TITLE: 03/26 Day Shift: 15:00-23:00 UTC (08:00-16:00 PST), all times posted in UTC
STATE of H1: Commissioning
INCOMING OPERATOR: Oli
SHIFT SUMMARY: Maintenance day activities concluded just before noon and we made it back to low noise at 21:11 UTC. Since then there have been detchar injections, PEM inj, PRM/PR2 spot centering.
LOG:
Start Time | System | Name | Location | Lazer_Haz | Task | Time End |
---|---|---|---|---|---|---|
15:01 | FAC | Ken | osb roof | n | Catwalk lights | 18:14 |
15:05 | SUS | Jeff.dave.jonathan | cr | n | Triples WD model changes | 19:02 |
15:07 | FAC | Karen | EY | n | Tech clean | 16:28 |
15:09 | FAC | Kim, Emma | FCES | n | Tech clean | 17:08 |
15:22 | FAC | HFD | Xarm | n | Tumbleweed burning, no Xarm access!! | 15:24 |
15:40 | LAS | camilla | LVEA | YES | Laser HAZARD!! | 18:49 |
15:42 | ias | jason.ryanC.tyler | LVEA | n | FARO | 18:39 |
15:49 | ee | fil.marc | EY | n | accelerometers | 16:56 |
15:50 | tcs | tj.camilla | LVEA | YES | TCSx Table beam profiling | 18:27 |
15:50 | vac | gerardo.janos | LVEA | n | LOUD purge air +x-beam manifold test | 17:51 |
16:02 | pem | robert | ex | n | PEM Injections (set-up) | 20:12 |
16:16 | sus | rahul | cr | n | etmX+Y charge meas | 18:00 |
16:17 | ee | fernando | ex.ey.lvea | n | oplev cabling labeling | 18:08 |
16:25 | vac | norco | EY | n | LN2 @cp7 | 18:49 |
16:58 | vac | norco | Corner | n | LN2 @cp1 | 19:16 |
17:25 | fac | kim | LVEA | N | Technical cleaning | 18:36 |
17:52 | sqz | nutsinee, Daniel | sqz.rack | n | SQZ rack meas | 18:59 |
17:54 | sei | jim | LVEA | n | cps checks in CR & lvea | 18:15 |
18:03 | sus | jeff | cr | n | EX esd +charge offset | 18:51 |
18:21 | epo | cassidyand class! | CR | n | Field trip!!! | 18:31 |
18:30 | VAC | Gerardo | LVEA | - | Viewport notes | 19:10 |
18:32 | CDS | Marc | EY | n | Check on acc. cable | 19:16 |
18:38 | VAC | Janos | FCES | n | Purge | 18:39 |
19:02 | SQZ | Nutsinee | LVEA | n | SQZ rack meas. | 19:26 |
20:13 | PEM | Robert, Marc | EY | n | Acc. cable check | 21:20 |
21:46 | INJ | TJ | CR | n | Run detchar safety inj | 21:47 |
21:47 | ISC | Jenny | CR | n | PRM moves | 23:47 |
22:52 | PEM | Robert | LVEA | n | Turn on shaker | 23:02 |
22:59 | SQZ | Nutsinee, Naoki | FCES | yes | Center diode | 00:59 |
Following instructions in this google doc and here's a past alog70817 to reference running as well.
I started the injections the first time at 1395523038, but ran into an HTTP error when trying to upload the event to GraceDb. I also had forgotten to turn off the PCALX lines and Robert had a shaker going on during part of that time as well. Scrap this one.
Second round with PCALX lines off, no shaker injections, and still ran into the HTTP error at the end of the injections. Start time of these - 1395523842.
Looking at the PCAL AOM, it seems that it has had a lower voltage for ~1 hour before these were ran. PCAL team is currently looking into this and if it would have affected these injections.
Apparently I was somehow logged in as Corey yesterday. For the record this was done by me.
Also, a quick update. Sidd mentioned that they made some changes from GraceDb playground to just GraceDb, so he will verify on his end and then we will try again today.
