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Reports until 22:28, Wednesday 07 October 2015
H1 General
nutsinee.kijbunchoo@LIGO.ORG - posted 22:28, Wednesday 07 October 2015 - last comment - 22:50, Wednesday 07 October 2015(22324)
EVE late Mid Shift Summary

Sheila, Nutsinee

After we got passed all the problems Sheila mentioned earlier, we are still trying to acquire lock. Ifo lost lock at SWITCH_TO_QPDS twice in a row.

Comments related to this report
nutsinee.kijbunchoo@LIGO.ORG - 22:50, Wednesday 07 October 2015 (22325)

Back to Observing at 05:49 UTC

H1 ISC
sheila.dwyer@LIGO.ORG - posted 21:36, Wednesday 07 October 2015 - last comment - 22:03, Wednesday 07 October 2015(22322)
ALIGN_IFO guardian fix

Nutsinee started an inital alingment as part of recovering from the last lockloss.  The INPUT align WFS loops failed for an unknown reason, and caused the X arm to drop lock with out offloading the WFS.  At this point we noticed that the history in the suspension filters was not cleared in the down state of the ALIGN_IFO guardian, which caused the X arm to stay misalinged in this case.  I've now added clear history for the filters.  

Comments related to this report
sheila.dwyer@LIGO.ORG - 22:03, Wednesday 07 October 2015 (22323)

We got to DC readout transition this time, but had similar difficulties to last night where the OMC locked on a wrong mode, switched to the dither alignment and became misaligned.  I added a check on the DCPD sum in the OMC_LOCKED state, if the sum is below 14 mA it will give a notification and not move on the the dither aligment. 

We went through a couple of rounds of turning of the OMC ASC, clearing the history, and turning it back on.  I think this failed the first time because I didn't wait for the suspension to stop swinging before turning the ASC loops on again.  The last time everything seemed fine, but we had been sitting at DC readout transition for a while.  Like last night we lost the lock when we tried to transition.  

H1 General
nutsinee.kijbunchoo@LIGO.ORG - posted 20:06, Wednesday 07 October 2015 - last comment - 20:59, Wednesday 07 October 2015(22319)
Lockloss 02:48 UTC

All the environment monitors didn't show anything that could have caused the lockloss. Sheila's investigating.

Comments related to this report
sheila.dwyer@LIGO.ORG - 20:59, Wednesday 07 October 2015 (22321)

ITMY saturated in this lockloss, caused by angular drives that were somewhat large.  It looks like many ASC loops have large drives in the 200 ms before the lockloss, but DHARD goes bad first.  

Images attached to this comment
H1 INJ (DetChar, INJ)
christopher.biwer@LIGO.ORG - posted 18:59, Wednesday 07 October 2015 - last comment - 17:24, Tuesday 03 November 2015(22316)
Tested PCALX with new inverse actuation filter
Summary:

We had single-IFO time so I tested the new inverse actuation filter for PCALX. WP5530

Sudarshan and I believe we tracked down the factor of 2 and sign error from the initial PCALX test, see aLog 22160. We wanted to do this test to confirm that.

CBC injections:

The waveform file is: https://daqsvn.ligo-la.caltech.edu/svn/injection/hwinj/Details/Inspiral/H1/coherenttest1from15hz_1126257408.out

The XML parameter file is: https://daqsvn.ligo-la.caltech.edu/svn/injection/hwinj/Details/Inspiral/h1l1coherenttest1from15hz_1126257408.xml.gz

I did three CBC injections. The start times of the injections were: 1128303091.000000000, 1128303224.000000000, and 1128303391.000000000.

The command line to do the injections is:
ezcawrite H1:CAL-INJ_TINJ_TYPE 1
awgstream H1:CAL-PCALX_SWEPT_SINE_EXC 16384 coherenttest1from15hz_1126257408.out 1.0 -d -d >> 20151006_log_pcal.out
awgstream H1:CAL-PCALX_SWEPT_SINE_EXC 16384 coherenttest1from15hz_1126257408.out 1.0 -d -d >> 20151006_log_pcal.out
awgstream H1:CAL-PCALX_SWEPT_SINE_EXC 16384 coherenttest1from15hz_1126257408.out 1.0 -d -d >> 20151006_log_pcal.out

I have attached the log. I had to change the file extension to be posted to the aLog.

