May 2025(84548)
Tested the SR3 OSEM calibration [It works!]

Oli, Edgard.

On Tuesday, Oli tested the SR3 OSEM calibration factors mentioned in the comments of [LHO:84296] and summarized in [LHO:84531] and took a new suite of HAM5 ISI to SR3 M1_DAMP transfer functions (the measurements also live in /HLTS/H1/Common/Data/ and are dated for May 21st of 2025). 

The calibration factors from [LHO:84531] (taken on May 7th) featured a seemingly crazy change on the T1 OSEM calibration of 2.4539 x. So we wanted to doublecheck that the numbers actually made sense before proceeding with OSEM estimator work.

The measured SUSPOINT V to M1_DAMP_{ V , R , P } show that the calibration factor was largely correct. 

The first attachment shows the SUSPOINT V to M1_DAMP_{ V , R , P } in measured on May 7th before using the new OSEMINF gains. In it, it can be seen that there is a very clear crouss-coupling from V to R, which is mediated by the T1 OSEM in SR3. Dividing the length-to angle over the length-to-length at 10 Hz to get a sense of the cross-coupling we get 3.3 rad/m for R and 0.65 rad/m for P.

The second attachment shows the SUSPOINT V to M1_DAMP_{ V , R , P } measured on May 21st after using the new OSEMINF gains. The V to R (and to P) improves significantly with the new calibration factors. This is best seen by comparing the relative amplitude of the V to V transfer function (in red) with the V to R (in blue), and the V to P (in green), through which we get 0.4 rad/m for R and 0.1 rad/m for P. Therefore, the apparent cross-coupling has been greatly reduced, which confirms that the T1 factor was likely correct, and we can proceed with the rest of the procedure.

[NOTE: We use relative factors for the comparison, because all OSEMs were miscalibrated by a factor of 1.3-1.4, so directly comparing the amplitudes from may 7th to May 21st would be inaccurate]

These improvements are encouraging enough that we feel comfortable moving forward with the M1 OSEM calibration for SR3. To do so, Oli is hard at work rescaling the gains of the SR3 loops. We will post when that steps is ready

 

 

 

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edgard.bonilla@LIGO.ORG - 14:52, Thursday 22 May 2025 (84549)

As a sidenote, I ran the calibration script from [LHO:84531] on the May 21st HAM5 to SR3 data to see how stable the ISI to OSEM calibration is likely to be.

The TL;DR is that most OSEM gains are estimated to remain almost the same, the only suggested gain change above 1% is the T1 OSEM which is suggested to change by 6%, which is small enough that we will leave it alone for now. These results imply that the calibrations are good enough that they won't change by much on a weekly basis.

We will NOT adjust the SR3 M1 OSEMINF gains again with the values listed below

 

This is the output of the script:

%%%%%%
We have estimated a OSEM calibration of H1 SR3 M1 using HAM5 ST1 drives from 2025-05-21_0000 (UTC).
We fit the response M1_DAMP/HAM5_SUSPOINT between 5 and 15 Hz to get a calibration in [OSEM m]/[GS13 m]

The H1:SUS-SR3_M1_OSEMINF gains at the time of measurement were:
(old) T1: 3.627
(old) T2: 1.396
(old) T3: 0.952
(old) LF: 1.302
(old) RT: 1.087
(old) SD: 1.290

The suggested (calibrated) M1 OSEMINF gains are
(new) T1: 3.435
(new) T2: 1.389
(new) T3: 0.952
(new) LF: 1.296
(new) RT: 1.088
(new) SD: 1.292

To compensate for the OSEM gain changes, we estimate that the H1:SUS-SR3_M1_DAMP loops must be changed by a factors of:
L gain = 1.002 * (old L gain)
T gain = 0.998 * (old T gain)
V gain = 1.029 * (old V gain)
R gain = 1.029 * (old R gain)
P gain = 1.003 * (old P gain)
Y gain = 1.002 * (old Y gain)

This message was generated automatically by OSEM_calibration_SR3.py on 2025-05-22 20:49:42.062366+00:00 UTC
%%%%%%

 