Naoki, Nutsinee
Since we see the 0.4 Hz motion in FC IR error signal, we added a boost filter for FC IR. The new boost filter is p0.1z5 and it is in FM9 of FC_LSC_DOF2. The first attachment shows the improvement of FC IR error signal with the boost filter. The rms is reduced by a factor of 3. We modified the SQZ_FC guardian to add this filter as follows.
line 393: ezca.switch('SQZ-FC_LSC_DOF2','FM1','OFF','FM2','OFF','FM3','OFF','FM9','OFF') #disable IR sus boost
line 424: ezca.get_LIGOFilter('SQZ-FC_LSC_DOF2').only_on('FM1','FM2','FM3','FM4','FM5','FM6','FM9','FM10','INPUT','OUTPUT','DECIMATION')
The SDF is accepted as shown in the second attachment.
I noticed in the summary pages spectrogram that the low frequency sensitivity was changing during one of the A2L step experiments (this is ETMX ITMX test).
The first plot shows the strain spectrum (GDS-CALIB_STRAIN_CLEAN) for 900 seconds for each available step of P2L and Y2L for the x arm. Some steps were repeated twice. In each panel, the title shows what A2L gain is being changed, and what's the nominal value. The second plot shows the ration of strain spectrum for a given A2L gain over the averaged strain spectrum with the nominal A2L value. So lower than one means the A2L value is improving the sensitivity.
There is evidence that yaw values away from nominla make the nosie below 30 Hz better.
TJ, Camilla, WP 11746, LLO did in LLO#14419
Using Matlab code from LLO#14419 with edit to parameter x = 4:1:26
J. Kissel ECR E1700387 IIET 9392 WP 11743 After - yesterday's front-end code model prep (LHO:76696), - TJ and I's prep for front-end code installation (LHO:76703), and - Dave's code installation (LHO:76706) I spent the rest of the morning filling in the upgraded watchdog infrastructure for the HAM Triples, i.e. MC1, MC2, MC3, PRM, PR2, PR3, SRM, SR2, SR3, FC1, and FC1. All HAM Triples' WD RMS MAX thresholds have been set to 150 [um_RMS] As with the QUADs and Beam Splitter -- please feel free to edit as we gain more experience with normal things that happen during IFO operation. The following has been committed / was affected by today's upgrade. MEDM SCREEN MODS /opt/rtcds/userapps/release/sus/common/medm/hxts/ SUS_CUST_HXTS_M1_WD_OSEMAC_RMSLP.adl SUS_CUST_HXTS_M2_WD_OSEMAC_RMSLP.adl SUS_CUST_HXTS_M3_WD_OSEMAC_RMSLP.adl SUS_CUST_HXTS_WD.adl SUS_CUST_HLTS_OVERVIEW.adl SUS_CUST_HSTS_OVERVIEW.adl FOTON FILE MODS /opt/rtcds/userapps/release/sus/h1/filterfiles/ (all of the above mentioned foton filter files) SDF FILE MODS /opt/rtcds/userapps/release/sus/h1/burtfiles/ (all relevant _safe.snap and _OBSERVE.snap files) GUARDIAN MODS /opt/rtcds/userapps/release/sus/common/scripts/ sustools.py Attached are my detailed notes.
This morning I took the OPLEV charge measurements on both ETMX and ETMY suspensions. I will post the results below after processing the data.
Both the suspensions were restored to their nominal state after the measurements were complete.
Later, Jeff flipped the sign on ETMX ESD bias voltage once the above measurements were done.
H1 SUS ETMX L3 ESD Bias was held at +430 [V_ESD] in order to mitigate the charge build up identified in LHO:76326 for ~1 hr today, 2024-03-26, between 17:46 and 18:46 UTC. Attached is a trend of the ESD bias offset (calibrated in [V_DAC] rather that [V_ESD]) throughout today's maintenance.
I processed the measurement, ETMYs charge appears low and doesn't have any major trends, ETMXs charge is around 40 [V] on most DOFs and appears to have a slight upward trend.
TITLE: 03/26 Day Shift: 15:00-23:00 UTC (08:00-16:00 PST), all times posted in UTC
STATE of H1: Preventive Maintenance
INCOMING OPERATOR: Oli
SHIFT SUMMARY:
Covered the morning for TJ while he did TCS work & here are the activities from when I was in the chair.
