TITLE: 03/27 Eve Shift: 2330-0500 UTC (1630-2200 PST), all times posted in UTC
STATE of H1: Microseism
OUTGOING OPERATOR: TJ
CURRENT ENVIRONMENT:
SEI_ENV state: USEISM
Wind: 17mph Gusts, 11mph 3min avg
Primary useism: 0.05 μm/s
Secondary useism: 0.51 μm/s
QUICK SUMMARY:
In OMC_WHITENING and damping violins. Hopefully we'll be back to Observing soon.
After this morning's SRCL offset change and SQZ NLG change 83589, I returned FC de-tuning to -34Hz, SQZ angle to 171, and OPO trans setpoint to 80uW. Adjusted OPO temp and measured NLG to be 12 following 76542
opo_grTrans_ setpoint_uW | Amplified Max | Amplified Min | UnAmp | Dark | NLG (usual) | NLG (maxmin) | OPO Gain |
80 | 0.0110211 | 0.0002941 | -0.000023 | 0.0009199 | 11.7 | 12.7 | -8 |
FranciscoL, SheilaD, JeffK
I compared the sensing functions from calibration reports 20250327T160138Z, and 20250322T190652Z to look for correlations with the SRCL offset change done before the routinely Thursday calibration measurement. We see a decrease of the detuned SRC spring frequency from 7.343 Hz to 2.191 Hz.
I am attaching each sensing model generated by pydarm. Second attachment (20250322T190652Z_sensing_mcmc_compare) is for the measurement done last Saturday, third attachment (20250327T160138Z_sensing_mcmc_compare) for the measurement done today. We trust the model because the fit (orange trace) and the data (green dots) match well above the 10 Hz fit range. Additionally, the data on both measurements below 10 Hz shows a similar behavior. This gives us (1) confidence that the change in the sensing function was indeed from SRCL detuning and (2) we may have other sources of coupling into the sensing function -- thinking about DHARD as the main culprit.
The first attachment (sensing_ratio) shows the relative change of each measurement labeled by their report id. We see that the latest calibration measurements (orange and black), have been consistent with the latest front-end calibration (blue) -- more confidence towards SRCL changing the sensing function.
While this improves the detuning of the interferometer, the overhead to update the calibration has deemed to high for the few days left that will be running. We will reassess when we are close to coming back into observing mode (June)
What I did to make plots:
(1) Get the report from the calibration measurement this morning:
In the terminal -- no need to activate any environments or configuring the terminal in any way -- running
will create a report of the latest measurement that was done. This command will not change FE calibration so, for now, this is a safe way to get data and manipulate/evaluate it.
(2) Used script to retrieve sensing function measurements from calibration reports:
The script located at
will load the measurements as provided by their report id. I personally chose a dictionary to add comments for labeling purposes. The function 'sensing' will load the measurement and get the response. The rest is plotting aesthetics.
NOTE To enable the pydarm package -- and run the script -- run in terminal
Also -- side note -- I'd been skeptical of the accuracy of the live spring frequency calculation, H1:CAL-CS_TDEP_F_S_OUTPUT. Looks like it *is* a good measure, or at least the same measure as the sweeps, of the spring frequency. See attached trends of f_s, surrounding the times of these calibration measurements. Nice!
