Displaying reports 56181-56200 of 86875.Go to page Start 2806 2807 2808 2809 2810 2811 2812 2813 2814 End
Reports until 16:49, Wednesday 16 November 2016
H1 SUS
sheila.dwyer@LIGO.ORG - posted 16:49, Wednesday 16 November 2016 (31553)
more notching of triple modes in top mass damping

Although Jeff and I reduced the appearance of triple bounce and roll modes in DARM by adding notches to the top mass damping for the HSTS (30970), there are still a few modes that show up. 

The largest in our last lock was at 28.2 Hz, which belongs to PR3 according to the resonances wiki and Jeff's measurement in 30646.  We had no notches for the HSTSs so I have added notches 1 Hz wide centered around 28.2Hz and 44.2 Hz for PR3 and SR3.  

The other thing which is large in our spectrum from last night is the remaining 40.9375 Hz mode from PR2.  I am not sure why the PR2 mode shows up in DARM larger than the others.  I looked at spectra of the osems to see if there is more noise on the PR2 osems.  The attached screenshot shows that the top mass osems for PR2 aren't any more noisy than PRM, but there is extra noise in the lower stage osems for PR2, and a large comb.  This might be noise in the readback only.  

I made the notches in the damping loops 20dB deeper for PR2, we will see if this helps in the next lock. 

Images attached to this report
H1 SUS
nutsinee.kijbunchoo@LIGO.ORG - posted 16:35, Wednesday 16 November 2016 (31552)
First harmonics violin mode table is now up-to-date

Last updated Nov 11, 2016

https://lhocds.ligo-wa.caltech.edu/wiki/Violin_Mode_Table_v2

LHO General
thomas.shaffer@LIGO.ORG - posted 16:20, Wednesday 16 November 2016 (31539)
Ops Day Shift Summary

TITLE: 11/17 Day Shift: 16:00-00:00 UTC (08:00-16:00 PST), all times posted in UTC
STATE of H1: Lock Acquisition
INCOMING OPERATOR: Corey
SHIFT SUMMARY: 16hr lock ended a few hours before the end of my shift. Things seemed to be misaligned after and it took me a bit, and with much help, to get it through an initial alignment. Handling off to Corey who may need to do another IA.
LOG:

LHO General
corey.gray@LIGO.ORG - posted 16:20, Wednesday 16 November 2016 (31551)
Eve Transition Summary

TITLE: 11/16 EVE Shift: 0:00-08:00 UTC (16:00-0:00 PST), all times posted in UTC

STATE of H1: Lock Acquisition
OUTGOING OPERATOR: TJ
CURRENT ENVIRONMENT:
    Wind:  under 5mph
    Primary useism:  Not changing much over last 24hrs
    Secondary useism:  --
QUICK SUMMARY:

TJ is still here and he & Jenne are addressing issue with Initial Alignment (current issue is with SRC Align).  This is all after a 16hr lock.  

Next up:  IM alignment tweak from Cheryl (& then tweak Initial Alignment to address that tweak....so skip Green Arms/ALS & start with INPUT_ALIGN).

Then we'll go back to locking.

LHO VE
kyle.ryan@LIGO.ORG - posted 15:53, Wednesday 16 November 2016 (31550)
Manually (remotely) over-filled CP3
Significant exhaust thermal couple response in 19 seconds after changing the as found control valve setting of 16% open to 50% open.  


Chandra's adjustment to 16% following yesterday's LN2 delivery looks to be an ideal value for the current LN2 column height in the storage tank.
H1 TCS
nutsinee.kijbunchoo@LIGO.ORG - posted 14:55, Wednesday 16 November 2016 (31547)
Corner station HWS code running again

After I left them off for camera glitch investigation (alog31456). Both IX and IY. ETM hws code also restored after hwsmsr restarted. I don't remember having to restart ETMY by hand. Maybe I did but I just forgot that I did.... Or it could be a glitch in the Matrix. I'll keep this in mind for next time.

