Displaying reports 9101-9120 of 84064.Go to page Start 452 453 454 455 456 457 458 459 460 End
Reports until 16:00, Tuesday 16 April 2024
LHO General
ibrahim.abouelfettouh@LIGO.ORG - posted 16:00, Tuesday 16 April 2024 (77219)
OPS Day Shift Summary

TITLE: 04/16 Day Shift: 15:00-23:00 UTC (08:00-16:00 PST), all times posted in UTC
STATE of H1: Commissioning
INCOMING OPERATOR: Oli
SHIFT SUMMARY:

IFO is in NLN and COMISSONING - the squeezer is having lock issues and a team of comissioners, fellows and other staff are in the control room and working on fixing it.

19:29 UTC: Began Locking (No initial alignment)

20:15 UTC: Began Initial Alignment (after 3 IR_COMM based locklosses)

IR COMM Weirdness:

Once we started locking, ALS locked fine but IR_COMM was not found, prompting a troubleshoot of this part. There was extremely noise behavior in the relevant channel (H1:LSC-TR_X_NORM_INMON) where the usually normalized (to 1) values were showing up bizarrely high. (Screenshot 1). After initial alignment, this issue was resolved.

20:36 UTC: Initial Alignment Complete

21:21 UTC: Reached NLN

21:24 UTC: H1 is OBSERVING

21:36 UTC: Dropped out of observing due to squeezer lockloss - a team of commissioners are on the case.

22:55 UTC: Trying to get into OBSERVING without squeezing while we troubleshoot the squeezer.

LOG:

Start Time System Name Location Lazer_Haz Task Time End
15:02 FAC Ken FCES N Electronics work 20:00
15:03 CAL Dave remote n WP11812 h1calcs cal_hash_ioc chan move 17:31
15:04 DAQ Dave Remote n DAQ Restart for cal work 17:31
15:10 VAC Jordan, Norco EY, Corner, EX N Nitrogen tank inspection 19:22
15:18 ISC Jennie LVEA N Turning off PSL Sidebands 15:23
15:19 FAC Kim, Karen FCES N Technical Cleaning 15:53
15:19 ISC Camilla LVEA N Laser Hazard Transition 15:26
15:39 TCS Camilla,. TJ LVEA YES TCS Table Work 18:49
15:39 OMC Jennie, Sheila Ctrl Rm N Aligning OMC 17:38
15:40 FAC Christina OSB Patio N Transporting pallets and moving tables 17:38
15:41 OMC Sheila LVEA YES Turning off PSL sidebands 16:40
15:45 FAC Ace Portapotty End Stations N End Station Portapotty Inspection 16:45
15:45 IAS Jason, Tyler, Ryan C LVEA YES IAS Alignment Work 18:42
15:46 LVEA HAZARD LVEA YES LVEA IS LASER HAZARD 19:11
15:53 FAC Kim EX N Technical Cleaning 16:53
15:53 FAC Karen EY N Technical Cleaning 16:39
15:54 EE Fil LVEA YES Cable tray inspection 16:23
16:08 SEI Jim FCES N HAM7 Dissassembly of CPS Cards 17:39
16:42 PEM Marc EX N Accelerometer chassis 18:50
16:48 EE Fil LVEA YES Table Tray Inspection 17:14
16:53 FAC Kim Hi-Bay N Technical Cleaning 17:34
17:09 OMC Sheila LVEA YES Turning sidebands back on 17:59
17:14 EE Fil EX, EY N Equipment Inventory 19:20
17:34 FAC Karen, Kim LVEA YES Technical Cleaning 18:44
18:49 OPS Camilla LVEA YES Detransitioning to LASER SAFE 19:19
18:54 FAC Nolan Y-Arm N Y-End Ecology Check 21:54
18:54 IAS Jason Optics Lab N Finishing up optics work 19:00
19:05 OPS TJ LVEA YES Maintenance End Sweep 19:16
20:07 FAC Ken FCES N Bolting 21:07
Images attached to this report
H1 SQZ (SUS)
camilla.compton@LIGO.ORG - posted 15:35, Tuesday 16 April 2024 - last comment - 08:33, Friday 19 April 2024(77218)
Trouble locking SQZ FC again. Checking on FC SUS

Shiela, Naoki, Rahul, Kar Meng, Terry

Same as yesterday (77188), we are again today having trouble locking the FC. Wind is again constant at 0-20mph. Can get green flashes but no locking, even with FC feedback turned off, VCO locking also fails. 