J. Kissel, S. Dwyer Sheila and I were finally able to use an SR785 by HAM6 ISC-R5 (see setup and discussions in LHO:83523, LHO:83466, and LHO:83468) to inject a loud sinusoidal excitation into the OMC DCPD transimpedance amplifier TEST inputs via analog interface of the OMC DPCD whitening chassis. Remember, this is in hopes to mimic a PI ring-up and identify whether or not this would cause ~10-100 Hz broadband noise increase in the detector sensitivity, as was seen on 2025-03-12 (LHO:83335). We saw NO broadband low frequency noise increase with an excitation amplitude that results in a factor of 5x *higher* photocurrent on the DCPDs than during the PI ring-up. I attach a four-panel plot, and because that makes each panel small, I also attach the same plots zoomed in to each panel. In the plots, I'm comparing four different times: - (RED) 2025-03-12 17:32 UTC -- the time of the 10.4 kHz PI mode ring-up from LHO:83335 - (BLUE) 2025-03-20 16:13 UTC -- the time I used in LHO:83468 to assess how much drive I should be able to put in, - (GREEN) 2025-03-27 17:16 UTC -- a time during the loudest, 250 [mVpk_SE, SR785 SRC output] excitation - (BROWN) 2025-03-27 17:30 UTC -- just after we're done with our tests and everything is unplugged in the nominal configuration Upper panels of 1st Attachment (zoomed in with 2nd and 4nd attachment)-- the 65 kHz version of the OMC DPCD A channel that has NO digital anti-aliasing (under the obfuscated channel name H1:OMC-PI_DCPD_64KHZ_AHF_DQ), calibrated into photocurrent on DCPDA (which needs only a conversion of 0.001 [A/mA]). - Left panel (and 2nd attachment) is zoomed in around the 10.2 - 10.5 kHz region, showing the excitation, The acoustic mode forest, and except for the unthermalized data, the 02 (or 20) optical mode hump. - Right panel (and 4th attachment) is the full ASD across the 10 Hz - 25 kHz frequency range. Lower panels of 1st Attachment (zoomed in with 3rd and 5th attachments) -- GDS-CALIB_STRAIN converted to DARM displacement (which needs only a multiplication by the length of the arms, L = 3995 [m]). - Left panel (and 3rd attachment) zooms in on the 10-100 Hz frequency region, and - Right panel (and 5th attachment) shows the whole 10 - 7000 Hz sensitivity. There's NO change between BLUE (excitation OFF) and RED (excitation ON), and thus no evidence of broadband noise increase we saw in BROWN (during PI ring-up). %%%% Measurement notes - For no particular reason, we turned on BOTH DCPDA and DCPDB test excitation relays (see LHO:83466 for how). That means our single-ended qqq [mVpk] analog excitation from the SR785, converted to qqq [mVpk] differential by the SR785 Accessory Box (whose TF is 1 [V_DIFF] / 1 [V_SE]), was driving that qqq [mVpk] amplitude into BOTH A & B channels' TEST inputs within the TIA. So, the excitation seen in OMC DCPDA's ADC input is also in DCPDB, and thus the sum of the the two, OMC_DCPD_SUM, the DARM error signal, actually sees twice this amplitude. But, the sum is done digitally, after down-converting to 16 kHz, so it's not relevant to "is the ADC getting saturated" discussions; just important to bring up in "how much of this excitation can the IFO handle" discussions.
As an aside, here I attach a trend of the H1:OMC-DCPD_[A,B]_WINDOW_[MAX/MIN] channels (the details of which can be found in LHO:62310). In short they're looking at the 4-channel SUM of each DCPD's 4x analog copies of the voltage going into the the ADC, in units of 4x ADC counts. In the attached trend, I divide these by 4 (or scale by 0.25), to compare against the saturation limit of a single ADC channel, which is what we really want. Remember this the General Standards Low Noise Fast ADC, which spreads its 40 Vpp input range across 18 bits, so the saturation limit is +/-2^17 = +/- 131072 [ADC ct]. In the trend, I highlight when we engaged the relays (without any SR785 excitation on) and when we turned them off to show how loud that is. We did *not* break lock from those glitches, but it sure made the ETMX actuators sad for a bit and caused a big glitch in the detector. I also highlight the period over which we increase the amplitude of our excitation from 0.1 to 250 [mVpk_SE, SR785 SRC Output]. Our excitation doesn't start to show up as contributing to this ADC channel MIN/MAX time-series until we hit excitation amplitude of 50 [mVpk_SE, SR785 SRC Output]. It reaches at most 40k [ADC ct] = 6.1 [Vpp_DIFF, ADC Input] (again, of 40 Vpp_DIFF, so 15% of the range) at our loudest excitation amplitude of 250 [mVpk_SE, SR785 SRC Output]. I also attach the same OMC DCPDA photocurrent ASD in the main entry, but I add what the DCPD photo current ASD looks like under lesser excitation amplitudes; 10 mVpk in BLACK, 50 mVpk in ORANGE, and the one I've already shown, 250 mVpk (again in BLUE). Again, the 250 [mVpk SRC Output] excitation is a factor of 5x above the amplitude that this PI mode was at the time of the low frequency broadband noise. Sheila reminds me that we've seen PIs *louder* than this time and *not* seen any broadband low-frequency noise increase. But anyways, even at 50 [mVpk_SE, SR785 SRC Output] -- which according to this ASD (a) The equivalent to a photocurrent of 4.07e-7 [A/rtHz] at 10.3 kHz (b) Comparable to the height of 4.04e-7 [A/rtHz] at 10.428 kHz (for a 0.1 Hz frequency resolution, which DTT turns into an 8 sec FFT or 1/8 = 0.125 Hz resolution, and Hann window; ENBW = 0.187) -- this starts to dominate the ADC's RMS, since there is a noticeable change in the WINDOW MAX/MIN channels. But it's a small fraction of the ADC range. I note that the OMC DCPD analog whitening was ON at all times during our measurements today, and during each of the old data sets. So that means, at these frequencies, there's an extra gain of 10x on the TIA output voltage.
