Displaying reports 1-20 of 86953.Go to page 1 2 3 4 5 6 7 8 9 10 End
Reports until 23:37, Friday 13 March 2026
H1 IOO (IOO, ISC)
masayuki.nakano@LIGO.ORG - posted 23:37, Friday 13 March 2026 (89514)
JAC heater on

The JAC heater turned on at 8:00 PM PT. JAC-HEATER_POWER_SET is set to 3.

H1 General
ryan.crouch@LIGO.ORG - posted 19:56, Friday 13 March 2026 (89510)
OPS Friday EVE shift summary
Start Time System Name Location Lazer_Haz Task Time End
23:24 Cheta Sophie Cheta Lab local Workign on Cheta 00:42
00:27 OPS Oli LVEA LOCAL Unplug laptop charger 00:33
Images attached to this report
LHO VE (VE)
gerardo.moreno@LIGO.ORG - posted 19:02, Friday 13 March 2026 (89511)
HAM1 Pumpdown Update

Pumpdown continues on HAM1 and it is progressing.  The chamber is currently being pumpdown with the SS500 cart aiding the turbo pump up on top of the chamber.  We are very close to opening the ion pump for this chamber.  Vacuum pressure is currently at 8.95x10-07 torr.  The aux carts to pumpdown the annulus for both chamber HAM1/2 were disconnected Monday, see aLOG entry 89440.

Images attached to this report
LHO VE (VE)
gerardo.moreno@LIGO.ORG - posted 18:34, Friday 13 March 2026 (89508)
Test of Power Consumption of Y2-8 Ion Pump Controller

I used a power meter to measure the power consumption of a Gamma ion pump controller (Digitel MPCq type) to power the 1200 l/s ion pumps (this one located at Y2-8), I concentrated on startup of the controller, then on startup of the high voltage (7kV) for the ion pump..

During the initial startup of the ion pump controller the consumption goes up slow, it creeps up to 12.04 Watts max, then it drops a bit after.  The second part of the test was to see the consumption spike when turning on the high voltage for the ion pump, for this test the meter immediately goes up to 40.69 Watts, then after a few seconds the power drops slowly.

A side effect of running this test can be appreciated on the attached trend data, because we powered off the ion pump the vacuum pressure internal to the main volume went up, it can be appreciated by the gauges along the Y-End station as well as Y2-8 gauge.

To do the test I powered the unit off and back on 3 times.

Images attached to this report
H1 ISC
sheila.dwyer@LIGO.ORG - posted 18:07, Friday 13 March 2026 (89501)
PRMI locking today, DRMI also now locking

Sheila, Oli, Jennie, Tony, Ryan Crouch

Summary: Today we found that the 9MHz modulation depth was low because of a wrong setting, and that the beam was misaligned on the LSC REFLAIR A diode. After these changes and some gain adjustments we were able to lock DRMI.  

Details:

After restoring the 9MHz modulation depth this morning (89497), we went on to locking PRMI, using the notes from 89491, but scaling for the increased modulation depth.   Once it was locked, Oli and I went to ISCT1 to double check the alignment onto the POPAIR diodes, we slightly improved the alignment onto POPAIR A, but POPAIR B was already well aligned.  We measured 0.55mW in the POPair path before the splitter using a power meter. 

Oli phased POP18 + POP90 to maximize the I ERR signal with PRMI locked, and we put a 132 Hz, 3000 count exitation into PRM LOCK L to phase REFLAIR 9 and 45 to minimize the PRM signal in Q.  (userapps/lsc/h1/templates/phase_REFLAIR.xml)  We then adjusted the gain in REFLAIR 9 to match the ugf to the PRMI reference (screenshot).  In O4, we used a whitening gain of 12dB and then a digital gain of 0.25 before the phase rotation, and LSC input matrix of 1.75 .  Now we are using 30dB of whitening gain and a digitial gain of 4.4 to reproduce the same ugf (input matrix unchanged 1.75), so we are missing a factor of 140 signal strength compared to O4.  For MICH the ugf is also right on the reference, screenshot.  This is with 30dB of whitening gain and a digital gain of 4 before the phase rotation, compared with 0dB of whitening gain an a digital gain of 1 in O4, so this signal is too small by a factor of about 126.  So this is pretty similar to the signal loss for REFLAIR 9.  

Oli and I went back to ISCT1, removed the ND filter, and realigned reflair A.  This gave us 2.5 counts on REFLAIR A LF, and we were able to relock PRMI with the whitening gains for REFLAIR back to normal.  We adjusted the phase of reflair, and added some digital gains to set the ugfs to what they used to be.  