Rahul changed the M1 coil driver state on FC1 and FC2 from state 1 (usually only used in TFs) to state 2: IFO nominal for other triples. State 2 contains a low pass filter. 

Rahul took FC2 P and L transfer functions, look healthy and same as 66414.

Rahul took FC2 OSEMINF spectrums and checked ther health, as previously had issues with FC1 BOSEMS  (72563). Can see the 0.3 to 0.4Hz peak, Rahul's not worried about it but we could check old data for this peak.

Images attached to this report
Comments related to this report
camilla.compton@LIGO.ORG - 16:39, Tuesday 16 April 2024 (77221)

Jim found that the HAM8 ISI has a resonance at the same place as FC2, peak at 0.375Hz see attached. He edited a gain and the motion seemed to improve enough to lock the FC.

During this time Ibrahim, Oli and I had followed ObservationWithOrWithoutSqueezing wiki and edited all the SQZ guardian code nominal states and accepted no squeezing sdfs. We then reverted these changes once the FC locked. 

Images attached to this comment
victoriaa.xu@LIGO.ORG - 16:49, Tuesday 16 April 2024 (77225)

From HAM8 summary pages, I don't see this 0.36 Hz peak between Dec15 - Jan15. Peak is basically exactly where FC2_L is oscillating in yesterday's screenshot. Since Jan 15 2024, the peak looks intermittently there or gone, pretty variable. Maybe exciting this peak is related to wind? Or maybe this is all totally unrelated to wind.. I don't think this was an issue in O4a, maybe something changed after Jan 15.

Images attached to this comment
jim.warner@LIGO.ORG - 17:10, Tuesday 16 April 2024 (77226)SEI

Seems like another broken GS13 on HAM8, this time a horizontal sensor. I took some driven measurements looking at the l2l cps to gs13 transfer functions and the H1 cps to gs13 tfs is lower than the other 2 sensors by about 2x, see first attached image. This affects the stability of the blend cross-over, which changes the gain peaking in the blends. I've compensated for now with a digital gain, but this may not work for long.

I tried compensating with a digital gain in the calibration INF filters for the ISI, this seems to have improved things, shown in the second image. Top subplot is the M3 pit witness for FC2, second line is the gain I adjusted, third line are LOG BLRMS for the X, RZ and RX GS13s on HAM8. X and RX don't improve much, but the RZ motion improves a bit after changing the gain. Fourth line is the RZ cps residual, which is much quieter after increasing the gain to compensate for the suspected low response of the H1 GS13.

To add to Vicki's comment, the peaks behavior seems complicated, it started at .6hz in January, then some time around March it moved down to its current frequency ~.37hz. Lots of days missing from the summary pages in that time, so it's hard to track. The transience of the peak is also consistent with broken seismometers we've seen in the past. The gain tweak I put in may not be a stable fix.

Images attached to this comment
oli.patane@LIGO.ORG - 17:43, Tuesday 16 April 2024 (77227)

SDFs that were accepted for observing w/ sqz

Images attached to this comment
brian.lantz@LIGO.ORG - 08:33, Friday 19 April 2024 (77284)

FYI - FRS ticket 31005 is tracking the 1/2 gain GS-13

H1 PEM (PEM)
marc.pirello@LIGO.ORG - posted 15:07, Tuesday 16 April 2024 (77217)
EX Accelerometer Conditioner Repaired

I pulled EX Accelerometer Power Conditoiner S2300070 per WP11813 to investigate a bad channel and the restult was that the input resistor had blown on that channel.  The symptom was that the channel was completely off, no LED activity on the front panel for that channel.  The current draw per channel at 24V is < 63mA, the 10 ohm resistor is rated at 1/4 watt which gives us an upper limit of 160mA current.  It could have been inrush current that blew this resistor as they have only been tested on bench and not with kepkos' higher current rating.  This is part of the low pass filter for these accelerometer channels.  I replaced the 10 ohm 1/4 watt resistor with a 5W resistor.  I will keep an eye on these, if this becomes an issue, we might consider replacing the resistors with higher wattage versions as there is space on the board for it.