DetChar injection:

I injected Jordan's waveform file: https://daqsvn.ligo-la.caltech.edu/svn/injection/hwinj/Details/detchar/detchar_03Oct2015_PCAL.txt

The start time of the injection is: 1128303531.000000000

The command line to do the injections is:
awgstream H1:CAL-PCALX_SWEPT_SINE_EXC 16384 detchar_03Oct2015_PCAL.txt 1.0 -d -d >> 20151006_log_pcal_detchar.out

I have attached the log. I had to change the file extension to be posted to the aLog.
Non-image files attached to this report
Comments related to this report
christopher.buchanan@LIGO.ORG - 20:16, Wednesday 07 October 2015 (22318)DetChar

Chris Buchanan and Thomas Abbott,

Quick follow-up with omega scans. It looks like most of the power is seen in GDS-CALIB_STRAIN about eight seconds after each listed injection time, consistently for each of these three injections. Doesn't look like there are omicron triggers for these times yet, but omega scans for GDS-CALIB_STRAIN are attached.

Full omega scans generated here:
https://ldas-jobs.ligo.caltech.edu/~christopher.buchanan/Omega/Oct07_PCALX_Inj1/

https://ldas-jobs.ligo.caltech.edu/~christopher.buchanan/Omega/Oct07_PCALX_Inj2/

https://ldas-jobs.ligo.caltech.edu/~christopher.buchanan/Omega/Oct07_PCALX_Inj3/

Images attached to this comment
jordan.palamos@LIGO.ORG - 20:52, Wednesday 07 October 2015 (22320)

For complete documentation of the detchar safety injections:

The injections are 12 sine-gaussians, evenly spaced from 30hz to 430hz, 3 seconds apart with a Q of 6. There are three sets with increasing SNR of 25, 50, 100 (intended). However, the SNR is limited by the PCAL acuation range at higher frequencies.

To generate the waveforms I used the script written by Peter Shawhan / Andy located here: https://daqsvn.ligo-la.caltech.edu/websvn/filedetails.php?repname=injection&path=%2Fhwinj%2FDetails%2Fdetchar%2FGenerateSGSequencePCAL.m

I tuned the injections to stay within the PCAL actuation limits referenced in Peter Fritschel's document https://dcc.ligo.org/LIGO-T1500484.

The intended time (seconds from start time of injections), freqency, snr, and amplitude (in units of strain) for all injections are pasted below:

 

__time__   __freq__   __SNR__    __AMP__

    0.50       30.0      25.0    5.14e-21

    3.50       38.2      25.0    4.96e-21

    6.50       48.7      25.0    2.15e-21

    9.50       62.0      25.0    2.07e-21

   12.50       79.0      25.0    1.75e-21

   15.50      100.6      25.0    1.78e-21

   18.50      128.2      25.0    1.92e-21

   21.50      163.3      25.0    2.06e-21

   24.50      208.0      25.0    2.39e-21

   27.50      265.0      10.0    1.11e-21

   30.50      337.6       5.0    8.39e-22

   33.50      430.0       5.0    8.51e-22

   36.50       30.0      50.0    1.03e-20

   39.50       38.2      50.0    9.92e-21

   42.50       48.7      50.0    4.31e-21

   45.50       62.0      50.0    4.14e-21

   48.50       79.0      50.0    3.51e-21

   51.50      100.6      50.0    3.55e-21

   54.50      128.2      50.0    3.85e-21

   57.50      163.3      50.0    4.12e-21

   60.50      208.0      50.0    4.77e-21

   63.50      265.0      20.0    2.21e-21

   66.50      337.6      10.0    1.68e-21

   69.50      430.0      10.0     1.7e-21

   72.50       30.0     100.0    2.06e-20

   75.50       38.2     100.0    1.98e-20

   78.50       48.7     100.0    8.62e-21

   81.50       62.0     100.0    8.27e-21

   84.50       79.0     100.0    7.01e-21

   87.50      100.6     100.0     7.1e-21

   90.50      128.2     100.0    7.69e-21

   93.50      163.3     100.0    8.24e-21

   96.50      208.0     100.0    9.54e-21

   99.50      265.0      40.0    4.43e-21

  102.50      337.6      20.0    3.36e-21

  105.50      430.0      20.0     3.4e-21

 

 

christopher.biwer@LIGO.ORG - 12:43, Thursday 08 October 2015 (22344)DetChar, INJ
Here are the SNR of the CBC injections using the daily BBH matching filtering settings:

end time               SNR   chi-squared  newSNR
1128303098.986  20.35  32.86            19.86
1128303231.985  22.62  32.73            22.10
1128303398.985  23.25  21.05            23.25

Expected SNR is 18.4.

