Displaying reports 50741-50760 of 85204.Go to page Start 2534 2535 2536 2537 2538 2539 2540 2541 2542 End
Reports until 11:58, Tuesday 11 April 2017
H1 ISC (ISC)
jenne.driggers@LIGO.ORG - posted 11:58, Tuesday 11 April 2017 - last comment - 02:44, Friday 14 April 2017(35464)
MC2 L2A decoupling filter installed, much better than previous

[Vaishali, JimW, Jenne]

During maintenance, while no one needed the IMC, we tried out our new L2A decoupling filter for MC2.  Recall that Jim found that it would be helpful in alog 35330, and we measured and fit TFs for it in alog 35397.

We found that (a) the pre-existing L2A decoupling was in fact worse than doing nothing at all, and (b) that our new filter works well

In the attached screenshot, the upper left corner is the Foton Bode plot of our decoupling filter.  In the other 3 DTT panels we have the coherence and transfer functions of 3 different MC2 L2A configurations. For these measurements, the IMC was unlocked, but MC2 still aligned.  The red traces in all panels are with no L2A decoupling at all.  The blue traces are with the old L2A "decoupling" gain.  That was a flat gain, and clearly was making things worse than doing nothing at all, over a pretty broad frequency range.  The green traces are with our new L2A decoupling filter on, and we win almost 20dB of isolation below a few hundred mHz.  

We have accepted the new L2A settings for MC2 in the safe and observe SDF files, so they should always be on now.   

Images attached to this report
Comments related to this report
jim.warner@LIGO.ORG - 16:16, Wednesday 12 April 2017 (35509)

I've looked at the coherence between MC2 M1 length drive and the two pitch witnesses (MC2 Trans qpd and MC2 M1 Pit) during locks before and after the install of the new L2P feedforward, and things look better. Attached plot shows the coherence between MC2 M1 L and MC2Trans (top plot, blue is before, red after) and MC2 M1 L and MC2 M1 P (bottom plot, blue is before, red after). Below .1 hz the coherence is much better, which should help for wind and earthquakes, which is what I was looking at originally anyways. Above .1hz  the coherence is pretty much unchanged, not sure why, maybe the motion is dominated by the table motion at those frequencies?

jim.warner@LIGO.ORG - 02:44, Friday 14 April 2017 (35543)

Always useful to actually post promised plots... 

Images attached to this comment
H1 CDS
david.barker@LIGO.ORG - posted 11:18, Tuesday 11 April 2017 (35463)
fixed filter files for h1susprocpi and h1ngn

these models' filter files were static files located in the chans/ directory. I put them into SVN control and made symbolic links from the chans/ directory to there new location under userapps.

H1 CAL (CDS)
aaron.viets@LIGO.ORG - posted 08:57, Tuesday 11 April 2017 - last comment - 20:31, Tuesday 13 June 2017(35462)
New GDS filters for LHO to compute SRC detuning parameters
[Jeff K, Aaron V]

I have produced new GDS filters for LHO that include new paramters (pcal correction factors and EPICS) necessary to compute SRC detuning parameters. It will also be possible to subtract the calibration lines from the strain, producing the additional channel GDS-CALIB_STRAIN_CLEAN, if we desire. The filters can be found in the calibration SVN at this location:
ligo/svncommon/CalSVN/aligocalibration/trunk/Runs/O2/GDSFilters/H1GDS_1175954418.npz

For information on GDS calculations of SRC detuning parameters, see:
https://alog.ligo-wa.caltech.edu/aLOG/index.php?callRep=35041  (note that we now compute Q-inverse instead of Q)
https://alog.ligo-la.caltech.edu/EVNT/index.php?callRep=11785

The filters were produced using this Matlab script in SVN revision 4537:
ligo/svncommon/CalSVN/aligocalibration/trunk/Runs/O2/H1/Scripts/TDfilters/H1_run_td_filters_1175954418.m

The parameters files used (all in revision 4537) were:
ligo/svncommon/CalSVN/aligocalibration/trunk/Runs/O2/H1/params/2017-01-24/modelparams_H1_2017-01-24.conf
ligo/svncommon/CalSVN/aligocalibration/trunk/Runs/O2/H1/params/2017-01-24/H1_TDparams_1175954418.conf
ligo/svncommon/CalSVN/aligocalibration/trunk/Runs/O2/H1/Scripts/CAL_EPICS/callineParams_20170411.m

