Edgard, Oli
We took measurements to get the above-resonance OSEM response of the PR3 and SR3 suspensions to characterize the gaines. This is a follow up to the in vacuum measurements on 80863, and to the estimated calibrations from 83605.
For PR3, the measurements were taken with
- all of the M1 damping loops at a gain of -0.2 (instead of the nominal -1).
-The coil driver filter in state 1 (similar to the measurements that Jeff took).
- The ISI state was ISOLATED, but HEPI is locked, so we circumvented guardian by sliding off the Isolation Gain on HEPI. This should not affect the measurements for the OSEM calibration.
The results are saved in:
/ligo/svncommon/SusSVN/sus/trunk/HLTS/H1/PR3/Common/Data/
2025-04-15_1431_H1ISIHAM2_ST1_WhiteNoise_PR3SusPoint_L_0p02to50Hz.xml 2025-04-15_1431_H1ISIHAM2_ST1_WhiteNoise_PR3SusPoint_T_0p02to50Hz.xml 2025-04-15_1431_H1ISIHAM2_ST1_WhiteNoise_PR3SusPoint_V_0p02to50Hz.xml
The similarly named _tf.txt files are stored in the same folder, and they export the measured M1 transfer functions using the [ L T V R P Y ] order.
Back in August 2023 the damping gains for SR3 were reduced from -1 down(up?) to -0.5 to help with noise in DARM (72130). Since that change, we had never taken a set of transfer functions with the damping loops on with these new gains, so today I took those. The resulting transfer functions don't show too much damping, which is expected.
The data can be found in ../HLTS/H1/SR3/SAGM1/Data/2025-04-15_2000_H1SUSSR3_M1_WhiteNoise_{L,T,V,R,P,Y}_0p01to50Hz.xml, and has been committed to svn as r12228.
The results can be found in ../HLTS/H1/SR3/SAGM1/Results/ as 2025-04-15_2000_H1SUSSR3_M1_ALL_TFs.pdf and 2025-04-15_2000_H1SUSSR3_M1.mat, and have been committed to the svn as r12229.
Linking analysis pdf showing cross coupling between all DOFs
Also adding a comparison between this measurement and the last time that we took damped transfer functions since those previous measurements would have been taken with a different set of damping gains.
The last time a damped measurement was taken was back in 2015, and those transfer functions look a lot different than the model and this recent measurement, so I also looked at the next previous damped measurement, from 2014. This one was in phase 2b, so not in chamber, but here at least we see that these damped measurements match up pretty well both with the model and with the recent measurement.
This PDF along with a zoomed in version of some of the plots can be found at /ligo/svncommon/SusSVN/sus/trunk/HLTS/Common/Data/ as
allhltss_DampingOnComparison_H1SUSSR3_M1_Apr25vsFeb15vsMar14_ALL_TFs.pdf
allhltss_DampingOnComparison_H1SUSSR3_M1_Apr25vsFeb15vsMar14_ALL_ZOOMED_TFs.pdf
and have been committed as r12251.
TITLE: 04/15 Day Shift: 1430-2330 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Planned Engineering
INCOMING OPERATOR: None
SHIFT SUMMARY:
ISI is installed , but more work need to be completed before Optics can be installed.
PSL & SPI team are still in the PSL & anti Room, they have installed a beam splitter nut more work may be required.
Jason setup some Faro equipment.
Vacuum team started to pump down the BSC8 annulus door volume.