Sheila, Camilla
This morning we changed SRCL offset from -191 to -306 and FC detuning from -34 to -28, as discussed in 83570. Decided to take a SQZ dataset here.
Increased SHG launch, turned OPO trans setpoint up from 80uW to 95uW to increase NLG from 11 to 19 (as we had earlier in O4). Measured NLG with 76542. OPO gain left at -8.
Had some strange HAM7 CPS glitches and WD trips. Think we manged to avoid these effecting the data.
Forgot to turn of SQZ ASC, realized and then we lost lock, this data is not good as the AS42 and ZM alignment offsets were moving around a lot.
opo_grTrans_ setpoint_uW | Amplified Max | Amplified Min | UnAmp | Dark | NLG (usual) | NLG (maxmin) | OPO Gain |
95 | 0.0179401 | 0.000271566 | -0.00002333 | 0.000906905 | 19.3 | 20.8 | -8 |
Type | Time (UTC) | SQZ @1kHz (dB) | Angle | DTT Ref |
No SQZ | 18:11:30 - 18:20:00 | N/A | N/A | ref 0 |
MeanSQZ w/o ADF | 18:22:30 - 18:25:30 | 13.3 | N/A | ref1 |
FIS Mid SQZ + | 18:28:30 - 18:31:30 | (CLF-) 195 | ref2 | |
FIS Mid SQZ - | 18:38:30 - 18:41:30 | (CLF-) 127 | ref3 | |
FIS ASQZ | 18:44:00 - 18:47:00 | 15.8 | (CLF-) 68 | ref4 |
FIS ASQZ +10deg | 18:47:30 - 18:50:30 | 15.2 | (CLF-) 78 | ref5 |
FIS ASQZ -10deg | 18:51:00 - 18:54:00 | 15.2 | (CLF-) 58 | ref6 |
J. Kissel, S. Dwyer When we apply a large SRCL offset, as we did today LHO:83583, we get more 45 MHz sideband field in the POP port. The POP A LSC RFPD (in HAM1) is demodulated in analog at 45 MHz, and its I & Q signals are piped into a standard 16 bit ADC whose saturation limit is +/- 2^15 = 32768 [ct]. The I channel is used as the error signal for SRCL, and the Q is used as the error signal for MICH, so if we get anywhere near that saturation limit, these loops lose there error signals and the IFO loses lock. So, just a sanity check, here's the POP A I & Q raw ADC channels across the transition from -191 [ct] to -306 [ct] SRCL offset. -306 [ct] does not saturate the POP A I or Q ADC channels.
While the SQZ team was commissioning in the control room, the HAM7 ISI tripped 4 times on the CPSs. Looking at the trip plots this looks like the CPS glitches that we have seen in the past (attachment 1).
HAM7 definitely trips more forequently than other ham chambers (attachment 2), and we know that we have seen these when there are people working in the racks nearby, but today the sqz team was adjusting TEC temperatures, closing beam diverters, or just doing nothing when these happened.
FRS33714 filed since I couldn't find one specifically for this, though we do have tickets open for other HAM6 CPS gltiching: FRS: 11640 FRS: 11642 Aggregate IIET: 11643.
Thu Mar 27 10:13:56 2025 INFO: Fill completed in 13min 52secs
Followed the usual wiki instructions.
