Displaying reports 35201-35220 of 89220.Go to page Start 1757 1758 1759 1760 1761 1762 1763 1764 1765 End
Reports until 10:04, Tuesday 17 March 2020
H1 CDS (SEI)
david.barker@LIGO.ORG - posted 10:04, Tuesday 17 March 2020 (55647)
Latest HEPI and HAM-ISI models installed

WP8554 senscor addition to HEPI and ISI models

Jim, Dave:

The SEI front end models were restarted in the following order:

2020_03_17 09:08 h1hpietmx
2020_03_17 09:08 h1hpietmy
2020_03_17 09:10 h1hpiham1
2020_03_17 09:10 h1hpiham2
2020_03_17 09:10 h1hpiham3
2020_03_17 09:10 h1isiham2
2020_03_17 09:11 h1hpiham4
2020_03_17 09:11 h1isiham3
2020_03_17 09:13 h1hpiham5
2020_03_17 09:13 h1hpiham6
2020_03_17 09:13 h1isiham4
2020_03_17 09:13 h1isiham5
2020_03_17 09:15 h1hpibs
2020_03_17 09:15 h1hpiitmy
2020_03_17 09:15 h1isiham6
2020_03_17 09:16 h1hpiitmx
In some cases the filter module file was slightly modified by a reordering of the header modules list (no actual filter change).

No DAQ restart was necessary.

H1 PSL
jason.oberling@LIGO.ORG - posted 09:25, Tuesday 17 March 2020 (55646)
PSL Power Watchdogs Reset (FAMIS 10754)

I reset both PSL power watchdogs at 16:21 UTC (9:21 PDT).  This completes FAMIS 10754.

H1 General
jeffrey.bartlett@LIGO.ORG - posted 08:14, Tuesday 17 March 2020 (55645)
Ops Day Shift Transition
Ops Shift Transition: 03/17/2020, Day Shift 15:00 – 23:00 (08:00 -16:00) - UTC (PT)
State of H1: Unlocked for maintenance
Intent Bit: Maintenance
Weather:  Skies are mostly clear, temps are in the lower 20s. The winds are Light Breeze.     
Primary 0.03 – 0.1Hz: 0.01um/s
Secondary 0.1 – 0.3Hz: 0.2um/s
Outgoing Operator: Corey
Quick Summary: The IFO is unlocked for Tuesday maintenance
H1 General
corey.gray@LIGO.ORG - posted 05:53, Tuesday 17 March 2020 - last comment - 06:35, Tuesday 17 March 2020(55643)
12:12utc (5:12amPT) Lockloss & IR Not Found

Initial NOTES:

Comments related to this report
corey.gray@LIGO.ORG - 06:35, Tuesday 17 March 2020 (55644)

13:29 took H1 back to Observing for tne next 80min before Maintenance.  (no intervention needed for the two lock attempts)

And since it's close to Maintenance, running the Revert script for my alerts.

H1 General
corey.gray@LIGO.ORG - posted 02:41, Tuesday 17 March 2020 (55640)
9:41utc (2:41amPT) H1 Relocking Notes

SUMMARY of H1 locking/recovery after lockloss:

H1 General
corey.gray@LIGO.ORG - posted 01:24, Tuesday 17 March 2020 - last comment - 02:05, Tuesday 17 March 2020(55641)
8:12utc (1:12amPT) Running Initial Alignment

H1 was having issues at CHECK MICH FRINGES and not locking PRMI.

8:12 Began an Initial Alignment.

Comments related to this report
corey.gray@LIGO.ORG - 02:05, Tuesday 17 March 2020 (55642)

1st locking attempt after Initial Alignment had lockloss at ENGAGE ASC FOR FULL IFO (looks like POP18 & PR Gain both drift down before lockloss; see attached screenshot).

NOTE:  There was a 5.7 Chilean EQ inbound, but don't really see any reason this was the cause for the lockloss.

On to 2nd lock...