Though a recovered SNR of 20 (about 10% percent difference from 18.4) is comparable to some of the SNR measurements when doing injections with CALCS in aLog 21890. Note this is the same waveform injected here except in aLog 21890 it starts from 30Hz. In both cases the matched filtering starts at 30Hz. The last two have a bit higher SNR though.
christopher.biwer@LIGO.ORG - 13:42, Thursday 08 October 2015 (22348)DetChar, INJ
I edited Peter S.'s matlab script to check the sign of these PCAL CBC injections.

Looks like the have the correct sign. See attached plots.

To run code on LHO cluster:
eval '/ligotools/bin/use_ligotools'
matlab -nosplash -nodisplay -r "checksign; exit"

Also in hindsight I should have done a couple CALCS CBC injections just to compare the SNR at the time with the PCAL injections.
Images attached to this comment
Non-image files attached to this comment
jordan.palamos@LIGO.ORG - 17:01, Friday 09 October 2015 (22383)
I checked for overflows using TJ's script with the following command:

gwdetchar-overflow -i H1 -f H1_R -O segments -o overflow --deep  1128303500 1128303651 124

It returns an empty table, so no overflows.

peter.shawhan@LIGO.ORG - 20:27, Saturday 10 October 2015 (22400)
A time-domain check of the recovered strain waveforms is here: https://wiki.ligo.org/Main/HWInjO1CheckSGs.  I found that the sign is correct, the amplitude matches within a few percent at most frequencies, and the phases are generally consistent with having a frequency-independent time delay of 3 or 4 samples (about 0.2 ms).  Details are on that wiki page.
christopher.biwer@LIGO.ORG - 17:24, Tuesday 03 November 2015 (23079)DetChar, INJ
Thomas Abbot, Chris Buchanan, Chris Biwer

I've taken Thomas/Chris' table of recovered omicron triggers for the PCAL detchar injection and calculated the ratio of expected/recovered SNR and added some comments:

Recovered time      time since                 frequency recovered expected  recovered/expected        comments
                               1128303531 (s)          (Hz)           SNR        SNR           SNR
1128303531.5156	0.515599966	         42.56	34.07	25	            1.3628
1128303534.5078	3.5078001022	        61.90	39.41	25	            1.5764
1128303537.5039	6.5039000511	        64.60	28.29	25	            1.1316
1128303540.5039	9.5039000511	        79.79	23.89	25	            0.9556
1128303543.5039	12.5039000511	1978.42	21.38	25           	0.8552                                  suspicious, the frequency is very high
1128303546.502	15.5020000935	 144.05	26.24	25	           1.0496
1128303549.502	18.5020000935	 185.68	26.38	25	           1.0552
1128303552.502	21.5020000935	 229.34	26.29	25	           1.0516
1128303555.501	24.5009999275	 918.23	27.34	25	           1.0936
1128303558.501	27.5009999275	 315.97	11.05	10	           1.105
1128303564.5005	33.5004999638	 451.89	6.76	          5     	1.352
1128303567.5156	36.515599966	        50.12	68.53	50	          1.3706
1128303570.5078	39.5078001022	 61.90	78.23	50	          1.5646
1128303573.5039	42.5039000511	 76.45	52.04	50	          1.0408
1128303576.5039	45.5039000511	 91.09	48.42	50	          0.9684
1128303579.5039	48.5039000511	 116.63	47.73	50	         0.9546
1128303582.502	51.5020000935	 144.05	52.59	50	         1.0518
1128303585.502	54.5020000935	 177.91	52.3	        50	         1.046
1128303588.502	57.5020000935	 261.81	54.8	       50	          1.096
1128303591.501	60.5009999275	 323.36	55.64	50	          1.1128
1128303594.501	63.5009999275	 414.01	19.67	20	          0.9835
1128303597.501	66.5009999275	 390.25	9.55	       10	        0.955
1128303600.5005	69.5004999638	 481.99	9.34	        10	          0.934
1128303603.5156	72.515599966	         48.35	136.81	100	          1.3681
1128303606.5078	75.5078001022	 71.56	156.91	100	         1.5691
1128303609.5039	78.5039000511	 76.45	102.72	100	         1.0272
1128303612.5039	81.5039000511	 138.03	102.85	100	          1.0285
1128303615.5039	84.5039000511	 134.83	95.52	100	         0.9552
1128303618.502	87.5020000935	 1283.14	104.17	100	         1.0417                 frequency seems a bit high
1128303621.502	90.5020000935	 211.97	107.18	100	         1.0718
1128303624.502	93.5020000935	 261.81	104.53	100	         1.0453
1128303627.501	96.5009999275	 323.36	109.66	100	         1.0966
1128303630.501	99.5009999275	 414.01	42.15	40	        1.05375
1128303633.5005	102.5004999638	 959.39	19.11	20	        0.9555                  this last injection had some kind of glitch on it

