Displaying reports 70221-70240 of 85044.Go to page Start 3508 3509 3510 3511 3512 3513 3514 3515 3516 End
Reports until 16:00, Friday 21 November 2014
LHO General
patrick.thomas@LIGO.ORG - posted 16:00, Friday 21 November 2014 (15237)
Ops Summary
07:03 Karen cleaning in LVEA
08:11 Jeff B. and Andres to LVEA west bay
08:23 Jeff B. and Andres back
08:41 Jeff B. and Bubba to LVEA to look at container
08:43 Filiberto and Aaron to end Y to work on PEM
08:52 Cris checking mid and end stations for cleaning
08:56 Jeff B. and Bubba moving storage containers in LVEA (no craning)
08:57 Travis to LVEA teststand to work on suspension
09:21 Keita to end X to work on green WFS
09:32 Jeff B. and Bubba done
09:32 Travis done
10:10 Cris done
10:40 Jeff B. turned on dust monitor 10 (under cleanroom for 3IFO work)
11:02 Gerardo to H2 PSL laser enclosure to work on OFI
11:09 Cris dropping off frocks at end X
11:22 Bubba taking U.S. Linen to mid and end stations (not in VEAs)
11:25 Keita done
12:04 Hugh and Jim W. checking boards at ITMX
12:13 Filiberto and Aaron done (also labeled cables at end X)
12:25 Hugh and Jim W. done
12:25 Gerardo done
13:48 Corey looking for cables in squeezer bay
14:06 Corey done
15:02 Gerardo back to H2 PSL laser enclosure to continue work on OFI
H1 SEI
jim.warner@LIGO.ORG - posted 15:32, Friday 21 November 2014 (15236)
ITMX CPS issues still a mystery

Sheila noted a while ago ITMX was having weird CPS trips. Hugh and I went out during lunch and checked all of the chamber CPS cable connects as best as we could, but we didn't find any loose cables. Some of the the corner 1 cables (over the TCS table) are missing nuts, but the power boards are all secure on all 3 racks, and all cables seem to be well connected otherwise. On Tuesday, we plan on going out with a Genie and look at fixing the missing connectors on corner 1, if possible.

H1 SEI
jim.warner@LIGO.ORG - posted 15:28, Friday 21 November 2014 - last comment - 16:05, Friday 21 November 2014(15235)
Beamsplitter sensor incorrection

While commissioners were MIA this morning I took the time to try sensor correction at the beam splitter again. Previously, I had found that it pretty much just made stuff worse, at least when I tried HEPI Z. Unfortunately, that still seems to be the case. This time I tried HEPI Z, and ISI X & Y, and in every case it just made things slightly worse. My attached plot shows a comparison between the ISI X for the BS (red) and ETMX (blue). Sensor correction is off  for the dashed traces, on for the solid. ETMX shows our expected improvements, but the BS gives no joy. Also interesting that the BS doesn't seem to be performing as well as the ETMX generally, but the mechanical and controls configurations are quite different. I've talked to Hugh, and the input and output matrices have errors on the BS (not on ETMX), and the STS2 the BS uses is a little wonky, it reads ~2000 cts, while the other cornerstation seismometers are in the hundreds. The STS spectra all  look similar in the .1hz and above region, but they disagree a bit below, see my second plot. When I get a chance, I'll try using a different seismometer, but I'm pretty sure I've gotten positive results at ITMX using the BS seismometer.

Images attached to this report
Comments related to this report
krishna.venkateswara@LIGO.ORG - 16:05, Friday 21 November 2014 (15238)

K. Venkateswara

It looks like you may have the sign of the sensor correction wrong. It looks like you are adding instead of subtracting the ground, hence the result looks a factor ~2 higher. Have you tried the opposite sign?

H1 SUS
travis.sadecki@LIGO.ORG - posted 14:38, Friday 21 November 2014 (15232)
3IFO QUAD 07 Spectra and improvement attempts

In an attempt to improve (?) previous TF data from QUAD 07, today I checked the cabling connections to both chains and added wipes around connectors that were touching the structure/test stand.  I then retook the RO R TF (which showed an unexpected DC offset).  The results showed no improvement and looked identical to the previous round of measurements.

