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Reports until 16:17, Tuesday 20 May 2025
H1 SUS (GRD)
oli.patane@LIGO.ORG - posted 16:17, Tuesday 20 May 2025 (84488)
New SUS guardian state for taking health check transfer functions

TJ, Jeff, Oli

It was brought up that it would be nice if we had a guardian state for taking our regular suspension health check transfer functions, since it requires a few different things to be changed, some of which differ from sus type to sus type. So I created three new states, PREP_HEALTH_CHECK (67), which gets everything in the correct state for running our default transfer functions, HEALTH_CHECK (70), which is just an idle state, and REVERT_HEALTH_CHECK (73), which reverts the changes made in PREP_HEALTH_CHECK. I set the edge of PREP_HEALTH_CHECK to come off of FULLY_ENABLED, and then REVERT_HEALTH_CHECK comes back around and goes into FULLY_ENABLED (state graph).

The things that need to be true for every suspension type are:

Additionally, there are some sus specific requirements:

I've updated SUS.py, (in $(USERAPPS)/sus/common/guardian/), sustools.py (in $(USERAPPS)/sus/common/scripts), and susconst.py (in $(USERAPPS)/sus/h1/guardian/) with the new states, function additions, and dictionary additions needed to get everyone in the right state for taking transfer functions.
 
Examples:
SUS ALIGNED HEALTH_CHECK Extra changes (on top of default req)
PR3 aligned health check None
ITMX aligned health check Turn off any Main Chain L2 to Reaction Chain R0 damping/tracking (R0 L2 witness damp)
BS aligned health check (BSFM) Turn off any optical lever damping loops
TMSX aligned health check (TMTS) Turn off any QUAD to M1 damping / tracking
OMC aligned health check (OMCS / OMs / RMs) Turn off any ISC DC centering input

Every suspension's guardian has been reloaded and tested, and the scripts have been committed to svn as r31488 (SUS.py), r31489 (sustools.py), and r31483 (susconst.py).

I will be talking to Stuart Aston at LLO to make sure they update their susconst.py when they decide to pull this newest version of the SUS code.

Images attached to this report
X1 SUS
ibrahim.abouelfettouh@LIGO.ORG - posted 15:43, Tuesday 20 May 2025 (84489)
BBSS Shear Plates Installed

Ibrahim, Betsy

Today Betsy and I successfully installed the shear plates onto the BBSS. In the attached pictures, you can see:

Next, I intend to install the HRTS mount, the HRTS itself and start B&K (with Rahul)

Images attached to this report
H1 SEI
ryan.short@LIGO.ORG - posted 13:59, Tuesday 20 May 2025 (84486)
ISI CPS Noise Spectra Check - Weekly

FAMIS 26044, last checked in alog84268

The script reports BSC high frequency noise is elevated for the following sensors:

ITMX_ST1_CPSINF_V1
ETMY_ST2_CPSINF_V2

Non-image files attached to this report
LHO VE
jordan.vanosky@LIGO.ORG - posted 13:41, Tuesday 20 May 2025 (84485)
Morning Purge Air Checks 5-20-25

Dry air skid checks, water pump, kobelco, drying towers all nominal.

Dew point measurement at HAM1 purge inlet port, prior to pumpdown, -43.7 °C

The HAM1 purge exhaust dewpoint at top of chamber was measured to be -40.3C just before turning off the purge and starting pumpdown.

Images attached to this report
H1 CDS
david.barker@LIGO.ORG - posted 12:52, Tuesday 20 May 2025 - last comment - 14:13, Tuesday 20 May 2025(84482)
HAM1 pump down, monitor vacuum pressure with temporary EPICS IOC

Jonathan, Patrick, Janos, Ryan, Dave:

The HAM1 pressure gauge PT100 is temporarily only available as a raw voltage signal (H0:VAC-LY_X0_PT100B_PRESS_VOLTS).

I wrote an EPICS IOC which reads this voltage signal, converts it to a pressure (Torr) and exports it as a "H1" version of the PT100B cold cathode signal. The new EPICS channel is:

H1:VAC-LY_X0_PT100B_PRESS_TORR

The new IOC is currently running in a tmux session on opslogin0. It was started at 11:31 Tue20may2025, at which time HAM1 was still at atmospheric pressure (10.0V, 750Torr)

WP12558 was opened to add this new channel to the DAQ so that this week's HAM1 pump down could be trended.

