Randy T., Camilla C., TJ S.
After the chiller was found tripped off and water was found in the plastic "leak containment apparatus" last week (alog89931), we expected to have to replace the expansion joint as we did in January 2024 (alog75657). Turns out, the expansion joint is okay but the fittings have loosened themselves overtime not just on this line but some of the others as well. More details below.
Today when Randy went to go swap the joint out for a used spare, he noticed that the fittings were very loose, not only on the TCSX supply line, but on a few others. He re-tightened all fittings and we decided to test it out slowly with water. Camilla tried to turn on the chiller, but it would shut itself off saying "low flow". She and I then closed the 3way valve in back which makes the chiller run in a closed loop within the chiller. This worked to get it to run. We then slowly opened that valve to slowly allow water to start flowing down the supply line. Randy was waiting and watching at the joint and never saw any water leaking out during the ~5 min test.
At this point we think that the water just leaked out of the loose fittings when the quick connect was disconnected last week. The updated chiller settings most likely helped and turned off the chiller before the pressure reached levels that could cause damage to the system. We will add checking the tightness to the quarterly pipe check FAMIS task.
Next steps - start on replacing the TCSX table flex lines, and work on making a unistrut cage around the quick connects to avoid bumps in the future.
TITLE: 04/21 Day Shift: 1430-2330 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Planned Engineering
INCOMING OPERATOR: None
SHIFT SUMMARY:
Covering the morning Ops shift & handing off to RyanS.
LOG:
Tue Apr 21 10:10:27 2026 INFO: Fill completed in 10min 24secs
WP13186 TJ, Dave, Erik:
10:07 h1guardian1 powered down for OS upgrade to Debian13.
Upgrade to debian 13 is completed. Nodes are running, communicating via epics and NDS and controllable from the workstations. Some more testing is needed of git archiving etc.
TITLE: 04/21 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, 2mph 3min avg
Primary useism: 0.01 μm/s
Secondary useism: 0.29 μm/s
QUICK SUMMARY:
BSC2 work continues, CDS work. HAM5 & 6 HEPI has been down overnight due to HEPI pump system issues noted yesterday.
Workstations were updated and rebooted. This was an OS packages update. Conda packages were not updated.
Madi, Camilla
Started ETMX Ring Heater test for HWS testing, turned up from 1W/segment to 2W/segment. Plan to leave until tomorrow.
TITLE: 04/20 Day Shift: 1430-2330 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Planned Engineering
INCOMING OPERATOR: None
SHIFT SUMMARY: Some BSC2 and cabling work done today. HAM5 and HAM6 HEPI are going to be down overnight since the HEPI pump is having issues.
LOG:
| Start Time | System | Name | Location | Lazer_Haz | Task | Time End |
|---|---|---|---|---|---|---|
| 14:40 | FAC | Kim, Nellie | LVEA | n | Tech clean | 15:32 |
| 15:09 | FAC | Randy | MidY | n | Rock cleanup on aisle MY | 16:10 |
| 15:51 | FAC | Nellie | HAM Shack | n | Tech clean | 16:34 |
| 16:01 | VAC | Jordan | LVEA | n | CP1 RGA work | 16:29 |
| 16:44 | SEI | Jim | LVEA | n | BSC2 work | 17:49 |
| 16:57 | IAS | Jason | LVEA | n | FARO scoping | 17:28 |
| 17:20 | FAC | Randy | LVEA | n | Just looking at HAM6 cleanroom | 18:07 |
| 17:21 | VAC | Jordan, Gerardo, Travis | LVEA | n | CP1 pump work | 18:44 |
| 17:34 | SEI | Mitchell | LVEA | n | BSC2 work | 17:49 |
| 19:10 | EPO | Jeff, +1 | LVEA | n | Tour | 20:17 |
| 19:47 | EE | Fil | MER | n | HAM6 cabling | 00:20 |
| 20:18 | VAC | Travis, Jordan, Gerardo | LVEA | n | CP1 pump work | 23:29 |
| 20:23 | CDS | Dave | EX | n | Reboot BRSX | 21:30 |
| 20:25 | FAC | Randy | LVEA | n | Looking at HAM6 some more | 21:43 |
| 20:29 | Jennie | Optics Lab | n | Looking for laptop | 20:40 | |
| 20:37 | Betsy | LVEA | n | Looking at HAM6 with Randy | 21:46 | |
| 20:44 | IAS | Jason | LVEA | n | Grabbing FARO parts | 20:57 |
| 21:10 | SEI | Jim | LVEA | n | Talking with Betsy / SEI work | 23:28 |
| 21:19 | TCS | Madi, Camilla, Maya | OpticsLab, LVEA | n | Grabbing parts | 21:51 |
| 21:30 | CDS | Dave | EY | n | Verifying 24V power supply | 22:02 |
| 21:44 | SEI | Mitchell | LVEA | n | BSC2 work | 23:28 |
| 21:52 | TCS | Camilla, Madi, Maya | EX | y(local) | HWS work | 23:06 |
| 22:12 | IAS | Jason, RyanC | LVEA | n | Setting up FARO for tomorrow | 22:40 |
| 22:22 | TCS | TJ | LVEA | n | Draining TCS chiller line | 23:19 |
| 23:15 | SUS | Ibrahim | LVEA | n | BBSS ExpreSS | 23:33 |
In prep for WP13185 to replace the flex lines on the table and the expansion joint, I've drained and vacuumed the TCSX table and then I just used gravity to drain most of the water in the supply line, enough so that the expansion joint is free of water.