H1 CAL
jeffrey.kissel@LIGO.ORG - posted 14:46, Wednesday 16 November 2016 (31546)
PCALX Roaming Calibration Line Frequency Changed to 4301.3
After a week's worth of struggle with the h1oaf computer, and alignment loop instabilities, we've been blessed with another 16 hour lock stretch. As such, we've got sufficient amount of data for the roaming calibration line to move it from 4001.3 Hz to 4301.3 Hz. 

Though the line has been at 4001.3 Hz for 5 days, I recommend only using data from the two long lock stretches in that time from Nov 12 2016 05:00:00 UTC to Nov 12 2016 21:00:00 UTC and Nov 16 2016 06:00:00 UTC to Nov 16 2016 22:00:00 UTC. However, note that the mean laser power is different from the one lock stretch to another -- 29.5 [W] for the Nov 12 stretch, and 31.1 [W] for the Nov 16th stretch.

Current Schedule Status:
Frequency    Planned Amplitude        Planned Duration      Actual Amplitude    Start Time                 Stop Time                    Achieved Duration
(Hz)         (ct)                     (hh:mm)                   (ct)               (UTC)                    (UTC)                         (hh:mm)
---------------------------------------------------------------------------------------------------------------------------------------------------------
1001.3       35k                      02:00                   39322.0           Nov 11 2016 21:37:50 UTC    Nov 12 2016 03:28:21 UTC      ~several hours @ 25 W
1501.3       35k                      02:00                   39322.0           Oct 24 2016 15:26:57 UTC    Oct 31 2016 15:44:29 UTC      ~week @ 25 W
2001.3       35k                      02:00                   39322.0           Oct 17 2016 21:22:03 UTC    Oct 24 2016 15:26:57 UTC      several days (at both 50W and 25 W)
2501.3       35k                      05:00                   39322.0           Oct 12 2016 03:20:41 UTC    Oct 17 2016 21:22:03 UTC      days     @ 50 W
3001.3       35k                      05:00                   39322.0           Oct 06 2016 18:39:26 UTC    Oct 12 2016 03:20:41 UTC      days     @ 50 W
3501.3       35k                      05:00                   39322.0           Jul 06 2016 18:56:13 UTC    Oct 06 2016 18:39:26 UTC      months   @ 50 W
4001.3       40k                      10:00                   39322.0           Nov 12 2016 03:28:21 UTC    Nov 16 2016 22:17:29 UTC      days     @ 30 W
4301.3       40k                      10:00                   39322.0           Nov 16 2016 22:17:29 UTC                                  
4501.3       40k                      10:00
4801.3       40k                      10:00  
5001.3       40k                      10:00

Images attached to this report
H1 PEM (PEM, SYS)
richard.mccarthy@LIGO.ORG - posted 14:30, Wednesday 16 November 2016 (31545)
Anemometer Replacement
Began replacing the Anemometers on the weather stations.  Taking longer than anticipated as the stations are not in the same orientation as they were pre roofing.
The corner station is done and EndX is complete.  I had to rotate the mounting hardware so the Anemometer could point in the proper direction for 0deg.
Everything seems to be functioning.  This may also explain the complaints about the wind direction being broken in previous posts.
H1 DetChar (DetChar, ISC)
gabriele.vajente@LIGO.ORG - posted 13:38, Wednesday 16 November 2016 (31544)
BruCo scan

Here's a BruCo scan for last night lock:

https://ldas-jobs.ligo.caltech.edu/~gabriele.vajente/bruco_lho_1163325617/

Focusing on the band between 20 and 50 Hz, there isn't any large coherence. However:

Images attached to this report
H1 OpsInfo (OpsInfo)
jim.warner@LIGO.ORG - posted 13:30, Wednesday 16 November 2016 - last comment - 02:36, Friday 18 November 2016(31543)
FAMIS Weeklies tab added to Sitemap

I've added a Weeklies screen to the Sitemap to make it easier for the operators to do FAMIS tasks. It can be found under the OPS tab. Pretty simple, there are a number of buttons that launch different scripts for different FAMIS tasks, so operators don't have to navigate from the command line. Operators and detector engineers should feel free to add tasks to this screen, I added the ones I could think of. Hopefully we can rely on this screen to make sure that operators use 1 version of a script, and give cognizant engineers some control over which version is used.

