Displaying reports 11041-11060 of 84723.Go to page Start 549 550 551 552 553 554 555 556 557 End
Reports until 15:55, Monday 19 February 2024
H1 CDS
david.barker@LIGO.ORG - posted 15:55, Monday 19 February 2024 - last comment - 19:51, Monday 19 February 2024(75887)
Beckhoff slow controls system is currently down, invalid alarms have been bypassed

Daniel, Dave:

h1ecatc1, the Beckhoff slow controls system, crashed at 15:38 this afternoon. The EDC is showing 35365 disconnected channels. The computer is completely unresponsive, including its management port. It will need a manual reset.

The alarms system restarted itself at this time. The ongoing HAM6 alarms remain bypassed, and in addition I have bypassed some invalid temperatures channels

Bypass will expire:
Tue Feb 20 03:49:26 AM PST 2024
For channel(s):
    H0:VAC-LX_Y0_PT110_MOD1_PRESS_TORR
    H0:VAC-LY_Y1_PT120B_PRESS_TORR
    H1:PEM-C_CER_RACK1_TEMPERATURE
    H1:PEM-C_MSR_RACK1_TEMPERATURE
    H1:PEM-C_MSR_RACK2_TEMPERATURE
    H1:PEM-C_SUP_RACK1_TEMPERATURE
 

Comments related to this report
daniel.sigg@LIGO.ORG - 19:51, Monday 19 February 2024 (75889)

Updated to the most recent svn, and restarted.

H1 CDS
david.barker@LIGO.ORG - posted 11:08, Monday 19 February 2024 (75886)
TW1 offload raw minute trend files completed

WP11702

The file copy completed at 12:23 Sun 18th Feb. This morning I reconfigured NDS1 daqd to serve the past 6 months of data from the permanent archive area, daqd was restarted at 08:44 this morning.

The old files were then deleted from TW1's SSD-RAID between 08:53 and 10:54, taking 2hours 1min.

LHO VE
david.barker@LIGO.ORG - posted 10:17, Monday 19 February 2024 (75885)
Mon CP1 Fill

Mon Feb 19 10:11:56 2024 INFO: Fill completed in 11min 52secs

Start time has been changed to 08:00 for tomorrow's early fill prior to CDS network upgrades.

Images attached to this report
LHO VE
david.barker@LIGO.ORG - posted 10:20, Sunday 18 February 2024 (75884)
Sun CP1 Fill

Sun Feb 18 10:10:41 2024 INFO: Fill completed in 10min 37secs

Images attached to this report
LHO VE
david.barker@LIGO.ORG - posted 10:23, Saturday 17 February 2024 (75882)
Sat CP1 Fill

Sat Feb 17 10:10:46 2024 INFO: Fill completed in 10min 42secs

Images attached to this report
H1 CDS
david.barker@LIGO.ORG - posted 10:21, Saturday 17 February 2024 - last comment - 13:27, Saturday 17 February 2024(75881)
Start process of raw minute trend offload from DAQ TW1

WP11702 TW1 offload

I've started the process of offloading the past 6 months of raw minute trends from TW1's SSD-RAID to h1ldasgw1's permanent storage.

The first step was to freeze the almost full directory and switch TW1 over to writing to a new empty area, and then temporarily configuring NDS1 to serve data from the frozen dir while the file copy is in progress.

To this end, NDS1 daqd was restarted at 10:14 PST this morning.

Comments related to this report
david.barker@LIGO.ORG - 13:27, Saturday 17 February 2024 (75883)

as of 13:23 copy is 9.3% complete, ETA 11:39 Sunday morning.

LHO VE
janos.csizmazia@LIGO.ORG - posted 21:09, Friday 16 February 2024 (75880)
2-16 vent vacuum diary
Today's activities:
- HAM7 pumpdown status: ~3.3E-6 Torr
- Corner pumpdown status: ~3.9E-1 Torr. On Tuesday, transitioning to Turbo (Y-manifold; OMC; HAM6)
- EX pumpdown status: 3.75E-8 Torr: the post-vent RGA scan is ready, the results will be in the comment comment section, once they are published. The comparison with past RGAs is also coming next week. If the results will be considered satisfactory, the Ion-pump will be valved in. The GV will remain closed during FAC works
- The purge air supply at FCES is switched on, in order to start HAM8 vent first thing next week
H1 SQZ
naoki.aritomi@LIGO.ORG - posted 19:28, Friday 16 February 2024 - last comment - 23:10, Monday 19 February 2024(75879)
PMC is locked with p polarization

Naoki, Nutsinee, Daniel

We installed all the optics for PMC and locked the PMC with p-polarization. We will lock the PMC with s-polarization and align SHG, CLF, seed next week.

