Displaying reports 61221-61240 of 85686.Go to page Start 3058 3059 3060 3061 3062 3063 3064 3065 3066 End
Reports until 20:35, Friday 22 January 2016
H1 General
edmond.merilh@LIGO.ORG - posted 20:35, Friday 22 January 2016 (25115)
Shift Summary - Evening

Apologies for no transition entry. I was tasked with locking as soon as I walked in.

TITLE: Jan 22 EVE Shift 00:00-07:11UTC (16:00-23:11:00 PDT), all times posted in UTC

STATE Of H1: Down

SUPPORT: Sheila,Evan, Gabriele

INCOMING OPERATOR: N/A

ACTIVITY LOG:

00:28  HFD on site as a matter of protocol for a faulty fire alarm panel

00:30 another fire unit on site

00:42  reloaded ISC_LOCK Guardian

00:45  HFD Off site. Three firetrucks drove past corner station during lock

00:46  Dave B called and informed me of an AC failure. He’s contacting the proper folks.

01:13  Dick out of optics lab

01:32  Bubba back on site to handle AC issue in H2 building

01:37 BS ISI St2 watchdog trip

01:38  cleared HAM6 ACT watchdog accumulation counter

02:18 GRB alert

02:51  Bubba has reported there’s nothing he can do about the AC in the H2 building tonight so he’s leaving it off. He also went into the CER to check on the AC in there. He didn’t think anyone had been in there to check since the power outage. It seemed ok.

04:xx Relocked at NLN. Gabriele has turned me loose into the world!

X1 DTS (DAQ)
david.barker@LIGO.ORG - posted 20:15, Friday 22 January 2016 - last comment - 21:46, Friday 22 January 2016(25118)
Test stand shut down for the weekend

We have a cooling problem with the H2 DTS building. Bubba came back in this evening to take a look at this, in the mean time we have powered down all DTS computers and DC power supplies for the weekend.

Comments related to this report
bubba.gateley@LIGO.ORG - 21:46, Friday 22 January 2016 (25119)
After an extensive search for the meaning of the error code displayed on both thermostats indicating a low pressure fault, which in and of itself is odd for both systems to have the exact same fault, I believe I have narrowed the problem down to faulty thermistors. This may have been caused by the recent power outage or may be simply coincidence.

Parts will need to be ordered next week.

I will follow up with a FRS.     
H1 ISC (ISC)
gabriele.vajente@LIGO.ORG - posted 20:12, Friday 22 January 2016 - last comment - 17:54, Saturday 23 January 2016(25117)
SRCL feed-forward retuning

 

I retuned the MICH feed-forward path. I injected noise in SRCL and measured the transfer function to DARM: TF_SRCL_DARM. Then I injected noise at the feed-forward input, with the FF shaping filters off, but with SBVio1 and SBVio2 on. I measured the transfer function from SRCLFF_IN2 to DARM: TF_SRCLFF_DARM. The optimal feed-forward filter should then be -TF_SRCL_DARM/TF_SRCL_FF. The first plot shows the measurement and the fit. Again, I decided not to fit the sharp features due to the  bounce and roll filters.

I implemented the new filter in the bank 'newFF' and engaged it. The performance improved, as shown by the  reduced coherence. The peak at 3 Hz also reduced a bit. See the second plot: green no feed-forward; blue old feed-forward, red new filter. The last plot compares the old (blue) and new (red) filters. With the new filter, I also switched on an AC coupling (double zero, double pole at 0.1 Hz).

Images attached to this report
Comments related to this report
gabriele.vajente@LIGO.ORG - 17:54, Saturday 23 January 2016 (25124)

Guardian code modified to load the new MICH and SRCL feedforward filters.

H1 ISC (ISC)
gabriele.vajente@LIGO.ORG - posted 19:33, Friday 22 January 2016 (25114)
MICH feed forward retuning

Sheila, Evan, Gabriele

We retuned the MICH feed-forward path. We injected noise in MICH and measured the transfer function to DARM: TF_MICH_DARM. Then we injected noise at the feed-forward input, with the FF shaping filters off, but with all the stop-band filters on and with the invBS filter on. We measured the transfer function from MICHFF_IN2 to DARM: TF_MICHFF_DARM. The optimal feed-forward filter should then be -TF_MICH_DARM/TF_MICH_FF. The first plot shows the measurement and the fit. We decided not to fit the sharp features due to the BS bounce and roll filters.

