Displaying reports 16941-16960 of 86691.Go to page Start 844 845 846 847 848 849 850 851 852 End
Reports until 07:37, Tuesday 01 August 2023
H1 General
ryan.crouch@LIGO.ORG - posted 07:37, Tuesday 01 August 2023 - last comment - 07:59, Tuesday 01 August 2023(71861)
OPS Tuesday day shift start

TITLE: 08/01 Day Shift: 15:00-23:00 UTC (08:00-16:00 PST), all times posted in UTC
STATE of H1: Lock Acquisition
CURRENT ENVIRONMENT:
    SEI_ENV state: CALM
    Wind: 4mph Gusts, 2mph 5min avg
    Primary useism: 0.01 μm/s
    Secondary useism: 0.05 μm/s
QUICK SUMMARY:

 

Comments related to this report
ryan.crouch@LIGO.ORG - 07:40, Tuesday 01 August 2023 (71862)

Injections finished at 14:39UTC

ryan.crouch@LIGO.ORG - 07:45, Tuesday 01 August 2023 (71863)

Inlock charge measurements start at 14:45UTC

ryan.crouch@LIGO.ORG - 07:59, Tuesday 01 August 2023 (71864)CDS, SUS

Inlock charges are having an ezca connection error, can't connect to H1:SUS-ITMX_L3_DRIVEALIGN_L2L. I've stopped to OP STOP and EXEC as suggested by the log but it gets the same error everytime. The inlock charge measurements were not able to be completed

Images attached to this comment
H1 CDS
erik.vonreis@LIGO.ORG - posted 06:54, Tuesday 01 August 2023 (71860)
Workstations rebooted

Workstations were updated and rebooted.  The update was only to OS packages.  Conda packages were not updated.

LHO General
ryan.short@LIGO.ORG - posted 00:00, Tuesday 01 August 2023 (71859)
Ops Eve Shift Summary

TITLE: 08/01 Eve Shift: 23:00-07:00 UTC (16:00-00:00 PST), all times posted in UTC
STATE of H1: Observing at 147Mpc
SHIFT SUMMARY: H1 has been locked and observing for 13 hours.

Noted in my mid-shift report that the MY AHU alarm started around 23:40; the AHU temperature has started to come down and has now dropped below 85 degrees so the alarm has stopped. Very quiet shift otherwise.

Incoming owl shift operator: TJ

LOG:

No log for this shift.

LHO General (FMP)
ryan.short@LIGO.ORG - posted 20:01, Monday 31 July 2023 (71858)
Ops Eve Mid Shift Report

State of H1: Observing at 147Mpc

H1 has been locked for 9 hours. The MY air handler alarm started around two hours ago; checking the medm it shows the cooling temp is around 86 degF and has been climbing over the past two days. Since the IFO doesn't much care about the mid station temperatures and a contractor will be out to check it tomorrow, this is not an urgent cause for concern (but I've notified Bubba and am tagging facilities anyway).

Images attached to this report
H1 PSL
ryan.short@LIGO.ORG - posted 17:56, Monday 31 July 2023 (71857)
PSL 10-Day Trends

FAMIS 19987

No major events of note.

Images attached to this report
H1 PSL
ryan.short@LIGO.ORG - posted 16:30, Monday 31 July 2023 (71856)
PSL Cooling Water pH Test

FAMIS 19964

pH of PSL chiller water was measured to be between 10.0 and 10.5 according to the color of the test strip.

H1 TCS
thomas.shaffer@LIGO.ORG - posted 16:12, Monday 31 July 2023 (71854)
TCS Chiller Water Level Top-Off

FAMIS 21126

I added no water to either chiller, they both were at or very near the values from the previous check on the 21st. Filters looked good and I saw no water in the leak-detecting Dixie cup.