First we put a HWP before PMC and changed the beam to the p polarization since the p-pol has much lower finesse in PMC and it is easy to align. The HWP angle is 152 for p-pol and 108 for s-pol. 

We aligned two steering mirrors before PMC. Fig. 1 and 2 show the PMC trans (blue) and refl (red) with PMC scan. The mode matching is 93% and the refl dip reaches 88% from the maximum.

We found that the label of the pick off mirror before PMC REFL PD says R=5% for s-pol, but it was actually R=90% for s-pol and R=70% for p-pol. The PMC REFL power is ~30mW and more than 20mW was injected to PMC REFL PD, which is a lot. So we replaced this mirror with the mirror which is R=8% for s-pol and R=1% for p-pol.

Then we adjusted the demod phase of PMC PDH signal and locked the PMC with p-pol. The UGF is 1.3 kHz and phase margin is 67 deg as shown in Fig. 3. We accepted the SDF related to PMC as shown in Fig. 4. 

Note that we will have 20 times more optical gain with s-pol because of higher finesse. Also we will have 8 times more power at PMC REFL PD with s-pol because of the pick off mirror. So we need to reduce the gain by 160 with s-pol to have the same UGF as p-pol.

Images attached to this report
Comments related to this report
nutsinee.kijbunchoo@LIGO.ORG - 17:50, Monday 19 February 2024 (75888)

After the pick-off mirror swap with 34mW input we have ~2mW hitting the PMC Refl. DC readout reads 75mW. The HWP before the PMC is set to s-pol at the moment.

Attached an updated picture of the SQZT0 table. All the optics are in.

Images attached to this comment
daniel.sigg@LIGO.ORG - 23:10, Monday 19 February 2024 (75890)

The PMC PZT trigger has the PMC TRANS PD wired to channel 1 and PMC REFL to channel 2.

The DC readback of PMC_REFL is saturating and the gain adjust is broken due to a missing ground wire in the controls of aux concentrator 11 (which pegs the adjustable gain to 40dB).

Nevertheless, we were able to engage the guaduan to lock the PMC using the dip in reflection.

LHO General
ryan.short@LIGO.ORG - posted 16:01, Friday 16 February 2024 (75877)
Ops Day Shift Summary

TITLE: 02/16 Day Shift: 16:00-00:00 UTC (08:00-16:00 PST), all times posted in UTC
STATE of H1: Planned Engineering
INCOMING OPERATOR: None
SHIFT SUMMARY: Another busy day; CS volumes still pumping down.

LOG:

Start Time System Name Location Lazer_Haz Task Time End
16:25 FAC Randy LVEA/FCES - Moving scissor lifts in/out of VEAs 19:21
17:23 IAS Jason, RyanC LVEA - Surveying in BG 19:13
17:29 VAC Jordan, Gerardo EX - RGA scans 19:21
17:42 FAC Karen, Kim FCES - Technical cleaning 18:05
17:47 SQZ Nutsinee Optics Lab - Gathering equipment 18:10
18:01 CDS Fil LVEA - Cabling cleanup 19:19
18:04 VAC Janos LVEA - Check on vacuum pump 18:45
18:10 SQZ Nutsinee, Daniel, Naoki LVEA Yes Local hazard work on SQZT0 21:24
18:21 FAC Karen, Kim LVEA - Technical cleaning 18:44
19:04   Ryan S LVEA soon Transitioning to Laser Hazard 19:19
19:20 CDS Fil, Camilla LVEA Yes Check power on HWS tables 19:51
19:22 SAF LVEA is Laser HAZARD LVEA Yes LVEA is Laser HAZARD Ongoing
20:05 VAC Janos LVEA Yes Checking on vacuum pump 21:05
20:14 TCS Camilla LVEA Yes Power on HWS tables 20:21
21:05 VIS Tony, Julian, Ibrahim, Dana, Dripta, Oli Roof - Showing visitors the view 21:13
21:06 VAC Jordan, Gerardo EX - RGA scans 22:31
21:41 IAS Jason, RyanC LVEA Yes FARO surveying in W-bay 22:28
21:50 SQZ Naoki, Daniel, Nutsinee LVEA Yes SQZ PMC work Ongoing
22:39 VAC Jordan, Gerardo FCES - RGA scans 23:36
22:40 VAC Gerardo LVEA Yes Looking for Janos 22:50
23:01 SQZ Camilla, Julian Optics Lab - Building spare SHG Ongoing
H1 TCS (CDS)
camilla.compton@LIGO.ORG - posted 14:14, Friday 16 February 2024 - last comment - 13:02, Tuesday 27 February 2024(75876)
Changed Wiring in HWS Camera External Power Supply - Have proposed coupling of combs!