We implemented the new filter in the bank 'newFF' and engaged it. The performance improved, as shown by the improved DARM noise and reduced coherence. See the second plot: green no feed-forward; blue old feed-forward, red new filter. The last plot compares the old (red) and new (blue) filters. With the new filter, we also switched on an AC coupling (double zero, double pole at 0.1 Hz).

Images attached to this report
X1 DTS (CDS, DAQ)
james.batch@LIGO.ORG - posted 18:20, Friday 22 January 2016 (25112)
Rearrange file server exports
Reconfigure x1fs0 to export individual directories under /opt, rearrange nfs mounts for front ends, x1boot, and x1 DAQ computers.  This is to test proposed changes for the h1 system.
LHO General
patrick.thomas@LIGO.ORG - posted 16:09, Friday 22 January 2016 (25111)
Ops Day Shift Summary
SHIFT SUMMARY: Some locking success in the morning, but trouble in the afternoon with high winds and microseism. Jim W. tried putting the end stations on Quite_90 and enabling sensor correction. Ed took over locking attempts in the mid afternoon. The winds have come back down.

ACTIVITY LOG:
19:59 UTC Jeff B. and Nicole W. to LVEA to look at 3IFO baffles
20:06 UTC Stopping locking attempts while Jim W. runs transfer functions on ETMX
20:36 UTC Jeff B. and Nicole W. done
20:48 UTC Phone call from Hanford Emergency instructing personnel in 200 West to take cover
21:38 UTC Phone call from Hanford Emergency reporting the lifting of the take cover alarm
21:44 UTC Dick G. to optics lab
21:45 UTC Resuming locking attempts. Jim W. has put the end stations on Quite_90 and turned on sensor correction.
23:35 UTC Gerardo to mid X to retrieve empty tote
23:54 UTC Filiberto to mid X to check alarm on fire panel

Tour group in the control room around 19:50 UTC
Dave B. changed the vacuum overview medm on video1
H1 CDS (OpsInfo)
thomas.shaffer@LIGO.ORG - posted 16:07, Friday 22 January 2016 (25110)
Fixed Bug in Verbal and Saturations now just say optic name

Fixed bug: Previously, when Verbal could not connect to a channel through ezca, it would crash with an EzcaConnectError. Now it will make a small noise and write a notification that it cannot connect to the channel and repeat. This will begin to get very useful now that we are in the commission era.

Saturations will now just say the optic name.

I also removed the acknowledgement feature for the CW inj. It should still alert if the inj status changes, but operators do not have to acknowledge.

H1 ISC (ISC)
matthew.evans@LIGO.ORG - posted 15:58, Friday 22 January 2016 (25106)
Unidentified Noise with Coating Thermal Noise removed

I included the coating thermal noise (CTN) in the estimate made in entry 25039, and find that this changes little the conclusion.  It seems that the unidentified noise source has a slope close to 1/f.  Increasing the CTN estimate by 1.4 changes the conclusion, in that noise is more like 1/f^2.  I do NOT mean to suggest that this indicates higher CTN; that extra junk could be anything.  What this does mean is that we cannot use H1 to set a better limit than this (yet).

Images attached to this report
Non-image files attached to this report
H1 General
edmond.merilh@LIGO.ORG - posted 15:15, Friday 22 January 2016 - last comment - 18:33, Friday 22 January 2016(25109)
Switched EX/EY ISI blends to 45mHz

uSeism is approaching 1um/s and the winds have dies down to below 10mph.

Comments related to this report
edmond.merilh@LIGO.ORG - 18:33, Friday 22 January 2016 (25113)

I hadn't been informed about the sensor correction/Quite_90 situation when I was asked to lock the interferometer upon my arrival. We have ben locking steadily on the 45mHz blends all evening. I've just changed everything back to Quite_90 to have a look. OK, it looks good so far. Apologies, Jim there was a lack of communication.

H1 CDS (VE)
david.barker@LIGO.ORG - posted 14:51, Friday 22 January 2016 - last comment - 19:46, Friday 22 January 2016(25107)
New vacuum controls overview screen

WP5692 FRS4202

John, Kye, Gerardo, Dave:

I have modified the H0 vacuum overview screen to show an alarm border around bar monitor widgets. If the widet has no content, the alarm color is now visible in the border.

Images attached to this report
Comments related to this report
kyle.ryan@LIGO.ORG - 19:46, Friday 22 January 2016 (25116)
 Thanks Dave!