I also swapped an L2 AOSEM that was showing low counts and retook spectra for all stages.

Attached are the spectra for QUAD 07.  L1 and L2 flags are not aligned.

Non-image files attached to this report
H1 SUS
alexan.staley@LIGO.ORG - posted 14:36, Friday 21 November 2014 (15233)
PRM offloaded hierarchy switch now

Alexa, Shiela, Nic

 

We forgot to post this yesterday ...

Our ASC offloading script had offloaded the wfs to the offset of M2_LOCK_P/Y. Once we ran the script, we noticed that we kicked SRM because SRM is under an offloaded hierarchy, whereas PRM is distributed (BS is also offloaded, but we never feedback to MO P, Y so these filters are off). Looking through all of the optics that we feed back to, only PRM is left under distrubted control, so we decided to swtich PRM from distrubted to offloaded. Our length control scheme for PRM is the same for both these configurations, so this transition was smooth.

We also modified the ASC offloading script to offload the wfs to the M2_DITHER offsets. This signal is always on and is not sent to another stage, so should be okay now. 

H1 CDS
patrick.thomas@LIGO.ORG - posted 13:17, Friday 21 November 2014 (15229)
Updated Conlog channel list
Removed the following channels:

H1:ALS-C_COMM_VCO_TUNEOFS
H1:ALS-Y_CAM_ITM_PIT_POS
H1:ALS-Y_CAM_ITM_SUM
H1:ALS-Y_CAM_ITM_YAW_POS

These have been added to the exclude list.
H1 SUS
betsy.weaver@LIGO.ORG - posted 11:59, Friday 21 November 2014 (15227)
MC bias saved

Over the last few days of Gabriele's MC WFS work the MC SUS bias sliders were tweeked.  We agreed to save these new slider settings since the WFS offsets are coming in via a different path anyways.  The guardians for MC1, MC2, MC3 are now green again.

H1 PSL
gabriele.vajente@LIGO.ORG - posted 11:53, Friday 21 November 2014 (15223)
Beams dumped on IOT2R - better, but not yet good

[Sudarshan, Gabriele]

Following up on yesterday's activity, today we properly dumped the beams on IOT2R. We tried different configurations: beam dump directly in place of the first mirror of the periscope, razor beam dumps, black glass plate, black galss beam dump. Finally, the best configuration is the one that lets the beams go through the periscope (recentering all three mirrors) and dump the REFL beam far away with a  black glass angled beam dump, and the IMC trans beam with a razor blade dump. See the attached pictures for more details.

With this configuration, we measured the out-of-loop intensity noise with MC2_TRANS, as before with the PRM aligned and the BS misaligned to avoid flashes. After many trials, we could geth the 18 Hz peak down by a factor 10, as shown in the 5th figure. Green is PRM aligned, ISS second loop off, before our modification. Brown is PRM aligned, ISS second loop on, before our modification. Red same as the last one, but aftr the modification.

The IMC transmission beam is not critical, and even leaving it undamped doesn't change much. Instead, the dumping of the REFL beam is critical. By simply tilting the beam dump of a very small angle (order of one degree), we could change significantly the amount of intensity noise. We tried many times to tweak the angle. Once we could make the 18 Hz completely disappear, but then just the action of clamping down the beam dump wornsed the situation. We think it's not really worth to spend more time on this, since a small change of the PRM alignment will in any case move the beam and probably spoil the noise reduction. The last figure shows a comparison of the intensity noise with different beam dump positions. Blue is before the modification, the other traces correspond to sligthly different beam dump positions. We also tried to rotate the beam dump 90 degrees, to have the black glass plates oriented "horizontally', but this didn't help either.

In conclusion, now the situation is much better than before, but the REFL beam transmitted by IM4 and collected on IOT2R is very critical. We should consider a better solution for the long term. For future reference, the last picture shows which beam we are talking about: the purple beam is the REFL beam transmitted through IM4 and sent otto IOT2R where it is reflected/scattered back to IM4, then reflected off the IM4 HR face and finally going to the ISS aray (green beam)

Images attached to this report
H1 AOS
edmond.merilh@LIGO.ORG - posted 10:28, Friday 21 November 2014 - last comment - 11:11, Friday 21 November 2014(15217)
Functionality Investigation of SUS Aux Channels/Monitors cont.