LOG:
Start Time | System | Name | Location | Lazer_Haz | Task | Time End |
---|---|---|---|---|---|---|
14:32 | FAC | Randy | LVEA | N | HAM1 Heavy lift Prep | 13:32 |
14:33 | FAC | Kim & Nellie | LVEA | N | Technical Cleaning & Supplies, Kim Out early | 16:25 |
14:54 | FAC | Eric | LVEA | N | Checking HVAC zone conditions | 14:57 |
15:02 | FAC | Eric | End X | N | Replacing Sensor | 15:43 |
15:17 | FAC | Christina | Staging | N | Moving Folklifts & matierals | 16:17 |
15:32 | Safety | Richard | LVEA | N | Settign up HAM1 Work Cam | 16:54 |
15:33 | VAC | Jordan | LVEA | N | Purge Air Checks. | 16:01 |
16:06 | EE | Marc | CER | N | Getting chassis for testing. | 16:09 |
16:11 | EE | Marc | EX & Y | N | Power supply testing | 17:25 |
16:15 | VAC | Travis & Jordan | LVEA | N | Closing GV7 and pump work | 17:15 |
16:22 | SPI | Jeff, Jason, Sina, RyanS, Josh | optics Lab , PSL | Yes | Installing SPI Optics, Jeff Out Early | 19:20 |
16:24 | SUS | Camilla & Matt | HAM5 | N | Pulling off First Contact off optics | 16:53 |
16:41 | SAFE T | McCarthy | LVEA | N | Running parts and Safety checks | 18:56 |
16:42 | SEI | Betsy | LVEA | N | Running parts | 20:28 |
16:49 | FAC | Nellie | Mid X | N | Tech cleaning | 17:20 |
16:54 | SEI | Jim, Randy Mitchell, TJ | LVEA | N | SEI Crew flying in an ISI | 18:07 |
17:20 | FAC | Kim | MY | N | Technical Cleaning | 18:35 |
17:24 | ISC | Dainel | LVEA | N | verifing Equipment in the ISC racks | 20:06 |
17:30 | FAC | Eric | PSL adjacent | N | Talking to Jason. | 18:12 |
18:04 | VAC | Jordan | LVEA | N | Preping Y arm RGA | 20:00 |
18:09 | VAC | Travis | BSC8 | N | Checking the anulus pump by ITMY | 18:16 |
18:21 | FAC | Christina | Water tank area & Recycling | Forklifting & dump run | 19:19 | |
18:21 | AOS | Camilla, Matt | LVEA | N | Pulling off first contact by HAM5 | 18:51 |
18:58 | SEI | Jim, TJ, Tyler, Randy, Mitchell | LVEA HAM1 | N | ISI Installation | 00:58 |
18:59 | SEI | Brian | LVEA HAM1 | N | Watching HAM1 Installation. | 21:03 |
19:51 | Safe T | Richard | LVEA | N | Safety checks. | 23:06 |
20:09 | VAC | Jordan | LVEA | N | Pump & RGA checks & bake out | 22:54 |
20:14 | PSL & SPI | Ryan S, Josh, Sina | PSL | YES | Installing SPI Pickoff of the ALS pickoff. | 00:14 |
20:16 | ISC | Camilla & Matt | HAM5&6 | N | cleaning parts | 23:49 |
20:46 | PCAL | Tony | PCal Lab | N | Delivery | 20:50 |
21:09 | ISI | Betsy | LVEA | N | Checking on the ISI team | 22:37 |
21:33 | VAC | Travis | LVEA | N | Table sneaking | 21:49 |
21:40 | IAS | Jason | West bay | N | Staging Faro Equipment | 23:40 |
It was a long day, but the HAM1 ISI is in the chamber. Mitch pointed out first thing this morning that the install fixture was still in the "short" configuration, with 2" spacer pads on the under side of the middle stand. We partially disconnected the I beams an swapped to the "tall" configuration, squared the I beams up to the chamber, including checking the height of the feet (procedure says 3", but could vary), centering on the HEPI piers with a plumb bob, checking I beam level with a bubble level and checking the vertical gap between the tightest point between the I beams and the chamber door, which the procedure recommended be 1.5". We then brought the ISI container into the LVEA, then realized the pallet jack was too close to the container to open the latches for the lid. We put the container on cribbing, adjusted the pallet jack then took lunch. After lunch, we took the lid off the can, flew the ISI over to the install cart by HAM1 and made a first attempt to slide the ISI in, at which point we realized the Stage 0 of the ISI would hit the tips of the HEPI springs. After much deliberation, we set the ISI back down on the cart and used the crane to lift the install fixture (I beams and stands) and extended the padded feet as muc has possible. We had to use the fork lift on the -Y side of the chamber, as the clean room blocked crane access. Clearance between the outside edge of the I beam and door was now about .5" and the feet were 4" above the floor. At this point the ISI sailed over the HEPI springs and we were able to proceed with the ISI install as normal, smooth sailing.
First two photos show the height of the feet and the clearance between the I beams and the chamber. Last one shows the clearance through receiving with the container, as we brought the ISI in. Others got pictures of other points and I hope will add.
We still have to pull the install fixture, then we can start plugging stuff in.
Months of build and testing, weeks-days of prep, 1 min 41sec to slide into chamber. In like Flynn.
Movie is too large so on One Drive: https://caltech.box.com/s/5p1eysbye8tmq2177x40tera254ezpl4 Good job Jim, Mitchell, TJ, Tyler, and the illusive Randy on the forklift (not shown)!
Woo Woo! Awesome job! Tagging EPO for photos.
