Displaying reports 48301-48320 of 83227.Go to page Start 2412 2413 2414 2415 2416 2417 2418 2419 2420 End
Reports until 12:29, Monday 01 May 2017
LHO VE
david.barker@LIGO.ORG - posted 12:29, Monday 01 May 2017 - last comment - 13:12, Monday 01 May 2017(35941)
CP3, CP4 manual running of Autofill 2017_05_01

(manual run of the scripts, crontabs were not operational)

Starting CP3 fill. LLCV enabled. LLCV set to manual control. LLCV set to 50% open. Fill completed in 40 seconds. TC B did not register fill. LLCV set back to 18.0% open.

Starting CP4 fill. LLCV enabled. LLCV set to manual control. LLCV set to 70% open. Fill completed in 630 seconds. TC A did not register fill. LLCV set back to 42.0% open.

Images attached to this report
Comments related to this report
david.barker@LIGO.ORG - 12:30, Monday 01 May 2017 (35942)

I've reconfigured the crontab for user vacuum on vacuum1, autofill should run automatically on Wednesday.

chandra.romel@LIGO.ORG - 13:12, Monday 01 May 2017 (35943)

Increased CP4 to 43% open.

LHO VE
logbook/robot/script0.cds.ligo-wa.caltech.edu@LIGO.ORG - posted 12:10, Monday 01 May 2017 (35940)
CP3, CP4 Autofill 2017_05_01
CP3 log file DOES NOT exist!
CP4 log file DOES NOT exist!
Images attached to this report
H1 CDS (VE)
david.barker@LIGO.ORG - posted 12:06, Monday 01 May 2017 (35939)
autofill of CP3/CP4 did not run today, re-installing code

The regular Monday 11am LN2 auto-overfill of CP3 and CP4 did not run this morning, presumably related to OS updates on Friday. Will run it manually for today.

H1 SEI
hugh.radkins@LIGO.ORG - posted 11:51, Monday 01 May 2017 (35938)
LHO LVEA Tilt Studies at Roam3--With wind from NW (+X)

Having moved the STS2-C (HAM5) from Roam2 (near NE BSC8{H2 ITMY} chamber leg/SEI Pier) to Roam3 (~2/3 distance to BSC4 {H2 BS}) on Friday during EQ downtime, some weekend wind has given a good comparison to examine.  Reference Traces are from the quiet period (0805utc May 1) and the current traces are  during the windy time beginning at 2300utc April 30.

See the first plot attached showing the wind velocity at the corner station.  180 degrees on the anemometer is pretty much right out of the +X to -X direction, i.e., no Y component and this may likely explain why the Y dof comparison of the ASD is nearly identical.  The coherence shows stronger frequency dependence.  On the X dof, the STS2-C at Roam3 is certainly noisier than STS2-B at its home location and a bit more so during the higher wind.  However, comparing the same plots from aLog 35848, Roam3 is a much less noisier location than Roam2.  Caveat: the wind may be a bit quieter (few mph) and the direction is nearly opposite.  But, we might feel the largest deal is ~doubling the distance from the south wall.  Still, the North wall which is getting the direct impact of the wind here is much farther (at least 3 times farther) than the South wall which was getting the direct hit from the aLog 35848 wind storm.  On the Z dof comparisons, the low wind time equity extends to lower frequencies and during high wind that breaks down around 10 or 20mHz.

Conclusion, Roam3 is a better position than Roam2 location, at least for this wind direction but the STS2-B location remains best.  Need a good SW wind (from +Y) to really fill in some holes.

Images attached to this report
H1 CDS
david.barker@LIGO.ORG - posted 11:10, Monday 01 May 2017 - last comment - 15:18, Monday 01 May 2017(35937)
front end lock-up summary

We had two more lock ups over the weekend. Luckily they were on non-dolphined corner station machines (SUS-AUX) and I was able to work remotely with the operator on getting these machines reset via the front panel reset button.