Images attached to this comment
H1 General (GRD)
camilla.compton@LIGO.ORG - posted 00:06, Tuesday 17 March 2020 (55636)
Shift Summary - Eve

TITLE: 03/17 Eve Shift: 23:00-07:00 UTC (16:00-00:00 PST), all times posted in UTC
STATE of H1: Lock Acquisition
INCOMING OPERATOR: Corey
SHIFT SUMMARY: Lost lock, ending a 31h15 lock stretch
LOG:

H1 General
camilla.compton@LIGO.ORG - posted 23:13, Monday 16 March 2020 (55639)
H1 Lockloss 06:06:47 UTC
Very fast unknown locklosses. Environment all fine.
H1 General
camilla.compton@LIGO.ORG - posted 20:11, Monday 16 March 2020 (55637)
Mid Shift Summary

Locked 28h20 at 120Mpc. Environment fine, microseism has crept up over the last 12 hours but still below the 90th percentile.

H1 TCS
camilla.compton@LIGO.ORG - posted 16:54, Monday 16 March 2020 (55633)
TCS Chiller Water Level Top Off - Weekly (FAMIS #11535)
FAMIS 11535
TCSx Chiller:  Had level of 29.5 cm.  Added 120mL for 30.0cm.
    We changed this filter 2020-02-25 (alog 55288) and it already has a slight green tinge. During the change we noted that the metal flow difuser was green which is proably causing the new filter to turn green. We are ordering replacements of the flow diffusers to hopefully solve.
TCSy Chiller:  Had level of 9.4 cm.  Added 50mL for 10.1cm.
H1 General
camilla.compton@LIGO.ORG - posted 16:03, Monday 16 March 2020 (55631)
Shift transition to Eve

TITLE: 03/16 Eve Shift: 23:00-07:00 UTC (16:00-00:00 PST), all times posted in UTC
STATE of H1: Observing at 119Mpc
OUTGOING OPERATOR: Travis
CURRENT ENVIRONMENT:
    SEI_CONF state: WINDY
    Wind: 14mph Gusts, 10mph 5min avg
    Primary useism: 0.04 μm/s
    Secondary useism: 0.33 μm/s
QUICK SUMMARY: Locked 24 hours 15

H1 General
travis.sadecki@LIGO.ORG - posted 16:03, Monday 16 March 2020 (55619)
Ops Day Shift Summary

TITLE: 03/16 Day Shift: 15:00-23:00 UTC (08:00-16:00 PST), all times posted in UTC
STATE of H1: Observing at 119Mpc
INCOMING OPERATOR: Camilla
SHIFT SUMMARY:  One Superevent candidate.  Otherwise, no issues to report.  Lock is 24+ hours old.
LOG:

18:30 Out of Observe, JeffK starting CAL injections

20:02 Robert to EY to setup equipment

20:09 Kyle to MX

20:15 JeffK done with CAL, Robert starting PEM work at EY

21:12 Gerardo to MY to pick up equipment

21:18 Back to Observing.  Robert done at EY.  WAP turned off.

21:29 Gerardo back

21:54 Robert to EX

22:04 Robert recalled from EX due to Superevent candidate, on his way back

 

H1 SUS (CAL)
rahul.kumar@LIGO.ORG - posted 15:23, Monday 16 March 2020 (55627)
several modes on the ETMX rung-up during CAL sweeps

Today, during the CAL sweeps (ISC lock state 700) several modes (2, 3, 4, 6, 7, 8, 9 in the 1st harmonic and 12, 13, 14, 16, 17 in the 2nd harmonic) ) on the ETMX were rung up by 2-3 orders of magnitude in the monitor levels. During this time Guardian did not switch-off damping for the rung-up modes and this is due to the settings made last Friday. The rung-up modes rose to their peak amplitude while the CAL sweeps lasted and then Guardian was successfully able to damp each one of them. 

I am attaching ndscope plots for the 1st and 2nd harmonic and the DARM spectrum from 3 different time today (a. before CAL sweeps started - which shows nominal noise floor, b. During CAL sweep: when the modes are rising, c. after CAL sweep when Guardian successfully damps them).

 

Images attached to this report
H1 AOS (AOS, SUS)
corey.gray@LIGO.ORG - posted 14:44, Monday 16 March 2020 (55630)
Optical Lever 7-Day Trends (FAMIS #11261)

Attached are trends for oplevs.

