Displaying reports 121-140 of 81331.Go to page Start 3 4 5 6 7 8 9 10 11 End
Reports until 11:18, Friday 28 March 2025
H1 PSL
jason.oberling@LIGO.ORG - posted 11:18, Friday 28 March 2025 (83616)
PSL FSS RefCav Remote Beam Alignment Tweak

I took advantage of the recent earthquake to tweak the beam alignment into the FSS RefCav from the Control Room to improve the transmission, which had been dropping for the last several days.  With the IMC unlocked the starting RefCav TPD was ~0.660 V, and after the alignment tweak (IMC still unlocked) the TPD is ~0.833 V.

H1 General
ryan.crouch@LIGO.ORG - posted 10:44, Friday 28 March 2025 - last comment - 13:40, Friday 28 March 2025(83614)
17:42 UTC lockloss

17:42 UTC lockloss from a 6.6 from Cape Verde, holding in down till the motion subsides.

Comments related to this report
ryan.crouch@LIGO.ORG - 13:40, Friday 28 March 2025 (83618)

20:40 UTC Observing

LHO VE
david.barker@LIGO.ORG - posted 10:22, Friday 28 March 2025 (83613)
Fri CP1 Fill

Fri Mar 28 10:13:33 2025 INFO: Fill completed in 13min 29secs

Gerardo confirmed a good fill curbside. Note TC adjustments during fill when ice was being removed.

Images attached to this report
H1 SQZ
camilla.compton@LIGO.ORG - posted 08:59, Friday 28 March 2025 (83594)
How to Take a SQZ Data Set

Sheila, Camilla

Aim to take 3 minutes of data peer point, watching BLRMs to check tere is no glitches. On DTT, set BW to 0.1Hz, 30 averages.
Example template is under camilla.compton/Documents/sqz/templates/dtt/20250327_SRCL_neg306.xml

Data to take and how each data is used in the model:

H1 PSL
ryan.crouch@LIGO.ORG - posted 08:20, Friday 28 March 2025 - last comment - 16:02, Friday 28 March 2025(83610)
PSL Status Report - Weekly

Closes FAMIS26379
Laser Status:
    NPRO output power is 1.864W
    AMP1 output power is 70.39W
    AMP2 output power is 140.2W
    NPRO watchdog is GREEN
    AMP1 watchdog is GREEN
    AMP2 watchdog is GREEN
    PDWD watchdog is GREEN

PMC:
    It has been locked 51 days, 18 hr 58 minutes
    Reflected power = 22.69W
    Transmitted power = 106.0W
    PowerSum = 128.7W

FSS:
    It has been locked for 0 days 0 hr and 59 min
    TPD[V] = 0.662V

ISS:
    The diffracted power is around 4.2%
    Last saturation event was 0 days 8 hours and 41 minutes ago


Possible Issues:
    FSS TPD is low

Comments related to this report
ryan.crouch@LIGO.ORG - 16:02, Friday 28 March 2025 (83620)

After Jasons touch up the TPD is now ~0.833 V

H1 General
ryan.crouch@LIGO.ORG - posted 07:32, Friday 28 March 2025 - last comment - 09:13, Friday 28 March 2025(83609)
OPS Friday DAY shift start

TITLE: 03/28 Day Shift: 1430-2330 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Lock Acquisition
OUTGOING OPERATOR: Ryan S
CURRENT ENVIRONMENT:
    SEI_ENV state: CALM
    Wind: 7mph Gusts, 6mph 3min avg
    Primary useism: 0.03 μm/s
    Secondary useism: 0.50 μm/s
QUICK SUMMARY:

Comments related to this report
ryan.crouch@LIGO.ORG - 08:29, Friday 28 March 2025 (83611)SUS

ETMY mode1 and 6 were both ringing up under nominal damping for the first 10 minutes so I've turned off the gain for now.

ryan.crouch@LIGO.ORG - 09:13, Friday 28 March 2025 (83612)

I found some new settings that are working, I added FM5 (-30 degrees) and switched the gain to negative. The working settings are FM1+FM5+FM10 G= -0.2

H1 General (Lockloss, SEI)
ryan.short@LIGO.ORG - posted 00:49, Friday 28 March 2025 - last comment - 07:05, Friday 28 March 2025(83606)
Lockloss @ 06:33 UTC from EQ and ISI Trips

H1 called for assistance at 07:13 UTC when ISIs tripped for every QUAD, BS, and HAM8 due to a M7.7 earthquake and M6.4 aftershock out of Myanmar. Lockloss happened earlier at 06:33 UTC because of the S-waves of this quake, I'm assuming. At the worst of the shaking, peakmon was at the highest I can recall seeing it at over 128,000 counts.

H1 will be down for a while. I'll check in after a bit and untrip platforms if the shaking has calmed enough and start locking.