Here is a summary of the lockups since Wednesday night:

h1susauxb123 Mon 11:24 01 mar 2017 UTC (04:24 PDT)
h1susauxh2 Sun 20:20 30 apr 2017 UTC (13:30 PDT)
h1susex Fri 12:43 28 apr 2017UTC (05:43 PDT)
h1seiex Thu 13:10 27 apr 2017 UTC (06:10 PDT)

 

Comments related to this report
david.barker@LIGO.ORG - 15:18, Monday 01 May 2017 (35946)

Extended table, and added recent h1seib2 lockup:

computer lock-up time (local) computer uptime at lockup timer reset date-time (local)
h1seib2 Mon 13:05 5/1 PDT 215 days Wed 22:07 4/26 PDT
h1susauxb123 Mon 04:24 5/1 PDT 215 days no data
h1susauxh2 Sun 13:30 4/30 PDT 214 days Wed 22:18 4/26 PDT
h1susex Fri 05:43 4/28 PDT 209 days Wed 23:34 4/26 PDT
h1seiex Thu 06:10 4/27 PDT 209 days Wed 21:53 4/26 PDT

 

H1 DCS (DCS)
gregory.mendell@LIGO.ORG - posted 11:02, Monday 01 May 2017 (35936)
Problem with DMT H1 lock segments ... fixed at LHO

John Zweizig has fixed the problem reported here,

https://alog.ligo-wa.caltech.edu/aLOG/index.php?callRep=35924

which was caused by the DMT RAID box running out of inodes.

John has fixed the problem by deleting older data to free inodes.

H1 General
edmond.merilh@LIGO.ORG - posted 08:09, Monday 01 May 2017 (35933)
Shift Transition - Day

TITLE: 05/01 Day Shift: 15:00-23:00 UTC (08:00-16:00 PST), all times posted in UTC
STATE of H1: Environment
OUTGOING OPERATOR: Jeff
CURRENT ENVIRONMENT:
    Wind: Calm
    Primary useism: EQ
    Secondary useism: EQ
QUICK SUMMARY: ops lazy script isn't doing transition (-t).

 

H1 General
jeffrey.bartlett@LIGO.ORG - posted 07:59, Monday 01 May 2017 (35932)
Ops Owl Shift Summary
Ops Shift Log: 05/01/2017, Owl Shift 07:00 – 15:00 (00:00 - 08:00) Time - UTC (PT)
State of H1: Unlocked       
Intent Bit: Commissioning/Earthquake
Support: Dave B.,
Incoming Operator: Ed

 

Shift Summary: Run A2L check script. Pitch is below reference, Yaw a bit elevated. Received GRB. Both sites in observing. Spoke with LLO. In one hour hold until 12:12 (05:12).

FE computer H1IOPSUSAUXB123 crashed. Spoke to Dave B. – Reset FE computer to recover.  Back into observing.

Received an EQ warning and shortly lost lock. USGS showing a Mag6.5 in Alaska. Both Primary and Secondary microseism are off the top of the charts. Tripped the WD on most SUS, all, ISIs, several HEIPs, and all four IMs. Have the IFO in DOWN until things settle down a bit. Have been resetting tripped WD as necessary. A dozen after socks in Alaska have been recorded. Primary and Secondary microseism are still above 1.0um/s.

As the seismic was ringing down tried relocking. After relocking ALS Green, hit with another Mag6.3 earthquake near Skagway Alaska. Seismic Primary and Secondary are off the top of the charts. Put the IFO back into DOWM and started resetting the SUS and SEI watchdogs.               

 

   Activity Log: Time - UTC (PT)
07:00 (00:00) Take over from Nutsinee
11:12 (04:12) GRB – Observe one hours hold
11:24 (04:24) Dropped out of Observing due to FE computer crash.
11:44 (04:44) Back in Observing after resetting H1IOPSUSAUXB123
12:35 (05:35) Lost lock – Mag6.5 Earthquake near Skagway, Alaska
15:00 (08:00) Turn over to Ed
H1 SEI
jeffrey.bartlett@LIGO.ORG - posted 07:00, Monday 01 May 2017 - last comment - 07:29, Monday 01 May 2017(35930)
Mag6.5 Near Skagway Alaska