Channel Order
CH1 - Cable 7 - AA7 - OPLEV-Y
CH2 - Cable 8 - AA8 - BSC9_X
CH3 - BLK_NL - U2_9 - Manifold1
CH4 - Cable 10 - AA10 - BSC9_Z
CH5 - Cable 11 - AA11 - TableX
CH6 - Cable 12 - AA12 - BSC_Floor
CH7 - Cable 13 - AA13 - Ebay_Floor
CH8 - BLK-NL - U2_11 - Manifold2
CH9 - empty - empty (ready to replace the Meggit single channel device)

H1 SQZ (ISC, SQZ)
jennifer.wright@LIGO.ORG - posted 14:10, Tuesday 16 April 2024 - last comment - 19:04, Thursday 18 July 2024(77204)
OMC Scan with PSL beam

Jennie W, Sheila,

 

We turned off the 9 and 45 MHZ sideband EOMs and unplugged the 118 MHz modulation at the PSL racks. See this alog for how to do this.

 

We locked the IMC and mis-aligned ITMX.

 

DC centering loops 3 and 4 were turned on.

 

Sheila took the OMC lock guardian to PREP OMC scan and turned on the OMC ASC.

We waited for this to converge then turned it off.

 

We turned input power up to 10W from 2W and then locked the OMC in length manually by using the PZT offset slider to search for a high peak ~ 15mA.

After finding it we turned on the locking with a gain of 24 and the boost and int filters on (we checked the settings we needed in the guardian as we couldn't get the OMC guardian to lock it for us).

 

Then we turned off the OMC ASC.

 

We tuned up the OM3 and OMC alignment slightly to maximise the power on OMC-DCPD_SUM_OUTPUT and minimise it on OMC-REFL_A_LF_OUT16.

OM3 was moved down in yaw only from -108 to -117 and OMC was moved down in yaw from 210.5 to 195.5 and down in pitch from 350.4 to 340.4. The final values for the sliders are here.

 

Quiet time locked after aligning 16:21:03 UTC - 16:24:13 UTC

OMC-REFL_A_LF_OUT16 = 0.652644 mW

OMC-DCPD_SUM_OUTPUT = 15.6162 mA

 

Quiet time unlocked 16:25:31 UTC -16:27:35 UTC

OMC-REFL_A_LF_OUT16 = 30.106 mW

OMC-DCPD_SUM_OUTPUT = 0.000456763 mA

 

We took the IMC guardian offline and shuttered the green light going into both arms at the ISC tables, and with ISC_LOCK guardian in idle so it wouldn't keep trying to relock IMC.

Quiet time dark measurement 16:43:38 - 14:46:19 UTC

OMC-REFL_A_LF_OUT16 = -0.0132979 mW

OMC-DCPD_SUM_OUTPUT = -0.00106226 mA

 

The scan template is saved as /ligo/home/jennifer.wright/Documents/OMC_scan/2024_04_16_OMC_scan.xml

With the references for the time series of the three pertinent channels as:

Ref 0 OMC-DCPD_SUM_OUT_DQ

Ref 1 OMC-PZT2_EXC

Ref 2 OMC-PZT2_MON_DC_OUT_DQ

 

Images attached to this report
Comments related to this report
jennifer.wright@LIGO.ORG - 19:01, Monday 06 May 2024 (77670)

I ran Sheila's code from this entry, altered with the measured input/output coupler transmission of the current OMC which can be found on Page 116 on LIGO-T1500060.

The output gives this for the cavity parameters:

Power on refl diode when cavity is off resonance: 30.138 mW

Incident power on OMC breadboard (before QPD pickoff): 30.589 mW

Power on refl diode on resonance: 3.879 mW

Measured effiency (DCPD current/responsivity if QE=1)/ incident power on OMC breadboard: 59.5 %

assumed QE: 100 %

power in transmission (for this QE) 18.203 mW

HOM content infered: 9.763 %

Cavity transmission inferred: 66.439 %

predicted efficiency () (R_inputBS * mode_matching * cavity_transmission * QE): 59.509 %

omc efficency for 00 mode (including pick off BS, cavity transmission, and QE): 65.948 %

round trip loss: 3504 (ppm) Finesse: 335.443

 

I will cross-check the HOM content inferred by analyaing the C02 mode height from a cavity scan.

jennifer.wright@LIGO.ORG - 19:04, Thursday 18 July 2024 (79229)

The mode-matching inferred from the height of the carrier 02 mode vs. the carrier 00 mode from the scan is 0.0983 mode mis-match = 9.83%.

