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Reports until 09:04, Thursday 15 May 2025
LHO VE
jordan.vanosky@LIGO.ORG - posted 09:04, Thursday 15 May 2025 (84406)
Morning Purge Air Checks 5-15-25

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

Dew point measurement at HAM1 -43.9 °C.

Images attached to this report
H1 General
anthony.sanchez@LIGO.ORG - posted 08:57, Thursday 15 May 2025 (84405)
HVAC Fans Vibration Sensors Health check Weekly

FAMIS - 26378 Checking HVAC Fans Vibrometers.

Fans dont look too bad aside from H0:VAC-MY_FAN_270_1_ACC_INCHSEC which seems to be a  Noisier fan.

Images attached to this report
H1 General
anthony.sanchez@LIGO.ORG - posted 07:50, Thursday 15 May 2025 (84404)
Thursday morning Ops shift start

TITLE: 05/15 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: 12mph Gusts, 8mph 3min avg
    Primary useism: 0.02 μm/s
    Secondary useism: 0.08 μm/s
QUICK SUMMARY:

LVEA is LASER Safe. Hartman Lasers are on but are Eye safe and are ~780nm green/blue in color.

HAM1 ISI is currently unlocked.

Today's  Agenda:
CS:
HAM1 optical Alignment checks
HAM1's Glamour shots.
HAM1 Ground Checks.
Cable Tray work.
GOUI phase measurements in the output arm
TCS work?
 

EX
More wind fence work.

EY
SEI BRS work.

H1 SEI
jim.warner@LIGO.ORG - posted 17:03, Wednesday 14 May 2025 - last comment - 16:11, Thursday 15 May 2025(84403)
HAM1 ISI testing so far

Now that ISC is done with their alignment, I have been working on testing the ISI. Last night TJ and I unlocked and balanced the ISI, I did some quick tests to make sure the actuators were pushing where I expected them and found the horizontal and vertical actuator for each corner was swapped, so I switched the cables at the chamber. This morning I did some tests like range of motion and CPS linearity and some quick spectra to check that all of the sensors looked more or less the same and a quick set of tfs to look for rubbing. Now starting my long overnight tfs, so hopefully there are no big eqs overnight. If those go well, I hope to have everything for the testing report by the afternoon tomorrow.

Attached images are some of the tests I did today. First image is CPS linearity, which looks kind of ratty because I think the purge was too high, but otherwise looks okay. Second image shows unlocked asds for the CPS, GS13s and L4Cs. No glaring issues, but the kind of noisy V2 GS13 and CPS made me think some rubbing or high purge was happening. Last image is a set of tfs I used for chamber closeout comparing the measurements on HAM8 from last year to HAM1 today. Looks okay for a quick measurement.

Images attached to this report
Comments related to this report
jim.warner@LIGO.ORG - 09:24, Thursday 15 May 2025 (84407)

L2L tfs look good. Still have some other information to collect.

Images attached to this comment
jim.warner@LIGO.ORG - 16:11, Thursday 15 May 2025 (84420)

My testing is done. Testing report is uploaded to E2500128. Payload was light by a lot during testing, it did not get better in chamber and there were a lot of beam dumps that got added that I don't have weights for, so the payload section of the report should be taken with a grain of salt.

H1 TCS
camilla.compton@LIGO.ORG - posted 17:00, Wednesday 14 May 2025 - last comment - 09:46, Thursday 15 May 2025(84401)
Corner Station Ring Heater and SR3 Chassis back on. ITMX RH back to 0.44W/segment

Fil, TJ, Camilla. WP 12533

We turned back on the RH and SR3 heater chassis which were turned off for venting. After these were turned on, ITMX came back to it's nominal value of 0.44W/segment.

TJ and I played with the inverse RH filters for a while on ITMX (instructions 50777),  turning ITMX up to 0.5W for a couple of hours, it doesn't really make sense to us what it was doing as it drops the power lower than the requested power which seems un-intuitive 68549. Now back at nominal 0.44W/segment with the RH inverse filter guardian back to NOMINAL (off). 

ETMY had come back to the incorrect value after the April power outage (last saved Beckhoff value maybe), so TJ turned that back to the nominal 1.3W/segment on ETMY too. 

Comments related to this report
camilla.compton@LIGO.ORG - 09:46, Thursday 15 May 2025 (84408)

The HWS signal from this RH turn does not look very clear plot, I removed a few dead pixels (wiki). The HWS spots on the  ITMX camera are not very bright plot (even set to minimum frequency 1Hz), so TJ and I plan to replace the SLEDs.

Images attached to this comment
H1 General
anthony.sanchez@LIGO.ORG - posted 16:56, Wednesday 14 May 2025 (84402)
Wednesday Day ops shift End

TITLE: 05/14 Day Shift: 1430-2330 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Planned Engineering
INCOMING OPERATOR: None
SHIFT SUMMARY:
HAM1 Purge air has been turned Down.
HAM1 ISI is Currently Unlocked.
It got too windy to work on the Wind Fence  while elevated at EX, so wind fence work was postponed.
SEI BRS team found a broken cable on the BRS System.