H1 SUS (CDS, SUS)
jeffrey.kissel@LIGO.ORG - posted 14:30, Thursday 22 May 2025 (84547)
Greenlighted sush2b HAM1 Software Watchdog (SWWD)
J. Kissel

Now that PM1, RM1, and RM2 are safely functional on the new ISI HAM1, in the h1iopsush2b front-end model, I've
    - set H1:IOP-SUS_${OPTIC}_DK_BYPASS_TIME to 600 seconds H1:IOP-SEI_HAM1_DK_BYPASS_TIME
    - set H1:IOP-SEI_HAM1_DK_BYPASS_TIME to 999999999 (~1e9) seconds, as is seemingly common in most SWWDs
    - hit RESET on each of the SUS DACKILLs and the SEI DACKILL to arm them
    - initialized the PM1 channels in the safe.snap and accepted and monitored their current values
H1 SUS (ISC)
jeffrey.kissel@LIGO.ORG - posted 14:10, Thursday 22 May 2025 (84545)
PM1 Accepted in h1sushtts safe.snap with settings in the ALIGNED state
J. Kissel, T. Shaffer

In the current O4 paradigm of SDF practice, we've minimized the number of .snap files to track by accepting the settings of some suspension whose setting don't change between "IFO down" and "Observing." That includes SUS RM1 and RM2, which live on the sushtts model -- that also now is home to PM1. RM1 and RM2 are ALIGNED at the moment, with damping loops and alignment offsets ON, and yet their settings do not show up as "different" from the safe.snap. This disagrees with the principle of "safe" but it's how we're doin it. 

As such, I've accepted PM1's settings in the ALIGNED state into the sushtts safe.snap.

Images attached to this report
H1 ISC
camilla.compton@LIGO.ORG - posted 13:36, Thursday 22 May 2025 (84544)
ISCT1 Moved back into Place and Bellows Reattached

TJ, Ryan C, Oli, Camilla. WP#12561

Randy had forklifted ISCT1 just outside of the cleanroom. We pushed ISCT1 back into place and checked it's location and height. Removed yellow VP covers and replaced bellows, then removed guillotines.

H1 SUS (SEI, SUS)
edgard.bonilla@LIGO.ORG - posted 12:34, Thursday 22 May 2025 - last comment - 13:50, Monday 23 June 2025(84531)
M1 SR3 OSEM calibration [revisited]

Oli, Edgard, Jeff, Brian

This post is meant to give a clearer explanation of the work in [LHO:84296] and its many comments. We are trying to find a new set of gains for the M1_OSEMINF filter banks for SR3 to calibrate the OSEMs to be in agreement with the HAM5 GS13s.

To do so, we drive the HAM5 ISI in { X , Y , Z } and record the response of the relevant OSEMs between 5 to 15 Hz.  At these frequencies, the M1 stage of the suspension should start to become inertial, and the M1_DAMP / SUSPOINT response of each individual OSEM should asymptote to -1, because the OSEMs would be measuring their support point on the cage [barring internal dynamics of the cage itself].

To increase the accuracy of the calibration, we use the MATLAB model of the HLTS and use the full extent of the 5-15 Hz data instead of only the asymptotic behavior.

I post here the code used to generate these results. The code requires the new Common/MatlabTools/ExportedModels folder from the SusSVN [LHO:84458]. The detailed results of the calibrations mentioned is shown below.

_____

Images attached to this report
Non-image files attached to this report
Comments related to this report
edgard.bonilla@LIGO.ORG - 17:06, Tuesday 27 May 2025 (84605)SUS

Adding hera a few bits of information that were missing from the original post, together with an updated version of the script.