LHO General
ryan.short@LIGO.ORG - posted 16:06, Monday 31 July 2023 (71852)
Ops Eve Shift Start

TITLE: 07/31 Eve Shift: 23:00-07:00 UTC (16:00-00:00 PST), all times posted in UTC
STATE of H1: Observing at 142Mpc
CURRENT ENVIRONMENT:
    SEI_ENV state: CALM
    Wind: 17mph Gusts, 13mph 5min avg
    Primary useism: 0.03 μm/s
    Secondary useism: 0.06 μm/s
QUICK SUMMARY: Taking over from Ryan C. H1 has been locked and observing for 5 hours.

H1 General (SQZ)
ryan.crouch@LIGO.ORG - posted 15:55, Monday 31 July 2023 (71844)
OPS Monday day shift summary

TITLE: 07/31 Day Shift: 15:00-23:00 UTC (08:00-16:00 PST), all times posted in UTC
STATE of H1: Observing at 146Mpc
SHIFT SUMMARY: The squeezer lost lock a few times and kicked us out of observing, 1 lockloss with an automated relock. Handing off to RyanS

Lock#1:

Squeezer ISS took us out of commissioning from 15:59UTC to 16:09UTC

Lockloss @ 16:31UTC

Lock#2:

Couldn't get DRMI or PRMI, went to CHECK_MICH then back to PRMI then lockloss 16:54 UTC

Lock#3

Couldn't get DRMI or PRMI (2nd try) so H1MANAGER took us to initial alignment as expected, which went smoothly. We were then able to lock DRMI within 30 seconds during the following relocking.

Back into NLN at 18:05TUC and Observing at 18:26UTC. **Fully automated relock with an automated initial alignment**

We lost connection to the CDS_WAP_{EX,EY,LVEA}_STATUS briefly (~50 seconds) at 21:55UTC which are and were all off

Superevent S230731an

LOG:                                                                                                                   

Start Time System Name Location Lazer_Haz Task Time End
17:34 FAC Karen Optics lab, VAC prep N Tech clean 17:53
19:01 SEI Jim Mezz N Parts/tools search 19:06
19:27 CAL Gabriele Remote N CHARD_Y measurement 20:48
20:28 VAC Travis & Jordan Optics lab N Disassembly of a setup 21:56
21:09 FAC Ken MY n Light fixtures back 22:10
H1 SEI
thomas.shaffer@LIGO.ORG - posted 14:49, Monday 31 July 2023 (71851)
H1 ISI CPS Sensor Noise Spectra Check - Weekly

FAMIS 19669

Script reports ITMX_ST2_CPSINF H3 &V1 high freq noise is high! I agree that H3 looks higher, but V1 looks OK.

 

Non-image files attached to this report
H1 ISC
gabriele.vajente@LIGO.ORG - posted 14:00, Monday 31 July 2023 - last comment - 08:27, Tuesday 01 August 2023(71848)
CHARD_Y open-loop gain measurement

Today between 19:25 UTC and 20:45 UTC I measured the CHARD_Y open-loop gain with two broadband noise injections (different shapes). The result is a pretty good measurement that will enable a better design of the CHARD_Y controller.

Right now: the controller has little gain at 2.6 Hz, and a very large (10 dB) gain peaking at 1 Hz.

The template is available in /ligo/home/gabriele.vajente/ASC/CHARD_Y_shaped_exc_2023_07_31b.xml

Images attached to this report
Comments related to this report
gabriele.vajente@LIGO.ORG - 14:58, Monday 31 July 2023 (71850)

Here's a fit of the CHARD_Y plant (open loop gain divide by controller, including gain 60). zeros and poles in s-domain below (rad/s)

z = [-4.27268475+16.14989614j, -4.27268475-16.14989614j,
        -0.84677811+11.7910939j , -0.84677811-11.7910939j ,
        -0.15001959 +3.1577398j , -0.15001959 -3.1577398j ,
        -0.14073526 +2.60978661j, -0.14073526 -2.60978661j,
        -0.89432965 +1.06440904j, -0.89432965 -1.06440904j]
p = [-1.26172189+18.71400182j, -1.26172189-18.71400182j,
        -0.42125296+16.04217932j, -0.42125296-16.04217932j,
        -1.88894857+14.52668064j, -1.88894857-14.52668064j,
        -0.17624191 +6.42823571j, hisproduces -0.17624191 -6.42823571j,
        -0.08126954 +3.12803462j, -0.08126954 -3.12803462j,
        -0.33177813 +2.74361234j, -0.33177813 -2.74361234j,
        -1.01199783 +0.j        , -0.20377166 +0.j        ]
k = -2608.840762444897