TCS team Turned on the Hartman Wave front lasers. These are Eye safe lasers that have a power output of less than a mW. So if you see a blue-green ~780nm beam it MAY be from that.

Bees are still at EX.

LOG:                                                                                                                                                                 

Start Time System Name Location Lazer_Haz Task Time End
14:33 FAC Randy EX N Wind fence work 17:46
14:45 FAC Kim & Nellie LVEA N Technical cleaning 15:31
15:18 SEI Corey EX N Wind fence work 17:46
15:52 EE MARC EE LAB N Control Room Quiet Time for TEST N EE Lab 16:52
16:02 Bees Mitchel EX N Moving a box of Bees 17:47
16:09 VAC Jordan LVEA N Purge Air checks. 16:29
16:18 sei Jim Remote N HAM1 SEI health checks STAY AWAY 18:18
16:31 PEM Robert , Carlos, Keit EX N Getting parts 16:51
16:52 FAC Nellie EY N Technical cleaning 18:12
17:53 SEI Randy EX N Getting Equipment. 18:33
18:12 FAC Nellie LVEA N Technical Cleaning 19:10
19:11 FAC Nellie EY N Dropping off supplies 19:41
19:23 TCS Camilla LVEA No Turning on an Eyesafe Hartman laser 19:26
19:38 SEI Michael R & Shoshana EY N Pumping Down BRS 20:33
19:43 TCS Camilla LVEA N Power cycling the Hartman cameras 19:47
19:55 SEI Jim LVEA Ham1 N Locking ISI & Adjust CPS 21:14
20:09 VAC Jordan LVEA N Looking for parts 20:18
21:08 VAC Travis MidY N Looking for Eye bolts 21:20
21:13 FCA Mitchell & Randy LVEA n Liberating totes from their resting place 23:13
21:14 SEI Jim LVEA N Turned down Purge air 21:14
21:21 VAC Travis & Jordan LVEA N Craning over the X arm 21:49
21:42 TSC Camilla & TJ CER N Turning on HighVoltage for the Ring Heaters. 21:46
21:50 Guard TJ & Olli Control rm N Testing new guardian code 23:12
22:05 SEI Michael R & Shoshanna EY N BRS Wiring 22:40
23:18 VAC Janos Mid X&Y N Cryo pump survey 01:18

 

H1 ISC (OpsInfo)
thomas.shaffer@LIGO.ORG - posted 16:45, Wednesday 14 May 2025 (84387)
ALS Beckhoff vs Guardian locking error codes and expanded thresholds

Sheila D, TJ S.

Summary: the ALS arm guardians will now log the Beckhoff fiber locking error messages (untested though, testing later), and I've relaxed some of the thresholds set in Beckhoff. This is all nice, but I don't anticipate major gains from this.

Why: Our ALS locking has not been as reliable as it once was and has been one of the primary reasons for our locking not being fully autonomous. We have been discussing ways to help our ALS locking without large scale ALS table mode matching efforts, that would be very time and resource heavy, and has the chance to impact the ALS system negatively while we are still in a run. One issue that Sheila pointed out was that there were some times before this recent break that the Beckhoff automation code would flag some type of error and then stop the locking automation, the guardian node would see this and drop to the unlocked state and then start over. Sheila thinks that the Beckhoff errors are often based on far too strict of thresholds, and we should rely more on the guardian node for the error checking.

Guardian Changes: While the Beckhoff error codes for fiber locking are in the DAQ (H1:ALS-X_FIBR_LOCK_ERROR_CODE), this binary value needs a map to convert it back to something human readable. The guardian node doesn't look at these directly either, so we don't currently have an easy way to see what the Beckhoff automation is failing on...until now! The binary first has to be converted to hex, then the hex values and their associated error codes were found in a table from E1300482. I wrote a quick dictionary with a string message for the different binary values that are in epics. I've added this into the ALS nodes as a decorator to many different locking states. It will frequently check if there are any errors and log them so we can track what is happening a bit better. It won't be perfect though since it's just a decorator and it's possible that we will miss some of these error messages.

What codes have we been seeing? So in terms of error codes, what has been happening? In 2025, there was a trend in the X arm error codes that was seen during some times where ALS was fussy. Attachment 1 is an example where there is a "beat note out of range of frequency comparator" followed by a "laser error" code. This generally only lasts a few minutes though, and it looks like there were issues before these codes popped up. For the Y arm, the error codes are up for <1second and will often happen a minute or more after the arm loses lock, so I don't think this is too useful. The most common error codes that pop up are: Reference cavity transmission PD error, Reference cavity transmission below the limit, Beat note power too low.