_______________________________________________________________________

To compensate for the OSEM gain changes, we estimate that the H1:SUS-SR3_M1_DAMP loops must be changed by a factors of:
L gain = 0.743 * (old L gain)
T gain = 0.724 * (old T gain)
V gain = 0.549 * (old V gain)
R gain = 0.549 * (old R gain)
P gain = 0.691 * (old P gain)
Y gain = 0.743 * (old Y gain)

The calibration will change the apparent alignment of the suspension as seen by the at the M1 OSEMs
NOTE: The actual alignment of the suspension will NOT change as a result of the calibration process

The changes are computed as (osem2eul) * gain * inv(osem2eul).
Using the alignments from 2025-05-07_0000 (UTC) as a reference, the new apparent alingments are:

DOF    Previous value     New value       Apparent change
---------------------------------------------------------------------------------
L          -4.3 um                 -2.6 um                     +1.7 um
T          -19.7 um              -14.2 um                 +5.4 um
V          -24.0 um              -8.4 um                   +15.6 um
R          -490.6 urad          -219.3 urad          +271.4 urad
P          -300.2 urad          -203.8 urad          +96.5 urad
Y          -569.3 urad          -422.5 urad          +146.8 urad

Non-image files attached to this comment
edgard.bonilla@LIGO.ORG - 18:21, Tuesday 27 May 2025 (84607)SUS

Here I post the coherence and transfer functions between the excitations of HAM5 in X, Y, and Z to the SUSPOINT degrees of freedom.

The band from 5-10 Hz seems to be low enough amplitude that I think we can claim that the drives are clean enough in the SUSPOINT basis to perform the calibration.

Note that the high coherence between L/T and HAM5_ISO X/Y is expected, since the SR3 euler basis does not perfectly align with the cartesian basis of HAM5.

 

 

Images attached to this comment
jeffrey.kissel@LIGO.ORG - 13:50, Monday 23 June 2025 (85255)
J. Kissel (for O. Patane and E. Bonilla)

Also during this barrage of measurements, Oli and Edgard gathered Open Loop Gain (IN1/IN2), Loop Suppression (IN2/EXC), and Closed Loop Gain (IN1/EXC) tfs under the presence of DAMP_EXC. 

Within the templates mentioned below, there're two data sets.
The "New OSEMINF gains" data is with with the above mentioned
    H1:SUS-SR3_M1_OSEMINF_T1_GAIN  3.627
    H1:SUS-SR3_M1_OSEMINF_T2_GAIN  1.396
    H1:SUS-SR3_M1_OSEMINF_T3_GAIN  1.345
    H1:SUS-SR3_M1_OSEMINF_LF_GAIN  1.719
    H1:SUS-SR3_M1_OSEMINF_RT_GAIN  1.490
    H1:SUS-SR3_M1_OSEMINF_SD_GAIN  1.781

The "OG OSEMINF gains" data is with the OSEMINF gains that have been present throughout O4 (as they were reverted post-measurement) 
    H1:SUS-SR3_M1_OSEMINF_T1_GAIN  1.478
    H1:SUS-SR3_M1_OSEMINF_T2_GAIN  0.942
    H1:SUS-SR3_M1_OSEMINF_T3_GAIN  0.952
    H1:SUS-SR3_M1_OSEMINF_LF_GAIN  1.302
    H1:SUS-SR3_M1_OSEMINF_RT_GAIN  1.087
    H1:SUS-SR3_M1_OSEMINF_SD_GAIN  1.29

The raw .xmls for both these data is 
    /ligo/svncommon/SusSVN/sus/trunk/HLTS/H1/SR3/SAGM1/Data/
        2025-05-21_1800_H1SUSSR3_M1_WhiteNoise_L_0p02to50Hz_OpenLoopGainTF.xml
        2025-05-21_1800_H1SUSSR3_M1_WhiteNoise_P_0p02to50Hz_OpenLoopGainTF.xml
        2025-05-21_1800_H1SUSSR3_M1_WhiteNoise_R_0p02to50Hz_OpenLoopGainTF.xml
        2025-05-21_1800_H1SUSSR3_M1_WhiteNoise_T_0p02to50Hz_OpenLoopGainTF.xml
        2025-05-21_1800_H1SUSSR3_M1_WhiteNoise_V_0p02to50Hz_OpenLoopGainTF.xml
        2025-05-21_1800_H1SUSSR3_M1_WhiteNoise_Y_0p02to50Hz_OpenLoopGainTF.xml