A comparison time with PRMI locked in November 14th 2025, 22:23:00 UTC

  Nov 14th 2025 22:23 UTC PRMI locked today PRMI locked nov/now ratio taking gain changes into account
POPAIR A LF ~17 counts 16 counts fine
POPAIR B LF 12 counts 8 counts 1.5
POPAIR B 18 100 counts, whitening gain 12dB, digital gain of 2  80 counts, whitening gain is 36dB, digital gain of 2 20 (improved with aligment)
POPAIR B 90 70 counts, whitening gain 6dB, digital gain 4 90 counts, 18dB whitening gain, digital gain 4 3
ASC POP X  DC SUM 40 counts -1 running raster on PM1
reflair A LF 2.5 2.5 after today's realignment
reflair B 5.5 5.3 yay?
reflair A RF9 signal  whiten gain of 12dB, digital gain of 0.25 whiten gain 12dB, digital gain of 0.31 1.25
reflair RF45 signal whiten gain 0dB, digital gain 1 whiten gain 0dB, digital gain of 2.17 2.17

We ran SRY alignment manually, (the WFS don't work since we have not rephased them).  

This screenshot shows the gains I had manually adjusted when we got a 3 second DRMI lock, March 13th at 23:28:21 UTC.  

DRMI locking references: trigger levels: 44348  filter states and loop measurements: 87768   When DRMI grabs for a few seconds, it looses lock due to a 20Hz oscillation (screenshot), which suggests the MICH gain is too high.  I tried a few changes to MICH gains.  In this grabbing attempt, it seems that the MICH filter changes are what is making things unstable.  

Edited to add: We have locked DRMI, with three manual changes, to the POP18 digital gain (set to 3 as in screenshot), RF9 gain set to 0.31, and RF45 gain set to 2.17.  We think that this was too high for RF45, and instead it should be left as SDF will set it at 1.  We stepped through the DRMI_locked guardian state manually which was fine.  

 

 

Images attached to this report
H1 IOO
jennifer.wright@LIGO.ORG - posted 17:36, Friday 13 March 2026 (89509)
Added error message to JAC GUARDIAN for shutter

I added a check for the JAC shutter to the 'LOCKING' state to its guardian. This was because it was closed when the guardian was trying to lock JAC this morning and it took us a while to figure out.

We haven't had a chance to check this today due to efforts to lock DRMI but I will check it on Monday.

Its on lines 207-209 of the script.

 if ezca['SYS-MOTION_C_SHUTTER_M_STATE'] != 0:#added to notify if shutter closed. J Wright 2026-03-13.
            notify('Shutter closed. Check shutter trigger values.')
            self.timer['waiting'] = 5

Thanks to Tony for helping me debug gedit.

H1 SUS (CDS)
oli.patane@LIGO.ORG - posted 17:11, Friday 13 March 2026 (89507)
RM2 WD bypassed for now

Control room

RM2 SWWD has been bypassed temporarily until we offload some of it since we're near the end of the ADC range for one of the channels.

The ADC reaching the end of its range isn't what actually caused the trips though . The HAM1 ISI SW watchdog tripped after being triggered by RM2's LP SWWD. It looks like the LOCK filter bank integrators had started raking up counts, eventually causing large oscillations in the suspension that surpassed the LP SWWD threshold. The integrators for RM1, RM2, and PM1 all started building up at the same time, but for whatever reason the build ups on RM2 were much larger.

Jim says that he doesn't care for the HAM1 ISI whether any of the little tip tilts on there trip, so we're bypassing RM2 for now since its the closest to tripping.

LHO VE (VE)
gerardo.moreno@LIGO.ORG - posted 17:06, Friday 13 March 2026 (89506)
Survey Of Site Cryopump's Pumpout Port

Took a picture of the pumpout port for each of the cryopumps.

The attached pictures below are from CP1 to CP8 from left to right.

 

Images attached to this report
H1 ISC
jennifer.wright@LIGO.ORG - posted 17:04, Friday 13 March 2026 (89503)
POPAIR and REFLAIR checks

Jennie W, Sheila D,

 

I compared the RF monitor values for POPAIR and REFLAIR LSC photodioes between today during state 51 "PRMI LOCKED" and 2026-11-14 22:28:00 UTC in state 50 "ACQUIRE PRMI".

Note we re-aligned both POPAIR B and REFLAIR A yesterday.

POPAIR A RF9 and RF45 have not changed much.