J. Kissel, S. Koehlenbeck, J. Oberling, R. Short, J. Freed ECR E2400083 IIET 30642 WP 12453 After this morning's kerfuffle / belated power-outage recovery with the PSL HVAC system was resolved, Sina, Ryan, and Josh began the procedure we're walking thru outlined in Section 1 of T2500024. We're keeping running notes on the fly at the bottom of the google-doc for now. In summary here, with more details to come, we got as far as - Clearing out some old IO equipment that unused and in the way of the SPI pick-off path - Measuring the power around ALS-PBS01 - Installing the new ALS/SPI 80R/20T beam splitter - Measuring the beam profile along the future SPI path, in reflection of this 80R/20T beam splitter.
Among the first things we did was measure the power at various places along the ALS beam path to get a good starting point. For the ~2W beams we used an Ophir 20C-SH (datasheet says accuracy of +/- 3%) and for ~100 mW beams we used a S401C, (datasheet says accuracy of +/- 7%). For laser safety, we would unlock the PMC and shutter the laser while we were placing these power meters, so I also kept track of the PMC TRANS to scale our measurements by input power appropriately. We did NOT turn on the PMC's intensity stabilization servo (ISS), for no particular reason other than we forgot to turn it on for the first measurement, and then wanted to stay consistent. This meant that the PMC TRANS itself was slowly noise at that +0.5 [w] level, so my reported values below are "eyeball averages." So, not exactly a NIST-level precision/accuracy setup, but good enough for sanity checks. As such, I'm not going to bother report uncertainty in the numbers below. Here're the results (again, this is prior to doing anything to the path). Times of measurements are all for 2025-04-15, and in UTC, such that trends of other PDs may be captured if need be. Location Power Meter [mW] PMC Trans [W] Time [UTC] (1) Going in to ALS-HWP2 2060 103.2 21:39 # expected: 2000 [mW]; good! (between ALS-L1 and ALS-HWP2) (2) p-pol in trans of ALS-PBS01 1970 102.8 22:17 # expected: 1950 [mW]; good! (between ALS-M2 and ALS-L2) (3) s-pol in refl of ALS-PBS01 49.4 103.2 21:44 # expected: 50 [mW]; good! (between ALS-L1 and ALS-M9) (4) s-pol in refl of ALS-M9 47.7 103.0 21:48 # 44.9 [mW] reported by ALS-C_FIBR_EXTERNAL_DC_POWERMON, which is in trans of ALS-M9 at this time; good! (between ALS-M9 and ALS-FC2) All of these powers match expectation quite exquisitely. My guess for the inconsistency of (4) with the EXTERNAL monitor PD is that the beam splitter ratio of ALS-M9 programmed into the beckhoff calibration of the PD's channel is a bit off, but this can be cross-checked later. We then installed SPI-BS1 (the 80R/20T BS), and cross-checked the reflectivity reported in LH0:83863. Location Power Meter [mW] PMC Trans [W] Time [UTC] (5) s-pol in refl of SPI-BS1 37.7 102.4 22:22 The PMC power is lower between (3) and (5), the input to the SPI-BS1 is different, so we need to scale the measurement a bit, Input Power to SPI-BS1 = 49.4 [mW] * (103.2 / 102.4) = 48.81 [mW] REFL power from SPI-BS1 = 37.7 [mW] Fractional reflection = 37.7 [mW] / 48.81 [mW] = 0.772 = 77% (from LHO:83863) = 77%. Thus, our results today are consistent with what Josh and Keita measured in the optics lab.
Pictures from the work on 2025-04-15. The first three attachments are without labels, just in case the pics are needed for something else in the future. The diagram we were working with (from the SPI ECR) is also attached here for convenience. The second three attachments *are* labeled, so I'll describe what happened using those. 20250415_some_optics_removed_labeled.jpg - This is (mostly) the how the team started the day: with the area where the SPI pick-off path is intended to go full of un-diagrammed spare/unused stuff. I highlight red circles everything that was removed in this first attachment. Additionally, before the picture was taken, ALS-M8 and ALS-FC1 were removed and the temporary large vertical beam block was installed. 20259415_all_optics_removed_labeled.jpg - This is the "after" all components cleared picture, and the table layout during the power measurements. As you can imagine, because of the lens tube on the SM1PD1A, there was no room between the PD and ALS-M9 to insert a power meter to measure the transmitted light thru ALS-M9. As such, we can't validate the beam-splitting ratio of that optic. Ah well. 20250415_end_day_1_labeled.jpg - This is how we left yesterday: We SPI-BS1 installed in its permanent location. Downstream, we sent the reflected beam into a WinCam head such that we could profile the beam incoming to the SPI path -- and assess whether we need lenses in order to adjust the beam size to match our fiber collimator. While we definitely saw the expected change in power and alignment at ALS-FC2, we elected to restore the power and alignment later.