The open loop gain transfer functions (IN1/IN2) have already been exported
    /ligo/svncommon/SusSVN/sus/trunk/HLTS/H1/SR3/SAGM1/Data/
        2025-05-21_1800_H1SUSSR3_M1_WhiteNoise_?_0p02to50Hz_OpenLoopGainTF_tf.txt     << exports of "OG OSEMINF gains" data

        2025-05-21_2000_H1SUSSR3_M1_WhiteNoise_L_0p02to50Hz_OpenLoopGainTF_tf.txt     << exports of "New OSEMINF gains" data

Also, I've exported the loop suppression of the "OG OSEMINF gains" data as
    /ligo/svncommon/SusSVN/sus/trunk/HLTS/H1/SR3/SAGM1/Data/
        2025-05-21_1800_H1SUSSR3_M1_WhiteNoise_?_0p02to50Hz_OLGTF_LoopSuppression_tf.txt     << exports of "OG OSEMINF gains" data
H1 SUS
oli.patane@LIGO.ORG - posted 11:50, Thursday 22 May 2025 (84543)
Closeout transfer functions confirm open questions on RM signs

Jeff, Oli

Looking into (1) from 84462.

Before this vent, although the cable pinouts were flipped for both RMs, the phase for the TFs were at 0. Now that the cables have been flipped (fixed), we are seeing that the closeout transfer functions that I took 84498 are showing that the phase for the RMs is now flipped, at 180. Additionally, both RMs are still needing the damping sign to be +1, instead of the usual -1.

Since there does still seem to be a sign issue somewhere in the sensor chain for RM2, we would have expected the 'after' transfer function phases to differ between RM1 and RM2, so it's strange that they both have switched over to 180.

I've attached the transfer functions for RM1 and RM2 comparing the after vent measurements to the last measurements we had done for them with damping loops off, which was in 2022.

Non-image files attached to this report
LHO VE
david.barker@LIGO.ORG - posted 10:23, Thursday 22 May 2025 (84539)
Thu CP1 Fill

Thu May 22 10:16:19 2025 INFO: Fill completed in 16min 15secs

 

Images attached to this report
H1 CDS
david.barker@LIGO.ORG - posted 10:20, Thursday 22 May 2025 (84538)
MC2 camera restarted, another instance of too many open files

Patrick, Jonathan, Dave:

MC2 camera went offline at 06:30 today, this was another instance of the new software eventually running into the 1024 limit for open files. This process is on h1digivideo4 and surprisingly had only been running for 8 days.

Jonathan increased the file limit on this machine to 40,000 and we restarted the process. MC2 h1cam07 did not need a power cycle.

H1 ISC (ISC)
raed.diab@LIGO.ORG - posted 09:00, Thursday 22 May 2025 (84536)
DARM sensing function - adding a digital offset

Summary: adding a digital offset to get a flat sensing function does not correspond to SRM detuning phase of 90, as modeled in FINESSE.

recap: I have modeled the SRCL DOF detuning due to mode mismatch. Nominally, we want the detuning phase of the SRM to be ø = 90˚ for resonant  sideband extraction conditions, where there are no optical spring effects. However, mode mismatches affect this phase, and consequently we can see optical spring effects showing up in the DARM sensing function.

On site, after locking we can add a digital offset to the SRM phase to flatten the sensing function, but then the question is “does the digital offset that flattens the DARM sensing function correspond to  ø = 90˚?”

And the answer is “no”, at least as modeled in FINESSE. 

I have added an offset to SRCL and looked at the corresponding sensing function, and it is clear that a ø = 90 is not necessarily a flat response (starting from 5 Hz), as the plot attached shows

In this case I’m looking at the RF readout (from DARM to AS45_Q), and where the average mismatch between all cavities is 0.01% (the start locking point is ø = 90.03˚). This also demonstrates that even a tiny mismatch can show optical spring effects.


 

Non-image files attached to this report
LHO General (VE)
ryan.short@LIGO.ORG - posted 08:02, Thursday 22 May 2025 - last comment - 17:36, Thursday 22 May 2025(84532)
Ops Day Shift Start

TITLE: 05/22 Day Shift: 1430-2330 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Planned Engineering
OUTGOING OPERATOR: None
CURRENT ENVIRONMENT:
    SEI_ENV state: MAINTENANCE
    Wind: 11mph Gusts, 6mph 3min avg
    Primary useism: 0.03 μm/s
    Secondary useism: 0.09 μm/s
QUICK SUMMARY: HAM1 pumping continued overnight, but starting about 1.5 hours ago the pressure started rapidly climbing. No cause determined as of yet. VAC team has been contacted.