We restarted the DAQ 0-leg at 12:16, the EDC at 12:17 and the 1-leg at 12:22

I took the opportunity to complete WP12523 and add the new CDS rack power strip EPICS channels to the EDC.

EDC details:

Addition of H1EPICS_VACHAM1.ini (3 channels) and H1EPICS_PWRSTRIP.ini (36 channels) for a total additon of 39 channels, which give a new total of 59,311 chans in the EDC.

I added the new HAM1 pressure channel to the vacuum overview (see attached).

The pump down was already on its way when we added it to the DAQ, attached trend shows data is available from 12:22 onwards, at which time the pressure was at 200Torr

Images attached to this report
Comments related to this report
david.barker@LIGO.ORG - 13:17, Tuesday 20 May 2025 (84483)

1-day pump down trend available CDS Ndscope Trender

david.barker@LIGO.ORG - 13:20, Tuesday 20 May 2025 (84484)

formula for converting Gauge voltage (v) to pressure in torr (p) is:

p = 10**(((v-7.75)/0.75) - 0.125)

The valid range for v is:

0.774 < v < 10.000

david.barker@LIGO.ORG - 14:13, Tuesday 20 May 2025 (84487)

gauge user manual pdf:

https://www.inficon.com/media/9695/download/Trigon%E2%84%A2-BCG552-TripleGauge%C2%AE-Operating-Manual-.pdf?v=3&inline=true&language=en

 

LHO VE
david.barker@LIGO.ORG - posted 10:40, Tuesday 20 May 2025 (84480)
Tue CP1 Fill

Tue May 20 10:05:48 2025 INFO: Fill completed in 5min 44secs

 

Images attached to this report
H1 CDS
david.barker@LIGO.ORG - posted 09:38, Tuesday 20 May 2025 (84479)
Loss of some h1digivideo5 cameras on Friday 16th May 2025

FRS34130

On Friday 16th May 2025 several cameras whose processes are running on one of the new AMD EPYC 9124 servers stopped working. Their MEDMs went "white-box" and their camera images went "blue-screen". The cameras and their last good data points are:

FC2 04:02

FC_TRANS_B 09:00

ETMX 10:03

ETMY 11:01

Note ETMX h1cam25 was not pingable, all the others were.

Yesterday I went to EX and EY to investigate. I power cycled both end station cameras by disconnecting their ethernet from the POE injector. After restarting their processes they came back online.

On the way back I did the same for the FC_TRANS_B from the CDS mezzanine in the FCES.

This morning I found that FC2 had also stopped (more about that laater) and got it running again by just restarting its process, no camera power cycle needed.

Looking at the logs we found 

"WaitObject duplicate failed (0): Too many open files. Reached open files limit"

type errors around these times. Debian has a limit of 1024 open file descriptors per process, and scanning the /proc/<pid>/fd/ dir sizes for h1digivideo5 showed that FC2 had 1024 open, which is how we found that camera had stopped working at 04:02 Friday.

Two immediate action items:

  1. install num_open_fd check in cds_report for camera processes to trend and alert on an hourly basis if we are getting close to the limit
  2. investigate if pylon code is responsible and if so can it be fixed.

 

LHO General
ryan.short@LIGO.ORG - posted 07:38, Tuesday 20 May 2025 (84478)
Ops Day Shift Start

TITLE: 05/20 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: 4mph Gusts, 1mph 3min avg
    Primary useism: 0.03 μm/s
    Secondary useism: 0.28 μm/s
QUICK SUMMARY: Pumpdown of HAM1 starts today as the main activity. The LVEA is currently Laser SAFE.

H1 CDS
erik.vonreis@LIGO.ORG - posted 07:32, Tuesday 20 May 2025 (84477)
Workstations updated

Workstations were updated and rebooted.  This was an OS packages update. Conda packages were not updated.

H1 CDS
david.barker@LIGO.ORG - posted 23:38, Monday 19 May 2025 (84476)
VACSTAT single alarm on BSC3 gauge glitch

VACSTAT went into sensitive mode after BSC3 PT132_MOD2 glitched, spending 2 seconds at 3.2e-07Torr before returning to 1.5e-07.