These are the results of the ETMX excitations to test for working channels. Again, 4hz/10cts/pitch

Images attached to this report
Comments related to this report
edmond.merilh@LIGO.ORG - 11:11, Friday 21 November 2014 (15221)

Here, also are the related TMSs

Images attached to this comment
LHO FMCS
john.worden@LIGO.ORG - posted 07:56, Friday 21 November 2014 - last comment - 14:26, Friday 21 November 2014(15212)
Temperature control LVEA/VEA

Bubba and I have stabilized the LVEA and VEA temperatures.

We still have known mechanical issues which are probably impacting the control loops so we should be able to improve things - especially XEND.

The one degree spike at XEND on the 19th was due to my attempt to outsmart the system.

Motorized variac heater controls are being ordered for the two end stations which should allow for better control and transient behavior.

We may be asking to raise the set point at XEND - so if anyone has thoughts on this please let us know.

Images attached to this report
Comments related to this report
daniel.sigg@LIGO.ORG - 11:08, Friday 21 November 2014 (15219)

On the evening of the 19th commissioners noticed large angular drifts on ETMX, see alog 15193. The attached plot shows temperature in end X over the past 3 days as well as the optical lever readouts. There is a clear correlation between temperature and optical lever readouts. The trace of the 0.8 C excursion on the 19th in the optical levers is obfuscated by several re-alignments of ETMX. One might wonder, if the optical lever temperature fluctuations correspond to actual optical alignment changes, or if they are just an optical lever feature. Since large alignment drifts were reported on the 19th, one might suspect the former.

Alignment changes of the order 0.5–1 µrad will require a re-alignment of the arm cavity.

Non-image files attached to this comment
daniel.sigg@LIGO.ORG - 11:29, Friday 21 November 2014 (15224)

Looking at a trend from 3 weeks ago shows that the temperature is now oscillating with a ~2.25 h period and an amplitude of ~0.15ºC.

Non-image files attached to this comment
daniel.sigg@LIGO.ORG - 11:58, Friday 21 November 2014 (15225)

Here is an LLO alog describing a measurement of the angular misalignment when their HVAC system was shut off. One can deduced a temperature dependency around 35 µrad/°C in pitch, see alog 13817. Yaw seems relatively stable. With a requirement of 0.5–1 µrad the temperature stability would need to be around 0.02ºC.

The other thing noteworthy is that it takes less than an hour for the vertical position to turn around after the HVAC system was engaged. This would indicate that the dominant thermal coupling is radiative through the chamber walls, and not conductively through the ISI. The reaction time of the ISI is of order 36 hours—which could be responsible for the long tail seen in restoring the position.

peter.fritschel@LIGO.ORG - 12:36, Friday 21 November 2014 (15228)

The calculation made by Brett in the above referenced link, as well as the measurements of pitch vs temperature that are reported by Stuart A in the LLO log, correspond to the pitch of the TOP mass of the quad suspension. According to the suspension model, the test mass pitch is 25% of the TOP mass pitch. So, the 30-40 urad/C for the TOP mass translates to 8-10 urad/C for the test mass. So 1 urad corresponds to 0.1 C. Still quite sensitive, but not so bad.

daniel.sigg@LIGO.ORG - 14:26, Friday 21 November 2014 (15231)

Not sure, if this still agrees with the observed optics drift. If I interpret the plot in alog 13639 correctly, the HVAC system was off for about 20 h, in which the temperature was rising by ~3.2 F. Assuming a linear trend we get 90 mK/h, or 15 mK in 10 minutes. The optics was drifting 0.5 µrad in 10 minutes. So, we get ~34 µrad/K at the optics.