ASD plots comparing GDS and the front-end CALCS model are attached. These agree with those on the summary pages from the same day (4/10), as expected. Also, time domain vs. frequency domain comparison plots of the filters are attached. Lastly, a time series plot of the kappas from GDS and CALCS is attached, as well as histograms. These show the expected output.
Images attached to this report
Comments related to this report
aaron.viets@LIGO.ORG - 20:31, Tuesday 13 June 2017 (36864)
It was discovered that the output of these filters did not agree with the C01 frames. These GDS filters have been regenerated with SVN revision 4781, and the discrepancy has disappeared. For more details on this issue, see https://alog.ligo-wa.caltech.edu/aLOG/index.php?callRep=36863 .
H1 General
jeffrey.bartlett@LIGO.ORG - posted 08:48, Tuesday 11 April 2017 (35461)
Ops Day Shuift Transition
Ops Shift Transition: 04/11/2017, Day Shift 15:00 – 23:00 (08:00 - 16:00) - UTC (PT)
State of H1: IFO unlocked for maintenance  
Intent Bit: Commissioning/Maintenance
Weather: Wind is a Gentle to Moderate Breeze, Cloudy and lower 30s  
Primary 0.03 – 0.1Hz:   
Secondary 0.1 – 0.3Hz:    
Quick Summary: In maintenance window.      
Outgoing Operator: Nutsinee
H1 CAL (CAL, DetChar)
sudarshan.karki@LIGO.ORG - posted 08:32, Tuesday 11 April 2017 - last comment - 00:05, Monday 17 April 2017(35441)
High Frequency Pcal Injections

There were number of high frequency calibration lines injected using the automated Guardian scripts. These lines are injected using the Pcal at ENDX (ENDY is used for calibration purpose). The GPS time at which these lines were running are listed below:

Frequency Starttime Endtime
2001.3 1174765755 1174843009
2501.3 1174843010 1175048873
3001.3 1175048874 1175185602
3501.3 1175185604 1175280996
4001.3 1175280998 1175367396
4501.3 1175367398 1175532906
5001.3 1175532908  

 

Comments related to this report
sudarshan.karki@LIGO.ORG - 14:21, Tuesday 11 April 2017 (35479)

Rick, Sudarshan

Th high frequency line was moved to 5501.3 Hz. The guardian script was designed to go upto 5001.3 Hz so Rick moved the frequency to 5501.3 Hz manually during the maintenance period.  We will move this line to 6001.3 Hz when we have enough data and the ifo goes out of lock next time.

sudarshan.karki@LIGO.ORG - 00:05, Monday 17 April 2017 (35579)

Updated list of lines with their start and endtime.

Frequency Starttime Endtime
5001.3 1175532908 1175971199
5501.3 1175971561 1176156175
5751.3 1176156177 1176255835
5251.3 1176255837 1176350524
4751.3 1176350525  
H1 General
nutsinee.kijbunchoo@LIGO.ORG - posted 08:03, Tuesday 11 April 2017 (35460)
Ops Owl shift summary

TITLE: 04/11 Owl Shift: 07:00-15:00 UTC (00:00-08:00 PST), all times posted in UTC

STATE of H1: Observing at 65Mpc

INCOMING OPERATOR: Jeff

SHIFT SUMMARY: Not much going on. PI Mode 23 rung up. I flipped the phase 180 degree and it seemed to stop ringing up. I later found an alog that operator shouldn't damp this mode. So what's the status now?

LOG:

13:56 Briefly out of Observe (accidentally). See alog35458

H1 PSL (PSL)
peter.king@LIGO.ORG - posted 06:58, Tuesday 11 April 2017 - last comment - 07:14, Tuesday 11 April 2017(35458)
Front end watch dog accidentally re-enabled
~13:56 UTC, I accidentally re-enabled the front end laser watchdog.
Comments related to this report
peter.king@LIGO.ORG - 07:14, Tuesday 11 April 2017 (35459)
The laser output power has slowly been decaying over the past week or so - see attached plot.  Most of the
power decay is due to the deterioration in the output of diode box 1 (head 1).