Simulines command run:
gpstime;python /ligo/groups/cal/src/simulines/simulines/simuLines.py -i /ligo/groups/cal/H1/simulines_settings/newDARM_20231221/settings_h1_20250212.ini;gpstime
Simulines start:
PDT: 2025-03-27 08:35:50.875109 PDT
UTC: 2025-03-27 15:35:50.875109 UTC
GPS: 1427124968.875109
Simulines stopped prematurely due to some SCRL offsets getting changed midway through:
PDT: 2025-03-27 08:54:32.154549 PDT
UTC: 2025-03-27 15:54:32.154549 UTC
GPS: 1427126090.154549
Simulines started again:
PDT: 2025-03-27 09:01:37.213384 PDT
UTC: 2025-03-27 16:01:37.213384 UTC
GPS: 1427126515.213384
Simulines end:
PDT: 2025-03-27 09:25:15.138110 PDT
UTC: 2025-03-27 16:25:15.138110 UTC
GPS: 1427127933.138110
Files:
2025-03-27 16:25:14,982 | INFO | File written out to: /ligo/groups/cal/H1/measurements/DARMOLG_SS/DARMOLG_SS_20250327T
160138Z.hdf5
2025-03-27 16:25:14,990 | INFO | File written out to: /ligo/groups/cal/H1/measurements/PCALY2DARM_SS/PCALY2DARM_SS_202
50327T160138Z.hdf5
2025-03-27 16:25:14,995 | INFO | File written out to: /ligo/groups/cal/H1/measurements/SUSETMX_L1_SS/SUSETMX_L1_SS_202
50327T160138Z.hdf5
2025-03-27 16:25:15,000 | INFO | File written out to: /ligo/groups/cal/H1/measurements/SUSETMX_L2_SS/SUSETMX_L2_SS_202
50327T160138Z.hdf5
2025-03-27 16:25:15,004 | INFO | File written out to: /ligo/groups/cal/H1/measurements/SUSETMX_L3_SS/SUSETMX_L3_SS_202
50327T160138Z.hdf5
Tony created the PCAL{X,Y}_STAT nodes a few weeks ago, and has been monitoring and testing over that time. They look to be working as intended, flagging any major issues with the PCAL system. I've now removed them from the excluded nodes list that the IFO node looks at so that now if either of these nodes is out of its nominal state or the node is not OK==True, then the IFO node will not be OK and we will not be able to go to Observing.
J. Kissel, S. Dwyer, T. Shaffer TJ was diligently running at regularly scheduled calibration measurement suite with the current nominal configuration of the IFO. Sheila and I got too excited about what other measurements we needed to do during the commissioning period today, and I quickly and boldly made the assessment that the simulines sweeps were done by just looking at the front wall DARM FOM. And said "we can go ahead with the first [commissioning] measurements" and changed the SRCL offset to grab an augmented IFO configuration sweep as planned. We realized only ~2 mins after that the nominal configuration sweep *was* still going, and this is me eating my hat. Sorry team. TJ killed the simulines session, which apparently automatically cleans up the calibration sweep measurement report infrastructure, so there's no evidence of it. So, today's regular calibration has been spoiled. The broadband injection in the nominal configuration did go forward to completion, that's /ligo/groups/cal/H1/measurements/PCALY2DARM_BB/ PCALY2DARM_BB_20250327T153021Z.xml The "nominal" configuration -- compared to what we want to change today: Filter Cavity Detuning = -34 Hz offset SRCL Offset -191 [ct] Here's the measurements with the augmented IFO configuration, with Filter Cavity Detuning = -28 Hz offset SRCL Offset -306 [ct] /ligo/groups/cal/H1/measurements/PCALY2DARM_BB PCALY2DARM_BB_20250327T155611Z.xml /ligo/groups/cal/H1/measurements$ ls */*20250327*.hdf5 DARMOLG_SS/DARMOLG_SS_20250327T160138Z.hdf5 PCALY2DARM_SS/PCALY2DARM_SS_20250327T160138Z.hdf5 SUSETMX_L1_SS/SUSETMX_L1_SS_20250327T160138Z.hdf5 SUSETMX_L2_SS/SUSETMX_L2_SS_20250327T160138Z.hdf5 SUSETMX_L3_SS/SUSETMX_L3_SS_20250327T160138Z.hdf5 Due to the augmented SRCL offset, these measurements should *not* be included in the collection of measurements used for creating estimates of residual sensing function systematic error. The filter cavity detuning change only impacts the noise performance of the IFO, so if need be, you *can* still use the actuation function portion of the measurement suite.