On the other hand, looking at the temperature oscillations in EX we would expect to see 10 µrad-pp, but only see 1 µrad-pp. A time constant of ~1 hour would correspond to a pole frequency around 50 µHz which is abount 2.5 times slower than the observed oscillation. Assuming this leads to an attenuation of 8 dB, a reduction of 25% through the suspension chain would explain what we see in the optical lever.

H1 ISC
evan.hall@LIGO.ORG - posted 01:38, Friday 21 November 2014 - last comment - 12:17, Friday 21 November 2014(15209)
Some diagnostics on DRMI3f+arms

Kiwamu, Stefan, Nic, Evan

First, some troubleshooting:

After troubleshooting, we were able to get to DRMI3f+arms with a reasonable duty cycle, so we moved on to the problem of the CARM handoff.

Instead of pursuing sqrt(TRX+TRY), we looked at REFL9I. Surprisingly, we found no response in this signal in response to different CARM offsets. We thought this might be due to bad IR alignment into the arms, so we unlocked everything, then locked the Y arm in IR, and adjusted ETMY to maximize the transmitted IR power. This improved the buildup in Y by a factor of 3, but REFL9I continued to be nonresponsive. While locked, we tried some further tweaking of the ETM alignments, with no success. Relevant UTC times: 2014-11-21, from 09:00:00 to 09:30:00.

Comments related to this report
stefan.ballmer@LIGO.ORG - 12:17, Friday 21 November 2014 (15226)
Here are some REFL and arm TRANS signals from yesterday.

The span is 1h30min. The last 10 min or so was the "realigned" lock attempt last night. Still digesting.
Images attached to this comment
H1 SUS
nicolas.smith@LIGO.ORG - posted 23:33, Thursday 20 November 2014 - last comment - 11:09, Friday 21 November 2014(15208)
ETMX control was completely changed on Tuesday, no elog record

(Stefan Evan Kiwamu Nic)

We found the ETMX suspension was changed back to distributed control on Tuesday Nov 18, 2014 at 19:14. There was no elog documenting this. We expect this was an error (or maybe a BURT restore?). It's very surprising that we were still able to do ALS control at all in the interim.

The ETMs had been distributed for a long while, but were changed to offloaded while diagnosing ALS DIFF issues.

We've now changed it back to offloaded.

Comments related to this report
david.barker@LIGO.ORG - 11:09, Friday 21 November 2014 (15220)SUS

conlog reports only H1:SUS-ETMX_HIERSWITCH changed around this time on SUS ETMX, so no indication of a burt restore. Here is the conlog report of this channel from Tue morning until now

Images attached to this comment
H1 SEI (ISC, SEI)
sheila.dwyer@LIGO.ORG - posted 01:53, Thursday 20 November 2014 - last comment - 11:10, Friday 21 November 2014(15193)
sensor correction turned off, back on now.

Nic ran Jim's script. 

Earlier tonight, we had a large drift in ETMX pitch (1 urad over about 7 minutes).  I turned off the sensor correction (ETMX ISI X only) for the last several hours, this seemed to help.  Now I've turned it back on so we can see if this continues to happen overnight.  

We are leaving the arms locked in green, and the mode cleaner locked.  This should give a chance to see if the mode cleaner is really stable when there is no actuation on it.  

Comments related to this report
fabrice.matichard@LIGO.ORG - 08:00, Thursday 20 November 2014 (15194)

Thanks Sheila, for reporting this.

I looked for minutes long features into the ISI CPS, at 0am and 4am, but did not find anything obvious over such low frequencies. However, I don't understand why the vertical Stage 1 CPS signal is so low. The local CPS signals should be quite larger if the platform was well isolated. I am getting inertial sensors and optical levers data to look into more details.

Images attached to this comment
fabrice.matichard@LIGO.ORG - 08:51, Thursday 20 November 2014 (15196)

[Rich, Fabrice]

At  0am, the time series show a large drift in ETMX SUS top mass, not only in pitch but also in longidudinal, see first plot  (the ylabel should say "nm").  According to the Stage 1 T240s (second plot), the ETMX ISI was performing as well as the other units, but this doesn't tell us anything about slow drift, so we need to get back to CPS data (maybe look at the rotations in the cartesian basis for the non-corrected CPS signals).