EDIT: Had the wrong channel trended, corrected in current attachment.

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ryan.short@LIGO.ORG - 08:16, Thursday 22 May 2025 (84534)

The gate valve on top of HAM1 was closed and the pressure is now holding; trend attached.

Images attached to this comment
david.barker@LIGO.ORG - 09:23, Thursday 22 May 2025 (84537)

Note that we currently have a potentially confusing situation of two EPICS pressure channels for HAM1, only one of which is correct:

H1:VAC-LY_X0_PT100B_PRESS_TORR Is the correct channel, current value 1.3e-05

H0:VAC-LY_X0_PT100B_PRESS_TORR Is NOT the correct channel, unfortunately is misreports a better vacuum than we have, current value 1.5e-07

I went through all the vacuum MEDM screens and replaced the "H0" channels with the "H1" where ever I found them. Old MEDMs may still have the wrong value.

 

david.barker@LIGO.ORG - 10:43, Thursday 22 May 2025 (84540)

Vacuum FOM (nuc22) updated to new HAM1 gauge.

I've edited the caqtDM UI file for the Vacuum FOM to correct the HAM1 PT100B channel and remove the PT100A entry.

Images attached to this comment
janos.csizmazia@LIGO.ORG - 17:36, Thursday 22 May 2025 (84557)
Troubleshooted, see here: aLog no. 84556
H1 CDS
david.barker@LIGO.ORG - posted 07:53, Thursday 22 May 2025 - last comment - 08:20, Thursday 22 May 2025(84533)
Vacuum pressure in HAM1 rising rapidly, started around 6:00 today, Thursday 22nd May 2025

Starting around 6am today the vacuum pressure in HAM1, which had dropped to 6e-06 Torr, started rising rapidly. At time of typing it is up to 9.8e-04.

Richard is heading to the LVEA to investigate.

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Comments related to this report
david.barker@LIGO.ORG - 08:20, Thursday 22 May 2025 (84535)

VACSTAT detected the rise when the pressure slope exceeded its trip of 1e-07 at 06:48 this morning.

Images attached to this comment
LHO VE
janos.csizmazia@LIGO.ORG - posted 17:27, Wednesday 21 May 2025 (84530)
2025 April/May vent - VAC diary
Jordan, Travis, Janos

HAM1 pumpdown continued. The new Agilent leak checker is backing the turbo pump. We are waiting for the He-signal to be at least <5E-9 Torr, so we could start leak checking. After evaluating the trends, it is likely that tomorrow morning this happens. Also, regardless this happens, the Ion-pump (IP13) will be possible to be opened up. Also, an interesting note, that after achieving molecular flow in HAM1, the corner pressure suddenly decreased by ~5-6E-9 Torr, that suggests a E-3 Torrl/s gas load through the HAM1/HAM2 septum viewport O-rings, so there is indeed some communication between HAM1 and the rest of the corner.
The overall pressure in HAM1 in the end of the day is ~9E-6 Torr, which aligns well with fully gutted HAM chamber pumpdown speeds in the past.

The large Gate Valves, first GV7, then GV5 was opened. The fully open position was achieved at ~45 and ~47 psi, respectively. No issues were encountered during the process. The corner pressure went down quickly to ~3.5E-8 Torr. RGA scans are continuously being taken.
H1 ISC
thomas.shaffer@LIGO.ORG - posted 17:03, Wednesday 21 May 2025 - last comment - 11:14, Thursday 22 May 2025(84528)
Replaced shutter on ISCEX

FRS34149

Camilla and I removed the broken Model#VS35S2T0 Serial#3179 shutter and replaced it with Model#VS14S2T0 Serial#8796. The replacement unit had a slightly smaller outer diameter so we traded some posts with beam dumps that were on the side of the table not in use to get the correct height.