Images attached to this report
Comments related to this report
ryan.short@LIGO.ORG - 02:22, Friday 28 March 2025 (83607)

I've untripped all platforms and set up H1_MANAGER for the night. SEI_ENV is still in LARGE_EQ, but H1_MANAGER should wait until the seismic configuration is fully out of any earthquake mode before trying to lock.

ryan.short@LIGO.ORG - 07:05, Friday 28 March 2025 (83608)

H1 again called at 12:41 UTC as it wasn't able to finish an initial alignment. ALS-Y was having trouble staying locked, and I eventually ended up adjusting the BS in yaw to improve transmission as I noticed the ALS beam was clipped on the camera (it's still a bit clipped on the right, but less so now). After that, initial alignment was able to finish without issue, then relocking following that has been going automatically as well. H1 is currently relocking in MOVE_SPOTS.

H1 SUS (SEI, SUS)
edgard.bonilla@LIGO.ORG - posted 22:54, Thursday 27 March 2025 - last comment - 16:43, Tuesday 01 April 2025(83605)
Calibrating the PR3 OSEMs

Follow up to LHO alog 83200 and LHO alog 80863.

Brian and I thought of a better way of getting the M1 OSEMs in PR3 calibrated relative to the HAM2 GS13s: Use the ISI drives in L, T, V for frequencies above the suspension resonances to get an absolute calibration.

We can use the measurements Jeff took in LHO alog 80863 and project them in the OSEM basis, then use the translational (Longitudinal, Transverse, Vertical) drives to calibrate the OSEMs. Since the GS13s are calibrated to [m] all of the transfer functions (shown in the first attachment) are in [OSEM meters]/[GS13 meters]. At high frequencies (sufficiently above the resonances) the OSEMs should just be measuring (-1)*ISI motion, because the suspension is isolated. The calibration error will depend on how well we are able to drive L,T,V from the ISI without cross-coupling to any other DOF.

Figure 1 attached shows the 6x6 transfer matrix between the ISI drives and OSEMs (inputs are columns, and outputs are rows). We highlight the 6 translational transfer functions that can be used to calibrate the OSEMs in red. The drives seem decoupled enough to do the calibration (for example, we expect to see a length drive only in LF and RT, no motion anywhere else).

Figures 2,3, and 4 show a detail of the 6 transfer functions we will use for calibration, all of them should be scaled to 1 [OSEM m]/[GS13 m]. The scalings are:

            T1         T2          T3          LF          RT         SD
       1.544          0            0            0            0            0      T1
            0        1.394         0            0            0            0      T2
            0            0        1.273         0            0            0      T3
            0            0            0        1.411         0            0      LF
            0            0            0            0        1.588         0      RT
            0            0            0            0            0        1.366   SD
Two things to note:
1) The relative calibrations are consistent with the ~15% mismatch that led to the V to R and the L to Y couplings that Brian and I observed in the comments of LHO alog 83200.
2) The absolute calibrations being in the ballpark of 1.5 seem large, but they are close to the calibration factor in plotHLTS_ISI_dtttfs_M1.m that transforms between [um/drive cts] to [m/N]. The transfer functions plotted always seem about a factor of 1.5 off from the MATLAB model. Maybe there's a connection that explains why the calibration factor seems so large.
 
Figure 5 shows all of the diagonal ISI to M1 transfer functions after applying the calibration factors. They all asymptote to 1 at high frequencies even though we only used L, T, and V for calibration. A good sign that we're on the right track.
 
Figure 6 shows the effect of the calibration on the M1 to M1 transfer matrix (inputs are columns, and outputs are rows). The solid Black trace is the corrected M1 to M1, the dashed lines show what it was before the sensor calibration. A few of the cross couplings become significantly better: [L-Y], [V-P-R] are the best performing.
 
I think this gets enough benefit for the ISI - SUS estimatior. It also might be worth trying this scheme in other suspensions where we would benefit from eliminating more cross terms in the OSEM transfer matrix.
Images attached to this report
Comments related to this report
edgard.bonilla@LIGO.ORG - 13:51, Friday 28 March 2025 (83619)

Adding here the phases for the TFs used for the calibration. There's a 20 to 25 degree phase loss after the last resonance up to 20 Hz. I'm not sure what more to make out of it, I thought the phase loss would be an artifact of the OSEM readouts, but maybe someone with more knowledge can chime in.

 

 

Images attached to this comment
edgard.bonilla@LIGO.ORG - 16:43, Tuesday 01 April 2025 (83689)SEI, SUS

One way to fix the cross-coupling without having to get the absolute calibration is to slightly modify the M1 PR3 osem gains. They currently sit at:

    T1         T2          T3          LF         RT         SD

 1.161    0.998    1.047    1.171    1.163    1.062

 

Their new values would be at

    T1         T2          T3          LF         RT         SD

1.164    0.903    0.866    1.073    1.199    0.942

This change will still leave a scaling factor of 1.54 m/(OSEM m), but at least it should fix the L-Y and the V-P-R cross couplings.