Threshold Changes: One thing that has already been done was lower the PLL reference cavity transmission low limit (ref cav trans low limit) - alog83547. Today, I changed the PLL beat note frequency range from 3MHz-150Mhz to 2MHz-350MHz. The max frequency I saw was near 300MHz, so 350  seemed like enough to get it out of the way. Beat note minimum was already at -40dB, well out of the way already (see attachment 2 for examples). There might be some more places to relax the Beckhoff thresholds, but these related to the most common errors that we saw. Except for the very vague "Laser error" code. This will need more time to look into.

Images attached to this report
X1 SUS
oli.patane@LIGO.ORG - posted 16:25, Wednesday 14 May 2025 (84400)
BBSS TFs for new gold plated lower wire loop

Ibrahim, Betsy, Oli

Yesterday Betsy and Ibrahim swapped the wire loops for gold-plated wire loops (84378), so today Ibrahim took some top to top transfer function measurements and I've analyzed them (2025-05-14_1400_X1SUSBS_M1_ALL_TFs).

I have also made plots comparing them to our last measurements from February (83075). The new wire makes basically no difference (NoPlatingvsAuPlating).

I've also compared this latest measurement to LLO's latest measurement, and they are matching pretty well (AcceptanceReview).

These have all been committed to svn as r12307 and r12308 for the loop plating comparison.

Non-image files attached to this report
LHO General (EPO, PEM, SEI)
corey.gray@LIGO.ORG - posted 15:00, Wednesday 14 May 2025 (84396)
EX Windy Wind Fence Update

(CoreyG, MitchR, ChrisS, RandyT, JimW)

This week's wind fence work continues. With a couple of issues that continued from last week and were addressed:

  1. Soft Sand-- This has been an issue because it is fairly easy to get aerial lift wheels stuck in the sand.  Because of this, and since the big rental aerial lift was in position near the 1st panel (or "southernmost panel"), it was decided to do this panel's rework in one shot (vs the usual procedure of doing a step for all panel positions, and then moving to next steps for all positions, and so on)
  2. Bee Hive--Last Thursday, a beehive swarmed the wooden spool for the large wire.  A beekeeper was phoned in to help rehome this hive.  A beehive box was placed near the spool and today, this box was moved so the spool could be reinstalled in the trailer for use.

The first panel is mostly complete (on Tues) with one vertical cable remaining to be installed.  Old panels had thinner cables removed and are folded up for future availability and storage.

A water tank was delivered to EX (Tues) to allow daily soaks of the sand to help improve travel.

Today (Wed) was a windy day with sustained winds of around 15mph, so this morning mostly focused on non-at-height work.  The thick cables were cut for the remaining 3-panel locations

Images attached to this report
H1 SUS (SUS)
rahul.kumar@LIGO.ORG - posted 14:47, Wednesday 14 May 2025 (84397)
HAM1 vent work - PM1 transfer function measurement results look healthy

Attached below are the first set of transfer function measurement results for the Tip Tilt suspension PM1 in HAM1 chamber. The purge air flow in chamber was reduced to enable good coherence value and minimum cross coupling for this in-air measurements, and the results are very much visible when compared to earlier data (not posted here) which was very noisy. The plots attached below are for Length, Pitch and Yaw degree of freedom. Yaw dof. still shows some cross coupling/unwanted peak at 1.28Hz approximately, however it should go away in vacuum.

The templates for this measurement are stored at the following location,

/ligo/svncommon/SusSVN/sus/trunk/HTTS/H1/PM1/SAGM1/Data

2025-05-14_2100_H1SUSPM1_M1_WhiteNoise_L_0p01to50Hz.xml
2025-05-14_2100_H1SUSPM1_M1_WhiteNoise_P_0p01to50Hz.xml
2025-05-14_2100_H1SUSPM1_M1_WhiteNoise_Y_0p01to50Hz.xml

Hence, I can confirm that the suspension and the electronics chain is healthy.

Images attached to this report
LHO FMCS
eric.otterman@LIGO.ORG - posted 13:12, Wednesday 14 May 2025 (84389)
Chiller pump 1 overhaul
Chiller pump 1 at Mid X was overhauled; bearings and seal were replaced, stator was cleaned, and impeller was inspected. Current wear ring is in decent shape and was left in place. Pump was reinstalled this morning. 
H1 SUS
ryan.crouch@LIGO.ORG - posted 11:22, Wednesday 14 May 2025 - last comment - 15:44, Wednesday 14 May 2025(84386)
Misalignment GUI lock stretch gif

I branched and added some functionality to my misaligned GUI located on ASC IFO_ALIGN_COMPACTEST. I wrote another script to take a lock start and end and run the GUI every 5 minutes, take a screenshot then stitch them all together to make a gif of the lock so that we can see the changing alignments throughout lock stretches. It's a little slow, it was taking 20 minutes per hour till I realized I was redoing a large calculation each iteration unnecessarily, changing that brought it down to ~10 mins/hour of lock.