6.5 Magnitude EQ Near Skagway, Alaska at 12:31utc, (05:31PT).

Comments related to this report
jeffrey.bartlett@LIGO.ORG - 07:29, Monday 01 May 2017 (35931)
The Mag6.5 EQ was followed by 13 aftershocks. After seismic was starting to settle down tried relocking. However, at 14:18 USGS reported another Mag6.3 earthquake near Skagway Alaska. Primary and Secondary microseism are climbing again. Put the IFO back into down until this one passes. 
Most US, ISI, HEPI WD are tripping.  
H1 General
jeffrey.bartlett@LIGO.ORG - posted 03:59, Monday 01 May 2017 (35929)
Ops Owl Mid-Shift Summary
   Locked for 58.75 hours. All looking good at this time. 
H1 SEI
jeffrey.bartlett@LIGO.ORG - posted 01:34, Monday 01 May 2017 (35928)
Mag5.3 EQ Triple Junction Region, Galapagos

5.3 Magnitude EQ Triple Junction Region, Galapagos at 07:17utc, (00:17PT).

H1 General
jeffrey.bartlett@LIGO.ORG - posted 00:22, Monday 01 May 2017 (35927)
Ops Owl Shift Transition
Ops Shift Transition: 05/01/2017, Owl Shift 07:00 – 15:00 (00:00 - 08:00) - UTC (PT)
State of H1: IFO locked at NLN, 30.9W and 62.3 Mpc  
Intent Bit: Observing
Weather: Wind is up to a Moderate Breeze, clear, temps upper 40s  
Primary 0.03 – 0.1Hz: X Axis around 0.03um/s, Y & Z Axis at 0.01um/s 
Secondary 0.1 – 0.3Hz: At 0.1um/s   
Quick Summary:  Locked for 54.75 hours. A2L Pitch below reference, Yaw is slightly elevated.      
Outgoing Operator: Nutsinee

 

H1 General
nutsinee.kijbunchoo@LIGO.ORG - posted 00:03, Monday 01 May 2017 (35926)
Ops Eve Shift Summary

TITLE: 05/01 Eve Shift: 23:00-07:00 UTC (16:00-00:00 PST), all times posted in UTC

STATE of H1: Observing at 61Mpc

INCOMING OPERATOR: Jeff

SHIFT SUMMARY: Been locked for almost 55 hours. LLO joined us briefly but down again. Wind has pretty much died down. No issue to report.

 

H1 DCS (DCS)
gregory.mendell@LIGO.ORG - posted 22:04, Sunday 30 April 2017 - last comment - 22:11, Sunday 30 April 2017(35924)
Problem with DMT H1 lock segments and redundant hoft at LHO
FYI:

1. Note that the good news is I see H1 low latency hoft making it to CIT, and it is being aggregated. Also it seems the low-latency analysis can determine the lock segments from the hoft frames. 

Thus, the problems listed below are something we can investigate Monday morning. An email has been sent to DASWG and the relevant persons about this.

2. However, the redundant copy of hoft written by the DMT seems to have
stopped today at:

Apr 30 11:21 PDT.

Much earlier today, the DMT logs report Input/output error like this:

$ tail  logs/H1_rename_Frames-2017.04.25-09.43.log

‘/gds-h1/dmt/frames/hoft/H1/.temp/H-H1_DMT_C00-1177574268-4.gwf’ ->
‘/gds-h1/dmt/frames/hoft/H1//H-H1_DMT_C00-117757/H-H1_DMT_C00-1177574268-4.gwf’
mv: cannot move
‘/gds-h1/dmt/frames/hoft/H1/.temp/H-H1_DMT_C00-1177574268-4.gwf’ to
‘/gds-h1/dmt/frames/hoft/H1//H-H1_DMT_C00-117757/H-H1_DMT_C00-1177574268-4.gwf’:
Input/output error

3. Also, thus summary pages show dropout of the H1 lock segments

https://ldas-jobs.ligo-wa.caltech.edu/~detchar/summary/day/20170430/

and nagios reports errors like,

https://dashboard.ligo.org/cgi-bin/nagios3/status.cgi?host=all&servicestatustypes=28

"Known segments in frames that aren't in database"

Thus, low-latency data is making it to CIT, I think with the correct
locked segments, but these are not making into the segment database.

This is something we'll investigate Monday morning.

 

Comments related to this report
gregory.mendell@LIGO.ORG - 22:11, Sunday 30 April 2017 (35925)

This is not related to previous problems with the calibration code not reporting lock after a data dropout.

