Displaying reports 63041-63060 of 85745.Go to page Start 3149 3150 3151 3152 3153 3154 3155 3156 3157 End
Reports until 12:26, Wednesday 11 November 2015
LHO General
thomas.shaffer@LIGO.ORG - posted 12:26, Wednesday 11 November 2015 (23312)
Observing

Observing at 78MPc.

Environment:

LHO General
thomas.shaffer@LIGO.ORG - posted 11:27, Wednesday 11 November 2015 - last comment - 12:31, Wednesday 11 November 2015(23310)
Lockloss

Lockloss @ 19:22

Comments related to this report
thomas.shaffer@LIGO.ORG - 12:31, Wednesday 11 November 2015 (23313)

Possibly due to the injection testing. Everything else seemed calm. Attached the generic Lockloss tool set of plots.

Images attached to this comment
LHO General
thomas.shaffer@LIGO.ORG - posted 10:54, Wednesday 11 November 2015 - last comment - 12:36, Wednesday 11 November 2015(23308)
Out of Observing for Swept Sine Test

LLO is down with some "high" winds. Chris Biwer will run a swept sine while there is an opportunity.

Comments related to this report
thomas.shaffer@LIGO.ORG - 12:36, Wednesday 11 November 2015 (23314)

WP#5595

H1 AOS (CAL, INJ)
christopher.biwer@LIGO.ORG - posted 10:52, Wednesday 11 November 2015 - last comment - 12:12, Wednesday 11 November 2015(23307)
starting CAL-INJ swept sine test
Beginning swept-sine test for CAL-INJ while LLO is down.
Comments related to this report
christopher.biwer@LIGO.ORG - 11:24, Wednesday 11 November 2015 (23309)DetChar, INJ
Swept-sine for 500-2000Hz began at 18:55:45 UTC and finished. Lost lock at 19:23 UTC.
christopher.biwer@LIGO.ORG - 12:12, Wednesday 11 November 2015 (23311)DetChar, INJ
To do the swept sine from 500-2000Hz I used the template at: https://svn.ligo.caltech.edu/svn/aligocalibration/trunk/Runs/O1/H1/Measurements/INJ/template_cw_inj_sweptsine_500to2000_20151111.xml

I've attached the coherence and TF from CAL-INJ_CW_EXC to CAL-DELTAL_EXTERNAL_DQ.
Images attached to this comment
H1 PEM (DetChar, PEM)
robert.schofield@LIGO.ORG - posted 08:28, Wednesday 11 November 2015 (23305)
PEM injection report, summary and links to parts

Attached is a summary of PEM injections, with summary plots for both sites, estimates of environmental contributions to DARM and calibrated coupling factors. These are also useful for calculating the SNR in DARM from the SNR in the PEM channel, determining coupling sites for environmental events in DARM, and for comparing coupling between LHO and LLO. Links to the individual reports follow.

Magnetic

LHO: https://alog.ligo-wa.caltech.edu/aLOG/index.php?callRep=21272

LLO: https://alog.ligo-la.caltech.edu/aLOG/index.php?callRep=20599

RF

LHO: single f’s https://alog.ligo-wa.caltech.edu/aLOG/index.php?callRep=23252

         sweep https://alog.ligo-wa.caltech.edu/aLOG/index.php?callRep=22968

LLO: preliminary single f’s https://alog.ligo-la.caltech.edu/aLOG/index.php?callRep=20599

Vibration

LHO: https://alog.ligo-wa.caltech.edu/aLOG/index.php?callRep=22797

LLO: https://alog.ligo-la.caltech.edu/aLOG/index.php?callRep=22463

Site activities

LHO: https://alog.ligo-wa.caltech.edu/aLOG/index.php?callRep=21272

LLO: https://alog.ligo-la.caltech.edu/aLOG/index.php?callRep=20599

Robert, Anamaria

Non-image files attached to this report
LHO General
thomas.shaffer@LIGO.ORG - posted 08:18, Wednesday 11 November 2015 (23306)
Observing

Travis brought it all the way up, We are now in Observing. Winds <15mph, Seismic: 0.03-0.1Hz = 0.02um/s, 0.1-0.3 = 0.8um/s. The PSL power was 21.8W a second ago, but seems to have come up to 22.1W since I started writing this.  LLO is also up and Observing.