Using this model too predict the closed-loop gain underestimates a bit the gain peaking observed at about 1 Hz. So I did a refinement of the fit to better model the little gain and phase wiggles at 1.4 Hz:

z = [-4.27268475+16.14989614j, -4.27268475-16.14989614j,
        -0.84677811+11.7910939j , -0.84677811-11.7910939j ,
        -0.15001959 +3.1577398j , -0.15001959 -3.1577398j ,
        -0.14073526 +2.60978661j, -0.14073526 -2.60978661j,
        -0.89432965 +1.06440904j, -0.89432965 -1.06440904j,
        -0.55930335 +8.32753387j, -0.55930335 -8.32753387j,
        -0.13681604 +6.53617672j, -0.13681604 -6.53617672j,
        -0.75698522 +6.05299388j, -0.75698522 -6.05299388j]
p = [-1.26172189+18.71400182j, -1.26172189-18.71400182j,
        -0.42125296+16.04217932j, -0.42125296-16.04217932j,
        -1.88894857+14.52668064j, -1.88894857-14.52668064j,
        -0.17624191 +6.42823571j, -0.17624191 -6.42823571j,
        -0.08126954 +3.12803462j, -0.08126954 -3.12803462j,
        -0.33177813 +2.74361234j, -0.33177813 -2.74361234j,
        -1.01199783 +0.j        , -0.20377166 +0.j        ,
        -0.53443931 +8.46054777j, -0.53443931 -8.46054777j,
        -0.12110921 +6.58734716j, -0.12110921 -6.58734716j,
        -0.59423727 +5.96287439j, -0.59423727 -5.96287439j]
k = -2557.795730924652)

This reproduces pretty well the closed loop transfer function. So we can be confident that it will model well the performance of a new controller design. We'll include the refined fit in the model

Images attached to this comment
gabriele.vajente@LIGO.ORG - 16:04, Monday 31 July 2023 (71853)

Here's a compariison of the fit from the previous measurement and from the new measurement from today. They are quite different, and that explains why the previous controller design failed

Images attached to this comment
gabriele.vajente@LIGO.ORG - 08:27, Tuesday 01 August 2023 (71866)

Based on the measured CHARD_Y plant, I designed a new controller that would give us more supression at 2.6 Hz, and avooid gain peaking at 1 Hz. This comes at the price of about 10 times large noise injection at 10 Hz and above. This might be too much at 10-15 Hz, but ok above 15-20 Hz. Hopefully once the new controller is engaged and we have a more stable CHARD_Y, we should be able to fine tune the A2L to gain back some noise coupling at frequencies below 20 Hz.

Comparison of current controller with nominal gain at 60, current controller with higher gain at 180 and the new controller.

Comparison of the open-loop gain in the same three configurations

Comparison of the loop suppression in the same three configurations

The new controller can be engaged with the nominal gain of 60, and it is stable for an increased gain of 180. Even with a gain of 60, it removes completely the gain peaking at 1 Hz, and provides 3 dB of suppression at 2.6 Hz.

Images attached to this comment
Non-image files attached to this comment
LHO VE
david.barker@LIGO.ORG - posted 12:51, Monday 31 July 2023 (71847)
Mon CP1 Fill

Mon Jul 31 10:11:03 2023 INFO: Fill completed in 10min 59secs

Gerardo confirmed a good fill curbside

Images attached to this report
H1 General
ryan.crouch@LIGO.ORG - posted 11:27, Monday 31 July 2023 - last comment - 12:10, Monday 31 July 2023(71845)
Back into Observing

We've recovered NLN and Observing at 18:05 and 18:26 respectively fully automated, including an initial alignment!