The mode scan fit and the C02/C20 fit are attached.

The code is on labutils /dev branch

The code for the full scan can be ran using:

python OMCscan_nosidebands9.py 1397320410 80 "Cold OM2, 10W PSL, pre-output loss" "single bounce" --verbose -m -o 2

The code for the C02 fitting can be done using:

fit_two_peaks_no_sidebands9.py

Where the blue trace is the data, the orange is the fit, and the purple is the function plotted with the inital guesses for the fit parameters as a cross-check.

Non-image files attached to this comment
H1 SUS (ISC, OpsInfo)
jeffrey.kissel@LIGO.ORG - posted 14:09, Tuesday 16 April 2024 - last comment - 14:17, Tuesday 16 April 2024(77211)
H1 SUS IM Alignment Sliders now Calibrated into microradians
J. Kissel

EXECUTIVE SUMMARY

After having visited the calibration of the HAUX alignment sliders since 2016 (see LHO:30010), it's time to re-measure and recalculate what these gains should be, as we've lost confidence in their accuracy. 

I've recalibrated the IM1, IM2, IM3, IM4 alignment sliders today, such that one count offset in [pitch, yaw] produces 1 microradian in [pitch, yaw] according to the OSEMs. To correct from the previous incorrect calibration, slider values would have needed to be multiplied by factors of 20 to 30 [urad/"urad"].

METHODS AND RESULTS

In order get something in play quickly, I've used the OSEMs as my absolute angle reference, having been calibrated into microns [um] for years and cast into PITCH and YAW through trusted OSEM2EUL matrices to produce pitch and yaw in microradians [urad]. 

Recall the goal is to calibrate the output of the OPTICALIGN banks, which are nominally in Euler basis DAC counts [DAC ct] such that when you request the slider to move in your desired physical unit (in this case, [urad]) then the output of the bank requests the appropriate amount from the DAC. Thus, we need a gain, H where
    slider offset [urad] * H [DAC ct / urad] = DAC output [DAC ct]        (1)


In short, the method is:
    (i) Set the OPTICALIGN gain to 1.0 so there's no confusion during the measurement.
    (ii) Request the slider offset to be a range of values (I arbitrarily chose [-10000, -5000, -1000, 1000, 5000, 10000]; six data points such that a linear regression had plenty to grab on to)
    (iii) At each requested value, record the OSEM values.
    (iv) Fit a line to a plot of OSEM value vs. slider value, i.e. (slope * slider value + offset). The slope will be in units of [urad / DAC ct].
    (V) Invert the slope to obtain the slider calibration gain in units of [DAC ct / urad].
I used an ipython session interactively to do so for all IMs at the same time via for loops, while the IMC was unlocked and misaligned.

Here're the results in units of [DAC ct / urad] (rounded to the nearest 4th decimal place):
         PIT       YAW
IM1     9.9093    5.3457
IM2    10.1124    5.4868
IM3    12.5623    6.8758
IM4    10.9005    5.6289

Note that the results are not insignificantly different from suspension to suspension, even though every HAUX actuation chain should be the same. So, I've elected to install these suspension specific gains (like we have with other suspensions that have had recent attention), rather than a generic gain for suspension type based on a model of the actuation strength.

The first two pages of 2024-04-16_H1SUSIM_AlignmentSlider_Recalibration_GainFitPlots.pdf shows the plots of data, and their fits. As an aside, because I drove the slider requests programmatically via ipython, it was easy to measure both the pitch and yaw OSEM values during the other DOF's slider changes. As such, I also gathered the amount of cross-coupling between pitch drive and yaw response and vice versa, yaw drive and pitch response, in units of [urad / DAC ct]. This is shown on the last two pages. The good news is that the off-diagonal cross-coupling is an order of magnitude or two less than the expected diagonal coupling (I think auto-y-axis-scaling dataviewer or ndscope sessions have scared us for years). That being said, IM3 is the worst offender.