H1 General
oli.patane@LIGO.ORG - posted 22:08, Thursday 27 March 2025 (83604)
Ops Eve Shift End

TITLE: 03/28 Eve Shift: 2330-0500 UTC (1630-2200 PST), all times posted in UTC
STATE of H1: Observing
INCOMING OPERATOR: Ryan S
SHIFT SUMMARY: Just got to NLN and into Observing. When trying to relock earlier, we did have a lockloss from DHARD_WFS for some reason, but no issues after that. The wind is currently low but has had a couple instances of quickly spiking up above 20/25mph before dying back down, the second of which came with very heavy rain. Hopefully that doesn't happen again during the night. The secondary microseism is still very high, but doesn't look to be getting worse.
LOG:

23:30 Relocking and in OMC_WHITENING damping violins

00:33 NOMINAL_LOW_NOISE
00:34 Observing

03:03 Lockloss
    - Lost lock at DHARD WFS
    - Ran an initial alignment

05:06 NOMINAL_LOW_NOISE

05:07 Observing

Start Time System Name Location Lazer_Haz Task Time End
20:59 ISC Keita, Mayank Opt Lab Yes ISS PD array (Keita out 21:55) 01:27
21:23 TCS Camilla, Matt Opt Lab Yes CO2 laser testing 21:56
22:10 ISC Jennie OptLab Yes Looking for Keita 22:18
H1 General (Lockloss)
oli.patane@LIGO.ORG - posted 20:05, Thursday 27 March 2025 (83603)
Lockloss

Lockloss @ 03/28 03:03UTC after 2.5 hours locked. Of course right after I put in my midshift report saying that we were locked

H1 General
oli.patane@LIGO.ORG - posted 20:01, Thursday 27 March 2025 (83602)
Ops EVE Midshift Status

Observing at 155Mpc and have been Locked for 2.5 hours. Nothing to report

LHO General
thomas.shaffer@LIGO.ORG - posted 16:42, Thursday 27 March 2025 - last comment - 17:42, Thursday 27 March 2025(83590)
Ops Day Shift End

TITLE: 03/27 Day Shift: 1430-2330 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Microseism
INCOMING OPERATOR: Oli
SHIFT SUMMARY: Calibration and commissioning started the day. After a lock loss at 12PT we have been struggling to relock. We just recently made it to the last state before low noise, but the violins are very high from a few lock losses at Transition_From_ETMX and Move_Spots. Oli is damping those now and hopefully we'll be back to observing soon. It's not entirely clear why we had issues relocking. The primary and secondary useism are definitely elevated, but at levels that we have locked before. Wind is under 20mph, as well.
LOG:

Start Time System Name Location Lazer_Haz Task Time End
15:38 FAC Tyler EX n Adjust fan speed manually 16:08
16:29 ISC Sheila, Jeff LVEA n OMC DCPD injections, LVEA wifi on during this time 17:34
16:44 PSL Jason Opt Lab n Unpacking laser in lab and receiving 16:55
18:28 FAC Kim, Nelly MY n Tech clean 18:48
18:58 - Tony LVEA n Checking for water leaks 19:33
19:11 CDS Marc CER n Check on power supplies 19:33
19:11 CDS Fil LVEA n Check on CPS glitching 19:33
20:17 PSL Jason MX n Drop off 20:32
20:59 ISC Keita, Mayank Opt Lab Yes ISS PD array 22:18
21:23 TCS Camilla, Matt Opt Lab Yes CO2 laser testing 21:56
22:10 ISC Jennie OptLab Yes ISS help 22:18
Comments related to this report
oli.patane@LIGO.ORG - 17:42, Thursday 27 March 2025 (83601)CDS, SQZ

Back to Observing 03/28 00:34UTC after accepting a couple diffs for SQZ and IOPLSC0

Images attached to this comment
H1 SUS
marc.pirello@LIGO.ORG - posted 14:25, Tuesday 25 March 2025 - last comment - 11:53, Friday 28 March 2025(83554)
SUS-C4 Power Supply Chirping

The Kepco Power Supply for SUS-C4 started chirping at the end of maintenance today.  By 2pm the chirping is more regular.  The draw on the supply is 7A, typical failing fans last a few days once they get to this stage.  We should replace this one before the weekend, as a target of opportunity.  Down time will be 30 mins start to finish.

WP12406

M. Pirello, F. Clara

Comments related to this report
marc.pirello@LIGO.ORG - 11:53, Friday 28 March 2025 (83617)

Due to earthquake we took a window of opportunity to replace the SUS-C4 Kepco Power Supply which controls HAM1 and HAM2 suspensions.  These suspensions were placed into safe and the supply replaced.  We replaced only the -18V supply, the +18V matching supply was replaced in December 2022 so we left it in place.

WP12406

M. Pirello, F. Clara

 

 

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