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Comments related to this report
camilla.compton@LIGO.ORG - 11:14, Thursday 22 May 2025 (84542)
Both old and new models VS14 and VS35 use the same blade material (teflon coated SS) and have the same the max allowed energy density of <100mW/mm2 (https://www.uniblitz.com/blade-options/).
From D1800270 we expect the beam to be 14mW with a waist r=250um near the shutter, this gives an energy density of 70mW/mm2, which is within the shutter's specs. 
H1 CAL
anthony.sanchez@LIGO.ORG - posted 16:50, Wednesday 21 May 2025 - last comment - 17:08, Wednesday 21 May 2025(84524)
PCAL Y-End TX module maintenance

 Y-End TX Module Maintenance was performed today.
Everything went fairly well while following the instructions laid out in T1600436 -V12 Except the AOM Rejected Power measurement. This measurement inbetween PBSC2 and beam dump 2  is measuring the AOM power that we were dumping on to the beam dump. It didn't ever give us a static value like all the rest of the measurements. The max was a 18.5 mW  jump right after the we opened the shutter. Then the power would decay down to a lower value of 13.6 mw but over several minutes. The decay rate seemed to get longer after a while. The excitations were indeed turned off. We had zeroed the low power sensor with a shuttered background measurement. I'm not sure why that seemed to not be a steady number. We ended up taking the number that seemed like it had initially asymptote to before we saw the slow fall off.

The Beam Spots all look great. TX Sphere might be very slightly  to the right of perfectly center, but I think it's fine.
 

OLTF went well, Setup was well documented.

   
Date May , 21,2025
Laser Shutter Check pass
Max OFS Offset 8
95% OFS Offset 7.6
Operating OFS Offset 3.8
Laser Output Power 1.94 W
After-Laser Rejected Power 4.11 mW
AOM Input Power 1.91 W
Max Diffracted Power 1.60 W
Un-Diffracted Power 0.285 W
AOM Diffraction Efficiency 83.77%
After-AOM Rejected Power 15.5 mW
TxPD Power 6.51mW
OFSPD Power 6.64 mW
Outer Beam Power 0.355 W
Inner Beam Power 0.352 W
Output Beam Power Ratio 0.991549295774648
OFS Gain 38.5
OFS Phase Margin 58
Images attached to this report
Non-image files attached to this report
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anthony.sanchez@LIGO.ORG - 17:08, Wednesday 21 May 2025 (84529)

Updated the safe.snap files...... but not the observe.snap files because when loaded there were not any changes. because the files are linked and i had already saved the changes in the safe.snap file.

 

Images attached to this comment
H1 CDS
david.barker@LIGO.ORG - posted 14:21, Wednesday 21 May 2025 - last comment - 10:49, Thursday 22 May 2025(84521)
h1sush7 crash

13:25:11 Wed 21 May 2025 PDT all models on h1sush7 stopped running. The SWWD to h1iopseih7 started its countdown with 100% IPC receive errors.

I set a bypass time of 999999 on h1iopseih7 to interrupt the countdown.

We first restarted all the models. This did not clear the error, and we found a PCI bus issue whereby only one of the four ADCs could be found.

As a precautionary measure we fenced h1sush7 from the Dolphin fabric.

Next we power cycled the computer. This fixed the PCI bus issues, all cards are visible and all models starting running.

I cleared the SWWDs and handed the system over to the control room.

Note, there were TIMING error flashes during this recovery time which we have not traced down.

[Wed May 21 13:25:11 2025] h1iopsush7: ERROR - An ADC timeout error has been detected, waiting for an exit signal.
[Wed May 21 13:25:11 2025] h1susauxh7: ERROR - An ADC timeout error has been detected, waiting for an exit signal.
[Wed May 21 13:25:11 2025] h1sussqzin: ERROR - An ADC timeout error has been detected, waiting for an exit signal.
[Wed May 21 13:25:11 2025] h1susfc1: ERROR - An ADC timeout error has been detected, waiting for an exit signal.
 

Images attached to this report
Comments related to this report
david.barker@LIGO.ORG - 10:49, Thursday 22 May 2025 (84541)

Added this crash to FRS20317

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