In most cases looks like the ratio is within 0.1 of 1. On a quick glance I see 10 injections that were not within this range.
H1 INJ (DetChar, INJ)
christopher.biwer@LIGO.ORG - posted 18:27, Wednesday 07 October 2015 - last comment - 18:44, Wednesday 07 October 2015(22314)
Starting PCALX hardware injection test
Starting PCALX hardware injection tests. WP 5530. Intent mode is off. More details later.
Comments related to this report
christopher.biwer@LIGO.ORG - 18:44, Wednesday 07 October 2015 (22315)
Finished hardware injections. More details to come.
H1 General
nutsinee.kijbunchoo@LIGO.ORG - posted 16:29, Wednesday 07 October 2015 (22312)
Ops EVE Shfit Transition

TITLE: 10/7 [EVE Shift]: 23:00-07:00UTC (16:00-00:00 PDT), all times posted in UTC"

STATE Of H1: Observing at 72 Mpc. Been locked since yesterday.

OUTGOING OPERATOR: Ed

QUICK SUMMARY: Few people in the control room. Almost no wind. Nominal seismic activity in the earthquake band. Local seismic activities dropping to nominal.

H1 General
edmond.merilh@LIGO.ORG - posted 15:57, Wednesday 07 October 2015 (22311)
Shift Summary - Day

TITLE:   Oct 7 DAY Shift 15:00-23:00UTC (08:00-04:00 PDT), all times posted in UTC

STATE Of H1: Observing

LOCK DURATION: Entire Shift

SUPPORT: None required

INCOMING OPERATOR: Nutsinee

Activity log:

16:42 Changed the time period on Video1 FOM to 24 hours

17:46 Jim noticed that the .6Hz peak in the PRCL Live spectra (NUC4) has gone away.

17:49 Jody and John traveling to the X/Y mid stations.

18:30  Jody and John are back from the Mid stations

19:24 Peter into optics lab to find a neutral density filter. (Landry’s approval)

19:38 Peter out of the optics lab.

20:45  Joe D checked the emergency lighting in the Control Room

Shift Summary: Quiet day: IFO locked at 75Mpc (avg) for the entire shift. No excessive wind speeds. No obtrusive EQ activity. Microseism was steady all day.

SUS E_T_M_Y saturating (Oct 7 16:9:29 UTC)
SUS E_T_M_Y saturating (Oct 7 17:33:6 UTC)
SUS E_T_M_Y saturating (Oct 7 19:8:7 UTC)
SUS E_T_M_Y saturating (Oct 7 19:54:24 UTC)
SUS E_T_M_Y saturating (Oct 7 20:57:5 UTC)

H1 DAQ (CDS)
james.batch@LIGO.ORG - posted 13:59, Wednesday 07 October 2015 (22308)
Minor reconfigure of wiper script for h1fw0
The frame wiper script which runs on h1fw0 was changed to alow the disk to become 95% full to match the configuration of h1fw1.  The previous setting allowed only 90% disk usage.  

The setting of 90% was most likely left over from a test configuration when the Ubuntu frame writer was first created.
H1 DAQ (CDS)
david.barker@LIGO.ORG - posted 13:56, Wednesday 07 October 2015 (22306)
LHO DAQ lookback times for framed data

Here are the LHO DAQ lookback times for framed data served by the internal NDS protocol-1 servers (data taken at 13:25 local time).

h1nds0 (disks in LDAS server room). Disk usage 91% (33TB used). 

data type days hours mins
Commissioning (full) 10 06 08
Science 02 09 58
second 24 18 25
minute 03 03 36

h1nds1(default-nds) (disks in MSR). Disk usage 96% (35TB used).

data type days hours mins
Commissioning (full) 11 00 32
Science 02 14 24
Second 26 13 58
Minute 03 09 39

Note underuse of disks on h1nds0, being changed to use 95% of available disk space.