LHO General
thomas.shaffer@LIGO.ORG - posted 08:02, Wednesday 11 November 2015 (23304)
Ops Day Transition
H1 General
travis.sadecki@LIGO.ORG - posted 08:00, Wednesday 11 November 2015 (23303)
OPS Owl shift summary

Title: 11/11 Owl Shift 7:00-15:00 UTC (0:00-8:00 PST).  All times in UTC.

State of H1: Lock acquisition

Shift Summary:  Wind dropped like a rock at ~15:00 UTC.  I began an initial alignment since it had been down for 4 hours and had been through a windstorm.  Microseism is trending up but still at a manageable level. 

Incoming operator: TJ

Activity log:

8:33 GRB alert, LLO was down

12:03 Adjusted X and Y arm ALS fiber polarization

15:42 Chris to X arm for beam tube sealing

H1 General
travis.sadecki@LIGO.ORG - posted 04:16, Wednesday 11 November 2015 (23302)
OPS Owl Mid-shift Summary

Still down after the lockloss earlier due to high winds.  Winds are in the 30s with gusts to over 40 mph, and the forecast predicts it won't get better for the rest of the day.  But who believes the weathermen anyways?? (According to the NWS, they are off by a factor of 2 in their prediction at the moment, however in the wrong direction for GW science.  It is supposed to be 15 mph with gusts to 20.)

I had to call Keita at 4am PST to walk me through an ALS fiber polarization adjustment since I had never done one and could not find a procedure to do so (it is on my list to add to the OPS Wiki).  The wind did its typical thing where it calms just enough to lull you into the sense that you should begin locking again before it picks back up.  Sorry Keita, you should sleep in this morning or get a nice breakfast or something.

H1 General (Lockloss)
travis.sadecki@LIGO.ORG - posted 02:29, Wednesday 11 November 2015 (23301)
Lockloss 10:27 UTC

Lockloss, most likely due to winds which are gusting to over 50 mph.

H1 General
jeffrey.bartlett@LIGO.ORG - posted 00:06, Wednesday 11 November 2015 - last comment - 13:48, Wednesday 11 November 2015(23300)
Ops Evening Shift Summary
Activity Log: All Times in UTC (PT)

00:00 (16:00) Take over from TJ
02:40 (18:40) First of four large (mag 6.9 to 4.9) EQs in Chile. All four arrived within 30 minutes.
05:00 (21:00) Start initial alignment
06:19 (22:19) IFO locked at NOMINAL_LOW_NOISE, 22.1w, 78Mpc
06:24 (22:24) Cleared SDF and set intent bit to Observing
06:56 (22:56) Lockloss – mag 5.2 EQ on Mid-Pacific Ridge
07:30 (23:30) Relocked at NOMINAL_LOW_NOISE, 22.2w, 78mpc
	      No SDF differences flagged – Set Intent bit to Observing
08:00 (00:00) Hand off to Travis


End of Shift Summary:

Title: 11/10/2015, Evening Shift 00:00 – 08:00 (16:00 – 00:00) All times in UTC (PT)

Support: Keita, Betsy, Hugh, Vern, Marissa 

Incoming Operator: Travis

Shift Summary: Had problems locking the ALS green, mostly in X. Keita found the BSC-9 ISI had a large swing on the X platform location. (See #23293). The motion slowed down, and I was able to realign the ALS green for both arms. Tried relocking. Made it to DARM_1F before 4 large EQs hit Chile. Seismic motion is very high right now (See #23296). Waiting for things to settle and will try relocking. 