Pre-modecleaner could probably do with an alignment tweak.
Images attached to this comment
H1 General
nutsinee.kijbunchoo@LIGO.ORG - posted 03:53, Tuesday 11 April 2017 (35457)
Ops Owl Midshift Summary

Been locked and Observing since Travis handed off to me. Not much to report.

H1 General
travis.sadecki@LIGO.ORG - posted 00:00, Tuesday 11 April 2017 (35456)
Ops Eve Shift Summary

TITLE: 04/11 Eve Shift: 23:00-07:00 UTC (16:00-00:00 PST), all times posted in UTC
STATE of H1: Observing at 72Mpc
INCOMING OPERATOR: Nutsinee
SHIFT SUMMARY:  A pair of locklosses, one unknown and one due to PI.  Otherwise, nothing to mention.
LOG:  See previous aLogs.

H1 General
travis.sadecki@LIGO.ORG - posted 23:33, Monday 10 April 2017 (35455)
Observing at 6:33 UTC

No issues coming back up.

H1 General
travis.sadecki@LIGO.ORG - posted 22:54, Monday 10 April 2017 (35454)
Lockloss 5:54 UTC

PI mode 28 rang up and I couldn't find the right phase value fast enough.

H1 General
travis.sadecki@LIGO.ORG - posted 22:36, Monday 10 April 2017 (35453)
Observing at 5:35 UTC

Ran through a painless IA.  Adjusted ISS diffracted power as it was complaining that it was low.  Accepted SDF diffs in attached screenshots.  ISS refsignal was, of course, me. The other two I am not sure about.

Images attached to this report
H1 General
travis.sadecki@LIGO.ORG - posted 21:44, Monday 10 April 2017 (35452)
Lockloss 4:40 UTC

Cause unknown.  Lock gave up at 71 hours and 10 minute old.

H1 General
travis.sadecki@LIGO.ORG - posted 20:30, Monday 10 April 2017 (35451)
Ops Eve Mid-shift Summary

Wind has calmed down a bit and the range has come up some.  We just rolled over to 70 hours locked.

Images attached to this report
H1 IOO (IOO)
cheryl.vorvick@LIGO.ORG - posted 18:07, Monday 10 April 2017 (35449)
alignment shifts in L1 IMs continues after the vent

L1 alog #32936 describing an alignment shift of the L1 IM2 in pitch on March 27th, 2017.

H1 General
travis.sadecki@LIGO.ORG - posted 17:12, Monday 10 April 2017 (35448)
Ops Eve Shift Transition

TITLE: 04/11 Eve Shift: 23:00-07:00 UTC (16:00-00:00 PST), all times posted in UTC
STATE of H1: Observing at 51Mpc
OUTGOING OPERATOR: Patrick
CURRENT ENVIRONMENT:
    Wind: 33mph Gusts, 27mph 5min avg
    Primary useism: 0.18 μm/s
    Secondary useism: 0.33 μm/s
QUICK SUMMARY:  No issues handed off.  Lock going on 67 hours.

LHO General
patrick.thomas@LIGO.ORG - posted 16:02, Monday 10 April 2017 (35445)
Ops Day Shift Summary
TITLE: 04/10 Day Shift: 15:00-23:00 UTC (08:00-16:00 PST), all times posted in UTC
STATE of H1: Observing at 59Mpc
INCOMING OPERATOR: Travis
SHIFT SUMMARY: Abnormal noise in 3-10 and 10-30 Hz seismic BLRMS correlated with noise in range for a few hours before noon. Also heard an airplane at 20:08 UTC that may have correlated with noise in DARM.
LOG:

15:25 UTC Restarted video2.
16:00 UTC Karen driving car to warehouse.
16:45 UTC PI mode 23 came up coincident with large glitch in DARM. Spike in 3-10 and 10-30 Hz CS Z axis seismic BLRMS.
Chris driving green forklift? Christina at shipping and receiving?
17:14 UTC Marc and Filiberto to mid X.
18:24 UTC Marc and Filiberto back. Heading to vault.
19:53 UTC Marc and Filiberto back.
20:03 UTC Started darmBLRMS striptool and restarted range integrand on video0.
20:08 UTC Airplane heard in control room. Possible correlated noise in DARM.
20:41 UTC Gerardo to mid Y for scroll pump maintenance work. Nothing noisy.
21:43 UTC Chandra to CP3.
21:59 UTC Chandra back.
22:54 UTC Gerardo back.
LHO VE
logbook/robot/script0.cds.ligo-wa.caltech.edu@LIGO.ORG - posted 12:10, Monday 10 April 2017 - last comment - 15:01, Monday 10 April 2017(35439)
CP3, CP4 Autofill 2017_04_10
Starting CP3 fill. LLCV enabled. LLCV set to manual control. LLCV set to 50% open. Fill completed in 1072 seconds. TC B did not register fill. LLCV set back to 19.0% open.
Starting CP4 fill. LLCV enabled. LLCV set to manual control. LLCV set to 70% open. Fill completed in 128 seconds. LLCV set back to 37.0% open.
Images attached to this report
Comments related to this report
chandra.romel@LIGO.ORG - 14:42, Monday 10 April 2017 (35442)

Raised CP3 to 20% open.

chandra.romel@LIGO.ORG - 15:01, Monday 10 April 2017 (35443)

Verified that both thermocouples are inserted into CP3 and CP4 exhaust pipes, since TC B of CP3 didn't register fill for the last couple of times.

H1 CAL
jeffrey.kissel@LIGO.ORG - posted 11:44, Thursday 06 April 2017 - last comment - 16:26, Monday 17 April 2017(35361)
2017-04-06 New Calibration Sensing Function Measurement Suite
J. Kissel

Gathered regular bi-weekly calibration / sensing function measurements. Preliminary results (screenshots) attached; analysis to come.

The data have been saved and committed to:
/ligo/svncommon/CalSVN/aligocalibration/trunk/Runs/O2/H1/Measurements/SensingFunctionTFs
    2017-03-21_H1DARM_OLGTF_4to1200Hz_25min.xml
    2017-03-21_H1_PCAL2DARMTF_4to1200Hz_8min.xml

    2017-03-06_H1_PCAL2DARMTF_BB_5to1000Hz_0p25BW_250avgs_5min.xml
Images attached to this report
Comments related to this report
jeffrey.kissel@LIGO.ORG - 16:48, Friday 07 April 2017 (35398)
J. Kissel

After processing the above measurement, the fit optical plant parameters are as follows:

DARM_IN1/OMC_DCPD_SUM        [ct/mA]      2.925e-7
Optical Gain                 [ct/m]       1.110e6   (+/- 1.6e3)
                             [mA/pm]      3.795     (+/- 0.0053)
Coupled Cavity Pole Freq     [Hz]         355.1     (+/- 2.6)
Residual Sensing Delay       [us]         1.189     (+/- 1.7)
SRC Detuning Spring Freq     [Hz]         6.49      (+/- 0.06)
SRC Detuning Quality Factor  [ ]          25.9336   (+/- 6.39)

Attach are plots of the fit, and how these parameters fit in within the context of all measurements from O2. 

In addition, given that the spread of the course of the detuning spring frequency is between, say 6.5 Hz and 9 Hz, I show the magnitude ratio of two toy transfer functions, where the only difference is the spring frequency. One can see that -- if not compensated for, that means a systematic magnitude error of 5%, 10%, 27% at 30, 20, and 10 Hz, respectively.

Bad news for black holes! We definitely need to track this time dependence, as was prototyped in LHO aLOG 35041.
Images attached to this comment
Non-image files attached to this comment
shivaraj.kandhasamy@LIGO.ORG - 16:12, Monday 10 April 2017 (35446)

Attached are plots comparing the sensing and response function with and without detuning frequency.  Compared to LLO (a-log 32930), at LHO the detuning frequency of ~7 Hz has significant effect on the calibration around 20 Hz (see response function plot). The code used to make this plot is added to svn,

/ligo/svncommon/CalSVN/aligocalibration/trunk/Runs/O2/H1/Scripts/SRCDetuning/springFreqEffect.m
Images attached to this comment
shivaraj.kandhasamy@LIGO.ORG - 16:26, Monday 17 April 2017 (35596)CAL

Attached are plots showing differences in sensing functions and response functions for spring frequencies of 6 Hz and 9 Hz. Coincidentally they are very similar to the plots in the previous comment which show differences when the spring frequencies are 0 Hz and 6.91 Hz.

Images attached to this comment
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