TITLE: 03/27 Day Shift: 1430-2330 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Observing at 153Mpc
OUTGOING OPERATOR: Ibrahim
CURRENT ENVIRONMENT:
SEI_ENV state: CALM
Wind: 18mph Gusts, 10mph 3min avg
Primary useism: 0.03 μm/s
Secondary useism: 0.34 μm/s
QUICK SUMMARY: Locked for 3 hours. DIAG_MAIN is reporting "RefCav transmission low", tagging PSL. No other alarms or notifications. Planned calibration and commissioning time today from 1530-1900 UTC.
TITLE: 03/27 Eve Shift: 2330-0500 UTC (1630-2200 PST), all times posted in UTC
STATE of H1: Observing at 156Mpc
INCOMING OPERATOR: Ibrahim
SHIFT SUMMARY: Observing at 156Mpc and have been locked for almost 1 hour. One lockloss during my shift but relocking went well and was almost completely hands off besides me selecting an initial alignment.
LOG:
23:30UTC Observing at 156 Mpc and locked for almost 12 hours
01:55 Kicked out of Observing due to squeezer losing lock
01:59 Back into Observing after squeezer got back to FDS
02:41 Lockloss
- I immediately decided to start an initial alignment since the lock had been relatively long
04:13 NOMINAL_LOW_NOISE
04:15 Observing
Start Time | System | Name | Location | Lazer_Haz | Task | Time End |
---|---|---|---|---|---|---|
16:57 | ISC | Mayank | Opt Lab | Yes | ISS PD array | 00:53 |
21:46 | TCS | Camilla, Matt | Opt Lab | Yes | CO2 laser testing | 23:46 |
Lockloss @ 03/27 02:41UTC after just over 15 hours locked
04:15UTC Back to Observing
Sheila, Camilla
Reduced HAM7 rejected pump power and increased SHG launch, turned OPO trans setpoint up to 120uW and measured NLG with 76542 to be 58 (this was a little lower than with 120uW in 83370). OPO gain turned down from -8 to -12. ADF was on for all apart from "Mean SQZ w/o ADF".
Type | Time (UTC) | Angle | DTT Ref |
No SQZ | 16:01:00 - 16:15:00 | N/A | ref 0 |
SQZ | 16:56:30 - 16:59:30 | (CLF-) 174 | ref1 |
SQZ +10deg | 17:00:00 - 17:03:00 | (CLF-) 184 | ref2 |
SQZ -10deg | 17:03:30 - 17:06:30 | (CLF-) 164 | ref3 |
Mean SQZ w/o ADF | 17:07:30 - 17:10:30 | N/A | ref4 |
Mean SQZ w/ ADF | 17:11:00 - 17:14:00 | N/A | ref5 |
Mid SQZ + | 17:17:00 - 17:20:00 | (CLF-) 209 | ref6 |
Mid SQZ - | 17:21:30 - 17:24:30 | (CLF-) 152 | ref7 |
ASQZ | 17:27:30 - 17:30:30 | (CLF-) 80 | ref8 |
ASQZ +10deg | 17:31:30 - 17:34:30 | (CLF-) 90 | ref9 |
ASQZ -10deg | 17:35:00 -17:38:00 | (CLF-) 70 | ref10 |
Then went to FDS | |||
FDS SQZ, SRCL -191 | 17:46:00 - 17:49:00 | (CLF-) 174 | ref11 |
FDS SQZ +10deg, SRCL -191 | 17:49:30 - 17:51:30 (2mins) | (CLF-) 184 | ref12 |
FDS SQZ -10deg, SRCL -191 | 17:52:00 -17:54:00 (2mins) | (CLF-) 164 | ref13 |
FDS SQZ, SRCL -290 | 17:56:30 - 17:59:30 | (CLF-) 146 | ref14 |
FDS SQZ +10deg, SRCL -290 | 18:00:00 - 18:02:00 (2mins) | (CLF-) 156 | ref15 |
FDS SQZ -10deg, SRCL -290 | 18:02:30 - 18:04:30 (2mins) | (CLF-) 136 | ref16 |
Starting FC detuning -36Hz | |||
FDS SQZ, SRCL -290, FC detuning -40Hz | 18:08:30 - 18:11:30 | (CLF-) 146 | ref17 |
FDS SQZ, SRCL -290, FC detuning -32Hz | 18:12:00 - 18:15:00 | (CLF-) 146 | ref18 |