After I installed the new calibration, I've made sure to set the *actually* [urad] value to reproduce the same [DAC ct] output that had been requested with the previous incorrect ["urad"] values (generated with the incorrect [DAC ct / "urad"] gain, G). The method for doing so is revealed through a quick algebra exercise,
    slider offset [urad] * H [DAC ct / urad] = DAC output [DAC ct]                 (1)
    bad slider offset ["urad"] * G [DAC ct / "urad"] = DAC output' [DAC ct']       (2)

    want
    DAC output [DAC ct] = DAC output' [DAC ct'],

    so
    slider offset [urad] * H [DAC ct / urad] = bad slider offser ["urad"] * G [DAC ct / "urad"]
    
    slider offset [urad] = bad slider offset ["urad"] * G [DAC ct / "urad"] / H [DAC ct / urad]     (3)
or, in words, multiply the old bad offsets by the ratio of (old gain / new gain) to get the new well-calibrated offsets.

In addition to calibrating the offsets, I also updated the visual representation of the available range on the MEDM screen. In this case, given that the HAUX are driven with 18-bit DACs, then each OSEM can drive 2^17 - counts. The EUL2OSEM matrix elements for conversion of pitch and yaw to each of the four OSEMs is +/-8.594 [um / urad], so that means that a Euler basis pitch and yaw [DAC ct] drive cannot exceed 2^17 / 8.594 = 15251 [Eul DAC ct]. After dividing by the above calibration for each, that takes the slider limits to (roughly, taking the lowest range -- IM3 -- as the limiter) +/- 1200 [urad] for pitch and +/- 2200 [urad] for yaw.

2024-04-16_H1SUSIM_AlignmentSlider_Recalibation_OPTICALIGN_Screens_after_correctunits.png shows the final product after all of these changes,
    - the new slider gain values,
    - the new slider offset values to reproduce the same DAC output, and
    - the updated range of values.

Operators be aware: the amount of nudging you need to do on IM4 during initial alignment will need to change as a result of this re-calibration. Using the same math as Eq. (3) above, [1, 10, 100, 1000] "urad" nudges now are actually, roughly [0.05, 0.5, 5. , 50] "urad" nudges.

2024-04-16_H1SUSIM_AlignmentSlider_Recalibration_Notes.txt are my very rough notes from the morning's work, including all mistakes, as well as ipython code snippets to take actions, store information, and make plots. Could be cleaner for future users, but alas.
Images attached to this report
Non-image files attached to this report
Comments related to this report
jeffrey.kissel@LIGO.ORG - 14:17, Tuesday 16 April 2024 (77214)
As a result of this work, I have accepted the new OPTICALIGN slider calibration gains, which are "monitored" in the h1susim_safe.snap.
As is tradition, the OPTICALIGN slider offsets are *NOT* monitored, so I made sure to go to the "full table" and force accept the offsets as well.

Finally, I've also committed the update to the 
    /opt/rtcds/userapps/release/sus/common/medm/haux/
        SUS_CUST_HAUX_M1_OPTICALIGN.adl
because these values (a) are not too terribly different than the previous +/- 2500 ["urad"] range that was there, and (b) I expect the L1 HAUX to have similar calibration, when they get to it.
H1 General (SQZ)
thomas.shaffer@LIGO.ORG - posted 12:25, Tuesday 16 April 2024 (77210)
LVEA Swept

Swept the LVEA at the end of maintenance. All of the usual checks on  T1500386 were done, the only thing I noticed was that there were some cables plugged into the SQZT0 table that were not connect to anything else. These are for the hymodyne delta DC, PD1 DC, and PD2 DC according to their labels.

The items mentioned from last week's sweep (alog77058) are still there - pem setups, FARO, etc. as expected for the near future.

LHO General
ibrahim.abouelfettouh@LIGO.ORG - posted 12:02, Tuesday 16 April 2024 (77209)
OPS Day Midshift Update

IFO is in IDLE for TUESDAY MAINTENANCE

Maintenance work is wrapping up, Camilla is detransitioning our LVEA Hazard state and we will being locking as soon as maintenance activities end.