"no content", "no valid content", "value not valid for parameter represented", "something is broken" etc...
H1 SEI
hugh.radkins@LIGO.ORG - posted 14:29, Friday 22 January 2016 - last comment - 14:37, Friday 22 January 2016(25104)
Testing on Senscor Match Filters--leave SDF red unless we are going to observe--then accept, don't revert

Jim's testing some alternate filter on the ETM senscor Match filters for the beam line axis.  Leave the SDF red for SEI reminder of this.  If needing to green sdf for observation mode, please accept rather than reverting the settings on these.  Many thanks, TeamSEI.

Comments related to this report
hugh.radkins@LIGO.ORG - 14:37, Friday 22 January 2016 (25105)

Well, decided to go ahead and accept as the objective is to go to observe tonight.  We'll just have to remember.

LHO General
patrick.thomas@LIGO.ORG - posted 13:29, Friday 22 January 2016 - last comment - 13:40, Friday 22 January 2016(25101)
Hanford notification for 200 West
We received a phone call in the control room at 12:48 PST from Hanford Emergency instructing personnel in 200 West to take cover and close all doors and ventilation. Other personnel are instructed to stay clear.

Richard M. informs me that this does not affect us (other than to stay clear of 200 West).
Comments related to this report
patrick.thomas@LIGO.ORG - 13:40, Friday 22 January 2016 (25103)
We received another phone call in the control room at 13:38 PST informing us that the take cover was due to a false alarm and has been lifted.
H1 PEM (DetChar, PEM)
robert.schofield@LIGO.ORG - posted 11:38, Friday 22 January 2016 (25098)
End-O1 PEM injection report for LHO

Summary: most coupling at LHO was measured to be about the same as for the pre-run injections. Magnetic coupling was found to be lower in the CS ebay, and vibration coupling was found to be lower at the PSL periscope and at EX, as we were expecting. Since changes were for the better, we conservatively use the values from the start of the run and nothing has to change in estimates of noise from the environment. I also injected at locations we didn’t reach during the first round; there is low but interesting acoustic coupling at both mid-stations.

We make an abbreviated set of injections at the end of the run in case coupling changed after the pre-run injections (link to pre-run injection summary: Link). We made at least one magnetic and one acoustic injection in the LVEA, the 3 electronics bays, the two VEAs and the PSL. These were designed to show if any coupling changed significantly, in which case we would investigate using further injections.  For O1 end-of-run injections, all significant changes were improvements, so we change no estimates, and do not alter the coupling functions and estimated ambient levels from the beginning of the run.

In addition, we made several injections that were planned but that we did not get to in the September round. These included shaking of ETMX and Y, and of the beam tube at the mid station.

Vibration coupling at mid-station

The smallest clear aperture in the beam tube between the corner and end stations is associated with the mid-station cryopumps. For this reason, the beam tube is instrumented with accelerometers at the mid-stations. We first injected at the mid-station during the current round of PEM injections because of time limitations during the first round.

Shaker sweeps on the beam tubes revealed several sensitive frequencies, possibly resonances of scattering structures. Figure 1 shows a comb injection at MX with one of the lines centered on a putative resonance. The feature in DARM has the side-band structure that is typically produced by scattering coupling.  The acoustic line at 130 Hz is about 3 orders of magnitude above background, which was also the approximate excitation level needed to produce features in DARM at several other frequencies at MX (250, 315 & 170 Hz) and MY (150 Hz).

While the normal acoustic levels at the mid stations are not a problem, it is not difficult to increase the sound pressure level by 3 orders of magnitude. A loud bang in a mid-station VEA may show in DARM, as might bumping into the beam tube. I suggest that we emphasize that when we are in observation mode, we record in the log when people are working in the VEAs at the mid stations.

Shaking of ETMX and Y

I used piezo shakers mounted on the blue cross beams of the ETM BSCs. This increased the amplitude of motion by about 2 orders of magnitude between about 100 and 1800 Hz. No effect was noted in DARM.

Reduced magnetic coupling in CS electronics bay.

For pre-O1 PEM injections, the only magnetic coupling that would prevent us from reaching our sensitivity goals was magnetic coupling in the corner station electronics bay (Link).  The coupling function was not the highest, but in combination with the high magnetic noise level in the ebay, the pre-O1 coupling would limit us to about 1e-18m/sqrt(Hz) at 12 Hz. However, Figure 2 shows that this coupling was found to be greatly reduced during the post-O1 injections. It is not clear when this improvement was made, but Richard remembered several activities in the ebay that could have improved cable shield connections etc., during the two weeks between when the measurements were made and the start of the run. 

Reduced acoustic coupling at EX.