LOG:
Tue Mar 26 10:09:35 2024 INFO: Fill completed in 9min 31secs
TCs started lower, so I restored the trip temps to -120C (as shown on plot)
WP11786
Jeff, Joe, Jonathan, Dave
A new h1calcs model was installed, this adds two slow channels
++: slow channel H1:CAL-CALIB_REPORT_HASH_INT added to the DAQ
++: slow channel H1:CAL-CALIB_REPORT_ID_INT added to the DAQ
A DAQ restart was required.
As per ECR E1700387 these two channels were added to the h1daqgds[01] GDS broadcast streams. The h1daqgds[01] systems where restarted again as part of this process. This was around 8:50 am local time.
WP11743 SUS DACKILL removal
Jeff, Oli, TJ, Dave:
This morning we installed new HAM SUS and ISI models:
h1susmc[1,2,3], h1suspr[m,2,3], h1sussr[m,2,3], h1susfc[1,2], h1isiham[2,3,4,5]
All required a DAQ restart.
For h1sush2a and h1sush34, because we restarted all the user models, I elected to restart the IOP models as well to run a DAC AUTOCAL on these front ends. For all the other frontends, only the modified user models were restarted.
J. Kissel ECR E1700387 IIET 9392 WP 11743 Tomorrow, we continue on the adventure towards upgrading the suspension watchdog systems that Oli, Dave and I have been chugging along on for the previous two weeks (see, eg, LHO aLOGs 76305, 76269 and 76545). This week, we're tackling a big chunk -- all of the HAM triple suspensions, both large and smal, i.e. the 7 HSTS and 2 HLTS. Note :: these are the final suspensions that are hooked up to their respective ISIs, so this should be the last major upgrade. As such I've: In the SUS model library parts, - Converted the BLRMS trigger generating systems to include a trust-worthy RMS calculation, coupled with a down-stream low-pass filter, - Removed all evidence of the USER DACKILL watchdog aggregator system - While I was there, I removed remaining evidence of the long-defunct / depricated "online detector characterization" ODC system, long since replaced by guardian state information On the top level SUS models, - Removed all evidence of the USER DACKILL watchdog aggregator system - Removed the IPC sender of the USER DACKILL to the respective ISI - Verified that the removal of library block output ports didn't botch any of the top level connections, reconnecting and re-organizing as needed On the top level of the ISI models, - Replaced the IPC receiver of the USER DACKILL watchdog from all respective SUS which impacts all of the following models: Top Level ISI Top Level Optic Governing Library Part h1isiham2.mdl h1susmc1.mdl HSTS_MASTER.mdl h1susmc3.mdl HSTS_MASTER.mdl h1suspr3.mdl HLTS_MASTER.mdl h1susprm.mdl RC_MASTER.mdl h1isiham3.mdl h1susmc2.mdl MC_MASTER.mdl h1suspr2.mdl RC_MASTER.mdl h1isiham4.mdl h1sussr2.mdl RC_MASTER.mdl h1isiham5.mdl h1sussr3.mdl HLTS_MASTER.mdl h1sussrm.mdl RC_MASTER.mdl (no change to isiham7) h1susfc1.mdl HSTS_MASTER.mdl (no change to isiham8) h1susfc2.mdl HSTS_MASTER.mdl In addition, some of the lower level SUS library parts were also impacted, SIXOSEM_T_STAGE_MASTER.mdl FOUROSEM_STAGE_MASTER.mdl FOUROSEM_STAGE_MASTER_OPLEV.mdl All of the above model changes have been committed to the userapps SVN repo in revs 27310, 27311, 27312, and 27313.
This set of screenshots shows the typical edits to the top level HAM models, before vs. after. Note, because the "payload" is more that one suspension on the HAMs, I got lazy and started connecting two constants to four places, rather than putting in eight constants. In doing so, I harnessed the trickery of the bus creator / bus selector, and re-arranged the order hidden within. The screenshot highlights this debauchery in purple.
Here are some before vs. after, example top level model changes for the various types of HSTS and HLTS: PRM (an RC_MASTER) before vs. after MC2 (an MC_MASTER) before vs. after PR3 (an HLTS_MASTER) before vs. after
We aimed to do A2L steps over the weekend, 15 minutes/step 76630, 76683, but as Elenna points out with the camera servos running the beam spot stayed static on the mirror while the mirror actuation point changed.
