TITLE: 11/27 Eve Shift 2030-0200 UTC (1230-1800 PST), all times posted in UTC
STATE of H1: Planned Engineering
INCOMING OPERATOR: None
SHIFT SUMMARY: The last of the PEM measurements were done this evening when H1 was locked, but a couple of locklosses (both of which seemed to be caused by activity in sensitive areas in the LVEA) limited the amount of time at low noise. Following the most recent lockloss, I'm leaving H1 in 'IDLE' for the long weekend before the upgrade phase begins on Monday.
LOG:
| Start Time | System | Name | Location | Lazer_Haz | Task | Time End |
|---|---|---|---|---|---|---|
| 20:49 | PEM | Rene | CER | N | Moving magnetometers | 20:56 |
| 21:05 | PEM | Robert | LVEA | N | Running measurements | 22:51 |
| 21:50 | ISC | Kar Meng | Opt Lab | Local | OPO work | 00:17 |
| 01:41 | PEM | Robert | LVEA | N | Cleaning up | 01:55 |
TITLE: 11/26 Eve Shift: 0030-0600 UTC (1630-2200 PST), all times posted in UTC
STATE of H1: Planned Engineering
OUTGOING OPERATOR: Ryan C
CURRENT ENVIRONMENT:
SEI_ENV state: CALM
Wind: 8mph Gusts, 5mph 3min avg
Primary useism: 0.02 μm/s
Secondary useism: 0.16 μm/s
QUICK SUMMARY: H1 is relocking and currently up to LOWNOISE_ESD_ETMX. More PEM measurements ongoing today and into this evening.
TITLE: 11/26 Day Shift: 1530-0030 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Planned Engineering
INCOMING OPERATOR: Ryan S
SHIFT SUMMARY: We've had two locklosses today, both while people where out on the floor. Relocking has been fairly automated, we had a TCS CO2Y laser issue that we resolved. We are relocking at MOVE_SPOTS as of 20:30 UTC. LVEA zone4G got a bit warm but its leveled out.
LOG:
| Start Time | System | Name | Location | Lazer_Haz | Task | Time End |
|---|---|---|---|---|---|---|
| 16:47 | PEM | Robert | LVEA | N | Set up measurements, check on zone4 | 17:05 |
| 17:31 | PEM | Robert | LVEA | N | Setup shaker in *danger zone*, in and out | 20:18 |
| 17:34 | ISC | Kar Meng | Optics lab | LOCAL | OPO work | 19:27 |
| 18:56 | TCS | Sheila | LVEA | N | Reset CO2Y | 19:11 |
| 19:38 | FAC | Tyler | Mids | N | Find boom lift and inflate the tires | 20:06 |
| 19:54 | TCS | Daniel, Sheila | LVEA | N | Wiggle TCS CO2Y cable | 20:03 |
Both the pump (532nm) and fundamental (1064nm) have now been alignment to the VOPO cavity based on the mode matching setup described in this log.
From the mirror specification (C2500221), the theoretical escape efficiency is calculated to be 98.5% (derived from the decay rate of the mirror, k_in,r / k_in,tot).
The escape efficiency from the VOPO reflection is 97.9% (calculated from the photodiode reflection, trans/refl = (2nesc - 1)^2).
In short, input alignment done, rear seed injection is the next to go, escape efficiency checked, and the photons escaping the cavity with the enthusiasm of a PhD student during a conference lunch break.
For the escape efficiency measurement, the transmission field refer to the light entering and exiting the cavity via M1 (shown as the "dip" on the reflection photodiode). Whereas the reflected field refer to the promptly reflected light from the photodiode (shown at the flat line on the reflection photodiode).
The measured escape efficiency is consisted with the measurement done at MIT (E2500270), where escape efficiency of 97.9% to 98.2% was reported for various crystal position.
19:58 UTC lockloss, there was a big fuzzy oscillation in PR_GAIN right before LL
Wed Nov 26 10:05:20 2025 INFO: Fill completed in 5min 16secs
17:50 UTC lockloss, there was an ISI BS saturation a few seconds after the lockloss.
19:18 NLN but we've encountered a TCS CO2Y issue, the laser tripped off and doesn't want to come back.
Kevin, Sheila
Over the last few days we've run ADF sweeps a few times. Here's a record of what happened and file names.
The files are in /ligo/gitcommon/squeezing/sqzutils/data
Nov 22 08:31 HF_10kHz_11_2025.h5 IFO had been powered up for 11:00, sweep started at about 14:50 UTC Nov 22. NLG 24.3, measurement is in 88224. Something seemed to go wrong towards the end of the sweep, we aren't sure what.
Nov 22 12:38 HF_10kHz_11_2025_2.h5 IFo had been powered up for 15:10, same lock as the previous measurement, same NLG measurement, sweep started at about 19 UTC.