We expected that the high acoustic coupling measured at EX (Link) would be reduced when the beam diverter was finally closed (Link) on Oct. 6. Post run injections showed that it was indeed reduced by a factor of about 5 in the 50-120 Hz region.

Reduced coupling at PSL

The coupling in the PSL was changed Oct. 13 2015 when I epoxied the top mount on the periscope and fine tuned the peak frequencies using weights. This removed peaks around 300 Hz from DARM (Link). Figure 3 shows the new estimated levels of ambient noise. One peak is very near showing in DARM, but we hope that reductions in jitter coupling, towards the level at LLO, will keep this from limiting us.

Non-image files attached to this report
H1 CDS
evan.hall@LIGO.ORG - posted 10:52, Friday 22 January 2016 - last comment - 13:38, Friday 22 January 2016(25096)
Certain elliptic filters crash foton

Sometime between last night and today, foton seems to have become unable to generate certain elliptic filters of high order.

For example: choose elliptic band pass, first frequency 5 Hz, second frequency 500 Hz, fifth order, 1 dB ripple. Foton freezes as soon as you click ok. Same for a sixth-order elliptic bandpass, and a fifth-order elliptic low-pass.

Last night, we were able to generate fifth-order elliptic filters no problem. What happened between then and now?

Comments related to this report
jeffrey.kissel@LIGO.ORG - 13:38, Friday 22 January 2016 (25102)CDS
H1 ISC
kiwamu.izumi@LIGO.ORG - posted 13:24, Monday 18 January 2016 - last comment - 15:28, Wednesday 27 January 2016(25009)
f^{-0.5} noise in DARM ?

Evan, Kiwamu,

As some of us have already noticed, there is a broadband noise with a 1/f^{0.5} shape in frequency from 60 to 200 Hz. This noise is unidentified.

Do not believe any statements in this report until futher analaysis. Something is fishy with the claibration of the cross-spectrum.

We are planing to check how stable this noise level is over the course of the entire O1.

 


The below shows an example spectrum of DARM.

Blue curves are twenty spectra of DARM (aka C01 frame, converted into displacement), each of which is made by the Pwelch with Hanning, detrended, 50% overwrap for a 12 minutes time series. The data starts at a GPS time of 1134604817. Green curves are the square-root of twenty cross-power-spectra of DCPD A and B which are reconstructed from the sum and null streams of the DCPDs. The DARM suppression effect was removed from the sum signal. The cross-spectra are then calibrated to the displacement using the latest O1 DARM model of the calibration group. No time varying correction (i.e. kappas) is applied. Red line is a 1/f^{0.5} line to show how steep the slope of the green curves is. I also attach the fig file.

Images attached to this report
Non-image files attached to this report
Comments related to this report
kiwamu.izumi@LIGO.ORG - 20:42, Tuesday 19 January 2016 (25039)ISC

Gabriele, Evan, Kiwamu

The spectral shape seems to be 1/f in the range from 50 to 150 Hz rather than 1/f½.

There was a human-error in my code for calibrating the cross-spectrum. It was removing the loop suppression after the power spectrum of the null stream was subtracted from that of the sum stream. This was fixed such that the subtraction happens after the removal of the suppression in the sum spectrum. The below is the latest plot.

 

The plot shows the ampitude spectral desnsities of the calibrated darm displacement (aka C01) and the calibrated cross-spectrum. The cross-spectrum should represent noises which are coherent between two OMC DCPDs.

As a coarse verification, I have eye-ball-fitted the shot noise level with the fixed cavity pole frequency of 341 Hz (shown as a dotted line in cyan). Then I subtracted the shot noise component quadratically out from the actual displacement spectrum (in black). The residual (in blue) agrees with the estimation from the cross-spectrum. In order to check the slope of the cross-spectrum, I also drew a 1/f line. The cross-spectrum seems to follow 1/f from 50-ish Hz to 150 Hz.

The fig file is attached as well.

Images attached to this comment
Non-image files attached to this comment
matthew.evans@LIGO.ORG - 14:52, Friday 22 January 2016 (25108)

An update can be found in entry 25106

kiwamu.izumi@LIGO.ORG - 15:28, Wednesday 27 January 2016 (25211)

A higher resolution version is attached. The frequency resolution is set to 0.1 Hz, 50% overlap with Hanning for 1 hour data. No new findings.

The 1 Hz comb feature (see for example alog 24695) is becoming visible in 20-50 Hz. By the way, the legend in the plot is wrong.

Images attached to this comment
Non-image files attached to this comment
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