Comments related to this report
ryan.crouch@LIGO.ORG - 12:10, Monday 31 July 2023 (71846)SQZ

The SQZer lost lock at 19:07 and kicked us out of observing, it relocked at 19:10 and we went back to observing.

H1 General (CDS, Lockloss)
ryan.short@LIGO.ORG - posted 23:03, Sunday 30 July 2023 - last comment - 09:43, Monday 31 July 2023(71829)
Lockloss @ 05:50 UTC - Dolphin Crash

Lockloss @ 05:50 UTC, caused by Dolphin glitch.

First event I noticed was HEPI HAM1 watchdog tripping, then seeing IOP DACKILL tripped for iopsusb123, iopsush2a, iopsush34, and iopsush56 and a very red CDS overview (attached). Called Dave and we're now working on recovery.

EDIT: Attached CDS overview screenshot at time of glitch.

Images attached to this report
Comments related to this report
ryan.short@LIGO.ORG - 23:02, Sunday 30 July 2023 (71830)

At first glace Dave believes the glitch originated from the OMC model, causing everything else to trip. He's isolating it from the Dolphin network and restarting it now.

david.barker@LIGO.ORG - 23:46, Sunday 30 July 2023 (71832)

Ryan S, Dave:

After diag resetting which cleared a bunch of cached IPC errors we were left with:

1. Every receiver of IPCs originating from h1omc0 were continuously bad, including those at the end stations.

2. The IOP DACKILLs were permanently asserted on h1sus[b123, h2a, h34, h56]

So it looks like the IX Dolphin card on h1omc0 has gone offline and caused a glitch which took down the corner station SUS listed above.

Recovery:

Log into h1omc0 and check it can see its IO Chassis [it can] and see if the dmesg logs show anything from this time [they dont].

Fence h1omc0 from Dolphin and reboot.

When h1omc0 came back and its models restarted, all the outstanding IPC receive errors cleared.

Onto SUS. For each we safed the SUS, bypassed the SEI SWWD receivers, stopped all the models then started all the models. When the IOP was running again, I unbypassed the corresponding SEI SWWDs.

This worked well for h1susb123, h1sush2a and h1sush34. It did not work for h1sush56, the IOP model failed to restart.

I stopped the partially started h1sush56 models, checked the IO Chassis was visible [it was], fenced it from Dolphin and rebooted.

As h1sush56 came back from reboot, we saw a lot of IPC flashes on various systems. I had seen one or two flashes, but h1sush56 flashed the IPCs for many seconds until its IOP model got going. From that point onwards the Dolphin network was good, no new IPC errors.

 

Images attached to this comment
david.barker@LIGO.ORG - 09:43, Monday 31 July 2023 (71843)
H1 SQZ
victoriaa.xu@LIGO.ORG - posted 18:58, Wednesday 19 July 2023 - last comment - 16:53, Monday 31 July 2023(71533)
Collecting sqz / no-sqz times at hot, warm, cold, OM2 for quantum noise budgeting

Logging for Brina, who collected a bunch of relevant times to compare sqz vs. no-sqz at different OM2 settings. We aim to do some quantum noise budgeting with these times, to see whether/how much quantum noise is a contributor between 50-150 Hz, and to use the no-sqz data to look at ifo output losses for different OM2 settings. Looking at correlated noise budget from Craig recently, LHO:71333, hopefully we can understand what's going on with quantum noise ~30-200 Hz.. 