Fil, Luis, Camilla. FRS 26828#c11 Previous troubleshooting in alog 7495174750.

Today Fil went onto the HWS table and verified the HWS cameras are connected straight to the external power supply (photos in FRS26828#c8) via cables connected together. The HWS camera fiber CLink box is powered by the HWS breakout chassis D1200934 (originally designed to power cameras too).

Fil theorized that the HWS grounding is due to the power supply to fiber CLink connection grounding the cameras! With a multi-meter, we verified the HWS camera is grounded to the table when the CLink power cable is connected but when we disconnect CLink power, the camera is not grounded to the table (has Kapton tape and plastic bolts).

Step 1 (Completed): I removed the grounding cables from the HWS external power supply as Luis suggested in FRS 26828#c11, to avoid us holding the cameras negative terminal at mains ground. Photo of current connections attached. 

Step 2 (Planned): After verifying step 1 doesn't effect the combs (need overnight "quiet" data), Fil will make a new cable to power both the camera and CLink's via the external supply (14V is fine for both). 

Images attached to this report
Comments related to this report
camilla.compton@LIGO.ORG - 09:42, Wednesday 21 February 2024 (75911)

Preet, Camilla

It appears changing the cabling of the external power supply has removed/reduced the comb: compare blue trace before cabling change to red trace afterwards change in attached plot.

To verify this, we undid the cabling change, back to the old configuration this morning at 9:30am and turned the camera back to 7Hz each, we'll later check if the comb reappears. 

Images attached to this comment
camilla.compton@LIGO.ORG - 10:58, Tuesday 27 February 2024 (75996)CDS, DetChar, PEM

Preet, Camilla, FRS 26828 

With the swap back to the old cabling, we confirmed that the comb came back, see Feb 22nd data in attached plot. This morning I changed the cabling back to the "quiet" version, photo attached. 

Question for others, is the old cabling expected to push noise into DARM or is there an unknown coupling? Tagging PEM, CDS, Detchar. 

Images attached to this comment
luis.sanchez@LIGO.ORG - 13:02, Tuesday 27 February 2024 (76001)
Have you try using a different power supply or low the voltage to +12v? the camera also works with +12v and the rcx c-link only required +5v supply.
LHO VE
david.barker@LIGO.ORG - posted 11:10, Friday 16 February 2024 (75875)
Fri CP1 Fill

Fri Feb 16 10:11:32 2024 INFO: Fill completed in 11min 28secs

Gerardo confirmed a good fill curbside.

Images attached to this report
H1 ISC
elenna.capote@LIGO.ORG - posted 08:42, Friday 16 February 2024 - last comment - 20:20, Sunday 10 March 2024(75874)
Another look at the LSC Coupling

This log follows up some previous work that's been done to understand the LSC, in particular MICH, noise coupling that we have observed. The most recent work done on this front was by Dana, in alogs 74477 and 74787.  Notably, the MICH coupling follows an interesting shape here, especially below 20 Hz. For MICH, we expect a flat coupling depending only on the finesse, Gm = pi/2*F. Evan Hall made some great measurements of this coupling years ago and you can see the results in Fig 2.17 of his thesis(link to thesis)- without any feedforward the magnitude of the coupling is flat in frequency down to 10 Hz. However, Dana's measurements clearly show a frequency dependent coupling below 20 Hz. Also, Dana mentions that the MICH coupling is about 40% too high than we expect based on finesse.

I'll add here a quick note that currently the UGF of MICH is about 8 Hz and the UGF of SRCL is about 11 Hz, so I think it's safe to assume that we are not seeing any significant closed loop effects from either of these loops down to about 12 Hz in these measurements.

Something to remember here is that when we measure the MICH coupling we drive the beamsplitter which does induce a change in the MICH length, but it also changes the SRCL and PRCL length. Therefore, we should expect to pick up SRCL coupling along with the MICH coupling when we measure. Evan's thesis also includes the form of the SRCL coupling in Eq 2.29: Gs = 0.012 [m/m] * Pa/750 [kW] * dL/10 [pm] * F/450 * (10 [Hz] / f)^2 (I am only including the first term that dominates at low frequency). The SRCL coupling results from radiation pressure in the SRC due to the DARM offset (dL), power in the arms (Pa), and finesse (F) and follows a 1/f^2 slope (again, I am ignoring the second term here that rises like f^2 at high frequency). We are operating at much higher power and double the DARM offset, Pa=370 kW and dL = 20 pm (and F = 440).