POPAIR B RF18 and RF90 have reduced a lot.

As have REFLAIR A RF9 and RF45.

REFLAIR B RF27 and RF135 have gone up instead of down which seems less worrying for locking purposes.

Name 14th Nov[dBm] Today[dBm] P_today / P_Nov
POPAIR_A_RF9 -54.8

-54.9

0.98
POPAIR_A_RF45 -54.6 -55 0.91
POPAIR_B_RF18 -49.6 -53.9 0.37
POPAIR_B_RF90 -46.9 -51.4 0.35
REFLAIR_A_RF9 -45.4

-55.4

0.1
REFLAIR_A_RF45 -37.5 -54.6 0.02
REFLAIR_B_RF27 -53.1 -50.0 2.0
REFLAIR_B_RF135 -30.2 -28.0 1.7

 

After this Oli and Sheila re-aligned REFLAIR A (detailed in Sheila's log 89501).

Images attached to this report
H1 CDS
david.barker@LIGO.ORG - posted 16:53, Friday 13 March 2026 (89505)
SUS-AUX models' filter-module MEDMs now available

The SUS-AUX models have filtermodules, and until now the MEDMs for these have not been easily accessible.

With help from AI, I have written a python program which produces a set of MEDMs to permit navigation down the SUS-AUX tree to open MEDMs which display the filter modules.

To open the top level screen, which lists all the susaux models, a "SUSAUX Filters" button has been appended to the SUS pull down in the systems section of the SITEMAP (first attachment).

The second attachment shows the resulting FM screen when navigating from h1susauxb13 -> ITMX -> L2 -> NOISEMON

 

Images attached to this report
H1 General (IOO, ISC)
anthony.sanchez@LIGO.ORG - posted 16:43, Friday 13 March 2026 (89504)
Friday Ops Day shift report.

TITLE: 03/13 Day Shift: 1430-2330 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Planned Engineering
INCOMING OPERATOR: Ryan C
SHIFT SUMMARY:
The Commissioning crew today were focused on trying to get PRMI locked and stable for most of the day. Thye touched up the REFL A alignment which helped. 
But there seems to be some power lost somewhere.

This spreadsheet was created to document the difference in the ratio of  IMC Trans power/IMC input power back in the O4 run and now.  Specifically when the PSL is set to 2 Watts. Feel free to update this in the future.

 The Gain for H1:ALS-C_TRX_A_LF_GAIN has been bumped from 1.5 to 3 to get past FIND IR without issue.
This may not be the only gain that has been turnt to 11 to get DRMI to almost lock today,  Sheila will be posting an alog later with some laser power acounting that may shed more light on that situation. Yes the Pun was intended.

LOG:                                                                                                                                                                                 

Start Time System Name Location Lazer_Haz Task Time End
14:39 FAC Randy Xarm N Plowing the Tumbleweeds 17:02
15:06 H2O Water contrators Well N Testing the well water 18:06
17:04 VAC Travis Cleaning Racks & west bay, All ES and Mids N Looking for parts 19:34
17:26 FAC Randy LVEA N Walk about in the LVEA 17:49
18:28 PEM Ryan CER N Checking Dust mons 18:31
18:32 SPI Jeff & Josh Optics Lab Yes Working on SPI setup. 23:07
18:43 ISC Sheila & Oli LVEA Yes Tweaking alignments on ISCT1 19:09
18:50 OPS LVEA IS Birfurcated HAZARD HAM1 LOCAL LVEA Bifurcated LASER HAZARD 11:29
19:37 EE Marc LVEA & CER N placing stickers and parts. 20:07
20:36 EE Fil & Marc Mid Y N getting cables. 21:14
20:49 VAC Gerardo EndY N Anulus ion pump controller testing, unplug replug 21:24
21:15 PEM Ryan C LVEA N chasing cables 22:25
23:24 Cheta Sophie Cheta Lab local Workign on Cheta 00:24
H1 General
ryan.crouch@LIGO.ORG - posted 16:10, Friday 13 March 2026 (89502)
OPS Friday EVE shift start

TITLE: 03/13 Eve Shift: 2330-0500 UTC (1630-2200 PST), all times posted in UTC
STATE of H1: Planned Engineering
OUTGOING OPERATOR: Tony
CURRENT ENVIRONMENT:
    SEI_ENV state: CALM
    Wind: 6mph Gusts, 4mph 3min avg
    Primary useism: 0.02 μm/s
    Secondary useism: 0.21 μm/s 
QUICK SUMMARY:

H1 CDS
erik.vonreis@LIGO.ORG - posted 12:34, Friday 13 March 2026 (89500)
ndscope updated

There was a conda update on control room workstations to update ndscope from 0.20.7 to 0.20.8.