At  4amETMX SUS drift has stopped (third plot), though the sensor correction seems to be on (fourth plot).

Images attached to this comment
krishna.venkateswara@LIGO.ORG - 08:57, Thursday 20 November 2014 (15197)

K. Venkateswara

One thing to note is that turning sensor correction on is somewhat equivalent to blending at still lower frequencies than the normal 45 mHz. This makes it very sensitive to ambient ground tilt (caused by human activity or wind). It should not be used if there are people/activity near the ground seismometer.

Using tilt-subtraction makes sensor correction less susceptible to wind-induced tilt but unfortunately BRS is very sensitive to gravity gradients from people. So walking near the BRS when it is being used can cause very large low frequency signals to show up in the super-sensor.

sheila.dwyer@LIGO.ORG - 14:43, Thursday 20 November 2014 (15200)

Should we ask the operators to turn off the sensor correction at End X if they know someone is headed down there?

krishna.venkateswara@LIGO.ORG - 16:22, Thursday 20 November 2014 (15204)

Did you and Evan go there around 6 PM? The attached plot shows a spike at ~6:20 PM

In general, yes, it would be better to turn off sensor correction along the horizontal directions during the day if there is a chance of someone being close to the ground seismometers.

Images attached to this comment
richard.mittleman@LIGO.ORG - 07:28, Friday 21 November 2014 (15211)

Yes Sensor correction should not be on if there is any activity in the VEA.

 

 Sensor correction is a form of feed forward so it assumes that the chamber and ground sensor are seeing the same thing. So someone walking by the ground sensor, making a large local disturbance can produce  large motions in the platform

fabrice.matichard@LIGO.ORG - 08:18, Friday 21 November 2014 (15214)

[Rich, Seb, Fabrice]

We are now looking into HEPI to see if it caused the drifts that was observed on the ETMX suspension. Sebastien is processing the data. 

Please let us know if this is not anymore of interest because the cause of problem is now known (for instance related to John's comment on temmperature, or Nic's comment on suspension control).

 

 

daniel.sigg@LIGO.ORG - 11:10, Friday 21 November 2014 (15222)

A 1ºC temperature excursion was reported in alog 15212.

H1 SEI (SEI)
richard.mittleman@LIGO.ORG - posted 15:49, Wednesday 19 November 2014 - last comment - 14:47, Friday 21 November 2014(15168)
BSC-CPS Noise

There has been some concern that there might be excess cps noise in some of the channels. So i looked at 20 minutes of data at 1am sunday night/monday morning.

Looking only above 30Hz where the sensors have hit the noise floor, all of the coarse channels are similar and between 3.5-4.5E-10m/rrtHz about what we expect.

The stage 2 channels show two outliers, ITMX H2 and ITMX V1, maybe BS H2 also but that is close enough so that it could just be at a large offset (we expect the noise floor to go as the gap squared) I'll check that.

 

  The first thing to do is for me to look at another time, and to check the cables and connections for those sensors

 

I looked at a second data set calling it "B" (24 hours later)  ST2 ITMX H2 and ST2 ITMX V1 still show excess noise BS H2 is down to 4.5-5E-10m/rtHz which is a little bit noisy, but probably within what we are calling acceptable. I attached the data because Jeff asked to see the ADC noise on the plot

 

When I say large offset I mean > 10000 counts, so 1200 counts is centered for this discussion 

Non-image files attached to this report
Comments related to this report
hugh.radkins@LIGO.ORG - 11:57, Wednesday 19 November 2014 (15170)

ITMX Stage2 H2 & V1 CPS offsets are 900 & 3800 counts.  While V1 is actually the largest offset of all the BSC CPSs, H2 is 21st of 30 (towards the bottom) of Stage2 CPS offsets.  At 1200cts, BSC2 H2 ranks 17th of 30.  So the offset maybe an issue for ITMX V1 but the others...?  And, what about ITMY V1 at 3700 counts and ITMX V3 at 3200?

 

Attached are all the BSC medms showing the offsets.