Regarding the 40% excess MICH coupling, if you divide Dana's result by an additional sqrt(2), it lines up exactly how you would expect. Is there a chance the MICH calibration is missing a rt2 factor related to the fact that we measure from the beamsplitter?

Assuming I'm correct about the sqrt(2) factor, and plotting the magnitude of the expected MICH and SRCL coupling along with Dana's calibrated measurement, our expected O4 SRCL coupling lines up almost exactly with the response at 20 Hz and below (see first attached plot).

I think this effect has always been there, but not easily observable because the SRCL coupling was much lower due to lower operating power and smaller DARM offset. Comparing Evan's MICH coupling measurement (Fig 2.17) with his SRCL coupling measurement (Fig 2.18), the SRCL coupling at 20 Hz was close to an order of magnitude lower than the MICH coupling.

I think this understanding of the coupling better explains why we need to put so much work into the LSC feedforward. Specifically, we measure the coupling for MICH and SRCL, and then usually tune MICH first and then SRCL. Then, to do our iterative tuning, we redo the MICH coupling. It's likely we could do a better job first just tuning SRCL and then measuring and tuning MICH, since we need to subtract the SRCL coupling well enough to get a "true" measure of the MICH coupling.

Furthermore, the SRCL coupling is dependent on our DARM offset. When we make changes to OM2, for example, we change the mode matching at the output. Since we servo to keep the amount of light on the DCPDs constant, we could be changing the required length to achieve this amount of light slightly. In principle, this should only effect the SRCL coupling, but since SRCL shows up in our MICH coupling measurement, it effects both.

Finally, it appears in Dana's measurement that there is a rising trend above 30 Hz, which I have no explanation for. I don't think that can be explained by the SRCL coupling. A look at that second term in the SRCL coupling equation: Gs = 3e-5 [m/m] * phi_s/10 [deg] * dL/10 [pm] * F/450 * (f / 100 [Hz])^2 (Evan's thesis Eq 2.29), I estimate that with a SRCL detuning of about 1 deg, around 30 Hz the SRCL coupling term with an f^2 slope is about 5.3e-7 m/m. This is both too small and the wrong slope to explain that feature.

Images attached to this report
Comments related to this report
elenna.capote@LIGO.ORG - 16:53, Friday 16 February 2024 (75878)

I started poking around the CAL CS screens, and I noticed that the BS control path calibration screen has a "sqrt(1/2)" filter in M1 and M2 that is not engaged. Maybe that solves the rt2 mystery (screenshot attached).

Next, I took a look at the calibrated SRCL coupling. Thanks to Dana's fantastic documentation of the steps in 74477 I was able to generate the calibrated measurement of the DARM/SRCL transfer function (for the time of the SRCL excitation with no feedforward, use GPS time 1371490640). The DTT file is saved as "/ligo/home/elenna.capote/LSCFF/SRCL_DARM_cal.xml"

I exported the data and plotted it against my calculation of the SRCL coupling equation using both terms, Evan's thesis eq 2.29. For the high frequency term that is dependent on microscopic SRCL detuning, I used 0.5 deg (and darm offset 20 pm and finesse 440), which I got to by guessing and matching the trace. See the result in the second attachment.

Overall, the measurement magnitude is too low by a factor of 3. However, the slope matches up quite well. Given that we were apparently missing a rt2 in the MICH calibration, I am convinced that somewhere in the SRCL Cal screen, some filter magnitude is off by 3. Off the top of my head, I know that Gabriele updated the M1 offload filter for PRM and SRM, and that doesn't look like it has been updated in CAL CS. I'm not sure if other aspects are out of date as well. For those comparing the plots, the red SRCL trace in both LSC coupling plots is exactly the same.

Images attached to this comment
elenna.capote@LIGO.ORG - 20:20, Sunday 10 March 2024 (76238)

Reading Matt's alog calculating the DARM offset (alog 76236), I realized made a pretty big error in these noise coupling calculations. I incorrectly assumed "double darm offset" meant 20 pm instead of 10 pm, but it actually means 40 mW instead of 20 mW. Therefore, I need to calculate what the DARM offset was around the time of these measurements. Dan took some contrast defect measurements at 60W using the O4a TCS settings before we powered up in April (see pdf attachment). I also trended back in time to confirm that this measurement was indeed taken in the 60W configuration.