Today's activities:
There is an oplev chassis in SUS-R1 that isn't used for anything anymore. I powered it off and it will be removed soon.
TITLE: 04/15 Day Shift: 1430-2330 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Planned Engineering
CURRENT ENVIRONMENT:
SEI_ENV state: MAINTENANCE
Wind: 18mph Gusts, 10mph 3min avg
Primary useism: 0.03 μm/s
Secondary useism: 0.24 μm/s
QUICK SUMMARY:
Verbals Ops Remider to sweep the LVEA before relocking. Something tells me we are gonna have a long Tuesday maintenance today and may not get around to the LVEA sweep today. :)
Updates on the Upgrades the Following:
Install an ISI in HAM 1.
SPI in PSL - add ALS pickoff mirror - Update, The PSL team had some HVAC issues stemming from the poweroutage and were delayed.
VAC - HAM1 Top flange Gauge work table side - GM -- Travis has his hands on the new one and wants to install it..... but there is a flying ISI currently in the LVEA.
Norco arrived at exactly 15:00 UTC and drove to the CP2 N2 tank on the +X side of the corner station.
16:00 UTC Test T569591
Second Norco truck arrived 1700 UTC heading Down Y-ARM to Mid Y CP3
18:17 UTC PSL team makes it into the PSL room, after an hour
1 ton taken to dump to offload.
18:45 UTC 2nd Norco truck leaves.
Edgard, Oli
As a continuation from yesterday's work on getting the new noise estimators up and running for PR3 and SR3, we've copied over the filters used in the normal M1 damping for PR3 and SR3, H1:SUS-{PR3,SR3}_M1_DAMP_{P,Y}, for Pitch and Yaw over to new filter banks: H1:SUS-{PR3,SR3}_M1_{PIT,YAW}_DAMP_OSEM and H1:SUS-{PR3,SR3}_M1_{PIT,YAW}_DAMP_EST. These filter banks are found in the Pitch Estim and Yaw Estim screens under OSEM Damper and Estim Damper. The filters were copied over with a script that made sure that it was copying the filters that corresponded to the correct suspension and DOF (some of the filters differ between the suspensions as well as between DOF on the same suspension)..
The filters have all been loaded in but are currently off. The gains on these filter banks are currently set to 0.
I am attaching the script that I used to copy over these filters.
J. Kissel ECR E2400083 IIET 30642 WP 12453 We're getting started on installing the PSL Pick-off path for the future SPI, and we want to record the values of the ALS/SQZ fiber distribution path before any work gets started -- and also see how these PD's values depend on the PSL environment. These PDs are described thoroughly in LHO:83013, but in short, there's a monitor PD internal to the PSL, on the table, and a down stream fiber-coupled monitor PD inside the ALS/SQZ fiber distribution box. Note, because ISCT1 has been moved out of the way for the ISI HAM1 install, the ALS COMM 2f SHG power monitor PD is unexpected to be dead, reading zero. The good news: after the 2025-04-01 corner station vent and 2025-04-06 Power outage (LHO:83753), both ALS/SQZ path PDs report the same power as the did in Feb 2025 -- even though the PMC transmitted power is a few Watts less: Feb 24 2025 Today (Lights OFF) Today (Lights ON) H1:PSL-PWR_PMC_TRANS_OUTPUT [W] 105.0 104.6 104.6 H1:ALS-C_FIBR_EXTERNAL_DC_POWER [mW] 44.6 45.15 45.55 H1:ALS-C_FIBR_INTERNAL_DC_POWER [mW] 30.2 29.8 31.9 In LHO:83013, I reported the *log* of the power for the ALS path PDs rather than the absolute milliwats. Here, I quote both dates in absolute power [mW] for the record. Watching the long term trend of the PD internal to the ALS/SQZ fiber box, the power swings regularly by ~2 mW. The current max is ~31.5 mW, and min is 29.5 mW. During this morning's data, PSL environmental controls were on the fritz. My guess is that the optical fiber that feeds the ALS/SQZ internal monitor PD is quite sensitive to temperature, as you can see the INTERNAL power smoothly swing up and down. The free-space, on table EXTERNAL PD makes sharp 0.3 [mW] jumps when the lights are turned on and OFF, but otherwise no sensitivity to temperature. Finally, everything moves slightly with the PMC transmitted power, and the slightly