Date OM2 temp   gps_start gps_stop UTC   alog
2023/06/27 ~56 C no-sqz 1371910278 1371910578 14:11 to 14:16   1st hot OM2, LHO:70849
    sqz 1371910698 1371910698 14:18 to 14:22    
2023/06/28   no-sqz 1372017274 1372021147 19:54:16 - 20:58:49    70930 1-hour no-sqz, hot OM2, xcorr
    sqz 1372042818 1372046418 3:00 - 4:00 (6/29)    
               
2023/07/13 ~22 C no-sqz 1373320175 1373320818 21:49:17- 22:00:00   cold OM2, LHO:71302 ifo alignment tests
    sqz 1373322138 1373322738 22:22 - 22:32   sqz on, AS 36 Q yaw 50,000
               
2023/07/19 ~47 C no-sqz 1373812338 1373812938 14:32 - 14:42   warm OM2 (during pump iss failure, 71497)
    sqz 1373813118 1373813118 14:45 - 15:00   (should be more sqz times available)
               
2023/07/19 ~57 C no-sqz 1373839430 1373840398 22:03:32 - 22:19:40   2nd hot OM2, LHO:71518
    sqz 1373843778 1373844498 23:16 - 23:28    
Comments related to this report
victoriaa.xu@LIGO.ORG - 16:20, Friday 21 July 2023 (71598)ISC

So far I've just started comparing darm spectra (using GDS-CALIB_STRAIN_NOLINES) between the following times, some from the above table:
-- 'cold OM2' uses no-sqz = 1373320175 - 1373320818, fds = 1373322138 - 1373322738
-- 'warm OM2' uses no-sqz = 1373812338 - 1373812938, fds = 1373813118 - 1373814018
-- 'hot OM2 3' uses the recent hot OM2 no-sqz = 1374004600 - 1374005215 (LHO:71591), and fds = 1373984483 - 1373985483 from when range was ~150 this morning. Note FC detuning is -25 Hz for this trace, and many LSC FFs have been retuned here, compared to previous traces.

To start, I looked at compared both the DARM difference with squeezing for different OM2 settings (sqz compared to OM2), and also un-squeezed / squeezed DARMs for different OM2 settings (OM2_compared_to_sqz).

From this second pdf, OM2_compared_to_sqz, a few quick things I notice:
  - Hot OM2, >1 kHz (in the shot-noise-limited region at high frequencies), darm looks a bit worse; this is consistent with the decrease in optical gain at hot OM2.
  - Hot OM2, ~100 Hz, squeezing seems to give some noticeable improvement around and just above 100 Hz (??). This improvement is not that clear without squeezing. Unclear to me if related to FC detuning or OM2, but I wonder if this ~100Hz noise is in part related to quantum noise..
  - Hot OM2, < 100 Hz, low-frequency noise looks much better; the LSC FF tuning seems very effective at improving noise in this configuration.
  - At warm OM2, maybe low-frequencies < 100 Hz see some scatter shelves (?), but I might just be seeing things, not totally clear. 

Next I'll try to compare this with the quantum noise budget without squeezing, starting by comparing the no-sqz traces to look at IFO shot-noise based output losses, for different OM2s (as Sheila suggested). Ideally this will require independent knowledge of some IFO parameters like the readout angle and the SRCL detuning. Once it makes sense with no-sqz darm, I'll continue to work on making sense of both the full and the semi-classical quantum noise budgets with squeezing injected, and budgeting out the quantum noise contributions to get a sense of whether low-frequency quantum noise (e.g. from sqz misrotations) are plausibly showing up in darm, and what knobs we could turn if so.

Non-image files attached to this comment
victoriaa.xu@LIGO.ORG - 16:53, Monday 31 July 2023 (71849)

Edit: indeed the cold OM2 time had a glitch. Updated plots with the following cold OM2 no-sqz time (different day, early in lock.. but looks more reasonable).

Updated plots: effect of sqz at different OM2s, and sqz vs. no-sqz at different OM2s.

Times used:
cold OM2, no sqz, gps start = 1373371323 (2023-07-14, 12:01:45 UTC)
cold OM2, no sqz, gps stop = 1373372668 (2023-07-14, 12:24:10 UTC)

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