Dan's measurement shows about 1 mW of contrast defect and b=0.648 mW/pm^2. Therefore, the DARM offset during O4a was likely around 7.7 pm, using 40 mW of DARM offset light (dL = sqrt((40-1)/0.648)). Recalculating the expected SRCL noise coupling value in m/m shows it lines up very well with the calibrated SRCL measurement (see plot). Therefore, my assumption in my previous comment that the difference in expected versus measured value was due to miscalibration seems less likely.

However, this corrected result now casts doubt on my assertion that the MICH coupling behavior at low frequency can be explained by SRCL coupling. Using the corrected DARM offset value shows that the SRCL coupling is less than the observed coupling at low frequency by about a factor of 3 (see plot).

Images attached to this comment
Non-image files attached to this comment
LHO General
ryan.short@LIGO.ORG - posted 08:03, Friday 16 February 2024 (75873)
Ops Day Shift Start

TITLE: 02/16 Day Shift: 16:00-00:00 UTC (08:00-16:00 PST), all times posted in UTC
STATE of H1: Planned Engineering
OUTGOING OPERATOR: None
CURRENT ENVIRONMENT:
    SEI_ENV state: CALM
    Wind: 12mph Gusts, 10mph 5min avg
    Primary useism: 0.03 μm/s
    Secondary useism: 0.31 μm/s
QUICK SUMMARY: Corner volume continues to pump down; temperatures below freezing around 24F/-4.5C on-site.

LHO VE
janos.csizmazia@LIGO.ORG - posted 19:14, Thursday 15 February 2024 (75872)
2-15 vent vacuum diary
Today's activities:
- The Annulus Ion Pump of HAM7 - after ~1.5 days of pumping - is now switched on. There was a leak at the septum plug - temporarily it is solved, the annulus pressure now is in the E-5s
- HAM7 pumping status: ~7.8E-6 Torr
- Corner pumpdown status: ~1.2 Torr
- EX pumpdown status: 3.88E-8 Torr: ready for an RGA scan
- A pre-vent RGA scan was made on HAM8. The results will be available in the comment section, once they are published
H1 SEI
thomas.shaffer@LIGO.ORG - posted 16:25, Thursday 15 February 2024 (75871)
Added CPS noise test to DIAG_MAIN

Copied from LLO (LLOalog69495), I've added this test to our DIAG_MAIN. I haven't tested by putting the CPSs into a bad state, but Jim and I will do this next week.

LHO General
thomas.shaffer@LIGO.ORG - posted 16:23, Thursday 15 February 2024 (75870)
Ops Day Shift End

TITLE: 02/16 Day Shift: 16:00-00:00 UTC (08:00-16:00 PST), all times posted in UTC
STATE of H1: Planned Engineering
INCOMING OPERATOR: None
SHIFT SUMMARY: Pumpdown efforts continue, SQZ table work created a local hazard in the East bay.
LOG:

Start Time System Name Location Lazer_Haz Task Time End
16:02 FAC Karen, Kim LVEA n Tech clean 17:03
16:03 FAC Ken OSB/LVEA rec. n Light changes 23:44
16:39 VAC Gerardo, Jordan LVEA n Start HAM7 pumpdown, continue corner 19:14
17:01 FAC Randy FCES n Vent prep 21:01
17:27 CDS Fil LVEA-BG n Cable pulling in beir garten 00:47
17:53 FAC Karen MY n Tech clean 18:34
18:01 IAS Jason, Ryan C LVEA n Surveying 19:44
18:09 SQZ Nutsinee, Daniel, Naoki LVEA - SQZ LOCAL SQZ table work, LOCAL HAZARD 23:58
18:14 SEI Jim, Tony EX n BRS adjustment 19:34
18:35 FAC Kim H2 elec n Tech clean 18:57
18:57 FAC Karen, Kim FCES n Tech clean 19:44
19:00 VAC Gerardo, Jordan FCES n RGA scan 20:14
19:27 FAC Eric MY n Check on heating coil 19:58
21:33 IAS Jason, Ryan C LVEA n Surveying 00:06
21:39 FAC Randy LVEA n Move orange scissor lift to receiving 23:25
22:01 VAC Gerardo, Jordan LVEA n Leak checking near HAM5 01:11
22:47 ISC Julian Opt Lab n Optics lab SHG 23:36
22:59 FAC Ken EY n Grab scaffolding 23:09
23:20 SQZ Camilla LVEA local Check in with other squeezers 23:33
LHO FMCS
eric.otterman@LIGO.ORG - posted 14:01, Thursday 15 February 2024 (75869)
Mid Y chilled water temperature change
The temperature of the chilled water loop at Mid Y was lowered from 46F to 42F to bring it more in line with the other buildings. Other than the initial pulldown, the effect will be minimal but will allow for a more consistent temperature trend. 
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