Displaying reports 12161-12180 of 89162.Go to page Start 605 606 607 608 609 610 611 612 613 End
Reports until 17:38, Wednesday 24 July 2024
LHO VE (VE)
gerardo.moreno@LIGO.ORG - posted 17:38, Wednesday 24 July 2024 - last comment - 17:42, Wednesday 24 July 2024(79306)
Corner Station Dew Point Measurement

Dew point measurement taken this morning by Jordan, read at -43.9 oC.  Some demand by HAM5/6, small crew at work.

Images attached to this report
Comments related to this report
gerardo.moreno@LIGO.ORG - 17:42, Wednesday 24 July 2024 (79307)VE

End of the day dew point measurement, -43.6 oC.  No demand, all soft covers closed for HAM5/6 and HAM7 is under small pressure and isolated.

Note regarding HAM7: before the 10" gate valve is open, chamber needs a blow down, see a vacuum representative.

Images attached to this comment
H1 General
oli.patane@LIGO.ORG - posted 16:37, Wednesday 24 July 2024 (79305)
Ops Day Shift End

TITLE: 07/24 Day Shift: 1430-2330 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Corrective Maintenance
INCOMING OPERATOR: None
SHIFT SUMMARY: The OFI team was able to get the AUX laser aligned and verified that the SQZ beam can get to OM1. Tomorrow morning first thing we will be transitioning the LVEA to laser safe and continuing the OFI work by taking the KTP out and taking the HAM6 -X door off.
LOG:

- Continuing work on aligning AUX laser

- Aligning sqz beam

- Getting ready to transition to laser safe

Start Time System Name Location Lazer_Haz Task Time End
15:11 FAC Kim, Karen LVEA YES Tech clean, (Karen out at 1600) 16:23
15:20 VAC Jordan LVEA YES Checking purge air 15:31
15:41 OFI Camilla, Jason, Sheila HAM5 Y AUX laser work 19:41
16:10 OFI Keita LVEA YES OFI work 19:41
16:11 FAC Richard LVEA YES Checking in on OFI work 17:34
16:38 FAC Karen WoodShop n Tech clean 17:27
17:25 FAC Kim MX n Tech clean 18:27
18:09 FAC Karen EY n Tech clean 18:58
18:28 OFI Francisco LVEA YES Helping with OFI 19:41
19:12 ISI Jim EY n Recovering EY from HEPI/ISI trip 19:46
19:15   Richard LVEA YES Checking in on OFI peeps 19:41
20:41 OFI Camilla LVEA YES More AUX aligning for OFI 23:30
20:50 OFI Jenne, Naoki, Sheila, Jason LVEA YES Continue AUX alignment work for OFI (Sheila, Jenne out 22:55)(Naoki our 23:08)(Jason out 23:27) 23:27
21:51 VAC Gerardo LVEA YES Purge air for HAM7 22:02
21:29 VAC Janos EY n Purge air photos 21:48
21:49 FAC Tyler LVEA YES Prepping for HAM6 door removal 21:52
22:10 OFI Keita LVEA YES OFI help 22:55
23:08 EE Marc, Fil MY n Looking for parts ongoing
23:09 FAC Tyler LVEA YES More prep work for HAM6 door 23:13
H1 ISC
jennifer.wright@LIGO.ORG - posted 16:29, Wednesday 24 July 2024 (79304)
Mode-matching calculation for AUX laser injection from HAM6 to HAM5

Keita, Jennie W

Keita and I worked out the distance behind SRM we have to place the AUX launcher to match the beam radius the IFO beam normally has on SRM on its way into the OFI.

This is based on measurements of beam profile Keita made in the optics lab with the aux laser mounted with a collimator on it.

The code used to do this is saved in ligo/home/jennifer.wright/ModeMatching/beam_diverg.py

The graph attached shows the measured points in orange and the fitted points in blue.

Beam waist, w0 is 0.916 mm
Beam waist position in relation to front of launcher , z0 is -1.423 m
Rayliegh range for beam, z_R is 2.477 m
Move launcher 3.986 m away from SRM
Distance between OM1 and SRM is 3.646 m
 
Therefore we propose installing a steering mirror at right angles to OM1/SRM line to get this longer distance to SRM.
 
Images attached to this report
Non-image files attached to this report
H1 PSL
ryan.short@LIGO.ORG - posted 15:55, Wednesday 24 July 2024 (79303)
PSL 10-Day Trends

FAMIS 21009

The stabilization trends are especially interesting this week; PMC reflected power is steadily increasing while transmitted power (along with RefCav transmission and ISS diffracted power) is decreasing. This is particularly interesting as we thought this behavior might disappear when we swapped in the new PMC.

