Displaying reports 66821-66840 of 85402.Go to page Start 3338 3339 3340 3341 3342 3343 3344 3345 3346 End
Reports until 10:44, Thursday 11 June 2015
H1 SEI
hugh.radkins@LIGO.ORG - posted 10:44, Thursday 11 June 2015 (19074)
Compare Local Signals with EQ predictor

If you look at the Online EarthQuake Arrival Predictor, it shows the 5.7 mag EQ in Japan, along with many others.  This is just the largest in the last day or so.  I've overlayed the predicted arrival time of the Rayleigh waves on the STS2 ground seismometers and the BS stage2 inertial sensors--see attached.  Unfortunately the IFO was not in lock at the time.

Anyway, need a bigger EQ still to assess the prediction as the Ground sensors.  Just to be more thorough, I shifted and extended the plot a little and now include the predicted arrival times of the P & S waves, second attachment.  I got rid of the Z ground seismometer and added the transmitted arm power for a IFO indicator.  Did the arrival of the p wave ring up the BS ISI?  Ehh I don't think so given the ground seismo unless the prediction is off by ~90 seconds.  But I think the prediction could be off by that much given the complexity of travel paths and assumptions of the velocitys.  With this data set I'd say the ISI is being beat around by the locking attempts, not by this red earthquake.

Images attached to this report
H1 PSL
jeffrey.bartlett@LIGO.ORG - posted 09:35, Thursday 11 June 2015 (19071)
Adjust ISS Diffracted Power
Adjust the ISS diffracted power from 11.1% -2.06v to 8.3% -2.09v 
H1 General
jeffrey.bartlett@LIGO.ORG - posted 09:34, Thursday 11 June 2015 (19070)
Clear HEPI Watchdog Counters
Cleared the HEPI L4C watchdog counter for ITMY. All others were green and clear.
LHO VE
bubba.gateley@LIGO.ORG - posted 08:51, Thursday 11 June 2015 (19069)
Beam Tube Washing
Scott L. Ed P.
6/8/15
The following are some of the dirtiest area we have seen on the X-arm.
Cleaned 58 meters ending 8.4 meters north of HNW-4-068.

6/9/15
 Maintenance day which means we can use the Hilti HEPA vacuum, the most effective vacuum for cleaning out the support tubes. We have been holding off on using this vacuum during ER7 because of the loud thump emitted from the internal cleaning system of the hepa filter.
We will go back and clean 2 sets of support tubes and cap them, as well as move forward to clean as many supports as reasonable before the end of maintenance day at noon.
Cleaned 30 meters of tube ending at HNW-4-070. Test results posted on this A-log.
 
Robert Schofield came out to the area where we are cleaning to look at our procedure and methods of actual cleaning of the tube to investigate possible glitches seen by the control room operators during lock.

6/10/15
Remove lights, cords, vacuum machines, and all related equipment from enclosure and thoroughly clean all equipment, then relocate to next section north.
Started cleaning at HNW-4-070, cleaned 15 meters of tube.

To date we have cleaned a total of 3418 meters of tube. 



Non-image files attached to this report
H1 INJ (INJ)
peter.shawhan@LIGO.ORG - posted 08:32, Thursday 11 June 2015 (19068)
Ending scheduled burst hardware injections for ER7
Since we got a few coincident burst hardware injections this morning, and the rest of ER7 (now through Sunday 8:00 PDT) will be split between local measurements/commissioning and running, I have disabled the scheduled burst hardware injections for the rest of ER7.  To be precise, I left the next few dozen in the schedule but I set their amplitudes to zero, in order to test the long-term behavior and stability of tinj; tinj will call awgstream to inject them, but because awgstream will just add zero strain to the instrument, these should have no effect and will not appear in ODC bits or database segments.

There is still a plan to add a stochastic injection sometime before ER7 ends, if time permits.
H1 General
nutsinee.kijbunchoo@LIGO.ORG - posted 08:04, Thursday 11 June 2015 - last comment - 19:34, Friday 12 June 2015(19067)
Owl Shift Summary

00:00 The ifo locked right before I came in. Wind speed is <20 mph. 90 mHz blend filter is used for BSC2.

           I noticed the BS oplev sum is saturated (> 80000 counts). Is this alright? It's been around this value for 10+ days.