Looking at data from A2L tuning in April 2023 68384 attached plot, A2L steps are ~0.4 for a change of around 2 in the camera offset (TRAMP 120s). We'll keep around the steps same as the weekend: +/- 1.0 per 15 minutes to up to +/-2.0 in the H1:ASC-CAM_{PIT,YAW}{1,2,3}_OFFSET channels during observing with nominal TRAMPs extended from 10s to 120s. These offsets are already unmonitered in sdf as reset each lock, I unmonitered the TRAMPs.
These offfsets vary up to 3 counts lock to lock, see attached plot. Set based on ADS converging.
Script saved in /ligo/gitcommon/labutils/beam_spot_raster/camera_servo_offset_stepper.py Scheduled to run if we're in NLN via tmux session on cdsws26 at:
Tony will be here during the first set so can cancel the others if there is any issues.
Jennie, Camilla
I looked at the CAM3 test from 08:58:40 UTC to 12:46:33 UTC and can see that a high offset (ASC-CAM_{PIT3, YAW3}_OFFSET) in both pitch and yaw corresponds to high power build-ups in the PRC and arms. Yaw seems to have more of an effect than pitch. The range dips when the offset is away from its nominal state. See first image. The offsets don't seem to have much effect on KAPPA C.
During the CAM2 test the IFO unlocked and so only the P2L steps seem to have run, its hard to see a trend in the build-ups for this as the IFO was still thermalising - maybe this hsould be run again. See second image.
For the CAM1 test the yaw steps were interrupted by lockloss so we will have to redo these.
The pitch steps for CAM 1 show optimum build-ups/power recycling at Pitch offset = -231.6 counts and worst at -229.6 counts. The range is worst when the build-ups are best and vice versa.
I am not sure why lower circulating power makes the range drop for all these measurements.
J. Kissel, L. Dartez ECR E2400103 IIET 30760 WP 11786 To better coordinate and confirm the front end portion of the calibration pipeline and the GDS portion running on the DMT machines remain in sync in terms of calibration model installed, which is necessary for good calibration, we are adding two slow 16 Hz EPICS channels to the h1/l1calcs models (so both LLO and LHO) that will be added to the GDS broadcaster list so the GDS calibration pipeline can read them. These are H1/L1:CAL-CALIB_REPORT_ID_INT and H1/L1:CAL-CALIB_REPORT_HASH_INT. Louis and I created the top-level EPICs records today; see attached screenshot. The change has been committed to the userapps SVN under: /opt/rtcds/userapps/release/cal/h1/models/ h1calcs.mdl committed at rev 27307. It's in no way a complicated add to the model, but I've ran a test compile of the h1calcs.mdl on the build machine anyways just to check. The test compiled succeeded without issue.
J. Kissel This model changes have been installed this morning. As such, I've updated the safe.snap SDF system to initialize the H1:CAL-CALIB_REPORT_ID_INT and H1:CAL-CALIB_REPORT_HASH_INT channels. I've also chosen to monitor them, since we don't expect them to change during observation, and/or regulary, and this information will become critical for calibration librarianship.
Jason, Filiberto, Fernando.
Per the WP11763
Motor/Brake cable identification was perfromed for the TIMX/ITMY/BS OPLevers. The provisional Medm was tested as well. We took advantage of this opportunity to complete the internal wiring in the BS OPLEver with the inclusion of the RJ9 patches.
The WP will remain open to perform the activity in ETMX/ETMY next Tuesday.
ETMX and ETMY OPLever motors and brakes were identified. Medm tested and Beckhoff software updated with the right directions found.
Evan, Naoki, Nutsinee, Camilla
Today Sheila added nodes.set_managed() in INIT state of SQZ_FC guardian and let SQZ_FC guardian go through the INIT state. However, the FC2 M1 offload filter in the INIT state was old filter setting in 68914, which caused GR_SUS_LOCKING failure. We reverted it as shown in the attachment and updated the FC2 M1 offload filter in INIT state.
Attached a screen shot of the old (wrong) settings on top, correct one at the bottom.
In 76503, the limiter for FC2 M1 was not in INIT state of SQZ_FC guardian, but we added the limiter.