NOTE:

Images attached to this report
H1 CAL
jeffrey.kissel@LIGO.ORG - posted 11:39, Monday 16 March 2020 - last comment - 15:41, Friday 31 July 2020(55620)
OMC Whitening Change: On-going Now. Some Calibration Change at the 1.0-1.5%
J. Kissel, J. Driggers

More to come, but OMC Whitening Configuration change (using 1 whitening stage instead of 2 whitening stages and a low pass) is in testing now.

Quick answer from PCAL to DELTAL EXTERNAL broaband TF shows ~1.0-1.5% frequency dependent addition systematic error with the new configuration.
Magenta is nominal configuration (2 whitening stages and a low pass), and red is test configuration.

Sweeping now...
Images attached to this report
Comments related to this report
jenne.driggers@LIGO.ORG - 12:35, Monday 16 March 2020 (55621)

I have accepted in SDF the differences that this caused for the digital and analog filters (see screenshots of sdf files).

I have also modified the ISC_LOCK and OMC_LOCK guardians such that when we next acquire lock, it should come back to this state of only 1 stage of analog filtering.

  • ISC_LOCK I just removed the edges that were connected to the OMC_WHITENING state near the end of the acquisition sequence.  Lownoise_length_control now goes directly to Reduce_rf9_modulations_depth.  This prevents ISC_LOCK from asking the OMC guardian to add the 3rd stage of whitening.  Nothing else happened in this state.
  • OMC_LOCK I commented out the lines in OMC_LSC_on that would have turned on the 2nd stage of filtering.  Note that in Prep_omc_scan all 3 stages of whitening are turned off, so the OMC should now only have 1 stage of analog filtering.
Images attached to this comment
jeffrey.kissel@LIGO.ORG - 13:23, Monday 16 March 2020 (55623)CAL, DetChar
Calibration measurement suite sweeps are complete, and we are back in nominal low noise, but Robert has taken over the IFO for commissioning. 

We are remaining in this 1 stage of whitening only configuration.

We have resolved that it is not prudent to change the compensation filters, and/or update the calibration model parameter set, and we'll therefore just live with this increased systematic error in the low latency h(t). Eventually, after the systematic error is well quantified, we will create a new model parameter set, and re-calibrate the data -- starting at the next observation ready segment today.

I'll post the official time as to when we've gone back in to observation ready, so as to clearly define the first observation ready segment with this new change.
jeffrey.kissel@LIGO.ORG - 14:23, Monday 16 March 2020 (55629)DetChar, ISC, OpsInfo
The first observation ready segment that includes the above described OMC whitening chassis filter configuration change started at Mar 16 2020 21:18:54 UTC (GPS time 1268428752)
jenne.driggers@LIGO.ORG - 16:44, Monday 16 March 2020 (55632)

Not that there is anything profound here, but I caught a glitch.  This is the first one that I've caught to grab a screenshot of after our change this morning of the OMC DCPD whitening filter configuration. 

Note to self: compare the _OUT_DQ of this glitch with other glitches in the old nominal config that I have screenshots of, to (try to) see if these glitches were attenuated due to the new analog configuration. 

Images attached to this comment
jenne.driggers@LIGO.ORG - 17:26, Monday 16 March 2020 (55635)DetChar

The summary pages are reporting a significantly reduced range, but I'm not totally sure why. 

In the attachment, I've plotted ~an hour of data each for observing times this morning before we changed the whitening configuration, and for an observing segment after we made the change.  This is H1:GDS-CALIB_STRAIN, so has time dependent correction factors applied (although, as Jeff points out earlier in this thread those won't fully account for the small frequency dependent change that we've acquired).

Blue is an old nominal (3 analog filters) time, starting at 16 Mar 2020 16:24:40 UTC.  Orange is the new nominal (1 analog filter), starting at 16 Mar 2020 22:19:30 UTC.  The darker lines are the 50th %-ile, and the shaded regions are the 5th and 95th %-iles.  I can't tell much of a difference by eye.  Also, when I calculate the range from these median spectra, I get less than a 0.5 Mpc difference.  So, I'm not sure why the GDS range on the summary pages is so different now than it was this morning. 