This recent frame,

bash-4.4$ ls -l /scratch/frames/cache/hoft/H1/H-H1_DMT_C00-117764/H-H1_DMT_C00-1177648628-4.gwf
-rw-r--r--   1 40829    40829     392952 Apr 30 21:37 /scratch/frames/cache/hoft/H1/H-H1_DMT_C00-117764/H-H1_DMT_C00-1177648628-4.gwf

bash-4.4$ tconvert -l 1177648628
Apr 30 2017 21:36:52 PDT

reports a H1:GDS-CALIB_STATE_VECTOR of

67010559 = 0b11111111100111111111111111

which says H1 is in analysis ready mode.

H1 General
nutsinee.kijbunchoo@LIGO.ORG - posted 21:01, Sunday 30 April 2017 (35923)
Ops Eve Midshift Summary

Been locked and Observe for almost 52 hours. The wind is still~30 mph.

H1 ISC
terra.hardwick@LIGO.ORG - posted 18:20, Sunday 30 April 2017 (35837)
PI Mode23 coupling

Amplitude of 32761 Hz PI (Mode23 in LHO damping scheme) correlates with 3 - 30 Hz seismic motion. There is also a corresponding comb that rises in the PI OMC channel at 2*(Nyquist - PI frequency), where Nyquist = 32768 Hz and PI freq ~ 32761 Hz. 

Thanks to the summary pages, I'd noticed that the 28 - 32 kHz PI band somewhat correlated with SenseMon range. I narrowed this correlation down to 3 - 30 Hz seismic motion (which we now know correlates with range due to input beam scattering) and PI ETMY Mode 23 aka ~32761 Hz. Correlation seems to be only with this mode, ruling out electronics coupling since a mode sensed right next door in frequency world has no hardware difference - both are sensed with H1:OMC-PI_DCPD_64KHZ_AHF_DQ. First attachment is 32 hr stretch showing correlation between narrow OMC-PI band, seismic, and range. 

Kiwamu then did a drive/damp test of this mode and found narrow lines appeared in DARM while driving/damping well below saturation. Looking at the OMC channel, he actually saw just the first peak of a 14.5 Hz comb seen in OMC-PI, as well as 64, 78.5, 142.5 Hz lines. Second attachment shows comb while he was driving. This ~15 Hz comb is visible in OMC-PI anytime Mode23 is rung up enough (haven't quantified 'enough' yet) and first peak is always 2x the frequency difference of 32768 Hz (OMC-PI's Nyquist) and Mode23 frequency; I've confirmed this to within .01 Hz.  Third attachment shows presence of first peak in comb during a typical day's Mode23 non-driven ring up. I haven't seen the other peaks Kiwamu saw (64, etc.) any other time.

This is an actual mode ringing up (as opposed to just changing in sensing at OMC) as it's seen in the TransMon QPD's (and all feed forward is off for this mode). These have much lower SNR for PI so mode has to be unusually high to see. Fourth attachment shows a recent day with high 3 - 30 Hz seismic activity where amplitude correlations are visible everywhere. Fifth attachment shows spectrum during the peak just after 5 hours in previous attachment. Note that in TransMon channel, signal has been demoded with 32800 Hz, so two peaks are (32800 - 32761) = 39 Hz and (32800 + 32761 - 65536) = 25 Hz.

Images attached to this report
H1 CAL (CAL)
evan.goetz@LIGO.ORG - posted 16:44, Friday 28 April 2017 - last comment - 17:35, Friday 19 October 2018(35867)
Analysis of calibration measurements
Evan G., Jeff K.

Summary:
The calibration measurement data that was collected yesterday has now been analyzed using our Markov Chain Monte-Carlo (MCMC) methods. We detail the results below. Nothing abnormal was found, and we find that the time varying factors can track changes in sensing gain and coupled cavity pole and actuation coefficients.

Details:
We analyzed the data collected during yesterday's calibration measurements, see LHO aLOG 35849. We have simplified the process for analyzing the data; rather than running two separate Matlab script to generate the MCMC results, we can now run just one script to get the final model results.