H1 SEI
hugh.radkins@LIGO.ORG - posted 13:30, Wednesday 07 October 2015 (22305)
LHO HEPI Pump Out Pressures: why is the CS so much more quiet than the ends?

Under WP 5527, yesterday I switched the sensors on two of the CS HEPI Pump Skids.

On a Pump Station Skid, see first attachment for a medm depiction, there are pressure sensor ports. 1--right after pump, includes first capacitor accumulator; 2 & 3--after laminar flow resistors & includes accumulator; 4--after final 3u filter. In previous logs, see first plot of 21366, I show that at the corner station, pressure 1 right after the pump is super quiet, again only at the corner.  I checked with Barker and we looked at things and there is no reason the trends would be different for these channels.

Here the attached plot shows just the four impacted pressure sensors.  The first two plots I've zoomed into the quiet portions before and after the switch showing that the "quiet" is tied to the sensor not the channel; the shift in the reading is due to the AOFF (zero) of the individual channel.  On the next two graphs (PS4_PRESS1 & 3) I've zoomed into the noisier after and before the sensor switch.  Bottom line, the noise level is at the sensor, not the channel.  The next two graphs (channels 7 & 8) are the End stations' Pressure1.  Clearly EndX is out to lunch with super ugly noise from something we can't figure out.  This shows up on the EX control out, CH10, and the servo'd PV (not shown.)  The Ch8 graph shows the EY PRESS1 is much noisier than the corner press1s.  The last 3 graphs are the control outs for the corner, L0, and EX and EY.  Interestingly, despite the much quieter pressure on the CS vs EndY PRESS1s, the CONTROL_VOUTs of the CS and EY are very similar as is their servo'd PVs (the EndY shows the diurnal much more than the others.)  Even though the pressure out of the pump is quiet or noisy (CS or EndY) the RC Manifold of the Pump Station makes the signal noisier for the CS.  The noise level on the EndY Manifold pressures are about the same or only slightly noisier down the manifold (I looked.)

Still wondering about what is going on...

1) The Accumulator charge on the Press1 volumes are similar although the fluid pressures are different at the three locations.  Why?  The zero AOFFs are coarse and may be variable over time.  The resistances to get to PV setpoint are likely different even at Ends and especially at corner.  Why? Different crap in the resistor stacks, different length pipe runs to BSC, more Actuators at corner, different actuators everywhere, etc.

Solution?  Be more precise at setting accumulator pressures based on operating pressures?  Given the spec'd nominal accumulator charge of 60 to 93% (I shoot for 90%) of operating fluid pressure and the very unlikely(hood) that I would be so good(lucky) at the CS versus the Ends, I'd say this is not the issue.

2) The Corner station has 24 HEPI Actuators per Pump Station while the Ends have just eight.  This leads the CS pumps to run about twice as fast as the Ends, see VOUT channels.

I could manually slow down the CS pumps to End speeds and see what that does.  HEPI performance likely compromised if not completely hosed but might be informative.  Could we introduce additional resistances at the Ends to require the Pump to speed up?

3) Could the laminar flow Resistors be contributing to the down stream noise increase?  Does it make sense that the pressure out of the pump is the quietest?  This certainly would not explain why the Ends are noisier but might explain the down stream noise.

4) Could the End Station Pumps be cavitating?  Yes.  I've had a pump cavitate in July, 19699 & 19794, after maintenance in the CS and had to restart it.  I did so over 5 minutes and the cavitation stopped.  I'd have to mine to find the last time the Ends were restarted and figure out how they were ramped back on.  I try to do so slowly manually or with the servo but it's not typically 5 minutes.  I don't suspect this as the pump made an audible rumbling when the CS was cavitating and I don't hear this at the Ends.  But, maybe there are varying levels of cavitation and there could be benefit to restarting the End Pumps very slowly.

It really does not matter anyway.  Given what the servo pressure and control drive look like comparing the CS and EndY, those results are the same.  More important and maybe still not that important is to figure out why the EndX pressures are so noisy.

I'll restore the pressure sensor cabling when able and close out this WP.

Images attached to this report
H1 SEI (DetChar)
jim.warner@LIGO.ORG - posted 11:18, Wednesday 07 October 2015 - last comment - 11:09, Monday 26 October 2015(22304)
HAM3 .6 hz non-sense has fixed itself?