FDS SQZ, SRCL -290, FC detuning -32Hz | 18:18:00 - 18:21:00 | (CLF-) 149 | ref19 |
FDS SQZ, SRCL -290, FC detuning -28Hz* | 18:21:30 - 18:24:30 | (CLF-) 149 | ref20 |
FDS SQZ, SRCL -290, FC detuning -24Hz | 18:225:30 - 18:28:30 | (CLF-) 149 | ref21 |
OPO trans back to nominal 80uW, NLG 12 | |||
FDS SQZ, SRCL -290, FC detuning -28Hz | 18:46:30 - 18:49:00 (2m30) | (CLF-) 170 | ref22 |
FDS SQZ, SRCL -191, FC detuning -36Hz | 19:03:30 - 19:06:00 (2m30) | (CLF-) 171 | ref23 |
* For NLG of 58, SRCL -290, FC detuning -28Hz looked best.
Plots attached of FIS data showing SQZ, Mean SQZ, Mid SQZ and also SQZ and ASQZ, filename shown on screenshot.
Also did FDS SQZ, +/-10deg with nominal SRCL detuning (-191) and -290, plot attached. And adjusted the FC de-tuning with SRCL offset at -290, plot attached.
Finally we went back to the nominal NLG (NLG of 12 with 80uW OPO Trans setpoint) and checked FDS SQZ with the best found settings at high NLG: SRCL -290, FC de-tuning -28Hz and back to nominal settings, DARM plot attached. We didn't have time to fully tune the angle in both settings so could repeat this to check at which settings the range is best. Sheila ran a SQZ angle scan at these settings (SRCL -290, FC de-tuning -28Hz), see attached, it is less frequency dependent than than the scans taken the day before at SRCL -191 (nominal) and -190, FC de-tuning -36Hz (nominal), plot attached.
opo_grTrans_ setpoint_uW | Amplified Max | Amplified Min | UnAmp | Dark | NLG (usual) | NLG (maxmin) | OPO Gain |
120 | 0.0540944 | 0.00026378 | 0.000913452 | -0.0000233 | 57.75 | 58.68 | -12 |
80 | 0.010857 | 0.0002927 | 0.000904305 | -0.0000219 | 11.72 | 12.57 | -8 |
Here are some plots of Camilla's first dataset above, changing the SRC detuning while adjsuting the squeezing angle for high frequency squeezing, made with the same code used for 80318, which is available here
For the gwinc model, I've set the generated squeezing to 23 dB based on Camilla's measured NLG of 58. Based on the loss estimates from 83457, I've set the Injection loss to 0.178 (17.8% loss) and the PD efficiency (readout efficiency) to 0.815, and the phase noise to 0.
The third attachment shows the model where I've manually adjusted the SRC detuning to roughly match the subtracted squeezing, and the second shows a linear fit of SRCL offset to these detunings. This suggests that the SRCL offset should be at -306 counts to reduce the SRCL offset, and that we are currently running with a SRCL detuning of 0.013 radians.
This morning we put SRCL offset to -306, FC de-tuning -28Hz. I then ran SCAN_SQZANG which changed the angle form 171 to 161 and compare the before and after DARM, attached, SQZ looks alot better at higher frequencies, however the range, attached, is similar or a little worse, maybe the 300Hz (yellow BLRMs) squeezing is slightly worse.
Updated DTT legend as had typo.
Here are some preliminary plots from Camilla's data set of different squeezing angles taken at an NLG of 58 with the SRCL offset at it's nominal -191 counts setting, which we believe is about 13 mrad SRC detuning.