Nov 25 00:36 HF_10kHz_11_2025_b4_CO2_step.h5 IFO had been powered up for 4:20, in this sweep I didn't turn off the SQZ angle servo based on the ADF, so the demod phase was moved around during the sweep, making this data not useful.
Nov 26 01:56 HF_10kHz_11_2025_b4_CO2_step2.h5 last night's first scan, started only 38 minutes after power up at about 8:18 UTC Nov 26th. The amplified seed was 7.8e-3, unamplified seed didn't happen correctly with the script but the waveplate hasn't moved since previous measurements of that level at 2.9e-4 (88223), giving an NLG of 26.9. (Edit, I redid the unamplified seed measurement, it looks like 3.2e-4 now, making the NLG 24.4 for these last two measurements, which has been consistent (24.3 or 24.4) for the last week.
Nov 26 08:15 HF_10kHz_11_2025_after_CO2_1hour.h5 this morning's sweep, IFO had been powered up for 7 hours, CO2s had been stepped from 1.7W each to 0.9W each for 1.5 hours when the sweep started at about 14:37 UTC Nov 26th. NLG should be the same as for above, 26.9. 24.4
The goal of these measurements is to use the ADF to measure the rotation of the squeezed state around higher order mode arm cavity resonances as described in section IV.B of LIGO-P2500132. Ultimately we would like to be able to use such measurements to diagnose the thermal state as a guide in how to tune TCS in order to improve mode matching.
While we are still digesting the results, the first plot shows the preliminary inferred squeezed state rotation for the three good data sets that we got. pre-step 1 and pre-step 2 are the two taken on Nov 22. (Everything turned out to be fine with the first sweep.) post-step is the last one taken this morning after the CO2s had been stepped and the IFO had been up for 7 hours. There is a small arbitrary constant offset in the SQZ angle of order a degree, so all angles have been shifted to be zero at 10.450 kHz. The second plot shows the OMC DCPD spectra 5 min before the start of each of these three sweeps.
Two rotation peaks are visible rather than the one shown in Fig 7 of P2500132. This is expected since the arms are astigmatic in reality, and our more detailed models show the same behavior. Each eigenmode is resonant at a slightly different frequency and is responsible for a rotation as in Fig 7 which are superimposed as observed in this data.
The post-step rotation is slightly smaller in magnitude and is shifted to slightly lower frequencies. Since the CO2 is mainly a higher order actuator, this is consistent with our expectations that this rotation is predominantly sensitive to quadratic mismatch with higher order aberrations altering the detailed behavior. However, seeing as how the pre-step was not taken just prior to the CO2 step in the same lock, I think it's just as likely that this is due to it being in a slightly different thermal state before the CO2 step. The peaks in the OMC DCPD spectra also appear slightly lower in frequency for the post-step.
I think the main takeaway from these measurements so far is showing that we can measure this rotation and resolve changes on the scale that our modeling suggests would be useful.
This analysis was done in the aligoNB environment by running
pytest /ligo/gitcommon/squeezing/sqzutils/analysis/T_10kHz_ADF.py --tb short -s -k T_Nov_CO2_step
TITLE: 11/26 Day Shift: 1530-0030 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Observing at 146Mpc
OUTGOING OPERATOR: None
CURRENT ENVIRONMENT:
SEI_ENV state: CALM
Wind: 7mph Gusts, 4mph 3min avg
Primary useism: 0.01 μm/s
Secondary useism: 0.17 μm/s
QUICK SUMMARY:
15:33 UTC GRB-Short E619679
TITLE: 11/26 Eve Shift: 0030-0600 UTC (1630-2200 PST), all times posted in UTC
STATE of H1: Planned Engineering
INCOMING OPERATOR: None
SHIFT SUMMARY: We had 2 locklosses, the first was easy to recover from, the second is still in progress. We're at MAX_POWER right now.
LOG:
| Start Time | System | Name | Location | Lazer_Haz | Task | Time End |
|---|---|---|---|---|---|---|
| 00:16 | PEM | Rene, Alicia | CER | N | Setup measurement, huddle test | 00:33 |
| 00:20 | ISC | Kar Meng | Optics lab | LOCAL | OPO work | 01:13 |
| 00:21 | ISC | Marc | Optics lab | LOCAL | Help with osciliscope issue | 00:59 |
| 00:52 | PEM | Robert, Sam | EndX | N | Setup measurement | 01:20 |
04:10 UTC NLN
04:30 UTC We went into Obseving after I cleared a leftover EX PEM EXC
Last night I ran a longer version of the full magnetic injection suite starting at about 03:10 UTC, and it finished at 07:33 UTC. This used the same parameters as last week's run, except I doubled the injection time to 5 minutes each.