I have restarted VACSTAT to clear this glitch.

Images attached to this report
LHO VE
janos.csizmazia@LIGO.ORG - posted 17:36, Monday 19 May 2025 - last comment - 00:05, Wednesday 21 May 2025(84475)
HAM1 VAC works
Gerardo, Jordan, Travis, Randy, Janos

Today between 10 am and 2 pm both the Y+ and Y- HAM1 doors have been installed. The installation went smoothly, no issues were found.
A valve on the new interlock gauge-assembly was opened, and the HAM1 volume will be purged overnight. This is to clean the in-vacuum surfaces before pumpdown, resulting in lower gas load and therefore faster pumpdown.
After the door installation, the pumpdown of the joint HAM1/HAM2 Annulus volumes have been started. 2 turbo/pumping cart systems are pumping the volume, they are standing next to HAM1 and HAM2 - see attached photo.

Please do not move the pumping carts, as it can result in immediate damage in the turbo pumps. If you still need to do any activities which need these pumping carts to be moved, please talk to vacuum team members first!
Images attached to this report
Comments related to this report
gerardo.moreno@LIGO.ORG - 00:05, Wednesday 21 May 2025 (84502)VE

Door crew in action, -Y door for HAM1.

Images attached to this comment
H1 General
oli.patane@LIGO.ORG - posted 16:36, Monday 19 May 2025 (84474)
Ops Day Shift End

TITLE: 05/19 Day Shift: 1430-2330 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Planned Engineering
INCOMING OPERATOR: None
SHIFT SUMMARY:

Doors are on HAM1 and things are being wrapped up in order to start pumping down!
LOG:

Start Time System Name Location Lazer_Haz Task Time End
14:15 FAC Kim, Nellie LVEA n Tech clean 14:58
15:20 VAC Jordan LVEA n Turning down purge air on HAM1 15:27
15:51   Oli LVEA YES Transitioning LVEA to laser hazard 16:06
15:59 - Corey EX n Wallet hunt 16:19
16:00 FAC Kim, Nellie EX n Tech clean 17:08
16:11 OPS RyanC LVEA Y Restart DM5 16:11
16:00   Camilla LVEA YES Turning down power 16:37
16:00 SUS Jeff, Rahul LVEA YES Checking RM pointing (Jeff out 16:40) 16:43
16:00 EE Fil CER YES Checking if PM1 is jumpered 16:14
16:39 EE Fil LVEA n Running cables 18:21
16:40 EX Eric EX n Looking for hot breakers 17:59
16:40   Camilla LVEA YES Transitioning us back to laser safe 16:48
16:44 ISC Betsy LVEA n Last minute checks on HAM1 table 17:40
16:57 SUS Jeff CER n Checking SUS coil drivers 17:00
17:04 VAC Travis LVEA n Prepping for doors 18:34
17:09 FAC Kim, Nellie EY n Tech clean 17:50
17:09 PCAL Tony PCAL Lab y(local) Packing up standards 18:28
17:24 VAC Jordan, Janos LVEA n HAM1 doors 18:41
17:26 VAC Gerardo LVEA n HAM1 Doors 18:41
17:44 FAC Chris MY n Checking noisy bearing 18:24
17:45 EE Jackie LVEA n Helping Fil with cables 18:21
17:53 SUS RyanC CR n OpLev charge meas for ends 19:21
18:16   Elenna LVEA n Watching doors get put on 18:21
18:22 EE Fil, Jackie CER n ISC cabling for HAM1 19:36
18:34 ISC Camilla, Betsy LVEA YES Transitioning to Laser Hazard and checking beams at ports 19:07
18:57 FAC Nellie LVEA CERish YES Restocking garb 19:26
19:24 VAC Jordan LVEA N Door work 21:51
19:33 VAC Janos, Gerardo, Travis, Randy LVEA n Putting on second door (Janos, Travis, Randy out 21:30) 21:51
19:44 FAC Eric EY n Checking breaker panel temps 21:16
20:15 CDS Jonathan, Dave MSR n Swapping frame writer power supply 20:47
20:46   Jeff LVEA n Returning laptop 20:48
20:47 TCS Camilla LVEA n Checking CO2X table parts (laser is off) 21:13
20:48 CDS Dave EY n Checking cameras 21:56
21:13 PCAL Tony PCAL Lab y(local) Starting measurement 22:46
21:40 FAC Randy LVEA n Helping with doors 21:51
21:46 EE Fil LVEA n Finishing up HAM1 cables 23:34
21:46   Richard LVEA n Trying to not help out 21:55
21:56 CDS Dave EX n Checking other cameras 22:58
22:26 SEI Jim, Mitchell LVEA n Moving Class A stuff out of HAM3 cleanroom 22:43
22:41 VAC Jordan, Gerardo LVEA n Prepping HAM1 for pumpdown 23:34
23:17 TCS Camilla LVEA n Measuring a distance and looking in the TCS cabinets 23:34
H1 TCS
thomas.shaffer@LIGO.ORG - posted 15:14, Monday 19 May 2025 (84364)
TCS Chiller Sock Filters Replaced