Here's an example gif of a short 2 hour lock starting at 03/30/25 18:13

Images attached to this report
Comments related to this report
ryan.crouch@LIGO.ORG - 15:44, Wednesday 14 May 2025 (84399)

I've added PM1 to HAM1 since posting this.

X1 SUS
ibrahim.abouelfettouh@LIGO.ORG - posted 15:04, Tuesday 13 May 2025 - last comment - 15:03, Wednesday 14 May 2025(84378)
BBSS Gold Plated Wire Loop Installed

Betsy, Ibrahim

Today, Betsy and I replaced the non-plated BBSS bottom wire loop with the gold plated wire loop, which was done successfully and took roughly two hours. We've confirmed the BBSS is centered and aligned. We will monitor and inspect the BBSS in the next few days and coming week. Stay tuned for new transfer functions etc.

Gallery of the wire loop below!

Images attached to this report
Comments related to this report
ibrahim.abouelfettouh@LIGO.ORG - 15:03, Wednesday 14 May 2025 (84398)

Went in to monitor the BBSS alignment after pulling this new wire. All alignments were the same as yesterday. I have since covered the BBSS to take TFs, which have been saved as of writing this. Next, the plan is to compare the gold plated wire loop TFs with the non-plated wire loop TFs.

Images attached to this comment
H1 SEI (SEI)
shoshana.apple@LIGO.ORG - posted 15:54, Monday 12 May 2025 - last comment - 15:04, Friday 16 May 2025(84366)
BRS ETMY Mass Adjuster Install
[Shoshana, Michael]

We've started preparing to install the BRS mass adjuster to the End-Y BRS. The plan is to follow the same procedure/same parts as the End-X install outlined in LIGO-T2400043 and SEI log 1886 (https://alog.ligo-la.caltech.edu/SEI/index.php?callRep=1886).
 We've taken apart the BRS and discovered that doesn't match the designs on the DCC. How the parts are arranged blocks access to where the pico-motor mount should attach, but we think we have a work around that should work.
The electronics/wiring of the BRS is as expected and we've finished all the wiring for the pico-motor so that it should attach to the feed through.
Assuming all goes well we plan on installing the mass adjuster parts and begin testin.
Images attached to this report
Comments related to this report
shoshana.apple@LIGO.ORG - 16:51, Tuesday 13 May 2025 (84379)SEI
[Shoshana, Michael]

We've managed to get all of the hardware/parts installed in and we've closed up the BRS chamber. We had to add an inch of shims beneath to motor mount in order to get it to fit/align properly, but otherwise there were only minor complications during installation. We've tested the pico-motor and the mass adjuster using the pico-motor driver that we brought from UW and both seem to work fine. 
For in air balancing, we left the new mass adjuster centered to increase range for future adjustments for when the BRS is pumped down and running, and tried to just stick to moving masses that are inaccessible when the BRS chamber is pumped down. We unfortunately reached the maximum range with the internal masses and had to slightly move the manual mass adjustment system (what is currently used to adjust the center of mass) from center, but that might be returned to center after we re-balance it when it's pumped down. Right now the resonance frequency looks to be around ~7mHz (around 130 second period) which is about the same as it was before Mass Adjuster installation, but we'll check again after the chamber has been pumped down.
Tomorrow we'll finish all of the wiring and electronics to hook up the pico-motor to the LIGO system. The plan is to pump down the BRS chamber tomorrow and re-balance and test the pico-motor some more.

The reference pattern has a higher intensity than expected and we aren't sure why. Right now our best guess is that the light source drifted slightly, and we'll look into it more tomorrow.


Images attached to this comment
jennifer.wright@LIGO.ORG - 13:36, Wednesday 14 May 2025 (84391)EPO

EPO tag for BRS pics

shoshana.apple@LIGO.ORG - 16:05, Thursday 15 May 2025 (84411)SEI
[Shoshana, Michael]

Pumped down the BRS chamber overnight and started the ion pump this morning and got it down to 1.9e-6 Torr before we left end End-X. We also wired up the picomotor to the LIGO picomotor controller system. It is hooked up to the 7th channel X-direction and we tested it out and were able to hear it spinning for both directions. The BRS's thermal insulation was reapplied the box closed and the temperature sensors and heating plate were all re-attached and plugged back in. The reference beam's intensity has gone down to be closer to normal somehow, so it doesn't seem to be anything to worry about
We might go back to End-Y one more time tomorrow to clean up the wiring and do a final check of the vacuum pressure.
We waited for the temperature to equilibrate a bit before balancing  because we were hoping that as the temperature rises it would drift back to center, but we ended up using the mass adjuster to try and balance it.
It looks like the + - wires for the damping were switched, meaning when the damping was on it would ring up the BRS. Fixed by changing a line in the BRS code[IF H1_ISI_GND_BRS_ETMY_CAPDRIVE>=0] by switching the [>=0] to [<=0] and switching [H1_ISI_GND_BRS_ETMY_CAPOUTL] and [H1_ISI_GND_BRS_ETMY_CAPOUTR], and [H1_ISI_GND_BRS_ETMY_RELAYL] and [H1_ISI_GND_BRS_ETMY_RELAYR]