Images attached to this comment
jeffrey.kissel@LIGO.ORG - 15:41, Friday 31 July 2020 (56347)
I've used measurements of this OMC whitening chassis from (Sunday!) 2019-03-03 to predict the systematic error that transpired as a result of this configuration change. See further discussion in "PART II" of G2000527.

Making a *very* long story short, 
    (a) the systematic error incurred on the final DCS C01 calibration amounts to (a frequency dependent, but at maximum) 0.5% and 0.25 deg error at 100 Hz and 50 Hz, respectively.
    (b) the error arises from 
        - poor modeling of the super-Nyquist response of this chassis in the calibration pipeline, 
        - previously poor understanding of the circuit resulting in a poorly informed fit of the measurements, and finally 
        - the original data set only was taken down to 5 Hz, where the chassis (namely the first and third filters, which are the whitening stages) has response at 1 Hz and thus *any* fit (be it Stefan's original fit to update the compensation filters, or Lilli's fit for super-Nyquist poles) is fundamentally limited by the data.

Attached is a comparison of 
   - the ratio between the 2020-03-09 (pre-change) and 2020-03-16 (post-change) broad-band PCAL injections -- and thus the *measured* systematic error incurred by the change, and
   - the estimated systematic error derived from a re-fit to the original data.
Again, for further explanation of how this modeled error estimate was derived, see "PART II" of G2000527.

The script the accompanies the analysis for G2000527, from which all plots come, lives in 
    /ligo/svncommon/CalSVN/aligocalibration/trunk/Common/Electronics/H1/Scripts/
        fit_OMCDCPDWhiteningChassis_20190304_forG2000527.py

Non-image files attached to this comment
H1 SEI (GRD)
jim.warner@LIGO.ORG - posted 11:09, Monday 16 March 2020 - last comment - 17:14, Monday 16 March 2020(55618)
More tests of SEI_ENV earthquake transitions

Cheryl noted last night that the seismic system transitioned to earthquake last night without warning. This actually happened twice last night, I think the two attached earthquakes from USGS were the culprits. They were far enough away that we should have gotten some warning (5600 km, the closest seismon will give us early warning for is about 2000 km), but maybe the fact they were out in the middle of the ocean delayed the USGS reports. The later one is still on seismon, and gets a deceptive eq response "score", falling well into the blue region, so a good reminder to be kind of skeptical about what the plot tells you. Still, SEI_ENV caught both earthquakes and transitioned properly, and we stayed locked for both earthquakes.

Second attached plot shows SEI_ENV (in blue) jumping from CALM (index 10) to EARTHQUAKE (index 20), as both earthquakes cross 1000 nm/s on peakmon (in yellow). SEI_CONF (green) goes from WINDY to EARTH_QUAKE both times, in the IFO stayed locked for both earthquakes. It's possible that we could have ridden both of these earthquakes out without doing anything, but these earthquakes were both on the top end of the kind of earthquakes we were able to ride out for O2 before we had an actual earthquake control scheme. Both of these earthquakes would have been a challenge for a person to first realize what was happening, then make the decision to switch the seismic system before the earthquakes had come and gone.

Images attached to this report
Comments related to this report
camilla.compton@LIGO.ORG - 17:14, Monday 16 March 2020 (55634)

Great news! Well done SEI_ENV state!

H1 TCS
camilla.compton@LIGO.ORG - posted 05:53, Saturday 08 February 2020 - last comment - 14:40, Friday 03 December 2021(54980)
TCSy CO2 Laser has only Kicked us out of Observing Twice since Chiller Swap
Following on from FRS 13095.  Before October we were pushed out of Observing a few times by the TCSy CO2 laser loosing lock. TCSY chiller was swapped 2019-09-18 alog 51996. Flow meter was swapped 2019-10-10 alog 52406.
 