H1 AOS
david.barker@LIGO.ORG - posted 11:05, Tuesday 16 April 2024 (77208)
CAL HASH channels added to CDS SDF

New channels have been added to the CDS SDF, and h1cdssdf was restarted on h1ecatmon0. Current values have been accepted and are being monitored.

H1 CDS
david.barker@LIGO.ORG - posted 10:39, Tuesday 16 April 2024 - last comment - 12:56, Wednesday 17 April 2024(77207)
h1calcs, cal_hash_ioc and DAQ restarts

WP11812

Jamie, Jonathan, Erik, Dave:

The two CAL HASH channels (H1:CAL-CALIB_REPORT_HASH_INT and H1:CAL-CALIB_REPORT_ID_INT) were moved from the h1calcs model, where they were being acquired as single-precision floats, to a new custom EPICS IOC called cal_hash_ioc, where they are acquired as signed 32bit integers.

The h1calcs.mdl model was modified to remove the EPICS-INPUT parts for these channels. The model was then restarted.

The IOC, which was being tested with H3 channels, was modifed and rstarted to serve the H1 channels as integers.

The EDC was modified to add H1EPICS_CALHASH.ini to its master list. This added 5 channels the the DAQ, the two hash channels and three IOC status channels.

The EDC was restarted, followed in short order by a DAQ restart.

Comments related to this report
david.barker@LIGO.ORG - 13:31, Tuesday 16 April 2024 (77212)

Tue16Apr2024         
LOC TIME HOSTNAME     MODEL/REBOOT 
10:04:52 h1oaf0       h1calcs <<< Model change to remove channels
10:07:51 h1susauxb123 h1edc[DAQ]  <<< EDC has the new channels
10:08:43 h1daqdc0     [DAQ] <<< 0-leg restart, no issues
10:08:55 h1daqfw0     [DAQ]
10:08:55 h1daqnds0    [DAQ]
10:08:55 h1daqtw0     [DAQ] 
10:09:03 h1daqgds0    [DAQ]
10:11:55 h1daqdc1     [DAQ] <<< 1-leg restart, no issues
10:12:06 h1daqfw1     [DAQ]
10:12:07 h1daqtw1     [DAQ]
10:12:08 h1daqnds1    [DAQ] 
10:12:16 h1daqgds1    [DAQ] 

oli.patane@LIGO.ORG - 16:16, Tuesday 16 April 2024 (77222)
Images attached to this comment
louis.dartez@LIGO.ORG - 12:56, Wednesday 17 April 2024 (77250)
N.B. that changes to the channels H1:CAL-CALIB_REPORT_HASH_INT and H1:CAL-CALIB_REPORT_ID_INT will appear on the CDS SDF screen, *not the H1CALCS* screen. They get automatically re-populated each time pydarm export is used to update the calibration in the control room (which should be considered to happen atomically with GDS restarts). So, when updating the calibration both the H1CALCS and the H1CDS SDF screens need to be checked.
LHO VE
david.barker@LIGO.ORG - posted 10:21, Tuesday 16 April 2024 (77206)
Tue CP1 Fill

Tue Apr 16 10:12:16 2024 INFO: Fill completed in 12min 11secs

Jordan confirmed a good fill curbside. Plot looks strange because the DAQ was being restarted during the fill.

Images attached to this report
H1 IOO
sheila.dwyer@LIGO.ORG - posted 10:08, Tuesday 16 April 2024 (77205)
IM4 QPD centered with pico

I used the IM4 pico to center the beam on the QPD with 2W into the mode cleaner this morning (screenshot attached). We had some shifts of input alignment during the vent and difficulty recovering (see 76359 76291).  Now our range is 165 and locking seems reliable, so we are resetting the IM4 QPD to zero here so that we can use this as a reference in the future.  LLO tells us that they realign IM3 to this QPD every few months.

This increased the sum of IM4.  Since this sum is used to normalize our PRG channel, this will need a recalibration.

Images attached to this report
H1 ISC
gabriele.vajente@LIGO.ORG - posted 08:25, Tuesday 16 April 2024 - last comment - 09:40, Wednesday 17 April 2024(77201)
Why is it so hard to fit a good SRCL FF?