FAMIS 31406

The sock filters had slight discolorization, but there were floating string-like particulate in both reservoirs (pic1 & pic2). This isn't a new finding, but I was hoping after the last flush in October that it would have reduced the amount of floaters over time as they were filtered out, but this doesn't seem to be the case.

Images attached to this report
H1 DAQ
jonathan.hanks@LIGO.ORG - posted 13:55, Monday 19 May 2025 - last comment - 16:28, Monday 19 May 2025(84466)
WP 12455 Replace failed power supply on h1daqframes-1

As per WP 12455 Dave and Jonathan replaced the power supply on h1daqframes-1.  Due to the available space in the rack we decided to power off the system so that we could move it safely and replace the power supply.

We did some double checking to verify which machines where hooked together.  We followed the physical connections and cross checked them with the names and numbers for interfaces on each machine.  This was good as the labels on the front of the system where wrong.  This is the frame disk associated with h1daqfw1.

We powered down h1daqfw1, verified that the link to h1daqframes-1 had gone dark.  After that we powered off h1daqframes-1 pushed it forwared enought to replace the power supply, pushed it back in th place and restarted it.

After the disk server was back we restarted h1daqfw1 as well.

Dave will fix the labeling.

Comments related to this report
david.barker@LIGO.ORG - 16:26, Monday 19 May 2025 (84472)

Labels are now good. MSR-RACK09 U02-U03 (bottom unit) is h1daqframes-1. MSR-RACK09 U04-U05 (next to bottom unit) is h1daqframes-0.

david.barker@LIGO.ORG - 16:28, Monday 19 May 2025 (84473)

Closed FRS27399

H1 AWC
sheila.dwyer@LIGO.ORG - posted 15:58, Thursday 15 May 2025 - last comment - 16:44, Tuesday 03 June 2025(84419)
SR3 heater on overnight

TJ, Camilla, Sheila

TJ and Camilla got the HWSs working, and now we turned on the SR3 heater at 15:54 UTC, 2W requested power.  This is to do a check of the SR3 heater calibration and range similar to 27262

Comments related to this report
camilla.compton@LIGO.ORG - 10:53, Tuesday 20 May 2025 (84481)

SR3 heating up can be seen on the HWS signals but is not particulatly clear, see attached.

Images attached to this comment
jennifer.wright@LIGO.ORG - 10:12, Tuesday 03 June 2025 (84744)

Looking at when this test was done at LLO, the lens changing happened over a period of three hours and the lens power increased in the same direction on both HWS, so its possible our HWS are not a good witness for the SR3 curvature change.

jennifer.wright@LIGO.ORG - 10:25, Tuesday 03 June 2025 (84746)

Aidan calculated 2.45 uD/W at LLO, and we get 9.44 uD/W (from the H1:TCS-ITM{Y,X}_HWS_PROBE_SPHERICAL_POWER  trends with an estimated noise of 4.48e-12uD/W.

camilla.compton@LIGO.ORG - 11:43, Tuesday 03 June 2025 (84751)

Looked closer at these HWS signals during SR3 heater heat up and cool down. In all these plots, the two t-cursors are used as the reference and shown HWS live image.