01:55 There's a big bump at ~30 Hz that caused a big dip in the BNS range. SUS Oplev plots didn't show anything suspicious. The bump at this frequency happened through out the night, just not as big.

02:00 A 4.7 MAG earthquake in Ecuador shook PR3 a little and BNS range dropped slightly (from 61 Mpc to 60 Mpc), but that's all it did. No WD tripped. 

08:00 We've been locked for 8+ hours and still going strong at 61 Mpc! We had 5+ hours of coincidence with Livingston tonight. Handling the ifo to Jeff B.

Comments related to this report
daniel.hoak@LIGO.ORG - 17:16, Thursday 11 June 2015 (19083)

Judging from the normalized spectrograms on the summary pages, the 30Hz noise looks like occasional scattering noise, likely from the alignment drives sent to the OMC suspension.  Currently the Guardian sets the OMC alignment gain at 0.2 (for a UGF of around 0.1-0.5 Hz in the QPD alignment loops).  This is probably too high from a scattering-noise perspective, it can be reduced by a factor of two without ill effects.

daniel.hoak@LIGO.ORG - 19:34, Friday 12 June 2015 (19105)DetChar

To follow up on this noise, here is a plot of one of the noise bursts around 20-30Hz, alongside the OMC alignment control signals.  The noise has the classic scattering-arch shape, and it is correlated with the ANG_Y loop, which send a large signal to the OMC SUS.  We've seen this kind of thing before.  The start time for the plot is 09:27:10 UTC, June 11 (the time axes of the two plots are a little off, because apparently indexing for mlab PSDs is the hardest thing I've had to do in grad school.)

The second plot attached compares the OMC-DCPD_SUM and NULL channels at the time of the noise bursts in the first plot, to a quiet time one minute prior.  The scattering noise is largely coherent between the two DCPDs.

Images attached to this comment
H1 SEI
hugh.radkins@LIGO.ORG - posted 08:00, Thursday 11 June 2015 (19066)
BS ISI stage1 ISO running high wind blends

Jim must have switched these.  The 90mHz blends are on for X & Y rather than the 45s.  The SDF is red for this reason.

H1 CDS (DAQ)
david.barker@LIGO.ORG - posted 07:56, Thursday 11 June 2015 (19065)
CDS model and DAQ restart report, Wednesday 10th June 2015

model restarts logged for Wed 10/Jun/2015

no restarts reported

H1 INJ (INJ)
peter.shawhan@LIGO.ORG - posted 07:16, Thursday 11 June 2015 (19064)
Transient injections now running at LHO under the 'hinj' account
Dave Barker created a shared 'hinj' account for running hardware injections (alog 19057), and we restarted tinj (the transient injection process) under that account yesterday.  Unfortunately, the injections failed overnight due to awgstream errors.  That was puzzling because executing awgstream on the command line (with zero amplitude or extremely small amplitude) worked fine.  It turns out that different versions of the gds, awgstream and root packages are installed on the LHO injection machine compared to the LLO injection machine, so the environment setup that was copied over from LLO caused awgstream to fail when executed by tinj.  I made a separate environment setup script for LHO and restarted tinj under that, and now it seems to be working fine.

After doing a zero-amplitude test injection at 1118063333 (which should have had no effect on anything), I modified the schedule to more promptly do som burst injections (coincident at both sites), at GPS times 1118063933, 1118067123, and 1118067543.  (The actual signal comes a second or two later than those waveform file start times.  As of this writing, the first of those was picked up by the burst pipelines: see https://gracedb.ligo.org/events/view/G159516 .  We'll see about the others.
H1 SUS (ISC, SUS)
keita.kawabe@LIGO.ORG - posted 02:04, Thursday 11 June 2015 - last comment - 04:46, Thursday 11 June 2015(19060)
Charging localization measurement (Leo, Betsy, Evan, Kiwamu, Daniel, Keita)

Related:

Den's alog 16624

Den's alog 16727

Summary:

Many things are dubious.

  1. EX LL ESD is broken as the ESD to length response is 3 orders of magnitude smaller than the others. Probably shoddy connection somewhere between the driver and the ESD electrode, as the voltage readback looks normal.
  2. It looks as if either the sign of EX ESD output is flipped (positive digital out induces negative voltage) or the sign of EY ESD output is flipped but not both.
  3. I'm just assuming that the sign convention for CAL-CS_DARM_EXTERNAL_DQ is length(X)-length(Y), and that it's correct, without any confirmation.