FROM THE END-X INSTALL:
Coupling/decoupling move: 1.25k steps
Maximum: +-140k steps
Be careful: +-100k steps

NOTE: MOVING PICOMOTOR +(POSITIVE) DIRECTION TRANSLATES TO MOVING THE BRS UP

TOTAL MOVEMENT TODAY:+21k steps
shoshana.apple@LIGO.ORG - 11:49, Friday 16 May 2025 (84434)
Centered both ETMY and ETMX BRSs.
For ETMX net movement was +2200 steps, for ETMY net movement was -3200 steps.
For ETMX we saw that the DRIFTMON was moved by about ~3.27 counts per step, and ~2.3 counts per step for ETMY
shoshana.apple@LIGO.ORG - 13:55, Friday 16 May 2025 (84437)
Cleaned everything up for the ETMY BRS and relabeled all the wires. The final reading that we saw for the ion pump was 9.9e-7 Torr (186uA, 6950V) which seems about right. We left some extra mass adjuster parts with Jim just in case. 
michael.ross@LIGO.ORG - 15:04, Friday 16 May 2025 (84438)

Shoshana, Michael

We took tilt subtraction spectra as a final life check of the BRSs. Both BRSs appear to be in good working order and doing their jobs well.

Non-image files attached to this comment
H1 ISC
camilla.compton@LIGO.ORG - posted 12:46, Monday 12 May 2025 - last comment - 13:39, Wednesday 14 May 2025(84361)
ISC Alignment Work, Day 9 in HAM1 (May 12th): BeamDivs, POP Diodes

Sheila, Betsy, Tyler, Oli, Jennie, Camilla, 

Day 1: 84193, Day 2: 84228, Day 3: 84230 and 84239, Day 4: 84274, Day 5: 84292, Day 6: 84314, Day 7: 84334

POP/REFL: After the changes to the POP and REFL paths on Friday 84334, Betsy and I confirmed that the distance between the central and edge viewports is 22.5 to 23.5" on both the HAM1 door and VP simulator. We again checked the beams were easily making it though the VP simulator (attached).
Sheila and I installed and cabled the two beam divertors (REFL and POP), these are in different locations than the design to account for the close beams.
Daniel will swap the logic of the REFL divertor, POP is fine as is. Photos below:
Photos attached of: REFL (BDV1) POP (BDV2)
Location                                 photo
Open Position photo photo
Closed Position  photo photo
Beamdump Location  photo photo
Beamdump Name BD5 BD4
Beam dumped  photo photo

PSL ALS: we decided that the PSL ALS path was too close to the edge to the VP (84334) we tried moving M13 so the beam traveled in-between M11 and L2 but this didn't give enough separation at the bottom pericope mirror of ISCT1. We then put M1 back to a similar position to wear we started an decided that it was good enough away form clipping the VP. Photos attached of M15 locationbeam on M15, beam next to L2, VP simulator, UPM, LPM.

Images attached to this report
Comments related to this report
daniel.sigg@LIGO.ORG - 13:00, Monday 12 May 2025 (84362)

The logic of the REFL diverter has been changed to alternate beam. This required a restart of the slow controls software.

camilla.compton@LIGO.ORG - 17:13, Monday 12 May 2025 (84369)

Before lunch, Tyler, Oli and Betsy removed ISCT1 and the VP simulator. 

POP Beam to diodes: 

Jennie and I aligned the POP beam onto the POP X ASC diode (using flashes then single bounce, with 20W in). We needed to adjust the dark offsets (they are about the same size as the 1.5uW single bounced beam), sdfs accepted in safe attached, properly need to be redone and saved once we get to observe. All segments responded to the beam and a flashlight and we centered the beam in pitch and yaw using PM1 (alignment sliders P:100, Y:50).

Elenna and I aligned the POP beam onto the POP A LSC diode (using flashes then single bounce). We checked the POP LSC picomotor was working as expected. Checked beam was centered on the diode by it was centered by going to the middle of the edges of the diode. All segments responded to the beam and a flashlight and we centered the beam in pitch and yaw using PM1, ndscope. Note that we'll want to check this again tommor0w as we need to offload the picomotor in yaw as it doesn't have much range left. 

We couldn't see the didoe reflected beams (using POP flashes, sensitive IR card and IR viewer) so I dead rekon'ed the positions of beam dumps BD1 and BD2, see attached photo. 

Leaving IMC locked with 2W in. 

Still to do: offload POP LSC pico and check alignment, place BD6a, 6b, 7, 9 (couldn't see beams easily tpday at 2W), final checks (see other alog). 