Images attached to this report
H1 PEM
genevieve.connolly@LIGO.ORG - posted 12:10, Wednesday 24 July 2024 - last comment - 13:47, Wednesday 24 July 2024(79284)
~40 Hz peak(s) investigation in HAM ISIs and PEM accelerometers

Sam and I have been investigating a ~40 Hz peak in the HAM ISIs and PEM accelerometers, first noticed by Camilla and Sheila in alogs 79001 and 78879. Jim also investigated and suggested the peak may be caused by gain peaking from the isolation loops (alog 79145). The peak is strongest in HAMs 2, 6, and the LVEAFLOOR YCRYO Z accelerometer. We tracked the first appearance of the peak to May 20th. We've found there are actually two peaks roughly 0.2 Hz apart, which drift a bit in frequency from ~39.45 Hz (20/05/24 16:00 UTC) to ~40.2 Hz (20/05/24 22:00 UTC), measured from the point between the two peaks (see 1st attachment). The peaks consistently remain about 0.2 Hz apart in frequency but they do not always have the same magnitude ratio, even between channels measured at the same time (see 2nd attachment). Overall, the peaks vary in magnitude, occasionally disappearing altogether, but we have yet to find a time when one peak disappears and the other doesn't (see 3rd & 4th attachments for peaks disappearing and reappearing, respectively). We'll continue looking into surrounding peaks and the coherence with DARM.

Images attached to this report
Comments related to this report
jim.warner@LIGO.ORG - 13:47, Wednesday 24 July 2024 (79302)SEI

The extra drive on HAM2 is likely from a very thin phase margin on the HAM2 X feedback loop. I measured this yester day and found that it had something like 5 deg of phase margin with a 32-ish hz ugf. I backed this off quite a bit, phase margin is now around 20deg and the ugf is more like 27 hz. Might be worth doing some quick checks on these for all the ISIs. Measurements of the X ugf and phase margin are attached. Red is the modified loop I installed yesterday, blue is the loop with the filters that have been running up to that point, not sure when the last measruements were run, it's been a while.

Images attached to this comment
H1 CDS
david.barker@LIGO.ORG - posted 08:30, Wednesday 24 July 2024 (79299)
Atomic Clock out-of-sync with the timing system again

16:09 Tue 23 July 2024 PDT the atomic clock jumped to +0.42S out from the Timing system.

This is the third time this has happened in the past month. Prior to that it had only happened once in the past year, on 4th May. Here is a table of the atomic clock out-of-syncs for the past year

out-of-sync resynced uptime since last resync
23rd July 2024  still out 4 days
17th July 2024 19th July 2024 43 hours
15th July 2024 15th July 2024 2 months 11 days
4th May 2024 6th May 2024 +1 year

I have extended the timing comparator's tolerance to 0.9999999 seconds to 'green up' the corner station timing.

Images attached to this report
LHO VE
david.barker@LIGO.ORG - posted 08:14, Wednesday 24 July 2024 (79298)
Wed CP1 Fill

Wed Jul 24 08:05:48 2024 INFO: Fill completed in 5min 44secs

Jordan confirmed a good fill curbside.

Images attached to this report
H1 General
oli.patane@LIGO.ORG - posted 07:41, Wednesday 24 July 2024 (79297)
Ops Day Shift Start

TITLE: 07/24 Day Shift: 1430-2330 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Corrective Maintenance
OUTGOING OPERATOR: None
CURRENT ENVIRONMENT:
    SEI_ENV state: MAINTENANCE
    Wind: 4mph Gusts, 2mph 5min avg
    Primary useism: 0.01 μm/s
    Secondary useism: 0.05 μm/s
QUICK SUMMARY:

Close to getting the AUX laser aligned (79291)!

H1 ISC
sheila.dwyer@LIGO.ORG - posted 22:03, Tuesday 23 July 2024 - last comment - 10:18, Thursday 01 August 2024(79291)
HAM 5 alignment laser day 2

Sheila, Jason, Jennie, Keita, Jenne, Camilla, Naoki. Following 79274.'

Summary:  We still need more work on the alignment laser tomorow.  Today we believe that we understood the right process for setting it up, but we will need to iterate a few more times to get it set.