After seismic activities settled down to below 0.1 um/s and microseism dropped to 0.3 – 0.2 um/s, ran initial alignment. The IFO was locked at NOMINAL_LOW_NOISE. Cleared up several SDF issues, and set the intent bit Observing. Wind at the CS is a moderate breeze (13 – 18 mph) and light to gentle (4 – 12) at the ends and mids. 

Lockloss due to Mid-Pacific Ridge Earthquake. Seismic activity has rung up a bit, but is quickly coming down. Microseism did not change from 0.3 um/s. Wind is up to a fresh breeze (19 – 24 mph) in the CS. The wind at the ends and mids is still light to gentle breeze (4 – 12 mph). Will attempt to relock without doing an initial alignment.

IFO relocked easily without the need for a realignment. Back to Observing
   

 
Comments related to this report
thomas.shaffer@LIGO.ORG - 13:48, Wednesday 11 November 2015 (23316)

The SDF diffs that Jeff accepted were from the dark offset scripts that I ran at 23:28 UTC.

H1 General
jeffrey.bartlett@LIGO.ORG - posted 20:28, Tuesday 10 November 2015 (23298)
Ops Evening Mid-Shift Summary
   IFO is not locked. 

   Between the maintenance activities, problems with a swinging BSC-9 ISI (#23293), and a nine large EQs in Chile, locking has been unsuccessful. 

   After the motion of BSC-9 settled down, I did an ALS realignment, and was able to get the IFO to DRMI_1F, before the first two Chilean EQs (mag 6.9 & mag 6.6) arrived. Low frequency seismic activity jumped up to over 10 um/s, microseism was over 1 um/s. 

   There were at least nine large earthquakes in Chile (mag 6.9 to mag 4.8) within a one hour period. Things are starting to calm down. Will give it a bit more time to settle down and them will redo initial alignment. 

   At least the wind is just a light breeze (4 -7 mph).            
H1 SEI
keita.kawabe@LIGO.ORG - posted 18:30, Tuesday 10 November 2015 - last comment - 23:27, Tuesday 10 November 2015(23293)
relocking problems (TJ, Jeff, Keita)

People were having problem with relocking after the maintenance.

IMC VCO tune offset was railing at +-5V whenever COMM PLL was trying to enable slow feedback to IMC. TJ manually disabled it, not sure why this was turned on, it seems like the guardian does not touch this.

When both X and Y were unlocked, it was clear that X arm fringe velocity was much much larger than Y arm just by looking at the camera.

It seems like the EX ISI has been going crazy for the past 2 hours or so (first attachment left). I haven't checked if this is due to ground motion, It seems like the FOM for 0.03-0.1Hz band shows us that there's something going on (but EY looks noisier) (second attachment).

The dominant frequency of the noise is about 1/24 Hz, so the frequency is about right (first attachment right).

As I was talking to Jeff, however, ETMX ISI slowed down. We'll see.

(Update: As we were waiting, we are hit by another quake at around 2:10 or so UTC.)

Images attached to this report
Comments related to this report
arnaud.pele@LIGO.ORG - 20:18, Tuesday 10 November 2015 (23295)

Attached is a spectra comparing the ground motion between yesterday and today -EX first image, EY second image-. There is certainly 50mHz elevated motion, compared to yesterday.

Although it is strange how large is the ETMX motion on stage 1 at 40mHz, witnessed by the t240. Certainly much more than for EY.

Looking at the transmissibility at EX from ground to stage 1 -image 3- , it seems the motion is much more amplified (compared to yesterday) between hepi and stage 1 in x and y, cf green in 2nd row. 