Exact times and injection parameters are in the usual log directory for the magnetic injections: /ligo/www/www/exports/pem/WeeklyMagneticInjection/logs/1448075483.txt
The last batch of injections (all 7 of the ones at EY E-bay) mistakenly overlapped with a scheduled SQZ script, so last night I re-ran these between 05:29 and 06:06 UTC.
Analysis results and plots can be found here: https://ldas-jobs.ligo.caltech.edu/~ryan.short/pem/Weekly_Mag_Inj/H1_Injection_Results/O4/20251125_1448075483/
[Joan-Rene Merou, Alicia Calafat, Sheila Dwyer, Jenne Driggers] We have entered the LVEA and went to the Beer garden. There, we first turned off the Low Voltage ITM ESD Driver D1600092, first the 15V switch and then the medium voltage switch. In order to turn it on again, it should be reconnected in the opposite order. With the voltage request set to 0 and chassis powered off, we have unplugged the SHV cables going to the chamber and plugged into Robert's ground boxes, which we used to ground to the rack which is grounded to the chamber. This has been done at both drivers (See attached photos). Afterwards, we have changed the code at /opt/rtcds/userapps/release/isc/h1/guardian/ISC_LOCK.py in order that the LOWNOISE_COIL_DRIVERS will go to LOWNOISE_ESD_ETMY instead of TRANSITION_FROM_ETMX. This has been done by changing lines 6670 and 6674, moving the ", 15" step from line 6670 to 6674. Finally, we communicated the change to the operator and loaded the guardian.
It appears that the grounding did not decrease the amplitude of the combs. As seen in the attached figure, the relative amplitude of the first harmonics of the combs remains mostly the same before and after the change on November 13th.
I made plots of anti-symmetric power P_AS vs. power at reflected port of OMC P_OMC_REFL during the DARM offset step measurement on September 4th, (see LHO alog #86785 and 87629).
I had to use the Beckhoff reported power for this (H1:OMC-REFL_A_DC_POWER) as the front-end channel is calibrated wrongly (see LHO alog #87648).
I also plotted the P_OMC_REFL vs. P_DCPD, ie. reflected vs. transmitted power for the OMC.
The plots for our two measurements taken at different times during IFO thermalisation are below, both were taken when OM2 was hot.
I reran these plots as the axis limits of the P_REFL vs. P_DCPD plot were wrong and were cutting off end point, plus removed line that explained what the y-intercept was for each plot as different dependent on whether we plot P_REFL vs P_AS or P_REFL vs. P_DCPD.
I also switched the P_REFL channel being used in my code to H1:OMC-REFL_A_DC_POWER from H1:OMC-REFL_A_DC_POWERMON as this latter channel has a factor of 100 relative to the former that I don't really undestand. The DC_POWER channel seems to give a realistic reading for the OMC reflected power that is much less than the power into HAM6.
First link contains two plots when we were half-way thermalised:
First plot is power at the OMC reflected PD vs. power at the antisymmetric port (calibrated into the power into HAM6) for the case where we were 1Hr 25 mins into lock.
Second plot is power at the OMC reflected PD vs. power transmitted to the DCPDs for the case where we were 1Hr 25 mins into lock.
The second link contains two plots also when we were thermalised:
First plot is power at the OMC reflected PD vs. power at the antisymmetric port (calibrated into the power into HAM6) for the case where we were 3 hrs 59 mins into lock.
Second plot is power at the OMC reflected PD vs. power transmitted to the DCPDs for the case where we were 2 hrs 59 mins into lock.
We can write down an equation for P_REFL from the OMC in terms of P_DCPD, using our linear fit.
P_REFL = ( c*P_DCPD + d ) mW
We know the nominal setting for P_DCPD is 40mA, and we can take the responsivity of the DCPDs at 100 % efficiency to be
responsivity = e * lambda / (c * h)
From the squeezer budget (E2400269) we can get a number for the Q.E. of the PD that also includes OMC losses for the transmitted beam, transmissivity = 0.937
Therefore the power at the DCPDs at nominal DARM offset is 40mA/(responsivity*transmissivity) = 49.7 mW.
The reflectivity of the OMC breadboard is 2.75e-4 as calculated from parameters given in T1500060-v3.
The formula for the power measured at the reflected port of the OMC can also be expressed as:
P_REFL = R_cav [ P_00_arm + P_00_cd] + P_HOM_arm + P_sb + P_HOM_cd
where P_00_arm is the power in the fundamental carrier mode which changes with DARM offset, P_00_cd is the contrast defect light that is in the fundamental carrier mode, P_HOM_arm is light at higher order mode frequencies which also change with DARM offset, P_sb is power in the sidebands, P_HOM_cd is contrast defect light at higher order mode frequencies.
Whereas the formula for the power transmitted by the OMC can be described as:
P_DCPD = T_cav [ P_00_arm + P_00_cd]
As we assume that all HOM and sidebands are reflected by the OMC.