  • This morning when we went to the chamber we saw the reflection from one of the ITMs coming back near SRM, we were confused by this for a minute and misaligned the ITMs. 
  • Jennie found we needed to move SRM Yaw to 136 on the osems 79272, we did this (could see the beam slightly move but barely) and then touched the AUX laser BS to center the retrofection on the iris right after the laser.
  • Beam was on AS_C (170uW vs 100uW blocked) but not centered (-0.3 pit; +0.2 yaw)
  • Jennie found we were off 10urad in Pitch and moved SRM to 659.9 uradians on osems. This was not visible on the iris but we again touched the AUX laser BS to center the retrofection on the iris right after the laser (wasn't centered this morning <1mm off but was centered last night).
  • Sheila entered the chamber and walked to SR2, the beam was well centered in yaw but somewhat less than an inch too low.  Jenne moved SRM by about 350urad in pitch to bring the beam closer to center.
  • Jenne put SRM back half way to the starting place (so that we were half way between the alignment that gave us a good centering on SR2, and the one that we think should be close to what we had in lock.  Then Jason, Jenne, and Keita walked the temporary steering mirror and beamsplitter.  They moved the beam splitter to bring the beam lower on OM1, since they noticed that it was slightly high of center, and then walked the mirrors to restore the retroreflection on the iris right after the collimator. 
  • The combination of these moves meant that the beam was very low on SR2, clipping on the scrapper baffle and hitting the optic right at the bottom, around the level of the earthquake stops.
  • We took a lunch break, and installed an iris in front of OM1 to mark that position, and set SRM back to the alignment that we think that we were using for locking.  Jenne Jason and Naoki tried to move the beam the restore the retroreflection while keeping the beam on the OM1 iris, they found that in order to do that they had to move the beam visibly low on the Faraday aperture, on the temporary beam splitter (which Betsy set to 8.3", the SRM center height.).  We then realized that this might be because the beam has been high of center on OM1 while we have been locking, consistent with the fast shutter bouncing. 
  • We decided to move the beam closer to center in the OFI aperture, and the temporary beamsplitter, and allow it to be above center on OM1.  After this Jenne, Naoki and Jason realigned so that the beam was retroreflected with SRM aligned as we think it was for locking.  I went into the chamber again to look at the beam position, and found it was between 2 and 3 inches to low (a bit more than the height of the thorlabs beam card), and about 1 cm off in the -X direction.
  • When I left, the team was planning to reset the iris by OM1, and possibly make a move of SRM and walk the temporary mirror + BS to restore the retro reflection and spot position on OM1 iris.  If this worked we will check in the morning where the beam is on SR2. 

 

Comments related to this report
keita.kawabe@LIGO.ORG - 23:10, Tuesday 23 July 2024 (79292)

It's useful to know the geometry of this setup.

The SRM is a convex mirroor with R=5.678m ROC (and therefore a converging flat-convex lens with f=12.6m focal length).

All rays retro-reflected by the SRM HR surface converge at a single point. Because of the lensing effect of SRM, this point is NOT the center of the ROC but away from SRM by Rf/(R+f)=3.92m. OM1 is 3.65m away from SRM. These are all you need to know (plus a basic knowledge of thin lens), but I drew a cartoon for you (1st attached, top, but you can also see 2nd attachment for the math) where four different rays, all retro-reflected by SRM, are converging at one point.

Now, Sheila's 3rd bullet point from the bottom is like the green line in the cartoon. The green dot at the OM1 position marks the center of the OM1, however there's only one ray that is retroreflected and goes through the center of OM1 (green line), which happens to be VERY low on SRM.

Without touching SRM, we can walk the beam on SRM while keeping the retroreflection and bring up the position at SRM by deltax, and as a result the beam position goes up about 0.07*deltax at OM1 and about 3.7*deltax on SR2.

Note that a small pit offset on OM1 has a big effect on SRM and SR2, i.e. 1mm on OM1 will become 14mm at SRM and 54mm at SR2.

Images attached to this comment
keita.kawabe@LIGO.ORG - 23:41, Tuesday 23 July 2024 (79293)

SR2 beam position when Sheila left was 1cm to +X, too low by 3"~76mm (i.e. the beam needed to move to -X by 1cm, up by 3"~76mm).

Now the task is to rotate the SRM, maintain the retroreflection while keeping the beam position on OM1. This is explained in the attached cartoon again. Anyway, conclusion is that if we want to move the beam up by deltay at SR2, we have to rotate SRM by deltay/215m, i.e. deltay/[SRM rotation] ~ 2mm/10urad.

(The calculation in the attached assumes that we're fixing the OM1 beam position, but in reality the iris is maybe 50cm or so closer to SRM, so L=3.15 instead of 3.65. This should have a large effect on one of the important numbers d-L=3.92m-L, it changes from 0.27 to 0.77. Mostly because of this, my calculation is severely overestimating the deltay/[SRM rotaion] maybe by a factor of 3, roughly.)