Despite these things, it seems as if the charges on the back are on the same order as reported in Den's alog 16624.

If we assume that the sign of EY ESD is wrong and we still take 1. into account, the charges are calculated as:

  front back
X 4.4nC 1.1nC
Y 2.2nC 1.2nC

This looks semi-reasonable.

If we assume that the sign of EX ESD is wrong and we still take 1. into account, the charges are:

  front back
X 5.7nC -0.9nC
Y -6nC -0.4nC

I don't like that the signs are all over the place.

If we assume that everything is correct except that the EX LL is broken (i.e. we ignore the 2. above but take 1. into account), the charges based on are:

  front back
X 4.4nC 1.1nC
Y -6nC -0.4nC

Again the signs are all over the place.

These are based on the same calculation as Den's alog 16624.

I'm assuming that the sign convention of CAL-CS_DARM_EXTERNAL_DQ is length(X)-length(Y) (i.e. positive when X stretches and Y shrinks).

Anyway, no matter how you look at the data, the back surface charges are quite similar to what was reported in Den's alog (except for the signs that don't make much sense for the latter two tables).

We tried similar measurements as described in Den's alog 16727 but the angle data for X was unusable (no coherence at all). If you're interested in Y data, all measurements were saved in Betsy's template directory.

 

The gist of the measurements:

Differences between EX and EY measurements:

Fishy sign of ESDs (Go to the floor and figure out):

EY ESD length drivealign matrix has a negative DC gain while the corresponding matrix for EX is positive even though the LSC DARM output matrix already takes care of the sign difference necessary for DARM control for EX and EY.

It looks as if either the bias line has a wrong sign for one ETM but not the other, or LL/LR/UL/UR lines have a wrong sign for one ETM but not the other.

Raw-ish data and calculations:

Measured the zero-bias transfer coefficients from ESD segments and the ring heater (top and bottom combined) to the calibrated DARM channel in meters/volts at around 80Hz. After taking the TF of the drivers and the DAC V/cts into account, they are:

  LL [m/V] LR [m/V] UL [m/V] UR [m/V] ESD combined [m/V] Ring Heater [m/V]
EX +1.3E-18 +2.2E-15 +1.0E-15 +5.6E-16 +3.8E-15 * 4/3 -6.7E-16
EY +5.6E-16 +6.5E-16 +1.4E-15 +1.5E-15 +4.1E-15 +1.9E-15

Positive data is actually about 24 deg (Y arm) or 30 deg (X arm) delayed, while negative data is about 210 deg (X arm) delayed.

EX LL is not working. Coherence is very large, the voltage readback looks OK, but it has 3 orders of magnitude smaller response than the others. EX LL did not change much when the nominal EX ESD bias was put back on.

I multiplied the ESD combined data by 4/3 only for EX to take into account that the EX LL driver is not working.

Force to length transfer function at 80Hz is -1/M/(2*pi*80Hz)^2 = -1E-7[m/N] (negative as the phase is 180 degrees relative to DC).

Also, the above is the TF to DARM, which is supposed to be X length - Y length. In order to move to a sign convention where positive means that the ETM moves closer to ITM, the sign of the X data should be flipped.

Combining these, the above raw-ish data is converted to N/V as:

  LL [N/V] LR [N/V] UL [N/V] UR [N/V] ESD combined [N/V] Ring Heater [N/V]
EX +1.3E-11 +2.2E-8 +1.0E-8 +5.6E-9 +3.8E-8 * 4/3 -6.7E-9
EY -5.6E-9 -6.5E-9 -1.4E-8 -1.5E-8 -4.1E-8 -1.9E-8

The signs of this table don't really make sense (positive ESD electrode potential should move ETMX and ETMY in the same direction if the charge has the same sign).