The new version fixes a bug where old data could be left on the plot when changing the time window if there was no data for that window from NDS.  Thanks to Jenne for finding this bug.

It also fixes a bug where HDF5 and Matlab exports might be empty, and improves messaging around exports.

LHO VE
david.barker@LIGO.ORG - posted 12:00, Friday 13 March 2026 (89499)
Fri CP1 Fill

Fri Mar 13 10:15:08 2026 INFO: Fill completed in 15min 4secs

 

Images attached to this report
H1 ISC
sheila.dwyer@LIGO.ORG - posted 10:59, Friday 13 March 2026 (89497)
9MHz modulation depth was low

Tony, Filiberto, Sheila, Jennie Wright, Oli

This morning we tried to do an OMC scan to check the modulation depths.  The OMC high voltage was off, Filiberto found that the supply was powered on but the output disabled, so he enabled it.  

We used 10W input power single bounce off ITMX.  I compared this to a reference from 65828, it seems as thought the 9MHz is too small. 

  April 2022 this morning  (EOM driver 23.4dBm 9 Mz, 27dBm for 45MHz) now  (EOM driver 27dBm 9 Mz, 27dBm for 45MHz) modulation depth now (calculated by Oli and jennie W) modulation depth from April 2022 (alog 81816)
9MHz +/00 peak height 11.4e-3 5.04e-3 11.7e-3 .217 0.213
9MHz -/00 peak height 11.7e-3 5.4e-3 11.6e-3 .215  
45MHz +/00 peak height 1.9e-2 1.7e-2 1.7e-2 .266 0.275
45MHz -/00 peak height 1.9e-2 1.7e-2 1.7e-2 .265  

Jennie Wright checked modulation depths in 89456, at that time the EOM driver was set to 27dBm for 9MHz, on 10 am on March 10th it was set to 23.4dBm.  This was in SDF as 23.4dBm, but this channel is not monitored and this table is not in SDF revert. ISC_LOCK prep for locking sets these values because they get changed in low noise, I've changed it in lsc params now.  

Images attached to this report
H1 General
anthony.sanchez@LIGO.ORG - posted 07:44, Friday 13 March 2026 (89495)
Friday Morning shift report.


TITLE: 03/13 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: EARTHQUAKE
    Wind: 5mph Gusts, 3mph 3min avg
    Primary useism: 1.02 μm/s
    Secondary useism: 0.21 μm/s 
QUICK SUMMARY:

Site is wet, wind is low.
When I walked in there was an active 6.3M earthquake rolling through from Chile.
I'll give the earthquake about 10 more minutes to roll on through then start locking green arms and PRX for the comissioners.
 

LHO General (SUS)
corey.gray@LIGO.ORG - posted 21:21, Thursday 12 March 2026 (89490)
Thurs EVE Ops Summary

TITLE: 03/12 Day Shift: 1430-2330 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Planned Engineering
INCOMING OPERATOR: Corey
SHIFT SUMMARY:

Jenne/Jennies locked pseudo-PRMI earlier in the shift.  Ran trend plots of sus for comparison between today and Nov2025 (see Jenne's alog).
LOG:

H1 ISC
jenne.driggers@LIGO.ORG - posted 17:42, Thursday 12 March 2026 - last comment - 10:36, Friday 13 March 2026(89491)
PRMI locked 1f using REFLAIR, many analog gains cranked up

[Sheila, Jennie, Jenne, RyanS, Corey]

We have been able to get PRMI locked (with arms held off resonance using ALS).  To do this we:

PRMI locked without too much fuss.  Since we've effectively also increased the noise on the error signals, it's a bit delicate, and I lost lock twice while touching up alignment. The third lock I was able to go a bit slower when touching up BS and PRM alignment, and we've now been locked for more than 20 mins (aka infinity).  Jennie is taking PRCL and MICH OLGs.

The attached image shows all the things that I had changed. 

Nothing is in guardian (except maybe some trigger thresholds which should be reverted), and nothing is saved in SDF. 

Images attached to this report
Comments related to this report
sheila.dwyer@LIGO.ORG - 10:36, Friday 13 March 2026 (89498)

I did a sneaky phasing of POP18 yesterday, by 180 degrees, to make the flashes positive. 

jennifer.wright@LIGO.ORG - 18:06, Thursday 12 March 2026 (89493)

I used the lscparams to change the MICH triggers so I shave put these values back.