WP13182 BRS-EX recovery
Jim, Patrick, Dave
I tried to reboot, but ended up power cycling, h1brsex. Patrick started the code and IOC. Since then it has been attempting to damp over the past few hours.
FAMIS 31134
The ISS diffracted power has drifted down a bit over the past few days, so I'll bring that back up towards 4%. No other major events of note.
Mon Apr 20 10:09:19 2026 INFO: Fill completed in 9min 16secs
TITLE: 04/20 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: 9mph Gusts, 5mph 3min avg
Primary useism: 0.03 μm/s
Secondary useism: 0.19 μm/s
QUICK SUMMARY:
BSC2 work today
ETMY SWWD tripped at 01:17 PDT this morning due to an EQ. I have reset the DAC drives.
Sun Apr 19 10:06:23 2026 INFO: Fill completed in 6min 19secs
Closes FAMIS 28639
Last checked in alog 89720
TCSX read 30.8 - nothing added
TCSY read 10.6 - nothing added\
No water in small cup under the slow leak
TCSX is reading HIGH PRESSURE FAULT. See attached picture.
Betsy and I locked and tagged out the CO2X chiller, it will remain off until all needed repairs and safety documents have been completed next week.
At 15:44UTC the chiller tripped off with a HIGH PRESSURE fault, as found by Ibrahim. The CR verbal machine also alerted Ryan with a "low flow" warning.
I went out to the LVEA inspecting the pipes and found that the outgoing CO2X line was disconnected at the quick-connect, image. There was no water on the floor, so the quick-connect did it's job. Maybe this was already loose and we need to add the the pipe inspection FAMIS to inspect these connections, but. there was also lot of work in that area today. I inspected and reconnected the quick-connect, it did not seem damaged.
At out weak point in the chiller lines at the flexible baffle in the pipe bridge, the plastic sheeting that had been attached to catch any spilled water had a small amount of water in it photo, but none leaking out. Expect this water would have been pushed out a small break in the rubber while the chiller was trying to push water around the incomplete lines before the high pressure sensor in the chiller tripped it off. We will inspect and probably repair this part next week. In the meantime with water dripping out of the pipe bridge connection, we are fine to leave the chiller locked out with water in the lines.
TJ, Camilla. Trending the pressure values doesn't tell us much. The chiller appears to go to the high pressure fault and trip off before the pressure channels register a high pressure, see attached. ANALOG1 PSI starts at 65 PSI and ANOLOG2 started at 26 PSI, after the chiller trips off, these increase to 6500 PSI (unphysicial) and 44 PSI. The chiller must have an additional pressure sensor it uses to trip off. Current settings are to trip off at 80 PSI, see FRS 30283.
(Travis, Randy, Gerardo)
On Monday, the -Y door went on the HAM1 chamber with some minor issues not noted on previous installations, for some reason we had two minor misalignments: one, the door did not hung parallel to the HAM's flange,small tilt towards the outside on the upper part of the door, maybe the pick point slid forward. Two, the door required a clocking move, we pinned two holes spanning 5:12 O'clock, then rotated the door clockwise a bit until all of the holes aligned, then a small movement on the -Z to complete the alignment about 1/8". After all of that the door looks pretty concentric to the chamber flange.
Something to note, a dirty glove was found inside the chamber, yes inside the chamber under the support tube on the -Y side of the chamber, as I write, I nod, because it does not take much time to get this dirty thing out of the chamber.
HAM1 +Y door was installed today after replacing the inner o-ring, which had fallen out during door removal.
O-ring install went fairly smooth, only popped out of the groove a couple times, but we were able to get it seated properly and continued with door install.
No issues encountered, and we started pumping the HAM1/2 annulus volume to confirm there were no door o-ring leaks. Currently both aux carts are at ~2E-5 Torr.
