Displaying reports 10421-10440 of 84767.Go to page Start 518 519 520 521 522 523 524 525 526 End
Reports until 19:41, Wednesday 20 March 2024
H1 ISC
gabriele.vajente@LIGO.ORG - posted 19:41, Wednesday 20 March 2024 (76551)
OMC length noise guesstimation

Let's assume the additional flat noise in the ~100 Hz region that might be limiting now (w.r.t. to O4a) is due to OMC length noise. Either the OMC lenght noise is larger than before, and coupling through the residual OMC length RMS noise, or the OMC lock has an offset.

Let's assume that the OMC was locked at the top of the resonance (no offset, to be confirmed with the new demodulation phase).

According to 76137, the two PZT responses are PZT1 = 11.3 nm/V, and PZT2 = 12.7 nm/V.

Following Sheila's note in 30510, the normalized OMC transmission (RIN) is given by [after correcting for a mistake in the coefficient multipling F]

RIN = 1 / (1 + (2 F (x0 + dx)/ lambda)^2 )

where F = 400 is the OMC finesse (76386), x0 is a static lock offset (or equivalent RMS fluctuation) and dx is OMC lenght noise (form example due to dither).

The amplitude of the dither line is 0.23 V peak, corresponding to a dither amplitude (peak) of A = 2.6e-9 m, using the PZT1 calibration above.

The locking error signal is obtained using a length modulation dx = A sin(wt) that gives a RIN = (2F/lambda)^2 A sin(wt) x0, where x0 is the offsetf from resonance of the OMC length. Once demodulated, this gives

OMC-LSC_I = (2F/lambda)^2 A/2 x0 = 7.3e8 error_signal_demodulated_RIN / m (note that 30510 seems to be wrong and missing some factors, thank you Elenna for checking)

This allows me to calibrate the OMC-LSC input signal. The RMS with the OMC locked is 4.7e-5 RIN, corresponding to 6.4e-14 m RMS of residual OMC fluctuation around the lock point.

The flat noise in DARM is about 7e-21 m/rHz. Using the optical gain from the calibration measurement (3.4e6 LSC-DARM_IN cts/m) and the ratio LSC-DARM_IN / OMC_DCPD_NORM = 1.6e-5, I find an optical gain of 2.1e11 RIN/m for OMC-DCPD_NORM

Therefore the noise in DARM corresponds to a OMC-DCPD RIN of 1.5e-9 RIN/rHz

Noise coupling due to the residual OMC length RMS goes like (2F/lambda)^2 x_RMS dx_noise, where x_RMS is now the residual RMS motion computed above. Using this conversion, I found that the excess noise in DARM would correspond to a OMC length noise of 4e-14 m/rHz at 100 Hz. This still seems higher than the expected noise that should be in the 3e-16 m/rHz range (see for example section 8 of T1000276)

Tests to do:

  1. check if the new demodulation phase improves anything in DARM
  2. scan the OMC lock offset around 0, looking at DARM noise and at the optical gain (for example amplitude of the 410.3 Hz calibration line)
  3. change the locking gain to reduce / increase RMS and check DARM
Non-image files attached to this report
H1 PEM
evan.hall@LIGO.ORG - posted 19:05, Wednesday 20 March 2024 - last comment - 17:11, Thursday 28 March 2024(76575)
End station vibration over past 150 days -- EY BSC10 moves more than before

In addition to the BSC10 accelerometer, the amount of floor motion also increases over the past 6 weeks, though not in a sudden fashion.

This does not correspond to the time of the most recent fan swap, judging by fan accelerometers.

Images attached to this report
Comments related to this report
marc.pirello@LIGO.ORG - 09:36, Thursday 21 March 2024 (76586)

New EX and EY Accelerometer Power Conditioners were installed 30 January 2024.  This is roughly the same time as some of these jumps in the trend.  The EY BSC 10 accelerometer cable had a questionable connector but still functioned so I believe we left it, it may need to be replaced.

https://alog.ligo-wa.caltech.edu/aLOG/index.php?callRep=75592

marc.pirello@LIGO.ORG - 13:23, Thursday 21 March 2024 (76602)

We replaced the loose connector but did not see any effect on the signal.  While down there we looked at the output and found that channel 5 output was very noisy, and looking back at the notes in my prior ALOG, channel 5 = PEM EY BSC ACC X and back then it did not register as an accelerometer.  I assume this accelerometer is not functional or the cabling is not correct.  We plan to go back on Tuesday and track down the issue with this accelerometer and possibly repair the channel in the power conditioner chassis.