The mode-matching, MM, of the OMC to the differential arm mode is defined as:
P_00_arm / ( P_HOM_arm + P_00_arm )
This can be calculated using:
P_00_arm = (P_DCPD - d)/T_cav
P_HOM_arm = P_REFL - d - (R_cav*P_00_arm)
If we do this calculation for the half-way thermalised measurement we get
MM = 0.9975
For the fully thermalised case we get:
MM = 0.9978
The code to calculate this is in: Calculate_refl_power.py located at /ligo/home/jennifer.wright/git/2025/DARM_OFFSET/
Jennie W, Sheila,
I took a long time to post this as have been working on other things...
We carried out a test (see LHO alog #86785) to look at the effect of DARM offset stepping on the power at OMC-DCPD_SUMS and OMC-REFL (transmitted through and reflected from the OMC). We did this with the heater on OM2 off as is nominal.
We then meant to redo these measurements once we heated up OM2 to change the mode-matching of the IFO to the OMC.
Unbfortunately we lost lock at about 15:06 UTC while Corey was taking out first measurement before heating up the OM2.
The meausrement is shown in this image, I have mislabelled it as 'third measurement' but it was the first. The optical gain is shown just before this measurment to be 0.994.
Then we waited as long as we could under out initial parameters of being finished cooling the OM2 again by 1:45pm.
We took another measurement at 1 hr 25 mins into lock after two false starts where I forgot to turn off the ASC. The optical gain was measured right before we started the measurements to be 0.978 but was still thermalising.
And then we took a third 2 hrs 59 minutes into lock, the IFO should be thermalised but the temperature of OM2 was still trending upwards a bit. Optical gain was 0.986.
We can use the slope of the power at the antisymmetric port (P_AS) vs. the power at the DCPDs (P_DCPD) as the DARM offset changes to estimate the throughput of carrier through the OMC which allows us one estimate of the loss.
The plots of this throughput are here for the cold state (minus the points taken after we lost lock), here for the partially thermalised state, and here for the thermalised state.
I am also in the middle of using the plot of P_AS varying with power at the OMC reflected port (P_REFL) to get a better estimate of the mode-mis match between the interferometer and the OMC.
I plotted the loss between the antisymmetric port (calibrated into the power entering HAM6) to the power on the DCPDs. This is the inverse of the slopes in the graphs above.
All three are poltted on one graph, using plot_AS_vs_DCPD_changes.py in my own cope of the labutils repository at /ligo/home/jennifer.wright/git/local_git_copies/labutils/darm_offset_step/ .
Sheila and Camilla both agreed the loss for the two bottom lines (purple and red) are too high. These imply that a hot OM2 gives us over 20 % output losses.
If we look at the increase in loss from cold OM2 to hot OM2 this is a factor of 2.1 (210 % increase).
Compared to the decrease in optical gain squared (which we expect to reflect the change in output losses, which was:
(0.986^2 - 0.994 ^2) / 0.994^2 = -0.016 (1.6 % decrease).
We might have to check the alignment of out optics was not changing while we changed the darm offset.
Looking at OM1, OM2 and SRM alignment it did change during the darm offset steps with the biggest change (in the third offsset step measurement) being in OM2 pitch and yaw, this is only a change around 6 microradians (Elenna and Jeff state this calibration in correct to within an order of magnitude). Not sure if this enough to invalidate the loss values we measure. OM3 and OMC sus did not change much but this is because IU purposely unlocked the OMC ASC while changing the darm offset.
Jennie W, Matt T,
I plotted the antisymmetric power during the darm offset step vs. the power reflected by the OMC and am now very confused as the AS power looks to be smaller than the power reflected form the OMC. See the ndscope where I have zoomed in on the same time segment for both channels. The OMC-REFL channel is mean to be calibrated into mW and the ASC-AS_C channel is meant to be calibrated into W entering HAM 6 (even though the actual pick-off is the transmission through OM1).
The two plots attached show how the ratio between AS and OMC-REFL power changes during one of the DARM offset measurements we did right after I took this ndscope data.
Plot 1 hr 25 mins into lock.
Plot 2 hrs 59 mins into lock.
For each point the code returns the median of the time series at each step, this mioght be less valie for OMC-REFL as it is a lot noisier than ASC-AS_C.
I am still confused about the hogher power at OMC-REFL and wondering if:
a) I am confused about the calibration of one of these channels.
b) the calibration of one of these channels is wrong.
I plotted the three measurements of P_AS vs. P_DCPD during thermalisation on the same plot to make them easier to compare.
The code for this is in /ligo/home/jennifer.wright/git/local_git_copies/labutils/darm_offset_step/plot_OMC_REFL_changes/P_as_vs_P_DCPD__comp_Sep_04.pdf