The first plot shows some assumptions that go into making this model, we start with an assumption about arm power, use the noise budget estimate of non quantum noise at 2kHz (which may be out of date now), and set the readout losses to fit the no squeezing data at 2.1-2.3kHz. Then subtract this quantum noise model without squeezing from the no squeezing data, and use that as an estimate of the non-quantum noise, which can be added to all of the quantum noise models for different squeezing angles to compare to the measurement. (second plot is a somewhat overwhelming plot of all this added for completeness).
I've set the phase noise to 0 based on 83457. Using the level of sqz and anti-squeeze at 2.1-2.3 kHz, we infer that the NLG was 63 and the total efficency was 66.5%. Camilla measured the NLG to be 58, for 120uW circulating power, but in 83370 she measured 61-63 for 120uW. The third plot here shows the data that Camilla took with the LO loop unlocked, so that the squeezing angle is averaging and rotating freely. Using this and knowledge of the NLG, we should be able to infer the total squeezing efficiency as a function of frequency. Doing the subtraction of non quantum noise increases the infered efficiency, (compare thick lines to thin), the two different values of NLG suggest rather different efficiencies. There is evidence that the efficiency frequency dependent, which could be caused by a number of effects. Below 200 Hz there is some excess noise in the mean sqz trace, as you can see here, which causes the efficiency infered to be above 1.
The next two plots show the model broken into more readable plots, with the only thing I've adjusted by hand being the SRC detuning. There is a discrepancy between the model + noise for the anti-squeezing and anti-squeezing +/-10 degrees traces without the filter cavity, which seems like it could be some excess noise that is similar for the different traces. This is similar to the discrepancy seen in the last plot in 82097, but it is larger in this higher NLG dataset.
Jennie W, Sheila
Summary: We altered the offsets on the H1:ASC_OMC_{A,B}_{PIT,YAW} QPDs which are used to align the beam into the OMC. This was aiming to give us a improvement in optical gain. After doing this we aimed to measure the anti-symmetric port light changing as we chnage the darm offset. We are trying to use both these measurements to narrow down where we have optical loss in that could be limiting our observed squeezing. Performed both measurments successfully but the different alignment of the OMC made the squeezing less good so Camilla (alog #83009) needed to do some tuning.
Last time (alog #82938) I did this I used the wrong values as our analysis used the output channels to the loops instead of the input channels which come before the offsets are put in. The new analysis of our measurement of the optical gain as seen by the 410Hz PCAL line, changing with QPD offset, shows that we want the loop inputs to change to:
H1:ASC_OMC_A_PIT_INMON to 0.3 -> so we should change H1:ASC_OMC_A_PIT_OFFSET to -0.3
H1:ASC_OMC_A_YAW_INMON to -0.15 -> so we should change H1:ASC_OMC_A_YAW_OFFSET to 0.15
H1:ASC_OMC_B_PIT_INMON to 0.1 -> so we should change H1:ASC_OMC_B_PIT_OFFSET to -0.1
H1:ASC_OMC_B_YAW_INMON to 0.025 - so we should change H1:ASC_OMC_B_YAW_OFFSET to -0.025
We stepped these up in steps of around 0.01 to 0.02 while monitoring the saturations on OMC and OM3 suspensions and the optical gain, both to make sure we were going in the correct direction and that we were not near to saturation of the suspensions as hapenened last time I tried to do this.
Attached is the code and the ndscope showing the steps on each offset, (top row left plot, top row center right plot, second row left plot, second row center right plot). The top stage osems for OM3 suspension are shown in the third row left plot, the top stage osems for OMC suspension are in the third row center left plot, and the optical gain is shown in the third row right plot.
The optical gain improved from by 0.0113731 from a starting value of 1.00595, so that is an improvement of 1.13 % in optical gain.
Around 19:04:28 UTC I started the DARM offset step to see if the change in optical gain matches that we would see if we measured the throughput of HAM 6. Unfortuntely I forgot to turn off the OMC ASC which we know affects this measurement of the loss. We stood down from changing the OMC and Camilla did some squeezer measurements, then I made the same mistake again the next time I tried to run it (d'oh). Both times I control-C'd the auto_darm_offset.py form the command line which means the starting PCAL line values, and DARM offset had to be reset manually before I ran the script successfully after turning the OMC ASC gain to 0 to turn it off.