Anyway, from here, you solve Den's rough formula:

FRH / VRH = Afront Qfront + Aback Qback

FESD / VESD = Bfront Qfront + Bback Qback

Afront = 1 / 0.20 [1/m] ; Aback = -1 / 0.04 [1/m] 

Bfront = 1 / 0.20 [1/m] ; Bback = 1 / 0.04 [1/m]

Comments related to this report
rainer.weiss@LIGO.ORG - 04:46, Thursday 11 June 2015 (19063)
It is too confusing to be sure. My guess is also that there is charge on the back of the test mass. So let me suggest
that since you are now going to enter the chamber and use the top gun that the 10"flange with the off-axis nipple
be mounted on both x and y etm chambers with the associated small gate valves so that we have this capability
of best location for discharge in the future. Do not remove the gate valves from the middle flanges.
H1 AOS
jim.warner@LIGO.ORG - posted 00:03, Thursday 11 June 2015 (19062)
Shift Summary

~16:00 Locked IFO

~16:45 Winds pick up, lock loss

Many frustrating hours of lock losses at REFL_TRANS or there abouts

23:15 Lock IFO again.

H1 DetChar (ISC)
jim.warner@LIGO.ORG - posted 22:34, Wednesday 10 June 2015 - last comment - 23:33, Wednesday 10 June 2015(19059)
High-ish winds making locking difficult

When I took over from Jeff this afternoon, he had successfully damped down bounce and roll modes on various optics, so I was able to proceed with locking the IFO at 17:15. About 45 minutes after that, the DARM got glitchy and we noticed that the wind traces on the wall were all trending up. After 45 minutes we lost lock and I haven't been able to relock since. Winds seem to be slowly winding down, but it's not totally calm yet. Pretty consistenly the IFO will get o CARM reduction, then lose lock on REFL_TRANS. Attached plots show trends for the last 6 hours at EX and EY. We lost lock pretty much right as winds topped out at EY.

Images attached to this report
Comments related to this report
jim.warner@LIGO.ORG - 23:33, Wednesday 10 June 2015 (19061)

Winds have settled down. IFO is locked on LSC_FF, just 20 minutes after LLO went down. Oh, well, more data points about LHO locking and winds. I attach the last 7 hours of windspeeds for EX and EY, we were able to lock at roughly the beginning and at the end. So, roughly 0:00:00 UTC 6/11 and again at 5:45 UTC, and not betwixt the two. DARM is still kind of glitchy, but it seems to be holding up.

Images attached to this comment
H1 INJ
edward.daw@LIGO.ORG - posted 17:56, Wednesday 10 June 2015 (19058)
Files for simultaneous stochastic injection at both sites.
I've created 1 hour injection files intended for simultaneous injection at LHO/LLO. There is a single 3600 second text file on h1hwinj1 at this location:
h1hwinj1:/ligo/home/edward.daw/research/hardware_injections/dependencies/sources/virgo/NAPNEW/SCRIPTS/IsotropicSbGenerator/first_injframes/SB_H1_ER7_1hr.txt
This contains a single set of channel data for injection at the Hanford site. There is a corresponding one hour ascii text file at Livingston at this location:
l1hwinj1:/home/edward.daw/injections/SB_L1_ER7_1hr.txt
Both files were created using a single call to IsotropicSbGenerator.py on the l1hwinj machine as follows:
cd /ligo/home/edward.daw/research/hardware_injections/dependencies/sources/virgo/NAPNEW/SWIG/
./IsotropicSbGenerator.py -i IsotropicSbGenerator3.ini
The results were 2 frames, one containing the Hanford data, the other containing the Livingston data. The LLO file was copied by ftp
to l1hwinj1.ligo-la.caltech.edu. At each site, libframe and frgetvect were used to convert the frame data to ascii text.

The amplitudes of these injections are omega_GW=0.001 at 100Hz in each detector. This should be far more subtle than the previous injection, so no need (hopefully) for Jeff/Adam to rescale the amplitude this time.

Hope there is some simultaneous up time at the two sites to try this test; I will be delighted if this is possible, but understand of course if there isn't an opportunity.

Thanks for any help. I've left a copy of this entry on the LLO aLOG.
H1 CDS
david.barker@LIGO.ORG - posted 17:53, Wednesday 10 June 2015 (19057)
hinj user account created on h1hwinj1 machine

Following what was done recently at LLO, I have created a common hinj account on the LHO hardware injection machine h1hwinj1. To conform to security requirements, users cannot ssh into this machine using the common account, they must still use their own LIGO.ORG account. Once on the machine, they can set-user to access the hinj account. The plan is to run all injections (contuous and transient) using the hinj account.