Other notes

The INPUT to CH3 on the power conditioner is "TBL-Y" accelerometer cable.  When unplugged this affected "BSC-Y" signal plot.
The INPUT to CH4 on the power conditioner is "BSC-Z" accelerometer cable.  When unplugged this affected "BSC-Z" signal plot. (this one was correct)

Looking back at my analysis of the drawings in the linked ALOG, the above note matches the drawings in the DCC D1300773.  I propose we assume the cables are swapped incorrectly but labeled correctly, and we rearrange the cables to match the drawing.

Marc, Fil, Gerardo, Janos

 

evan.hall@LIGO.ORG - 17:11, Thursday 28 March 2024 (76782)

Refer to LHO:76728.

H1 SQZ (SQZ)
nutsinee.kijbunchoo@LIGO.ORG - posted 18:12, Wednesday 20 March 2024 - last comment - 11:35, Thursday 28 March 2024(76574)
High CLF in the IFO

Naoki, Daniel, Nutsinee

Today we increased RF6  from -22dBm to -13 dBm and 8 dBm. We saw excess noise at 8 dBm above 300Hz but no excess noise at -13dBm. REF 12 is the squeezing at -22dB before we started the test. Using the time from alog76553. REF9 and REF10 both show squeezing at -13dBm RF6 at different squeeze angle where one has a better sensitivity at low frequency bucket. REF13 shows squeezing at 8dBm RF6. The excess noise above 300Hz cannot be improved with squeeze angle. Investigation is required.

We turned off ADF sqz angle servo during the test. We readjusted the ADF squeeze angle demod phase and accepted the new value in the SDF.

We are parking RF6 at -12dBm. Since Daniel didn't like the unlucky number 13.

 

Loop Was (-22dBm RF6) Now (-12 dBm RF6)
CLF gain 10 0
LO gain -7 -12
FC LSC gain -2.6 -0.86
FC ASC gain 0.1 0.03
Images attached to this report
Comments related to this report
naoki.aritomi@LIGO.ORG - 18:32, Wednesday 20 March 2024 (76576)

The -22dBm, -12dBm, 8dBm RF6 correspond to 9 uW, 28 uW, 420 uW CLF REFL power.

camilla.compton@LIGO.ORG - 11:26, Thursday 21 March 2024 (76595)

We rechecked the FDS -22dBm time as the time in the above plot wasn't sqz opitmized to the bucket. Can see in attached plot, CLF at -22dBm and -13dBm have the same SQZ in the bucket, as expected.

Images attached to this comment
nutsinee.kijbunchoo@LIGO.ORG - 12:27, Monday 25 March 2024 (76686)

Looking back at the past data it seems we may not have adjusted the CLF ISS gain properly during the test causing our sqz level to be stuck at 3dB at kHz region. CLF_REFL_DC was oscillating when RF6 was at -13 dBm and at 8 dBm. This looks like an easy fix and we should try again at some point.

Images attached to this comment
nutsinee.kijbunchoo@LIGO.ORG - 10:11, Wednesday 27 March 2024 (76743)

Daniel Nutsinee

Reducing the gain didn't seem to fix the oscillation. We cranked up the CLF power so the RF6 read 6dBm and went out to look at the signal on the scope. We saw 60kHz beat note on the OPO refl and a crooked 105kHz sinewave on the CLF refl. We don't know where the 60kHz beat on the OPO refl came from. We couldn't make any improvement by changing the CLF ISS gain.

After some investigation we realized the oscillation disappeared when we unplugged the RLF. The oscillation came back when the RLF was plugged back in. The oscillation associated with the RLF seemed obvious only when we operated at high power. Next time we try high CLF power again we should attenuate the RLF RF output to the AOM.

 

The funny thing was PMC refl saw this oscillation as well. We hope this was just an electronics cross talk.

Images attached to this comment
daniel.sigg@LIGO.ORG - 11:35, Thursday 28 March 2024 (76771)

For even higher CLF power with +6dBm at the RF6 demod, we set the CLF servo IN2 gain to-18dB (from 0dB), the CLF ISS gain to 0dB (from 17dB), and the ISS input set point to 2.037 (from 0.347).

H1 ISC
jenne.driggers@LIGO.ORG - posted 17:13, Wednesday 20 March 2024 (76572)
SDFs for green initial alignment setpoints

SDFs from green initial alignment setpoints

Images attached to this report
H1 General (CAL, ISC, SUS)
corey.gray@LIGO.ORG - posted 17:12, Wednesday 20 March 2024 (76562)
SDF ACCEPT/REVERT Notes

Jenne was pecking away at SDFs (separate alogs), Jennie/Evan did OMC (I took screenshot below), Louis helped with PCal.....Squeezer work is currently active, so will wait for that team to ACCEPT Squeezer!