Lately it's been very difficult to fit an efficient SRCL feedforward filter, as reported many times by Camilla et al. (76993). Here I'm trying to figure out why. Spoiler alert: I don't have an answer yet.

The main problem with the SRCL FF filter (see first plot), is that the transfer function to fit has a large phase rotation, that looks basically like a phase advance (the opposite of a delay) of about 2 ms. This is very large, and being an advance, it can't be realized in a precise and simple wasy digitally.

First observation: we can fit a pretty good SRCL FF if we allow for unstable poles, i.e. poles with positive real parts (see second plot) Of course this is not something that can be implemented in the real time system. The fit ends up having a unstable complex pole at about 420 Hz and about 5 Hz. I have no intepretation for the origin of those poles, and they might very well be only a way to reproduce a phase advance (think of the Padé approximation for phase delays).

So the question is: what is the origin of this large phase rotation? It's not seen at LLO, for example see 70548

Second observation: this phase advance appeared after we switched the LSC FF from ETMX (full chain) to ETMY PUM. The third plot compares the MICH and SRCL feedforward to be fit in two cases: an old measurement when the FF was going to ETMX, and a more recent measurement with the FF going to ETMY PUM only. For both MICH and SRCL the orange traces (FF to ETMY) show a phase advanced with respect to the blue traces (FF to ETMX). For some reasons I don't fully understand, this rotation is more problematic for SRCL than for MICH, although fitting MICH has also been more difficult and the MICH FF is relevant at lower frequencies than SRCL, so maybe the phase advanced isn't that problematic.

Looking at the measurement of the MICHFF to DARM and SRCLFF to DARM, one can see that there seems to be an additional phase delay in the FF path through ETMY PUM with respect to the FF path through ETMX full chain. Since this transfer function is at the denominator when computing the ratio SRCLtoDARM/SRCLFFtoDARM that gives use the LSC FF to fit, this seems to explain the additional phase advance we observe.

The ETMY PUM L2 lock filter bank contains a "QPrime" filter module that compensates partially the additional 1/f^2 due to the actuation from L2 instead of L3. This filter however doesn't seem able to explain this additonal phase delay.

I'm now suspicious that there might be something wrong or mistuned in the ETMY L2 drive, maybe a whitening filter missing or not functioning properly or not properly compensated?

It would be worth doing a quick test in the next commissioning time with full IFO locked: inject some white noise on ETMX L2 L and ETMY L2 L and comapre the two transfer functions to DARM. In theory they should be equal, except for a sign difference. If they're not, then there must be something wrong with ETMY, since we're using ETMX L2 to lock without issues.

Images attached to this report
Comments related to this report
gabriele.vajente@LIGO.ORG - 14:35, Tuesday 16 April 2024 (77215)

This is a comparison of the LHO LSC FF and LLO LSC FF. The difference in the absolute scale might eb due to normalizations, but the SRCL FF does not show the large phase advanced visible at LHO

Images attached to this comment
gabriele.vajente@LIGO.ORG - 07:28, Wednesday 17 April 2024 (77236)

Maybe mistery solved...

The ETMY L2 DRIVEALIGN L filter bank has a "L2L3LP" filter engaged, whiel the corresponding ETMX L2 DRIVEALIGN L filter bank does not. This filter seems to be the origin of the phase rotation. At least it explains part of the phase rotation.

Anybody knows why this filter is engaged in ETMY? Should be turn it off and retune the LSC FF?

We should turn this filter off when we engage the FF (assuming it's needed some time during lock acquistion, to be checked) and retune the LSC FF. When we do that, we should reduce the excitation amplitude and reshape it, taking into account the filter we turned off.

Images attached to this comment
camilla.compton@LIGO.ORG - 09:40, Wednesday 17 April 2024 (77240)

Gabriele, Camilla. This ETMY_L2_DRIVEALIGN_L2L filter is used while locking in TRANSISTION_FROM_ETMX (when we control DARM on EY)  and then again when the LSC FF is turned on in LOW_NOISE_LENGTH_CONTORL, plot attached. To not need to change the sensitive TRANSISTION_FROM_ETMX state we should turn the filter off with ISC_LOCK  before turning the LSC FF's on. Will need to retune the LSC FF's (from scratch starting with both MICH and SRCL FF off, and adjusting the excitation to take this L2L3LP filter into account).