Below are OLG TFs I ran from userapps/lsc/h1/templates/PRCL and userapps/lsc/h1/templates/MICH

For PRCL the measurement is shown here where blue is the reference measurement in the tenplate, and red and green are the measurements I took today with different injection amplitudes.

We had to raise the injection in PRCL by a factor of 2.5 ti check the wiggles we can see in the gain between 10 to 30Hz are real.

Here is the measurement for MICH. Not sure we understand either of these yet. More investigation to come tomorrow.

 

Here is an ndscope with the 'good PRMI ACQUIRE time' we were using to scale gains and trigger levels. That is a prmi where we eventually locked and I picked the highest flash that occurred before we did.

Images attached to this comment
H1 SUS
thomas.roocke@LIGO.ORG - posted 16:12, Thursday 12 March 2026 - last comment - 19:12, Friday 13 March 2026(89487)
QOSEM Flag Gluing
[Tom R, Ibrahim]

We glued 6x of the QOSEM flags, attaching the lens (D2500277) to the aluminium body (D2500253). This was done using a jig (D2600054) to ensure the lenses were aligned to the body of the flag. We used EP30.

Only a tiny drop of glue is required, and was applied directly to the lip of the body using a thin wire. The flags will be left to dry overnight before another batch of 6 will be glued.
Images attached to this report
Comments related to this report
thomas.roocke@LIGO.ORG - 19:12, Friday 13 March 2026 (89513)
The flag gluing yesterday was successful, with a strong joint and nothing obscuring the lens itself. We continued and glued another 6x flags up, and will do 6x more next week
Images attached to this comment
H1 IOO (ISC)
jennifer.wright@LIGO.ORG - posted 17:26, Friday 20 February 2026 - last comment - 09:39, Friday 13 March 2026(89218)
JAC work today summary

Jennie W, Keita K, Rahul K, Ryan S,

 

This morning Keita turned the power up to 1 W and the purge air down in order to scan the OMC and measure the modulation index.

We had some work to do to lock the JAC, the cavity wouldn't scan properly when managed by the guardian code.

Ryan and I have looked back at it and think there may be something wrong with the feedback to the PZT. It can't be the PZT itself though, because Keita and I were able to lock on the TRANS PD signal with the dither locking done manually by tuning the PZT offset to find the resonance and then turning on the feedback.

I have enclosed a picture to aid problem solving next week.


We then had problems keeping the IMC locked so Keita had to change the threshold used to check if the cavity is locked down to 2. This was changed at line 133 in ISC_library.py at userapps/h1/isc/guardian/.

trans_pd_lock_threshold = 2

We then managed to do three scans,

one with 45 MHz off, one with both on, and one with 9 MHz off. Detailed analysis in progress.


After turning the power back down Keita and Rahul swapped the mirror we currently have in front of the TRANS PD, with the uncoated laser window that is meant to be there (JACT_BS1).

They had to top gun and swab it to remove two dust particles first.

This replacement means the power to the PD is lower and so we needed to power up to 1W to check this alignment.

I have left the mirror we took out on the table on the -Y side labelled as 'HR mirror taken out of JACT-BS1'. Need to check which exact mirror this is with Masayuki on Monday.

Keita locked the cavity manually with the REFL PD and optimised the amount of light falling onto the TRANS PD.

I powered down to 100mW and de-energised the rotation stage and closed the light pipe at the end of the day. We also had the rotation stage de-energised and locked out when we were working in chamber.

Images attached to this report
Comments related to this report
jennifer.wright@LIGO.ORG - 15:31, Monday 23 February 2026 (89230)IOO, ISC

FSR = 265 MHz (see this ref and table on P.110).

FSR in s on scan = 8.39 s

For the 9 MHz on the measurement with both sb at nominal power: : 0.0103mA is the upper 9 MHz sb  vs. 0.745 mA carrier (left-hand TM00 peak).

m_9 = 2*sqrt(0.0103/0.745) = 0.235

For 45 MHZ in same measurementdata : 0.0151 mA is the upper 45MHz carrier  vs. 0.745 mA carrier (left-hand TM00 peak).

m_45 = 2*sqrt(0.0151/0.745) = 0.285

 

The 9MHz seems similar to this (alog #89001) measurement with the previous crystal (0.26) but the 45MHz is different (0.31).

jennifer.wright@LIGO.ORG - 09:39, Friday 13 March 2026 (89496)

Here is the scan results pic which I forgot to include.

 

Images attached to this comment
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