I also encourage anyone with any artistic inclinations to make it look nicer. I got nothin'.

Images attached to this report
Comments related to this report
nutsinee.kijbunchoo@LIGO.ORG - 02:36, Friday 18 November 2016 (31581)

I gave the medm screen some colors. Blue indicates seismic related tasks, oplev gets red, and PSL gets purple. I can always organize them better if the number of tasks grow.

Images attached to this comment
H1 CDS (DAQ)
david.barker@LIGO.ORG - posted 11:54, Wednesday 16 November 2016 (31541)
CDS model and DAQ restart report Friday 4th - Tuesday 15th November 2016

model restarts logged for Tue 15/Nov/2016
2016_11_15 10:06 h1fw0
2016_11_15 11:45 h1susauxb123
2016_11_15 12:13 h1broadcast0
2016_11_15 12:13 h1dc0
2016_11_15 12:13 h1fw0
2016_11_15 12:13 h1fw1
2016_11_15 12:13 h1fw2
2016_11_15 12:13 h1nds0
2016_11_15 12:13 h1nds1
2016_11_15 12:13 h1tw1

Maintenance day. new frame-cpp version on fw0, new auxb123 model, daq restart.

model restarts logged for Mon 14/Nov/2016 - Thu 10/Nov/2016

Many h1oaf0 model restarts. Please see attached log text files for details.

model restarts logged for Wed 09/Nov/2016 No restarts reported

model restarts logged for Tue 08/Nov/2016
2016_11_08 08:24 h1iopoaf0
2016_11_08 08:24 h1oaf
2016_11_08 08:24 h1odcmaster
2016_11_08 08:24 h1pemcs
2016_11_08 08:24 h1tcscs
2016_11_08 08:25 h1calcs
2016_11_08 08:25 h1iopoaf0
2016_11_08 08:25 h1ngn
2016_11_08 08:25 h1oaf
2016_11_08 08:25 h1odcmaster
2016_11_08 08:25 h1pemcs
2016_11_08 08:25 h1susprocpi
2016_11_08 08:25 h1tcscs
2016_11_08 09:51 h1iopoaf0
2016_11_08 09:56 h1iopoaf0
2016_11_08 09:56 h1tcscs
2016_11_08 09:58 h1calcs
2016_11_08 09:58 h1oaf
2016_11_08 09:58 h1odcmaster
2016_11_08 09:58 h1pemcs
2016_11_08 09:59 h1ngn
2016_11_08 10:00 h1susprocpi
2016_11_08 10:06 h1pemex
2016_11_08 10:11 h1fw2
2016_11_08 12:32 h1iopoaf0
2016_11_08 12:34 h1calcs
2016_11_08 12:34 h1iopoaf0
2016_11_08 12:34 h1ngn
2016_11_08 12:34 h1oaf
2016_11_08 12:34 h1odcmaster
2016_11_08 12:34 h1pemcs
2016_11_08 12:34 h1susprocpi
2016_11_08 12:34 h1tcscs
2016_11_08 12:39 h1iopoaf0
2016_11_08 12:39 h1oaf
2016_11_08 12:39 h1pemcs
2016_11_08 12:40 h1calcs
2016_11_08 12:40 h1ngn
2016_11_08 12:40 h1odcmaster
2016_11_08 12:40 h1tcscs
2016_11_08 12:41 h1calcs
2016_11_08 12:41 h1iopoaf0
2016_11_08 12:41 h1ngn
2016_11_08 12:41 h1oaf
2016_11_08 12:41 h1odcmaster
2016_11_08 12:41 h1pemcs
2016_11_08 12:41 h1susprocpi
2016_11_08 12:41 h1tcscs
2016_11_08 13:00 h1dc0
2016_11_08 13:00 h1fw0
2016_11_08 13:00 h1nds1
2016_11_08 13:02 h1broadcast0
2016_11_08 13:02 h1fw1
2016_11_08 13:02 h1fw2
2016_11_08 13:02 h1nds0
2016_11_08 13:02 h1tw0
2016_11_08 13:02 h1tw1