Anyway,we used 2mm/10urad number at the time, and moved SRM in PIT by negative 380urad (PIT slider 2121 -> 1741, YAW slider -3492 no change).

At this point we reset the position of the iris to the beam. Naoki, Jason and Jenne adjusted the steering mirror and the BS so the beam hits the center of the iris while keeping the retroreflection. We stopped the work there.

Images attached to this comment
keita.kawabe@LIGO.ORG - 06:32, Wednesday 24 July 2024 (79295)

This is a picture of Sheila entering HAM4-HAM5 tube through the eye-shaped baffle.

Images attached to this comment
jason.oberling@LIGO.ORG - 06:31, Wednesday 24 July 2024 (79296)

Should also add that when restoring the aux laser alignment to OM1 position and the retroreflection iris in the afternoon, the alignment converged much quicker when using the beamsplitter to align the retroreflection and the steering mirror to align OM1 position.  In the morning we were doing the opposite (beamsplitter to OM1, steering mirror to retroreflection), and while we were able to get the alignment to converge it was picky and had a tendency to diverge if we made large steps.

After working through the math Keita had said this might be the case.  Our first run at restoring the aux laser alignment in the afternoon, still using beamsplitter to OM1 and steering mirror to retroreflection, was diverging when we were moving in the direction we clearly had to move, so we switched to beamsplitter to retroreflection and steering mirror to OM1; alignment went much smoother afterwards.

corey.gray@LIGO.ORG - 10:18, Thursday 01 August 2024 (79401)EPO

Tagging for EPO.

H1 General
oli.patane@LIGO.ORG - posted 16:33, Tuesday 23 July 2024 (79290)
Ops Day Shift End

TITLE: 07/23 Day Shift: 1430-2330 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Corrective Maintenance
INCOMING OPERATOR: None
SHIFT SUMMARY: Work today was just a continuation of work on aligning the AUX laser
LOG:                                                                                                                                                                                                                                                                                                          

Start Time System Name Location Lazer_Haz Task Time End
17:09 SAFE LASER HAZARD LVEA YES LVEA IS LASER HAZARD 03:49
14:49 FAC Kim, Nellie Optics Lab y(local) Tech clean 15:15
15:16 FAC Nellie, Kim LVEA YES Tech clean 16:35
15:47 OFI Sheila, Jason, Camilla LVEA YES Continuing OFI work (Camilla out 17:58) 19:21
16:01 FAC Tyler, Ivan LVEA YES Walking around 16:43
16:05 PCAL Francisco PCAL Lab y(local) PCALin 16:20
16:09 VAC Jordan LVEA YES Addressing HAM6 purge air and running an RGA 17:27
16:19 BIO Sabby Behind water tank n Taking soil for experiment 16:54
16:26 VAC Gerardo LVEA YES Joining Jordan at HAM6 20:07
16:32 FAC Chris MY, EY, MX, EX n Picking up old light fixtures 18:47
16:36 SUS RyanC, Rahul HAM Shack n Looking for parts 16:56
16:37 CDS Richard LVEA YES Checking on computers 17:00
17:03 SUS RyanC CR N ETM OPLEV charge measurement 18:46
17:04 OFI Keita LVEA YES Joining OFI team 19:21
17:09 OFI Jenne LVEA YES Joining OFI team 19:21
17:35 OFI Naoki LVEA YES Joining OFI work 19:00
17:51 FAC Richard LVEA YES Because he can (checking in on OFI work) 18:17
17:52 FAC Tyler LVEA YES 3IFO checks 18:07
18:15 ISI Jim HAM Shack n CPS work on HAM8 19:08
18:45 OFI Camilla, Josh Optics Lab y(local) Getting beam ready for KTP swap 20:24
18:45 FAC Richard LVEA YES Checking on OFI work status 19:14
18:52 PCAL Tony PCAL Lab y(local) Checking chassis for sending to LLO 19:20
18:58 PCAL Dripta PCAL Lab y(local) Joining Tony 18:59
19:46 FAC Tyler MX, MY n 3IFO checks 20:07
20:00 SUS RyanC LVEA YES Restarting dust monitor 20:12
20:12 FAC Chris MX n Finishing up light fixture pickup 21:29
20:45 OFI Sheila, Jason, Naoki LVEA YES Continuing OFI work (Sheila out 23:01) 23:30
20:55 OFI Jenne LVEA YES Continuing OFI work 23:30
21:21 OFI Camilla LVEA YES Helping out with OFI 21:54
21:34 VAC Jordan, Gerardo EX n Grabbing leak detector 22:45
21:35 SEE Tony, Genevieve, Sam, Mattia Roof n Looking at the beautiful landscape and arms 21:48
21:50 ISI Jim EX, EY n Recovering HEPI and ISIs 22:17
22:06 safe McCarthy LVEA YES checking on ofi work status 22:44
22:45 VAC Gerardo LVEA YES Doing vacuum checks 23:02
22:55 EE Jim, Fil EX n Figure out HEPI pump at EX 23:32
23:11 TOUR Camilla + 3 others LVEA YES Looking at OFI work