smaller, seemingly random 0.2 [W] blips in PMC transmitted power are a result of Jason / Ryan going in and out of the main PSL room to try to assess with the environmental controls and turning on/off the lights. Upsettingly interesting! So, here should be our goal powers for on-table EXTERNAL PD and fiber-coupled INTERNAL PD should be somewhere around Environmental Controls and Lights OFF EXTERNAL / ON TABLE / Free-space PD 45.2 +/- 0.1 [mW] INTERNAL / IN RACK / Fiber-Coupled PD 31.2 +/- 0.2 [mW] Environmental Controls and Lights ON EXTERNAL / ON TABLE / Free-space PD 45.5 +/- 0.1 [mW] INTERNAL / IN RACK / Fiber-Coupled PD 30.6 +/- 1.0 [mW]
UPDATE: Eric rescued the PSL environmental controls after a full system reboot. The systems communications to the actually HVAC had not been recovered since the power outage, so it required a full-system restart. This was complete and the system was functional by 2025-04-15 18:20 UTC. Attached are the same PD trends as the environmental controls turn on, and the temperature in the enclosure adapts. The PMC transmitted power went DOWN from 104.6 [W] to 103.7 [W]. The EXTERNAL, on table, free-space PD went DOWN from 45.5 [mW] to 45.2 [mW]. The INTERNAL, fiber-coupled ALS/SQZ distribution box PD became more stable at 31.2 [mW]. So... NEW GOALS for the PDs with the environmental controls on and functioning normally, with the lights on: H1:ALS-C_FIBR_EXTERNAL_DC_POWER 45.2 +/- 0.2 [mW] H1:ALS-C_FIBR_INTERNAL_DC_POWER 31.2 +/- 0.2 [mW]
Morning dry air skid checks, water pump, kobelco, drying towers all nominal.
Dew point measurement at HAM1 , approx. -42C
Tue Apr 15 10:07:33 2025 INFO: Fill completed in 7min 29secs
Edgard, Oli, Brian.
We added a folder with a script that calculates the noise budget for the OSEM estimator for an HLTS.
The folder lives in: sus/trunk/HLTS/Common/FilterDesign/Estimator/.
The script inside is called (at least for now) PR3_noise_budget.m, and it uses the simulink diagram in the same folder to run. The diagram doubles as a diagram for the estimator scheme itself, so it can be useful to look at.
We will post more commissioning scripts in this folder later in the week.
Just ensured the noise budget runs in an operator machine. It needs access to the SusSVN, to the matlabtools folder of the SeiSVN, and access to the ISI2SUS projection matrices saved in /opt/rtcds/userapps/release/isc/common/projections/
The changes are current as of SusSVN revision 12226.
Travis has asked for a temporary bypass on the GV7 cell phone alarms while this gate valve is soft closed
Bypass will expire:
Tue Apr 15 01:43:34 PM PDT 2025
For channel(s):
H0:VAC-LX_GV7_ZSM179A_VALVE_ANIM
Alarms has been reconfigured to expect GV7 to be soft closed.
SR3 Measurements:
I had a hard time trying to take data at first (no matter the excitation amplitude we were seeing no movement on the ISI sensors), and we figured out that it was because the SUSPOINT matrix for HAM5 ISI had never been populated! We found the correct matrix values in $(USERAPPS)/isc/common/projections/ISI2SUS_projection_file.mat as ISI2SUSprojections.h1.sr3.EUL2CART, and used /ligo/svncommon/SeiSVN/seismic/Common/MatlabTools/fill_matrix_values.m to fill them in. Then I was able to run the transfer functions.
Data files can be found at /ligo/svncommon/SusSVN/sus/trunk/HLTS/H1/SR3/Common/Data/2025-04-15_2100_H1ISIHAM5_ST1_WhiteNoise_SR3SusPoint_{L,T,V}_0p02to50Hz.xml, and have been committed to svn as r12227.
This morning we decided to do the rest of the DOFs for the SUSPOINT to M1 measurements of PR3 and SR3.
For SR3:
Same setup as before:
Data files can be found at /ligo/svncommon/SusSVN/sus/trunk/HLTS/H1/SR3/Common/Data/2025-04-15_2100_H1ISIHAM5_ST1_WhiteNoise_SR3SusPoint_{R,P,Y}_0p02to50Hz.xml, and have been committed to svn as r12232.
For PR3:
Same setup as before:
Data files can be found at /ligo/svncommon/SusSVN/sus/trunk/HLTS/H1/PR3/Common/Data/2025-04-15_1431_H1ISIHAM5_ST1_WhiteNoise_SR3SusPoint_{R,P,Y}_0p02to50Hz.xml, and have been committed to svn as r12249.