2016_11_08 19:35 h1calcs
2016_11_08 19:35 h1iopoaf0
2016_11_08 19:35 h1oaf
2016_11_08 19:35 h1odcmaster
2016_11_08 19:35 h1pemcs
2016_11_08 19:35 h1tcscs
2016_11_08 19:36 h1ngn
2016_11_08 19:36 h1susprocpi

Maintenance tuesday. New frame-cpp code for fw2. ADC install in h1oaf0 starts the instabilities. DAQ restart.

model restarts logged for Mon 07/Nov/2016 - Fri 04/Nov/2016 No restarts reported

Non-image files attached to this report
H1 CDS
hugh.radkins@LIGO.ORG - posted 10:16, Wednesday 16 November 2016 (31540)
SDF files must have precision to reflect the Front End

After switching to the down to check things and then going back to the OBSERVE, e-16 differences pop up that reflect the precision difference of the file and front end.  This will really hobble the commissioners/operators and jeopordize the configuration and IFO lock.  I know this is not a new problem.

The safe (for the lock) solution is to Accept the values in the FE to the file; but, this is temporary: the FE thinks the value in the file is the same even though it can not write that precision.  Next time the FE reads the file, the problem returns.  A more permanent fix is to revert the FE to the file but this requires the FE to change its value and potentially (maybe pretty small) break a lock.  Some argue we just not monitor these channels but I say that is risky for the configuration as we stop seeing actual problem channel changes.

The real solution is to have the FE code (RCG?) actually write the file at the precision of the FE so all these problems go away.

Images attached to this report
H1 ISC
hugh.radkins@LIGO.ORG - posted 09:22, Wednesday 16 November 2016 - last comment - 09:31, Wednesday 16 November 2016(31537)
Moving ALS-C_DIFF_PLL_CTRL_OFFSET to Not Monitored on OMC_SDF OBSERVE.snap

This channel will be different each lock (PerComm-JWarner.)

Here is the snap of the current 3 differences with the mask removed.

Images attached to this report
Comments related to this report
hugh.radkins@LIGO.ORG - 09:31, Wednesday 16 November 2016 (31538)

For the OMC safe/down, there are 114 Not Monitored channels and yet only 15 of those currently have differences.  FWIW.

H1 SEI
thomas.shaffer@LIGO.ORG - posted 09:05, Wednesday 16 November 2016 (31535)
Quick Evidence to Support BRS

We already know that the BRS's help us out, but here is a nice screenshot from yesterday of the ALS arm power in 40mph winds. Xarm (blue) has BRS sensor correction on and Yarm (green) had it turned on at around -50. The immediate difference really amazed me and I had to share.

Images attached to this report
H1 ISC
hugh.radkins@LIGO.ORG - posted 08:52, Wednesday 16 November 2016 - last comment - 09:10, Wednesday 16 November 2016(31533)
LSC-ASAIR__A/B_LF_GAIN accepted to OBSERVE.snap

Long lock, steady, looks like a good setting to call good.  This is not the safe, just the OBSERVE.

Attached are all the differences, even the not monitored channels.

Images attached to this report
Comments related to this report
hugh.radkins@LIGO.ORG - 09:10, Wednesday 16 November 2016 (31536)

As far as the safe or down, loading the down, (soft & down in target linked to userapps down,) there are 20 diffs--should not these be Not Monitored?  When I remove the mask, allowing all channels to be checked for differences, there are 60 total differences.  So only 40 of the Not Monitored channels have differences.  I would say that likely many of the 67 Not Monitored channels now showing No Differences could be monitored.  Sure, many channels might end up back where they started after all the scripts.  Still does it even matter?