23:33

 

H1 CDS
david.barker@LIGO.ORG - posted 15:29, Tuesday 23 July 2024 - last comment - 15:37, Tuesday 23 July 2024(79288)
Power glitch 13:43:30 PDT, took down both end station HEPI Pump Controllers

Site wide power glitch at 13:43:30 PDT (20:43:30 UTC) Tue 23rd July 2024. Lights in corner station flickered. Both end station HEPI Pump Controller VFDs tripped.

Jim untripped the EX VFD, but the HEPI pump controller does not seem to have control. Jim and Patrick are investigating.

Images attached to this report
Comments related to this report
david.barker@LIGO.ORG - 15:37, Tuesday 23 July 2024 (79289)

If it seems we have had a lot of power glitches recently, that's because we have, 6 in the past month.

(all times local PDT)

Tue 23 Jul 2024 13:43:30
Sun 21 Jul 2024 12:50:08
Tue 16 Jul 2024 10:58:55
Sun 07 Jul 2024 13:51:31
Mon 24 Jun 2024 09:46:28
Sun 23 Jun 2024 20:48:15

 

LHO VE (VE)
gerardo.moreno@LIGO.ORG - posted 11:55, Tuesday 23 July 2024 - last comment - 02:01, Wednesday 24 July 2024(79285)
Corner Station Dew Point Measurement

Dew point measurement done this morning, read at -43.4 oC.  There was some demand already on the system from HAM5, since both soft covers were off.  No demand from HAM6 or HAM7.  Flow was opened later to HAM6, since more personnel started working in-chamber.  HAM7 remains valved out.

Images attached to this report
Comments related to this report
gerardo.moreno@LIGO.ORG - 02:01, Wednesday 24 July 2024 (79294)VE

End of the day dew point measurement, -43.0 oC.

Images attached to this comment
H1 SEI
jim.warner@LIGO.ORG - posted 16:29, Monday 15 July 2024 - last comment - 12:14, Wednesday 24 July 2024(79145)
HAM2 moving a lot more than HAM3 around 40hz, probably time to do some re-tuning

Genevieve and Sam asked about HAM1 and HAM2 motion around 40 hz. I hadn't look in detail in this frequency band for a while, this is typically higher frequency than we are worried about with ISI motion. But it turns out HAM2 is moving a lot more than HAM3 generally over 25-55hz, and particularly around 39hz. It looks like it might be due to gain peaking from the isolation loops, but could also be from something bad in the HEPI to ISI feedforward. The extra motion is so broad I don't think it's just one loop has a little too much gain, so I'm not sure what is going on here. 

First image are spectra comparing the motion of the HEPIs for those chambers (HAM2 HEPI is red and HAM3 is blue) and the ISIs (HAM2 ISI is green, HAM3 is brown). The HEPI motion is pretty similar, so I don't think it's a difference in input motion. HAM2 is moving something like 10x as much as HAM3 over 25-55hz. The sharp peak at 39 hz looks like gain peaking, but I'm not sure that explains all the difference.

Second plot shows the transfer functions from HEPI to ISI for each chamber. Red is HAM2, blue is HAM3. The 25-55hz tf for HAM3  is not very clean probably because HAM3 is well isolated. HAM2 tf is pretty clean, it makes me wonder if maybe something is messed up with feedforward on that chamber. Maybe that is something I could (carefully) fix while other troubleshooting for the detector is going on.

Images attached to this report
Comments related to this report
jim.warner@LIGO.ORG - 17:00, Monday 15 July 2024 (79150)

I looked at some of my design scripts and realized that the HAM3 FF X filter is probably a bit better fit, so I copied that into the HAM2 foton file, loaded and engaged it on HAM2. It improved the 50ish hz motion quite a bit, but HAM2 is moving more than HAM3 still. Probably some tuning that could still be done here.

Images attached to this comment
samantha.callos@LIGO.ORG - 12:14, Wednesday 24 July 2024 (79301)

Looked further into the peak at ~40Hz and found an improvement in coherence after the re-tuning Jim did. Image 1 shows the peak pre-tuning, and image 2 shows it post-tuning.

Images attached to this comment
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