The darm offset measurement started at 19:20:31 UTC. The code to run it is /ligo/gitcommon/darm_offset_step/auto_darm_offset_step.py
The results are saved in /ligo/gitcommon/darm_offset_step/data and /ligo/gitcommon/darm_offset_step/figures/plot_darm_optical_gain_vs_dcpd_sum.
From the final plot in the attached pdf, the transmission of the fundamental mode light between ASC_AS_C (anti-symmetric port) DCPD is (1/1.139)*100 = 87.8 %. We can compare this to the previous measurement from last week with the old QPD offsets to see if the optical loss change matches what we would expect from such a change in optical gain.
Since the script didn't save the correct values for pcal ey and ex (due to the script being run partially twice before a siccessful measurement). I reverted the PCAL values back using SDF before we went into observing. See attached screenshots.
Sheila accepted the new ASC-OMC_A and B OFFSET values in OBSERVE and SAFE (only have the pic for OBSERVE).
Comparing OMC losses calculated by OMC throughput and optical gain measurements.
If we take the improvement in optical gain noted above and calculate the improvment in the optical gain ^2, ie.
(g_f^2 - g_i^2)/ g_i^2 = 0.023 = 2.3 %
And compare it to the gain in OMC throughput from this entry to the measurement after changing the OMC ASC offsets above
(T_OMC_f - T_OMC_i)/ T_OMC_i = 0.020 = 2%
Both methods show a similar improvement in the coupling to the OMC, or alternatively decrease in the HAM 6 losses. Since we improved the alignment of the OMC, it makes sense that the losses decrease and them agreeing validates our method of using darm offset steps to calculate OMC throughput and thus the loss in HAM 6.
The optical gain must be squared as it changes with the square root of the power at the output (due to the DARM loop).
For this comparison I was not able to use the measurement of optical gain from the same day as the initial measurement of OMC throughput, (alog #82938) as the calibration was exported to the front-end between these two dates which would have changed the reference value for kappa C.
The code I used for calcultions is attached.
As I did for the previous DARM offset measurement on the 20th Feb, in alog #83586, I checked that the DARM offset does not show a clear trend in the OMC REFL power. This would be another way of quantifying the mode-matching of the DARM mode to the OMC, but since the mode-matching is good, no trend can be seen in this channel (top plot) as we change the DARM offset.
Jennie W, Sheila
Today I got a chance to redo some of my output chain measurements (alog #82555) that gave us a confusing result when we were heating up and cooling down the OM2 heater. The confusiong was that our optical gain got better for cold OM2 compared to hot, but the loss through HAM6 predicted by stepping the DARM offset and comparing it to the power at the anitsymmetric port predicted that the loss was worse with cold OM2 and gave us unreasonably low (~65 %) throughput estimate for the fundamental TM00 mode through HAM6. We realised that the OM3 and OMC alignment are being changed by the ASC during this time so that could be affecting the comparison.
Steps:
Turn off OMC ASC at 18:43:00 UTC.
Run auto_darm_offset_step.py from /ligo/gitcommon/labutils/darm_offset_step at 18:45:01 UTC.
Results: P_AS = 62.996 mW + 1.162 * P_DCPD
This makes the throughput estimate for the TM00 mode through HAM6 to the DCPDs to be 86.0 % of the power at the AS port. Which seems more reasonable than the 65% we got last time. We need to do this measurements again when we have improved kappa C somehow to check it gives us the same loss estimate between two times.
We were then going to purposely change kappa C as a comparison to the estimate the DARM offset step gives us, byt changing the QPD offsets based on this measurement 82383(I got the sign wrong last time I did this).
I turned the OMC ASC back on before doing this, however when I changed the H1:ASC-OMC_A_PIT_OFFSET to 0.45 this saturated the OM3 suspension so this was set back to nominal.
I think I got signs wrong yet again so we will try what we now think are the correct ones another commissioning period but maybe do it slowly so as not to cause saturations.
Jennie, Sheila
Sheila wanted me to checked that we can't use the OMC REFL power as a calculation method for how much of the TM00 light does not make it through the OMC. If the mode-matching of the light at the AS port to the OMC is good, we would expect not to see much of a variation at the OMC REFL port as we change the DARM offset, and indeed we can't. See this image, with REFL power at the top.