Pecking away at some SDFs in preparation for OBSERVING tonight:

Easy Ones To ACCEPT

More Involved to ACCEPT:

Images attached to this report
H1 SQZ
daniel.sigg@LIGO.ORG - posted 17:05, Wednesday 20 March 2024 - last comment - 16:55, Tuesday 26 March 2024(76568)
ASC SQZ FC SDF

These changes were accpted, but need to be set again after aligning the FC IR transmission.

Images attached to this report
Comments related to this report
nutsinee.kijbunchoo@LIGO.ORG - 16:55, Tuesday 26 March 2024 (76730)

Naoki Nutsinee

We realigned IR trans diode. Accepted a new trigger values in the SDF.

Images attached to this comment
H1 ISC
jenne.driggers@LIGO.ORG - posted 17:04, Wednesday 20 March 2024 (76567)
ASC Camera servo gain SDF

Noaki added a gain increase to the CAM1 PIT loop for faster convergence.  It should be in the guardian, so I've accepted it in SDF.

Images attached to this report
H1 ISC
jenne.driggers@LIGO.ORG - posted 17:02, Wednesday 20 March 2024 (76566)
SDF for DHARD_Y

DHARD yaw new FM8, alog 76314.

Images attached to this report
H1 ISC
jenne.driggers@LIGO.ORG - posted 16:57, Wednesday 20 March 2024 (76565)
ADS for AS_A offset

Accepting AS_A offset engagement in Observe.snap.  Values from alog 76500

Images attached to this report
H1 ISC
jenne.driggers@LIGO.ORG - posted 16:52, Wednesday 20 March 2024 (76564)
SDF for new LSC FF

MICH and SRCL FF SDFs accepted.

alog for MICH: 76460

I think this is the alog for SRCL: 76279

Images attached to this report
H1 ISC
jenne.driggers@LIGO.ORG - posted 16:47, Wednesday 20 March 2024 - last comment - 17:11, Wednesday 20 March 2024(76563)
OBSERVE.snap SDFs for Dark Offsets

I've accepted dark offsets for the LSC and ASC PDs in SDF for the Observe.snap files. 

Images attached to this report
Comments related to this report
jenne.driggers@LIGO.ORG - 17:07, Wednesday 20 March 2024 (76569)

Dark offsets for ISCEX and ISCEY

Images attached to this comment
jenne.driggers@LIGO.ORG - 17:11, Wednesday 20 March 2024 (76571)

ALS X and ALS Y dark offset SDFs.

Images attached to this comment
LHO General
corey.gray@LIGO.ORG - posted 16:12, Wednesday 20 March 2024 (76559)
Wed EVE Ops Transition

TITLE: 03/20 Eve Shift: 23:00-07:00 UTC (16:00-00:00 PST), all times posted in UTC
STATE of H1: Commissioning
OUTGOING OPERATOR: Corey
CURRENT ENVIRONMENT:
    SEI_ENV state: CALM
    Wind: 13mph Gusts, 10mph 5min avg
    Primary useism: 0.03 μm/s
    Secondary useism: 0.19 μm/s
QUICK SUMMARY:

Engineering Run #16 (ER16) started this morning and Oli handed over an H1 in NLN with Camilla doing a Squeezer measurement and there is a possibility we may try to "squeeze" in a few other measurements (i.e. no squeezing quiet time) before the 6pm target for Observing.

H1 General
oli.patane@LIGO.ORG - posted 16:00, Wednesday 20 March 2024 (76555)
Ops Day Shift End

TITLE: 03/20 Day Shift: 15:00-23:00 UTC (08:00-16:00 PST), all times posted in UTC
STATE of H1: Commissioning
INCOMING OPERATOR: Corey
SHIFT SUMMARY: Commissioning all day with a few locklosses. Relocking took an average of 42ish minutes.
LOG:

15:00 Detector got to NOMINAL_LOW_NOISE
19:25 Lockloss

20:38 NOMINAL_LOW_NOISE
20:42 Lockloss in NOMINAL_LOW_NOISE from commissioners

21:31 NOMINAL_LOW_NOISE                                                                                                                                                                                                                                                                                                                                                                                                                                                                                             

Start Time System Name Location Lazer_Haz Task Time End
15:13   Elenna Remote n A2L tests 16:13
17:35 FAC Karen WoodShop n Tech clean 18:20
17:51 FAC Kim H2 n Tech clean 18:13
17:58 EE Fil EY n Check hotspot 18:25
18:25 EE Fil EX n Getting other hotspot 18:47
18:34 SHG Julian Optics Lab y(local) Working on SHG 19:46
18:43 FAC Tyler Water tower n Turning on tractor but not driving it 19:13
19:47 WLK Ibrahim along EY n Taking a nice walk 20:31
H1 SQZ
camilla.compton@LIGO.ORG - posted 15:53, Wednesday 20 March 2024 - last comment - 08:23, Thursday 21 March 2024(76556)
SQZ_ANG_ADJUST servo turned back on