Images attached to this comment
jeffrey.bartlett@LIGO.ORG - 23:27, Tuesday 10 November 2015 (23299)
   Took 24 hour plots of the ETM-X and ETM-Y ISI CPS X locations covering the time of the problems with ETM-X.  
Images attached to this comment
H1 SUS (SUS)
borja.sorazu@LIGO.ORG - posted 14:22, Tuesday 10 November 2015 - last comment - 12:55, Wednesday 11 November 2015(23283)
Ringdown Q measurements of the 3rd and 4th harmonic for the QUAD violin modes

This entry follows upon the entry 23167 where the frequency of the 3rd and 4th harmonic for the QUAD suspensions violin modes were identified. This entry is also complementary to Evan Hall's entry 22847 where similar Q's were measured with a different technique.

In this analysis, a line tracker (iWave) was applied over each of the identified 3rd and 4th harmonic frequencies (23167) on 21 hours of data during which the detector was continuously in Observing mode and with the damping filters turned off, data analysed started from 2015-10-21 21:30:00. The channel I used is H1:OMC-DCPD_SUM_OUT_DQ downsampled to 8192Hz in order to be able to handle the considerable ammount of data.

The line tracker was set to lock, on an automated way, to each of the monitored frequencies of interest. The tracker provides the frequency value which it is following and the amplitude of that frequency as a function of time. This information is provided in real time with the data being analysed. Although I automated the process the line tracker could not always lock to the mode of interest, in a few cases it locked to the wrong mode of higher amplitude and/or was not able to separate modes of high amplitude and close proximity. Therefore a targetted run had to follow the automated one.

The result of the analysis is summarised on the attached 'png' plots which shows; in each column the mode monitored with the top plot being the frequency tracked as a function of time and the bottom plot the 'log(Amplitude)' (Napierian or natural logarithm of the mode's amplitude). The red dashed lines are respectively the median of the tracked frequency and the fitted first order polynomial to the 'log' of the mode's ringdown.

Notice that monitoring 21 hours at 8192Hz resolution of 50 modes provide a huge ammount of data so here I only present a summary of the results, and this is also the reason why the plots shown are .png files.

The first order polynomial fitting of the ringdown was done using Matlab's 'polyfit' function which implements a least-squares minimization fitting. This function also provides an estimate of the covariance matrix of the fitted coeficients which is used to calculate the standard error or variance of the estimated coeficients for the linear fit of the log(Amp) ringdown. In particular only the slope of the fitted line is used to estimate Q = Pi * f0 / abs(slope_fit), where f0 is the median of the frequency tracked. The median of the tracked frequency has an observed uncertainty smaller than 1mHz which makes the Q relative uncertainty to be dominated by the slope fitting uncertainty as given by the covariance matrix of the fitted coefficients. Therefore the reported error on Q will be given by the uncertainty of the slope of the fit as:

(Delta(Q) / Q)^2 = (Delta(slope_fit) / abs(slope_fit))^2

Next I summarise the results in 4 columns (also on attached .txt files labelled 'Q_results_3Harm_1stFreq_2ndQ_3rdDeltaQ_4thEHresults' and ''Q_results_4Harm_1stFreq_2ndQ_3rdDeltaQ_4thEHresults); first is the mode frequency, second is my estimated Q, third is the estimated Q error, and 4th is Evan Hall's results from 22847 for comparison:

Mode frequency (Hz)          Q (line tracker)                Delta(Q)                Q_from_22847