For the sensing function, we run
${CALSVN}/trunk/Runs/O2/H1/Scripts/SensingFunctionTFs/runSensingAnalysis_H1_O2.m
while for actuation, we run
${CALSVN}/trunk/Runs/O2/H1/Scripts/FullIFOActuatorTFs/analyzeActuationTFs.m.
Note that for the actuation calibration script, we have not yet converted it to an IFO agnostic script. Once it is converted, this script will be renamed.

Below are the table of values and their associated uncertainties for yesterday's measurements. Also, for comparison, are the modeled values from the reference measurement 3 Jan 2017:

                                                       Reference Value     MAP     (95% C.I.)        MAP       (95% C.I.)
                                                       2017-01-03          2017-01-03 (MCMC)         2017-04-27 (MCMC)
 Optical Gain                K_C         [ct/m]        1.088e6             1.088e6 (0.0002e6)        1.124e6   (0.0002e6)
 Couple Cav. Pole Freq.      f_c         [Hz]          360.0               360.0   (7.6)             343.4     (2.6)
 Residual Sensing Delay      tau_C       [us]          0.67                0.67    (6.7)             -1.8      (1.8)
 SRC Detuning Spring Freq.   f_s         [Hz]          6.91                6.91    (0.1)             7.4       (0.04)
 Inv. Spring Qual. Factor    1/Q_s       [ ]           0.0046              0.046   (0.016)           0.009256  (0.0069)

 UIM/L1 Actuation Strength   K_UIM       [N/ct]        8.091e-8            8.091e-8  (0.2%)          8.0818e-8 (0.18%)
 PUM/L2 Actuation Strength   K_PUM       [N/ct]        6.768e-10           6.768e-10 (0.02%)         6.795e-10 (0.08%)
 UIM/L3 Actuation Strength   K_TST       [N/ct]        4.357e-12           4.357e-12 (0.02%)         4.537e-12 (0.07%)
 UIM/L1 residual time delay              [usec]        n/a                 n/a                       29.1      (35.5)
 PUM/L2 residual time delay              [usec]        n/a                 n/a                       7.7       (3.1)
 TST/L3 residual time delay              [usec]        n/a                 n/a                       10.2      (1.8)


These values are derived from MCMC fitting to the data values. The attached plots show these results for the sensing and multiple-stage actuation functions.

We have added a new feature to the MCMC analysis, modeling the residual time delay in actuation. We expect to have zero usec of residual time delay, provided the model accurately captures all dynamics of the actuation. Deviations from zero can reveal un-modeled dynamics. For example, the PUM and TST residual time delays are inconsistent with zero usec, but we expect that this is due to imperfect modeling of the complicated violin resonances of the quad suspension.

The time varying factors are doing a good job tracking the changes between the reference model and the currently measured parameters (see time varying factors summary page).

For reference, the parameter files were used as follows:
${CALSVN}/trunk/Runs/O2/H1/params/2017-01-24/modelparams_H1_2017-01-24.conf    (rev4401, last changed 4396)
${CALSVN}/trunk/Runs/O2/H1/params/2017-04-27/measurements_2017-04-27_sensing.conf  (rev4596, last changed 4596)
${CALSVN}/trunk/Runs/O2/H1/params/2017-04-27/measurements_2017-04-27_ETMY_L1_actuator.conf  (rev4596, last changed 4596)
${CALSVN}/trunk/Runs/O2/H1/params/2017-04-27/measurements_2017-04-27_ETMY_L2_actuator.conf  (rev4596, last changed 4596)
${CALSVN}/trunk/Runs/O2/H1/params/2017-04-27/measurements_2017-04-27_ETMY_L3_actuator.conf  (rev4596, last changed 4596)

Non-image files attached to this report
Comments related to this report
evan.goetz@LIGO.ORG - 10:42, Monday 01 May 2017 (35935)
A typo in the reference values for 1/Q_s above. It should be 0.046 (not 0.0046 as typed above).
jeffrey.kissel@LIGO.ORG - 17:35, Friday 19 October 2018 (44691)
For a bigger picture look at these 2017-04-27 actuation function measurements, I attach a plot of the model against measurement *before* dividing out the frequency dependence. This helps discern what the overall phase of the actuator stages should be relative to each other during O2.
Non-image files attached to this comment
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