Images attached to this comment
jennifer.wright@LIGO.ORG - 13:39, Wednesday 14 May 2025 (84393)EPO
H1 ISC
camilla.compton@LIGO.ORG - posted 16:25, Friday 09 May 2025 - last comment - 13:37, Wednesday 14 May 2025(84321)
Beamdumps on HAM1

Betsy, Camilla, Keita

We have started checking beams are sufficiently dumped on the HAM1 beamdumps by checking main beam is easily in the dump and first bounce of the  dumped beam if it's visible.
Progress below. Names as per D1000313 Cartoon.
 
Name Path Beam being dumped Checked?
BD1
POP
LSC POP_A Reflection 
 
BD2
POP
ASC POP_A WFS Reflection 
 
BD3
POP
RM3 Transmission 
 
BD4
POP
BDV2 Reflection 
 
BD5
REFL
BDV1 Reflection
 
BD6a
REFL
M7 Ghost
 
BD6b
REFL
M7 Ghost 
 
BD7
REFL
Unknown, beam from upstream of M2
 
BD8
REFL
M2 Transmission 
YES: photo
BD9
REFL
Unknown, beam from upstream of M2
 
BD10
REFL
ASC REFL_A Reflection
YES: photo
BD11
REFL
ASC REFL_B Reflection 
YES: photo
BD12
REFL
RM2 Transmission 
YES: photo
BD13
REFL
LSC REFL_A Reflection 
YES: photo
BD14
REFL
LSC REFL_B Reflection 
YES: photo
BD15
REFL
M2 Ghost (photo showing distance from main beam)
YES: photo
BD16
REFL
RM1 Transmission 
YES: photo
BD17
PSL
Nozzle Baffle on PSL-HAM1 VP
YES: photo
BD18
PSL
Nozzle Baffle on PSL-HAM1 VP
YES: photo
Images attached to this report
Comments related to this report
camilla.compton@LIGO.ORG - 15:24, Tuesday 13 May 2025 (84376)
Camilla, Betsy, Jenne
All beam dumps are now placed and checked as of this morning 84375, beams were confirmed in each BD apart from BD3 (PM1 transmission) as the beam is too faint to see.
Names as per D1000313 Cartoon, some edits to locations, details of new locations will be in other alog. 
 
Name
Path
Beam being dumped
Checked?
BD1
POP
LSC POP_A Reflection 
YES: photo
BD2
POP
ASC POP_A WFS Reflection, beam clears by ~15mm, photo 
YES: photo
BD3
POP
RM3 Transmission (Beam too weak, estimated placement)
Estimated: photo
BD4
POP
BDV2 Reflection MOVED LOCATIONS
YES: photo
BD5
REFL
BDV1 Reflection, alos catching 2 ghost beams, photo
YES: photo
BD6a
REFL
M14 Ghost MOVED LOCATIONS
YES, see BD6b.
BD6b
REFL
M14 Ghost 
YES: photo
BD7
REFL
Unknown, beam from upstream of M2, MOVED LOCATIONS 
YES: photo
BD8
REFL
M2 Transmission 
YES: photo
BD9
REFL
Unknown, beam from upstream of M2
Not using, dumped by BD8
NewBD
(BD9)
REFL
REFL ASC A low reflection, beam bounces off ISI, photo 
Call this new beamdump BD9 as now not using BD9
YES: photo
BD10
REFL
ASC REFL_A Reflection
YES: photo
BD11
REFL
ASC REFL_B Reflection 
YES: photo
BD12
REFL
RM2 Transmission 
YES: photo
BD13
REFL
LSC REFL_A Reflection 
YES: photo
BD14
REFL
LSC REFL_B Reflection 
YES: photo
BD15
REFL
M2 Ghost (photo showing distance from main beam)
YES: photo
BD16
REFL
RM1 Transmission 
YES: photo
BD17
PSL
Nozzle Baffle on PSL-HAM1 VP
YES: photo
BD18
PSL
Nozzle Baffle on PSL-HAM1 VP
YES: photo
HiPWR
REFL
M14 and M17 Reflection
YES: photo
Images attached to this comment
jennifer.wright@LIGO.ORG - 13:37, Wednesday 14 May 2025 (84392)EPO

EPO tag for pics of laser safety in practice.

H1 ISC
keita.kawabe@LIGO.ORG - posted 13:14, Friday 09 May 2025 - last comment - 13:41, Wednesday 14 May 2025(84334)
POP path alignment, Friday morning (Tyler, Betsy, Camilla, Sheila, Keita)

We ended up using pico in HAM3 to bring down green ALS beam as well as IR POP rather than raising the top periscope mirror after confirming that it was safe to do so.

We first confirmed that the X arm and corner alignment were still the same as yesterday. X arm was still locked to 00 green, and when I misaligned PRM the IR flash in H1:LSC-TR_X_IN1 was reaching 0.8 or more.