Naoki, Nutsinee, Camilla

We turned the SQZ_ANG_ADJUST servo back to it's O3a nominal ADJUST_SQZ_ANG_ADF.  Changed sqzparams.use_sqz_angle_adjust to True and reloaded SQZ_MANAGER and SQZ_ANG_ADJUST.

Set H1:SQZ-ADF_OMC_TRANS_PHASE as 133deg, new scan (as in 76434) running now to check what angle is best for total squeezing.

Comments related to this report
camilla.compton@LIGO.ORG - 16:16, Wednesday 20 March 2024 (76561)

Accepted at H1:SQZ-ADF_OMC_TRANS_PHASE = 120. This seems to give us the best range but not high frequency SQZ. Plot attached.

Images attached to this comment
nutsinee.kijbunchoo@LIGO.ORG - 17:46, Wednesday 20 March 2024 (76573)

We optimized the sqz angle after high CLF test and readjusted the AADF demod phase.

Images attached to this comment
camilla.compton@LIGO.ORG - 08:23, Thursday 21 March 2024 (76581)

We should check the ADF offset with a more themalized IFO as the SQZ angle servo seems to have pulled even the yellow BLRM to a worse location, see attached.

Images attached to this comment
H1 SQZ (SQZ)
nutsinee.kijbunchoo@LIGO.ORG - posted 23:52, Monday 18 March 2024 - last comment - 15:18, Wednesday 20 March 2024(76511)
Back to 5 dB of squeezing!

Naoki, Camilla, Evan, Sheila, Julian, Nutsinee

Many things happened with the squeezer this afternoon. A quick summary is we are back to 5 dB at kHz and we should be able to do this repeatedly. No PSAMs adjustment required at this time.

- When the IFO relocked this afternoon we adjusted ZM5 alignment to optimize ADF trans signal. By doing so we improved both the RF3 and the 42. However this made squeezing worse.

- We adjusted the SQZ angle. We couldn't make it better so we went the other way. This made squeezing worse and ADS TRANS went up with it. Note that this is the IQSUM channel. We didn't think that was a sensible behavior but we've seen it before.

- Sheila and Julian then optimized the crystal tempeature. The NLG for today was 17.3.

- Naoki measured the SQZ IFO sensing matrix. We found a big cross coupling between ZM5 P to AS42 B Y. Other than then everything else was sensible. A new improved sensing matrix has been implemented. 

- We lost hours tracking down why the filter cavity failed to lock on green. A reminder to check SDF next time we run into mysterious problems.

- After everything went back to normal we recovered 5 dB of squeezing. DARM plot said so. BLRMS seemed slightly off. We tried turning the ASC loop off and optimizing the ZM alignment by hand to see if we could do any better than the loop. We couldn't. SQZ IFO ASC loop now works as it should.

- We also optimized the filter cavity offset. Mostly to double checked that we were sitting at a good place. An offset of -28 (where we started) gave the best squeezing at low frequency.

 

We haven't got to increase CLF power today. 

After a new CLF VCO installed we should revert the CLF sign to make sure everything was the same as before. In theory this shouldn't do anything. 

 

 

Images attached to this report
Comments related to this report
nutsinee.kijbunchoo@LIGO.ORG - 00:35, Tuesday 19 March 2024 (76513)

Naoki Nutsinee

We changed "fcgs_trans_lock_threshold" to 120 today so FC wouldn't lock on higher order mode. The filter cavity was having trouble getting pass GR VCO lock so we have now reduced this power back to 80.

camilla.compton@LIGO.ORG - 15:18, Wednesday 20 March 2024 (76557)

Accepted the new ASC_INMATRIX settings in sdf, see attached. Aslo accepted ASC_POS_Y's new minus sign and AS_A_RF42_YAW_OFFSET.

Accpeted the SQZ_ASC WFS as OFF. As decided, we will start the ER with SQZ ASC IFO off.

Images attached to this comment
Displaying reports 10421-10440 of 84767.Go to page Start 518 519 520 521 522 523 524 525 526 End