H1 General
travis.sadecki@LIGO.ORG - posted 08:00, Wednesday 16 November 2016 - last comment - 15:00, Wednesday 16 November 2016(31527)
Ops Owl Shift Summary

TITLE: 11/16 Owl Shift: 08:00-16:00 UTC (00:00-08:00 PST), all times posted in UTC
STATE of H1: Observing
INCOMING OPERATOR: TJ
SHIFT SUMMARY:  Locked at NLN for my entire shift.  Darkhan doing some PCal line work for the first half of the shift.  Observing for the second half.
LOG:

11:53 Turned off PCal lines. Start Kissel's PCAL2DARM measurement.

Saved as /ligo/svncommon/CalSVN/aligocalibration/trunk/Runs/ER10/H1/Measurements/PCAL/2016-11-16_H1_PCAL2DARMTF_4to1200Hz_fasttemplate.xml

12:08 Start Kissel's DARMOLGTF measurement.

Saved as /ligo/svncommon/CalSVN/aligocalibration/trunk/Runs/ER10/H1/Measurements/DARMOLGTFs/2016-11-16_H1_DARM_OLGTF_4to1200Hz_fasttemplate.xml

12:28 Turned PCal lines back on.

12:57 Observing.

Comments related to this report
jeffrey.kissel@LIGO.ORG - 15:00, Wednesday 16 November 2016 (31548)
More details of the IFO conditions during this data set:
Mean Input Power: 31.1 [W]
SCR1 Loops P&Y Loops ON
Images attached to this comment
H1 ISC (ISC, OpsInfo)
sheila.dwyer@LIGO.ORG - posted 21:36, Tuesday 15 November 2016 - last comment - 12:27, Wednesday 16 November 2016(31525)
ASC changes, locking

Operator information:

I've added the Reduce RF9 modulation depth state back into the normal guardian path, but if you are having locklosses durring this state or right after you can try skipping it.  If you skip it, you might want to keep the beam diverters open so you can see that the SRC1 loops are OK (ie, the ratio of AS90/POP90 is staying reasonably high over the lock). You might need to open the SRC1 loops if you skip reducing RF9 modulation depth.  

I've also moved PR3 REFL WFS out of the normal path, so that it will be skipped for now if you just request nominal low noise. 

Comments related to this report
keita.kawabe@LIGO.ORG - 09:06, Wednesday 16 November 2016 (31534)

In the morning POPX DC PIT was routed to PRC2. Didn't make sense (POPX DC is controled by its own centering loop), so manually zero-ed it.

Should have had  no impact on anything as POPX DC is at least 4 orders of magnitude smaller than POPX RF over the entire frequency band.

Seems like this was puched in by hand last night.

Images attached to this comment
keita.kawabe@LIGO.ORG - 12:27, Wednesday 16 November 2016 (31542)

Combination of ASC-REFL_B_RF9I and 45I was routed to unused DC7 as a fake PRC2 on REFLB.

I measured the phase between this DC7 and PRC2 (which is POPX_I) in nominal low noise, and the YAW was out of phase for microseismic peak but not above 3Hz or so (first attachment left) though PIT was pretty good.

By changing the mixing ratio of REFLB RF9I and RF45I for YAW, the coherence between DC7 and PRC2 improves and the phase becomes saner (but never as good as PIT). The second attachment shows when the relevant input matrix components were [0.14, -0.08], i.e. 

DC7_YAW= 0.14*REFL_B_RF9I_YAW -0.08*REFL_B_RF45I_YAW.

(Nominally this was [0.14, -0.2].) The change was put in the guardian, I and Jenne were able to manually switch. Now PR3 is on REFL WFS instead of POPX.

This made ASAIR_B_RF90_I bouncier, but IFO seems to run. We'll run a2l and we'll also measure the sensing matrix

Images attached to this comment
Displaying reports 56181-56200 of 86875.Go to page Start 2806 2807 2808 2809 2810 2811 2812 2813 2814 End