Images attached to this comment
LHO General
ibrahim.abouelfettouh@LIGO.ORG - posted 08:14, Tuesday 16 April 2024 (77202)
OPS Day Shift Start

TITLE: 04/16 Day Shift: 15:00-23:00 UTC (08:00-16:00 PST), all times posted in UTC
STATE of H1: Preventive Maintenance
OUTGOING OPERATOR: Tony
CURRENT ENVIRONMENT:
    SEI_ENV state: CALM
    Wind: 12mph Gusts, 7mph 5min avg
    Primary useism: 0.04 μm/s
    Secondary useism: 0.13 μm/s
QUICK SUMMARY:

IFO was unlocked upon entry - now staying down for Planned Tuesday Maintenance

H1 General
thomas.shaffer@LIGO.ORG - posted 07:23, Tuesday 16 April 2024 - last comment - 07:42, Tuesday 16 April 2024(77199)
OWL Operator intervention

A lock loss this morning from unknown reasons had the IFO running an initial alignment after it struggled to lock in the main locking. I was alerted after it timed out locking green in initial alignment. By the time I logged in and accidentally restarted green locking, increase flashed had fixed it and it have moved on in the initial alignment sequence. I'll let it finish with the hopes that it will help maintance recover slightly quicker, but not start locking again since maintenance is about to start.

I'm not sure why green was struggling so much this morning, I'll have to dive deeper into it later it. It doesn't normally time out if it can lock this easily.

Comments related to this report
thomas.shaffer@LIGO.ORG - 07:42, Tuesday 16 April 2024 (77200)

SRC wouldn't lock, but flashes looked good. Somehow, it looks like the changes I made switching from POP_A to AS_C got reverted (<a href="https://alog.ligo-wa.caltech.edu/aLOG/index.php?callRep=77113">alog77113</a>). As soon as I switched back to using AS_C with 0.005 and 0.004 thresholds it locked right up.

I'll also have to check on why this was reverted when I get in.

H1 CDS
erik.vonreis@LIGO.ORG - posted 07:01, Tuesday 16 April 2024 (77198)
Workstations updated

Workstations were updated and rebooted.  This was an os package update.  Conda packages were not updated.

LHO General
corey.gray@LIGO.ORG - posted 16:10, Monday 15 April 2024 - last comment - 08:37, Tuesday 16 April 2024(77185)
Mon EVE Ops Transition

TITLE: 04/15 Eve Shift: 23:00-07:00 UTC (16:00-00:00 PST), all times posted in UTC
STATE of H1: Observing at 154Mpc
OUTGOING OPERATOR: Ryan C
CURRENT ENVIRONMENT:
    SEI_ENV state: SEISMON_ALERT
    Wind: 10mph Gusts, 5mph 5min avg
    Primary useism: 0.04 μm/s
    Secondary useism: 0.15 μm/s
QUICK SUMMARY:

Nicely Observing H1 handed off by RyanC.  He mentioned, same issue with SRC for alignment and needing to skip it (that's atleast 3x in a row).  He also mentioned a drop out of Observing due to SQZ_FC as observed last night (and tweaks Naoki made for this).  Currently, waiting for a M5.9 S.Korea earthquake to roll through with its R-wave in 10min.

Comments related to this report
ryan.crouch@LIGO.ORG - 08:37, Tuesday 16 April 2024 (77203)

Forgot my log                                                                                                                                                                                                                                                                                                                                                                                                                                                                                    

Start Time System Name Location Lazer_Haz Task Time End
15:20 FAC Chris FCES N Move snorkle lift to FCES 16:20
16:03 FAC Kim MidX n Tech clean 17:03
18:04 EE Fil MidY n Parts search 19:04
17:10 CAL Francisco PCAL lab LOCAL PCAL work 20:10
18:18 FAC Tyler AHU N AHU1 fan 18:35
Displaying reports 9101-9120 of 84064.Go to page Start 452 453 454 455 456 457 458 459 460 End