Images attached to this comment
fabrice.matichard@LIGO.ORG - 14:50, Wednesday 19 November 2014 (15177)

Some additional info regarding the CPS - On the figures are plotted time series, integrated RMS, and  ASD down to low frequencies. Somme comments:

 

- At high frequencies, not much to add on sensor noise (ITMX and BS both have two CPS untis with elvevated sensor noise on Stage 2).  I looked at data of the Nov 17th, 18th and 19th, and get similar results.

- All Stage 1 CPS units are within 1um p2p, except BS horizontal that is moving 4 times more. Something to look into.

- At the microseism, the three vertical sensors are moving in sync, on all stages of all platforms. Probably normal  (the platform is inertially decoupled down to the micro-seism with th 90 mHz blends)

- The low frequency motion amplification is about 100 times larger in the vertical directions than it is in the horizontal directions.

Images attached to this comment
fabrice.matichard@LIGO.ORG - 14:58, Wednesday 19 November 2014 (15182)

The 5 figures in the previous log are for data ten on the 17th at 3pm PT. 

Results and comments are similar for the 18th and 19th, except for ETMX (attached plot) that shows different behavior at low frequencies, as expected with the sensor correction that was turned on Tuesday. It also shows features on Stage 2 at the SUS resonances, that might need to be doubled checks.

Images attached to this comment
sheila.dwyer@LIGO.ORG - 14:47, Thursday 20 November 2014 (15201)

Could this be related to the trips on ITMX?  (alog 15021

richard.mittleman@LIGO.ORG - 14:47, Friday 21 November 2014 (15234)SEI

this log seems to have gotten hijacked

 

I check the HAM-CPS and they all seem to be good at high frequency

Non-image files attached to this comment
H1 SEI
sheila.dwyer@LIGO.ORG - posted 16:19, Wednesday 12 November 2014 - last comment - 19:17, Friday 21 November 2014(15021)
ITMX has a problem

Here is a collection of suspicious CPS trips on ITMX.  This is a problem only on this chamber, which has just cropped up in the last few weeks.  It needs to be investigated. 

Images attached to this report
Comments related to this report
sheila.dwyer@LIGO.ORG - 22:13, Wednesday 12 November 2014 (15026)

another example

Images attached to this comment
sheila.dwyer@LIGO.ORG - 19:19, Tuesday 18 November 2014 (15153)SEI

Still there, still a problem....

Images attached to this comment
nutsinee.kijbunchoo@LIGO.ORG - 19:17, Friday 21 November 2014 (15241)SEI
I made a few plots today. The spectrum of the CPS right before and right after the trip, and the zoom-in time series plot around the time of the trip. I notice that the time that the CPS signal goes down does not match the GPS time indicated the trip exactly (off by a few hundred milliseconds).

While making the spectrum I also notice the peak near 4Hz in the "beforetrips" spectrum plot. So I went and look at the LHO summary page and found that there's a small gaussian-looking bump around 4Hz that seems to appear everyday. Probably not very important but just wanted to point that out.

Also, please note that V2, H2, and H1 signals are almost perfectly overlapped (that's why you only see two colors). 

I'll start looking into other related channels that *should* have seen the signals. Although I believe this might be an electronics issue.
Images attached to this comment
H1 SUS
jeffrey.bartlett@LIGO.ORG - posted 16:01, Wednesday 24 September 2014 - last comment - 14:01, Friday 21 November 2014(14130)
Phase 1B Test Results for Quad-09
Ran a first set of TFs for 3IFO-QUAD09. The undamped plots look OK (pitch is a bit off). The damped plots measurements do not match the model between .1 and 20Hz very well, for both the Main and Reaction chains. Will investigate the cause. Plots are attached.  

As Betsy noted in aLOG 14128 the second pitch mode shift is present as for the other 3IFO Quads tested to date. 

All files, plots, and scripts have been commited to SVN.     
Non-image files attached to this report
Comments related to this report
travis.sadecki@LIGO.ORG - 14:01, Friday 21 November 2014 (15230)

Spectra for this quad attached.

Non-image files attached to this comment
Displaying reports 70221-70240 of 85044.Go to page Start 3508 3509 3510 3511 3512 3513 3514 3515 3516 End