By comparing H1:GRD-TCS_ITMY_CO2_STATE_N with our observation bit and checking logs, I have found only 2 cases since the swap (5months ago) where the TCSy CO2 laser has pushed us out of observing by loosing lock (2019-09-29 23:57 UTC and 2019-12-05 05:41 UTC). The first time being before the flow meter was swapped.
There were 15 times it pushed us out of observing from July 1st to the chiller swap (all between 2019-07-10 and 2019-08-31). Unless something else changed at the end of August I think we can confirm that the original chiller or new flow meter solved our problem.
Attached is the H1:GRD-TCS_ITMY_CO2_STATE_N from May 2019 to now (t1 line = chiller swap. t2 line = flow meter swap). The C02 laser now looses lock to search for a new lock point less regularly and seems to be able to wait until H1 is unlocked. 
Images attached to this report
Comments related to this report
camilla.compton@LIGO.ORG - 22:14, Monday 16 March 2020 (55638)

Happened a third time: 2020-03-17 05:04:09 UTC. Still much reduced since the chiller swap.

camilla.compton@LIGO.ORG - 11:28, Tuesday 02 November 2021 (60493)CDS

Looked back at this after TJ suggested we should check that both chillers are keeping constant temperatures and flow rates. Temperatures in ITMX and ITMY cCO2 chillers seems to be stable. See plot over last 2 years here. As the laser hasn't ben on recently we cannot check how stable it is.

Flow rate reported by ITMX chiller seems to regularly drop from the nominal 3.8 to 2 GPM to up to 10 times an hour. However these drops only last one data point which doesn't effect the laser controller safety controls. See zoomed plot here. The chiller has been like for the past 3.5 years (as far back as I can easily see in EPICS).

2021/09/21 Tuesday 17:30UTC Both ITMX and ITMY chiller temperatures decreased from 22 degC to 19.5 degC. The set point is still at 22degC but the channel H1:TCS-{ITMY/ITMX}_CO2_CHILLER_OUT_GAIN_OUT16 dropped to zero Simulink for h1tcscs . Ndscope trace here. This apears to be the day the h1tcscs model was installed on h1oaf0 - see alog 60002. Tagging cds.

Images attached to this comment
aidan.brooks@LIGO.ORG - 10:46, Wednesday 03 November 2021 (60511)

ECR for upgrading the CO2 controller is here: https://dcc.ligo.org/E1600312

Latest concept for redesigning CO2 controller is attached. Project is stalled right now due to lack of manpower.

 

Non-image files attached to this comment
camilla.compton@LIGO.ORG - 12:59, Tuesday 16 November 2021 (60663)

Daniel fixed this setpoint problem by finding the filters had been removed (see alog 60660).

Once the filters were added back in ~19.15UTC 11/16/2021, the filters seems to be maxed out. Daniel turned off the laser power servo loop (sitemap > TCS > CO2{X/Y} > LASER > ON/OFF for PZT_SERVO_GAIN) and they behaved as expected. These values are not recorded in SDF. It doesn't make sence for the chillers to be tied to the laser when the laser is off so will investigate if the matrix changed. 

 

camilla.compton@LIGO.ORG - 10:07, Friday 03 December 2021 (60842)

The PZT_SERVO_GAIN OUTPUT we turned OFF 2021/11/16 20UTC must have not being svn saved and turned back on on 2021/11/17 22UTC. See attached trend.

The design is to stabilize the laser PZT error signal by controlling the chiller temperature (E1300233p20). When the laser is off this seems to break down and change the have the setpoint given to the chiller (CHILLER_SETPT1) far from the ~20deg setpoint offset H1:TCS-ITM{}_CO2_CHILLER_SET_POINT_OFFSET (seen in TCS CO2 LASER screen). See table below.

TJ and I are looking into these settings. Maybe the matrix gain values or PZT gains are incorrect or the loop should be switched off when the laser is off.

Current values CHILLER_SET_POINT_OFFSET PZT_SERVO_GAIN CHILLER_SETPT1 (setpoint sent to chiller) 
CO2X 20.6 -111 16.6*
CO2Y 20.5 55 22.4

*Documentation states it's important not to let the chillers be +/- 5deg from 20deg otherwise there may be condensation formed in the laser. The chillers have limits to shut off if they get outside this range but only compared to the CHILLER_SETPT1 value. 

Images attached to this comment
camilla.compton@LIGO.ORG - 14:40, Friday 03 December 2021 (60850)

The PZT_SERVO_GAIN OUTPUT is turned off in the CO2 Guardian's DOWN state (well done guardian), running DOWN fixed the problem.

Now the lasers think the set point given to the chillers is 20deg but the chillers are receiving set point request of 22degC. So another issue to solve. 

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