We convinced ourselves that the alignmernt was reasonable and probably similar to the alignment before the vent, that the ALS beams were pretty high but was still hitting the top periscope mirror before just like ALSX beam is as of now. We discussed the use of the pico in HAM3 (instead of moving the top periscope mirror up) and decided that it's OK to do so as far as the IR beam is far from clipping somewhere in HAM2.

We moved the HAM3 pico for PIT in "Down" direction by 700 counts and the IR beam position looked about right. We moved the pico further down by 1000 counts (that's the total of 1700 counts down from the initial state) and the IR beam missed the bottom of the top periscope mirror but no sign of clipping in HAM2, so we were comfortable to go 1000 counts "UP" and search for an optimum positision. In the end we ended up going back to 700 counts "Down" relative to where we started.

Sheila and Camilla adjusted top and bottom periscope mirror. M10 (dichroich) was also touched up. Steering mirrors for in-air beams were also roughly adjusted, These are M7 (for REFL air), M11 (for green ALS), M13 (for IR ALS beam from the PSL) and M16 (for POP air).

Now we're ready to move ISCT1L in position to confirm that all beams hit the periscope mirrors on the table.

 

Comments related to this report
camilla.compton@LIGO.ORG - 13:56, Friday 09 May 2025 (84338)

Photos attached of the Green X-arm and POP beams on the HAM1 top periscope mirror before the HAM2 pico-ing and after the HAM2 pico-ing in the final position

Tyler fork-lifted ISCT1 into position and we correctly set the height. There was some confusion due to a typo by me on the -X-Y corner height measurement that we've now corrected.

PSL ALS and Green ALS Beams:

To get the PSL ALS and green ALS beams through the VP simulator and onto the top periscope mirror, Sheila needed to move both final steering mirrors (M11 and M13) to have the beams more centered on the VP simulator:

  • M11 (for green beams) was moved in +X. We had to carefully think about not centering the alignment of this beam on all mirrors as the Y-arm green beam will be ~8mm on the -X side of the X-arm beam. 
  • M13 (for the PSL ALS) was moved in -X, ideally we'd have moved it more to further center on the VP but it would have clipped on L2. 

Photos of the final positions attached, on the VP simulator (inner red circle is the location of the actual window),  on the upper periscope mirror, on the lower periscope mirror and on the ALS shutter, we expect to need to do some steering of the UPM to get the final beams better on the LPMs, this will be done once ISCT1 is installed and realigned. 

Images attached to this comment
keita.kawabe@LIGO.ORG - 21:18, Friday 09 May 2025 (84344)

POP air and REFL air alignment
(Note: At this point, HAM1 drawing https://dcc.ligo.org/D1000313-v19 was not useful for exact placement of the mirrors because, as was reported earlier, POP and REFL beam position coming from HAM2 into HAM1 are different from what the drawing suggests by an inch or so. )

POP air steering mirror (M16) had to be relocated closer to the periscope, otherwise the POP air beam hit the -X edge of the viewport simulator when we tried to center POP air on the periscope mirror on ISCT1. But then the REFL air beam became close to the M16 mirror mount, so we ended up moving M16 MUCH closer to the periscope and the REFL air steering mirror (M7) got further down in -X direction. As a result, two beams now crosses with each other inside the chamber. See the first attachment where the new POP air beam is in orange and the new REFL air path is in cyan. This is for illustration purpose only.

2nd attachment: Overview of the POP and REFL air path in chamber.

3rd and 4th attachment: Detailed location of M16 and M7, respectively.

5th attachment: REFL air beam is comfortably away from the M16 mirror holder.

6th attachment: Beam position on the viewport simulator. Dimmer beam is POP air.

7th and 8th: REFL and POP beam on the top periscope mirror of ISCT1.

This means that the beam diverters WILL have to be relocated and reconfigured.

Just swapping the positions might not work.

I wonder if using one diverter at the edge of the table will catch both beams. (That's not a good idea as we might want to use in-air POP WFS if in-vac one doesn't work well.)

 

Images attached to this comment
keita.kawabe@LIGO.ORG - 23:16, Friday 09 May 2025 (84345)

Distance from POP air steering mirror (M16) to the top POP periscope mirror in ISCT1 was: 34 1/4 + 30 1/4  = 64.5"

Distance from REFL air steering mirror (M7) to the top REFL periscope mirror in ISCT1 was: 13 3/4 + 30 + 31.5 = 75.25"

Measurement was done using long-ish ruler, but it wasn't long enough so we had to measure the distance in multiple segments. I'd say that the error bar of this is roughly +-3/4".

jennifer.wright@LIGO.ORG - 13:41, Wednesday 14 May 2025 (84394)EPO
H1 ISC
betsy.weaver@LIGO.ORG - posted 12:38, Thursday 08 May 2025 - last comment - 13:42, Wednesday 14 May 2025(84320)
ALS PSL path on HAM1