  • Heat up plot attached
  • Cool down plot attached (ITMX was misaligned so there's no HWS data)

Some strange things:

  • ITMX heat up ndscope spherical power looks the opposite direction of ITMY, this isn't physical. Looking at the HWS Live plot, this isn't really want's happening, it appears that the SR3 signal just appears if the edge of ITMX is heating up so the center that the calculations are made from isn't correct, making the calculated spherical power wrong.
  • In both the heat up and cool down of the ITMY signal, there appears to be two steps with a flat region in the middle. Looking at the the flat region only, attached, it appears that the spherical power is continuing to change in the expected direction, unsure why this change isn't shown in the calculated spherical power.
Images attached to this comment
jennifer.wright@LIGO.ORG - 11:54, Tuesday 03 June 2025 (84753)

With the numbers from ITMY HWS only, and looking at the 3hr 11 m cooldown in Camilla's photo, the lens change is 6.68e-6 Dioptres/W taking into account that the HWS beam passes twice through SR3.

jennifer.wright@LIGO.ORG - 16:44, Tuesday 03 June 2025 (84768)

After talking with Camilla, she reminded me the change in RoC (delta R) =/= 2/(delta D),

where D is defocus (1/focal length).

but instead delta R = 2/(2/R + delta D) - R

Where R=36.013m is given in https://git.ligo.org/IFOsim/ligo-commissioning-modeling/-/blob/main/LHO/yaml/lho_O4.yaml?ref_type=heads

delta R comes out as 4.3mm +/-  0.18 mm (which is the same order of magnitude as the change Aidan measured in alog #27262 at LLO). 

The error was estimated from looking at the noise on the spherical power and propagating through the calculation of delta R.

H1 ISC
sheila.dwyer@LIGO.ORG - posted 16:27, Wednesday 07 May 2025 - last comment - 15:21, Monday 19 May 2025(84307)
HAM1 POP path beam profile and distance measurements

location number on drawing

distance horizontal 13.5% diameter [um] vertical 13.5% diameter [um] photo of profiler location photo of profiles photo of beam scan measurements
1 52 mm from dichroic M10 6243 64040 here and here 9022 9023
2 147 mm from dichroic M10 6202 6365 9028 9026 9027
3 119 mm from HR of 50/50 BS M15, also 295mm from center of lens L2 870 874 9031 9030 9029
4 153 mm from HR of 50/50 BS, approximate location of LSC diode 279 284 9035 9032 9033
5 128 mm from HR of 50/50 BS 721 726 9036 9037 9038
6 139 mm from HR of 50/50 483 490 9041 9040 9039
7 353 mm from HR of 50/50 BS 3280 3372 9042 9043 9044

Camilla made these measurements with 20W input power into the IMC, PRM and ITMY misaligned single bounce beam.  We didn't place the 90/10 BS M12 in the pop path yet so that we would have about 35uW to measure beam profiles. There's a rough pen sketch of where these locations are in this photo.

Camilla also made ruler measurements of some distances:

Images attached to this report
Comments related to this report
elenna.capote@LIGO.ORG - 19:48, Wednesday 07 May 2025 (84313)

I think these measurements look pretty good, and the result is not that much different than the model (at least in terms of where to put the diodes). The biggest surprise is that Keita and I were pretty sure the beam coming into HAM1 is just over 2 mm in radius, when in reality it is more like 3 mm in radius.

I have attached plots of both the horizontal and vertical propagations, but you can see that the results for each direction are very similar. The black points are the measurements Sheila and Camilla took today, and I fit them with a la mode and the 2 inch POP lens (f = 334 mm), using the distances from the dichroic mirror that Sheila and Camilla measured.

If we place the POP LSC diode about 140 mm from M15 and the POP WFS about 200 mm from M15, we should get the beam sizes we want on each. I think these positions are a little closer to M15 than they are in the drawing, but I don't think that's a problem.

I also attached my a la mode script.

Images attached to this comment
Non-image files attached to this comment
sheila.dwyer@LIGO.ORG - 15:21, Monday 19 May 2025 (84471)

Linking here that Keita added distances to the refl air and popair periscopes here: https://alog.ligo-wa.caltech.edu/aLOG/index.php?callRep=84345

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