Update on annulus sytem
Pumping continues with two aux carts, one connected to each chamber (HAM1 and HAM2 annulus), last thursday we turned the ion pumps (see trend data attached), and HAM1 responded well, however the ion pump for HAM2 railed, after a couple of wake up hits it started working. Currently both systems are doing good, probably they'll be ready to run on ion pumps soon.
Both aux carts are now removed from the annulus system for HAM1/HAM2. The annulus system is back to nominal, at vacuum and under ion pump management, the main volume for HAM1 is at atmosphere and ready to pump down as soon as it is requested.
From the previous alog post, Sheila measured a power drop across BL2 lens.
Here I modeled the loss of the 700um beam waist across the 2.5mm BL2 lens aperture.
The expression for the transmitted power obtained by modifying the Gaussian beam equation to include a displacement d2 = dx2 + dy2 is shown here.
And here's the contour plot for the loss (1-T) across the lens aperture for a beam transversing across various spots on the lens.
Me and Sheila are checking on the geometry of the setup.
The BM3 mirror mount IXM100.2 has a 100 pitch screw adjustment ( correspond to 100 turn per inch translation), and the beam appeared to be clipped symmetrically for 1/8 rev. For the mirror mount of 1.87" width, this correspond to a mirror rotation of 1.3mrad.
The distance between BM3 and BL2 is 148mm, from the mirror rotation, the IR beam angular deflection is 2.6mrad, this implies an aperture size of 0.4mm. Something is not right, and it's a mystery that requires more investigation.
The aperture stop installed is D2000339: 0.2" (5mm) diameter.
Varun, Stefan
We measured the (one-way) SRC Gouy phase to be 28.97deg +-0.11deg (statistical) +-0.43deg (systematic).
We used a method pioneered in KAGRA (klog 9241 and 9246). A similar method was used for the PRC Gouy phase measurement(alog 52504).
Plots:
- Plot 1: SRC scan across 6 fringes. Blue: AS_C_SUM, Red: AS_C_SEG2 (both derived from IOP channels). Magenta: round trip Gouy phase fit from the two results.
- Plot 2: Raw data strech of 6 best fringes.
Method:
- Align BS and SRM (in SRY) carefully (especially BS)
- Misalign SRM by 70 urad (we did pos pitch)
- Let SRMI freely swing (i.e. SRM and BS aligned, PRC misaligned)
- SRCL1 and MICH1 gains 0 (we don't need the control loops)
- Put an offset in SRCL2_OFFSET (we used -1e6cts)
- Turn off all whitening on ASC-AS_C
- We want the LSC trigger to fire and stay latched (and apply the offset) when ASC-AS_C reaches the darkest possible spot.
This corresponds to the BS in the correct position, increasing the finesse of the SRC to its maximum.
- We achieved that with a negative trigger matrix element, a slightly positive enable threshold (since AS_C swing slightly negative), and a very negative disable threshold
We used: H1:LSC-TRIG_MTRX_4_14 =-100, H1:LSC-SRCL_TRIG_THRESH_ON = 0.015, H1:LSC-SRCL_TRIG_THRESH_OFF = -100
- To read the data we need the highest possible data rate. So in addition to H1:ASC-AS_C_NSUM_OUT we recorded the IOP channels
H1:IOP-ASC0_MADC6_TP_CH9, H1:IOP-ASC0_MADC6_TP_CH10, H1:IOP-ASC0_MADC6_TP_CH11, H1:IOP-ASC0_MADC6_TP_CH12
- Those IOP channels are before the fixed anti-whitening filter. So we did the anti-whitening filter in diaggui ('zpk([40],[0.4],1,"n")').
- The 4 quadrants of ASC-AS_C saw different combinations of the higher order modes.
- We used SEG4 (CH9) for finding the 00 modes.
- We used SEG2 (CH11) and the sum of all 4 segments for 10 modes (red and blue traces respecively).
- We chose a bank of 6 fringes with very low AS_DC values - those have the highest finesse.
- A spline fit was used to interpolate the time to degrees in-between 00 peaks.
- We calculated the mean from the red and blue traces separately. Their mean is reported as final value.
- We calculated the standard deviation of the mean from the red and blue traces separately. The maximum of the two errors is reported as statistical error.
- The difference between the red and blue result is reported as systematic error.
The code and raw data is found in /ligo/home/controls/sballmer/20191022.
Should add that the SR3 ring heater, as well as the ITM TCS system, was turned on during the measurement. Snap shots are attached.
The time of measurement was GPS 1255829128, Oct 23 2019 01:25:10 UTC.
At the time of this measurement, CO2 heating was central. The CO2 FLIP1MON was 0 and FLIP2MON was 1. Comparing this to the current values and the MEDM that says we are currently using annular heating, I believe this means that these measurements were done with central CO2.