Betsy, Camilla, Keita, Jason This morning, we took a closer look at eh small PSL-ALS beam path hitting the 1 and only mirror in HAM1 before heading to IOT1. It looked a bit clipped/elongated and was coming out of the light pipe toward the -Y side and veering off course onto the table (when compared to the new layout map). Given work on the path on the PSL table (for SPI), Jason and Keita went in to the PSL and revisited how the beam launches at the periscope. They could see scatter somewhere in the light pipe so it was probably clipping in there. Using the top ALS periscope mirror, Jason was able to yaw the beam back to the designed position of the mirror in HAM1 (Keita on the phone with Jason in the box, relaying to Betsy who moved the mirror and beam dump on HAM1). Now the beam looks nicely round, more centered in the entry viewport window, and runs along the table per the map we are aligning to D1000313-v19. We pointed the steering mirror so the beam leaves the table to also match the map. Next up is the X-arm peek and tweaking of alignments to get onto the IOT1 periscope mirrors.

Comments related to this report
keita.kawabe@LIGO.ORG - 13:30, Thursday 08 May 2025 (84322)

First attachment shows the beam right after the viewport, shot by Betsy's cellphone. The beam looked much worse to my eyes on the viewer card.

Anyway, Jason and I found that

  1. Nothing was clipping in the PSL room.
  2. The beam position on ALS-PBS01 and ALS-HWP2 was OK. Not excellent but OK.
  3. But the beam was significantly offset in YAW on ALS-L2 and downstream (2nd attachment).
  4. We were able to see two very bright beam spots somewhere inside the beam pipe viewd from the PSL room, though we couldn't tell what that was.

3rd attachment shows ALS-L2 where the beam was offset by about half of the open aperture radius of the lens mount (the lens itself is 1").

We used ALS-M2 and ALS-M3 to recenter the beam on two reference irises. 4th attachment shows ALS-L2 after this adjustment where the beam is more centered. Not perfect but much better.

On the 5th picture the beam shows no sign of clipping but the beam is close to the -Y edge of the baffle hole for the viewport.

Next Jason moved the top periscope mirror to steer the beam to where it's supposed to be in HAM1. The beam looked more centered on the baffle (6th picture).

7th picture: The location of the steering mirror for this beam on HAM1, which was set according to the HAM1 layout drawing.

8th and 9th show the PSL-ALS beam right after it is reflected by the steering mirror, and right before it leaves HAM1. We might have to fine-adjust this.

 

Images attached to this comment
jason.oberling@LIGO.ORG - 13:32, Thursday 08 May 2025 (84324)PSL

As Keita notes, before yawing the top periscope mirror he and I checked the 2 ALS alignment irises that sit under the periscope between mirrors IO_ALS_M3 and IO_ALS_M4 (the bottom ALS periscope mirror).  The beam was off on both alignment irises to the -Y side, suggesting a beam shift had occured sometime between the end of the PSL laser upgrade in Jan 2022 and now (the last time I recall looking at this alignment was at the end of the laser upgrade); using an IR viewer Keita looked at the beam on IO_ALS_L2 (the 2nd ALS mode matching lens) and the beam was off-center on the lens as well.  The beam looked decently well aligned (not perfect) along the IO_ALS_M1 to IO_ALS_M2 path, but beyond that it was well off.  It's unclear what casued this shift.  There was the recent SPI pickoff install last month that potentially could have bumped IO_ALS_M2, since they were working in that area, but I don't think that alone would be enough to cause the shift we saw.  The beam needed to be walked in the +Y direction using both IO_ALS_M2 and IO_ALS_M3 to re-center on the alignment irises, but bumping only a single mirror would more than likely have caused an angular shift in the beam and be easily corrected using only the mirror that was bumped.  This defintely was not the case, as we needed both IO_ALS_M2 and IO_ALS_M3 to walk the beam back to the irises.  So as of right now I cannot say what caused this misalignment, it's entirely possible the ALS beam has been misaligned for a while.

As noted above, we used IO_ALS_M2 and IO_ALS_M3 to re-center the ALS beam on the alignment irises, and at this point the beam was no longer clipping when traversing the ALS light pipe.  Back on the HAM1 table, the mirror that directs the ALS beam onto ISCT1 was still too far in the -Y direction for comfort (getting a little to close to the future home of the JAC and its associated optics).  I then went into the enclosure and yawed IO_ALS_M5 (the top ALS periscope mirror) until the mirror in HAM1 was in its as-designed location.  I've attached a picture I took of how the ALS beam now looks when entering the ALS light pipe; it's now a little closer to the +Y edge of the light pipe.  Before adjustment the outside edge of the beam was very roughly 1" or so away from the light pipe edge (did not get a picture of this), now it's very roughly 1/2" or so away from the edge.

Images attached to this comment
jennifer.wright@LIGO.ORG - 13:42, Wednesday 14 May 2025 (84395)EPO
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