Displaying reports 48721-48740 of 83194.Go to page Start 2433 2434 2435 2436 2437 2438 2439 2440 2441 End
Reports until 13:23, Tuesday 11 April 2017
H1 CAL (CAL, ISC)
jeffrey.kissel@LIGO.ORG - posted 13:23, Tuesday 11 April 2017 - last comment - 13:40, Tuesday 11 April 2017(35474)
Time-dependent SRC Detuning Infrastructure Installed, To Be Commissioned
J. Kissel, A. Viets
WP #6572
ECR E1700121
II 7828

Because I'm not sure how long it'll take to make the MED screens and fully commission the new parts' settings until we have results, I just want to get an aLOG in there that confirms we've installed the front-end infrastructure changes to begin tracking the SRC detuning as a function of time.

This required modifying 
/opt/rtcds/userapps/release/cal/common/models/CAL_CS_MASTER.mdl
to include many new EPICs records that store various DARM loop model component values at the already-existing PCAL line frequency (7.93 Hz), and as a bonus, I also installed all of the infrastructure to compute the SRC detuning frequency in the front-end as well -- it was an easy extension of the existing software to calculate the optical gain and cavity pole frequency, following the math in T1700106 and LHO aLOG 35105.

I've installed values for these new EPICs records using svn up'd versions of
/ligo/svncommon/CalSVN/aligocalibration/trunk/Runs/O2/H1/Scripts/CAL_EPICS/writeH1_CAL_EPICS.m
/ligo/svncommon/CalSVN/aligocalibration/trunk/Runs/O2/Common/Scripts/CAL_EPICS/writeO2_TDEP_EPICS.m
/ligo/svncommon/CalSVN/aligocalibration/trunk/Runs/O2/DARMmodel/Scripts/computeEPICS.m

To do/aLOG:
 - Take screen shots of the new model infrstructure to show the implementation
 - Update TDEP MEDM overview screen to include the new math
 - Install demodulation parameters and lowpass filters for new 7.93 Hz demod
 - Install low-passes on F_S and Q_S output banks
 - Compare against GDS pipeline output
Comments related to this report
aaron.viets@LIGO.ORG - 13:40, Tuesday 11 April 2017 (35476)
After an update to the frame broadcaster channel list and a minor correction to the write-EPICS code, we have restarted the primary and redundant calibration pipelines. The restart was at GPS second 1175976351. We can confirm whether the SRC detuning parameter algorithm is working once we have a lock stretch. For information on the new filters, see:
https://alog.ligo-wa.caltech.edu/aLOG/index.php?callRep=35462
For information on the new gstlal-calibration code release, see https://bugs.ligo.org/redmine/issues/5440
In addition, there are two small improvements I've noted:
1) The latency is reduced from ~12s to ~7s.
2) The CPU usage is reduced from ~55% to ~45%
H1 PSL
jason.oberling@LIGO.ORG - posted 12:19, Tuesday 11 April 2017 (35473)
PSL Power Watchdogs Reset (FAMIS 3645)

I reset both PSL power watchdogs at 19:16 UTC (12:16 PDT).  This completes FAMIS 3645.

H1 CDS
david.barker@LIGO.ORG - posted 12:17, Tuesday 11 April 2017 (35472)
DMT update progressing

Greg, Aaron and John are in the midst of the GDS/DMT update.

H1 DCS (CAL, DCS)
gregory.mendell@LIGO.ORG - posted 12:16, Tuesday 11 April 2017 (35471)
DMT updates
Re: WP 6567

The yum updates and reboots of the DMT computers is done. I've also restarted the dmt processes on each box.

The next step is for Aaron Viets to restart the calibration using gstlal-calibration-1.1.5.

 

H1 AOS (DetChar)
jason.oberling@LIGO.ORG - posted 12:14, Tuesday 11 April 2017 - last comment - 11:35, Tuesday 18 April 2017(35470)
ITMy Optical Lever Laser Swapped, Again (WP 6565)

This morning I swapped the ITMy oplev laser, per LHO WP 6565.  This was in response to this alog from K. Venkateswara and J. Kissel, indicating an ~0.44 Hz feature on the ITMy oplev (that showed up after the laser swap on March 7th) was possibly due to an issue with the laser and causing range issues.  The old laser SN was 189-1, the new laser SN is 191.  This laser will need a few hours to come to thermal equilibrium, once that is done I will assess whether or not the laser needs a power tweak for glitch-free operation; I will leave WP 6565 open until this is complete.

Comments related to this report
jason.oberling@LIGO.ORG - 11:35, Tuesday 18 April 2017 (35614)DetChar

Went out today to tweak the power of this laser, as it is still glitching, and found the interior of the box to be very warm.  This is highly unusual.  I also found the exterior mounted box that holds the DC/DC converter that powers the laser to be very warm as well.  My suspicion is that something, likely the laser, is drawing more current than it should.  I checked the other oplev lasers in the LVEA and none of them were running warm like this.  The quickest fix at this point is to swap in another laser.  Unfortunately the only laser currently ready for swap in is SN 189-1, which happens to be the laser I just removed from the ITMy oplev due to concerns over an ~0.44 Hz feature that might be from the laser.  Doing a quick spectrum of the new ITMy oplev laser SUM, pitch, and yaw signals after install on 4/11/2017 (attachment 1) and this morning (attachment 2) shows that the laser is currently very noisy compared to just after install (likely due to the increased operating temperature), but also still shows a feature at ~0.44Hz.  As this ~0.44Hz feature is still there with this new laser, the feature is likely either from the the electronics of the ITMy oplev (QPD, whitening chassis) or is something real that the oplev is only a witness for.  Assuming laser SN 189-1 checks out in the lab, I will re-install SN 189-1 into the ITMy oplev at the next available opportunity.

Images attached to this comment
H1 CDS
david.barker@LIGO.ORG - posted 12:14, Tuesday 11 April 2017 (35469)
HWS frame grabber pci-e card returned to h1hwsex

Carlos has returned the HWS card to h1hwsex (was in the spare machine h1hwsmsr1).

LHO General
thomas.shaffer@LIGO.ORG - posted 12:13, Tuesday 11 April 2017 (35468)
LVEA Swept

Unplugged one extension cord, but that is it.

H1 CDS (VE)
david.barker@LIGO.ORG - posted 12:12, Tuesday 11 April 2017 (35467)
vacuum dewar alarm levels lowered from 20% to 15%

The cell phone texter alarm system was reconfigured, all eight LN2 Dewar low level alarms will now start at 15% full instead of the previous 20%.

H1 CDS (CAL, DAQ, PEM)
david.barker@LIGO.ORG - posted 12:11, Tuesday 11 April 2017 (35466)
new models: h1pemcs and h1calcs. DAQ restart

h1pemcs was modified to return two test ADC channels to the frame, both at 2048Hz.

Jeff made his h1calcs model change. This only added slow channels to the frame (203 chans).

I changed the DAQ master to add the new H1EDCU_SEISMON.ini file.

11:44PDT: DAQ was restarted for the above.

LHO VE
chandra.romel@LIGO.ORG - posted 11:59, Tuesday 11 April 2017 (35465)
tested vertex VE

[Kyle, Chandra]

In preparation for anticipated vertex vent, we tested vacuum equipment:  QDP80 roughing pump, Kobelco purge air skid, and vertex turbo & scroll pumps. All ran satisfactorily. Purge air measured -43.7degC dew point. A few notes:

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.

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