H1 CDS
david.barker@LIGO.ORG - posted 17:41, Wednesday 10 June 2015 (19056)
GRB EPICS alarm

Dave Barker. WP5269

I have put together a quick EPICS alarm handler for Gamma Ray Bursts and Supernovae (GRB/SN) which runs on the operator alarm machine. It is called grbsn.alhConfig (in svn under cds/h1/alarmfiles).

The GRB alert system (which runs on h1fescript0) polls the GraceDB database every 10 seconds looking for External events (Gamma Ray Bursts and Supernovae). If an event is detected, its information is written to EPICS records which are hosted on the FE model h1calcs.

To put together a quick alarm system for ER7, I am using the alarm fields of the H1:CAL-INJ_EXTTRIG_ALERT_TIME record which records the GPS time of the trigger. By setting the HIGH alarm field to the current GPS time plus one second, when the next event is recorded this PV goes into the MAJOR alarm state.

The grbsn.alhConfig file provides the operator with two buttons:

[G] button opens the guidance text. It refers to the alog entry  https://alog.ligo-wa.caltech.edu/aLOG/index.php?callRep=19037

[P] button runs a script which resets the alarm level to the current event, turning off the current alarm

When a GRB/SN alarm is raised the operator should:

1. acknowledge the alarm to stop it beeping/flashing

2. press the [P] button to turn off the current alarm and prime the system for the next event

3. read the guidance to see if any further action is needed

Information on the current event can be obtained by running the script grb_latest_event_info.py. This gives you the event time as local time, so you can easily determine when the one hour stand-down time will expire.

Images attached to this report
H1 IOO
daniel.sigg@LIGO.ORG - posted 17:27, Wednesday 10 June 2015 (19055)
Strange IO alignment shift

(baffled control room crew)

After the most recent lock loss the IMC wasn't relocking and looked completely misaligned. The screenshot shows about 20 minutes of the previous lock, 30 minutes of confusion and 10 minutes on a new lock. The only dof which shows a signifcant change is the input pointing. Strange.

Images attached to this report
H1 General
jeffrey.bartlett@LIGO.ORG - posted 11:23, Wednesday 03 June 2015 - last comment - 10:26, Thursday 11 June 2015(18826)
Storage Dry Box May Data
Posted are data for the two long term storage dry boxes (DB1 & DB4) in use in the VPW. Measurement data looks good, with no issues or problems being noted. I will collect the data from the desiccant cabinet in the LVEA during the next maintenance window.   
Non-image files attached to this report
Comments related to this report
jeffrey.bartlett@LIGO.ORG - 10:26, Thursday 11 June 2015 (19073)
This is the data for the 3IFO desiccant cabinet in the LVEA.
Non-image files attached to this comment
H1 SUS
betsy.weaver@LIGO.ORG - posted 15:33, Thursday 28 May 2015 - last comment - 12:50, Thursday 11 June 2015(18669)
More ETM charge measurements

After a measurement of charge on each ETM yesterday, I took a few more on each today.  Attached show the results trended with the measurements taken in April and Jan of this year.  There appears to be more charge on the ETMs than in previous measurements, although there is quite a spread in the measurements.  The ion pumps at the end stations are valved in.

Images attached to this report
Comments related to this report
betsy.weaver@LIGO.ORG - 11:53, Friday 29 May 2015 (18695)

Note, the measurement was saturating on ETMy so Kiwamu pointed me to switch the ETMy HI/LOW Voltage mode and BIO state.  This made the measurement run with saturation.  Attached is a snapshot of the settings I used for the ETMy charge measurement.

Images attached to this comment
leonid.prokhorov@LIGO.ORG - 12:50, Thursday 11 June 2015 (19076)
1. I think that the results of charge measurements of ETMY on May, 28 are probably mistaken. I haven't see any correlation in dependence of pitch and yaw from the DC bias. 
2. It seems like there was very small response at ETMX LL quadrant at this charge measurements. Other ETMX quadrants are ok. It correlates with results of June, 10 https://alog.ligo-wa.caltech.edu/aLOG/index.php?callRep=19049 
Images attached to this comment
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