1.0e+09 *
   0.000001456177151   1.055261277139490   0.000021679047341   1.060000000000000
   0.000001456842619   1.011674961643711   0.000024977780728   1.020000000000000
   0.000001461409317   0.547106388691582   0.000007012695846   0.550000000000000
   0.000001461732469   1.000243995219630   0.000121822842175   1.000000000000000
   0.000001461859533   0.673721968942594   0.000056781365996   0.644000000000000
   0.000001462031866   1.015448724742734   0.000039055044799   1.030000000000000
   0.000001462313302   1.109264503070151   0.000020406518349   1.120000000000000
   0.000001462596624   0.879503445780186   0.000090574514768   0.921000000000000
   0.000001463096689   0.881010088452959   0.000383879344618   0.995000000000000
   0.000001463100039   0.990987050813072   0.000431799209313                   0
   0.000001467475846   1.089361798635816   0.000107769329936   1.130000000000000
   0.000001467964869   0.979770107952095   0.000024671825593   1.000000000000000
   0.000001470380790   0.886560854120574   0.000042794470546   0.894000000000000
   0.000001470826225   1.046162403099169   0.000070957888675   1.040000000000000
   0.000001471928631   1.433692732321030   0.000246428147278   1.280000000000000
   0.000001472216373   1.036874013551553   0.000319968824557   1.070000000000000
   0.000001472450299   1.116249774693906   0.000012761989599   1.130000000000000
   0.000001474079863   1.178125176004288   0.000086507667346   1.170000000000000
   0.000001475097416   1.001120432026481   0.000377881305540   0.935000000000000
   0.000001475251394   1.148066981481587   0.000155330486516   1.160000000000000
   0.000001478169574   0.781717093501666   0.000095725814070   0.830000000000000
   0.000001482585386   0.865266831531971   0.000049369138115   0.879000000000000
   0.000001484077440   0.912365853159565   0.000100741959112   0.914000000000000
   0.000001484430000                                   0                                 0   0.796000000000000
   0.000001484525699   0.821953404180692   0.000053588794283   0.836000000000000
   0.000001484668763   1.396430023353472   0.000359948050123   1.270000000000000


   0.000001922925589   0.806732893457201   0.000050155023271   0.812000000000000
   0.000001923612098   0.904079503131098   0.000101465317927   0.856000000000000
   0.000001923854589   0.730146274074320   0.000057632970265   0.741000000000000
   0.000001923861257   1.045943198261562   0.000286910927180   1.000000000000000
   0.000001924673359   0.656777206317145   0.000037377872702   0.675000000000000
   0.000001924914736   0.822610665784300   0.000055143089987   0.845000000000000
   0.000001926240582   0.877913538609440   0.000041733066792   0.888000000000000
   0.000001927465534   1.193131464187697   0.000196087122798   1.080000000000000
   0.000001928461859   0.491982285283618   0.000060799517584                   0
   0.000001929312799   1.014511076625149   0.000491391979504   0.742000000000000
   0.000001931573475   0.770986524485489   0.000120874236513   0.778000000000000
   0.000001932139817   0.721080850064806   0.000077175334498   0.739000000000000
   0.000001932335653   0.723984558093199   0.000083370684684   0.713000000000000
   0.000001932612502   0.802178526483954   0.000016727734773   0.806000000000000
   0.000001940322842   0.727877169848855   0.000210139484624   0.778000000000000
   0.000001940663844   0.923330707711907   0.000027923601820   0.941000000000000
   0.000001941349656   0.922491569137019   0.000274707300452   0.906000000000000
   0.000001942174877   1.171274720414585   0.000377051759607   1.050000000000000
   0.000001942390477   1.094325186350570   0.000475289691312                   0
   0.000001943777687   0.914373092200222   0.000483429769721                   0
   0.000001946732789   0.732800137163962   0.000093031972218   0.677000000000000
   0.000001954459289   0.803950536039718   0.000153319383649                   0
   0.000001955921818   0.684755442755530   0.000143761779921                   0
   0.000001957335075   0.651607142944878   0.000091322052084                   0
   0.000001959023577   0.785016144699797   0.000093723756453                   0

NOTE: Although there are not big differences in results with entry 22847 for the 3rd harmonics, however some difference is observed on the Q's of 4th harmonics, also 7 more modes are reported here for the 4th harmonics.

Images attached to this report
Non-image files attached to this report
Comments related to this report
borja.sorazu@LIGO.ORG - 12:55, Wednesday 11 November 2015 (23315)

Just to clarify, the period of time analysed in this entry was characterised by having the 3rd and 4th harmonics damping filters turned OFF but the filters for the fundamental and 2nd harmonics of the test masses were turned ON.

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