The LHO SEI team has known about a .6-ish hz peak on the HAM3 ISI for a long time (see my alog 15565, December of last year for the start, Hugh has a summary of LHO alogs in the SEI log for more). I was working with Ed on a DTT template for the operators when I noticed it was now gone. Very strange. Looking a little closer, it seems to have been decreasing over the last couple of days to a week, and disappeared completely this morning about 7-8:00 UTC. Attached spectra are from ~0:00 UTC (red) and ~16:00 UTC (blue, when I found it was missing). Looking at random times over the last week, it looks like it may have been trending down.

Could someone in Detchar look at this peaks longish term BLRMS, say over the last month, or even over the last year since we found it? Pretty much every sensor in that chamber saw this, but the GS-13s are the best witness.

Images attached to this report
Comments related to this report
guillermo.valdes@LIGO.ORG - 13:55, Monday 19 October 2015 (22644)DetChar

I checked the coherence of H1:SUS-PR2_M1_ISIWIT_L_DQ with some PEM sensors for frequencies around 0.6 Hz.

  • At ~0.64 Hz, H1:SUS-PR2_M1_ISIWIT_L_DQ shows strong coherence with the magnetometers:
    • H1:PEM-CS_MAG_EBAY_LSCRACK_Z_DQ. 
    • H1:PEM-CS_MAG_EBAY_SUSRACK_Z_DQ. 
  • At ~0.64 Hz, H1:SUS-PR2_M1_ISIWIT_L_DQ shows strong coherence with H1:PEM-CS_MAG_LVEA_INPUTOPTICS_Z_DQ, but not every time, even if the coherence is strong with the magnetometers in the electronics bay. 
  • I did not find strong coherence between the following PEM sensors and H1:SUS-PR2_M1_ISIWIT_L_DQ at ~0.64 Hz:
    • H1:PEM-CS_MIC_LVEA_BS_DQ
    • H1:PEM-CS_MIC_EBAY_RACKS_DQ
    • H1:PEM-CS_ACC_HAM3_PR2_Y_DQ
    • H1:PEM-CS_MAINSMON_EBAY_1_DQ
    • H1:PEM-CS_MAINSMON_EBAY_2_DQ
Images attached to this comment
brian.lantz@LIGO.ORG - 11:09, Monday 26 October 2015 (22841)
Note - it reappeared for a few hours on Oct 13 - picture at
https://alog.ligo-wa.caltech.edu/aLOG/index.php?callRep=22775
H1 ISC
sheila.dwyer@LIGO.ORG - posted 17:25, Tuesday 06 October 2015 - last comment - 06:02, Thursday 08 October 2015(22286)
EX beam diverter has been open since June(!)

Today we noticed that the EX beam diverter has been open since June 18th.  We don't normally switch this so it is not guardian controlled but we "usually" leave it closed.  It is beckhoff controlled so it is not monitored in SDF.  Today TJ added all the beam diverters we don't normally change in guardian to SYS_DIAG to prevent this from happening again (it was already checking the others).

We have now locked with the beam diverter closed, and see that the QPD spectra look the same between EX and EY.   (20418 and 21767 have some history.)  The peak in DARM at 78 Hz is also not here.  We will see if it stays gone, and check soon to see if the blinear coupling of ETMX ISI motion to DARM is gone with the beam diverter closed.  

Comments related to this report
evan.hall@LIGO.ORG - 17:34, Tuesday 06 October 2015 (22288)

Spectra attached. The performances of the X and Y QPDs are now comparable.

Non-image files attached to this comment
joshua.smith@LIGO.ORG - 07:34, Wednesday 07 October 2015 (22299)DetChar

Glad it was found. Attached are before/after spectra from good science times at 9UTC yesterday and today. The first two show the differences in the strain channel. The biggest feature removed is a nasty wide bump around 78Hz. The last three show the differences in the QPD signals. Very different. For detchar folks that might be wondering about what the beam diverter does, see the intro in T1100252. 

Finally, the last three plots shows another difference I spotted. There is a nasty feature at 640Hz that is gone today. I'm not sure if this is associated with the diverter and will keep an eye on it. 

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joshua.smith@LIGO.ORG - 10:43, Wednesday 07 October 2015 (22302)DetChar

Stan pointed out that a line around 1278Hz also disappeared. See spectrum below. The spectrogram of how this line varies is quite similar to the 640Hz line, and lo and behold 640*2 = 1280.

I still don't know if the 640 and 1278 are for sure from the diverter. If the diverter was switched off during lock, and I knew the exact time, I could tell. But I haven't been able to find the time or the diverter switch channel to read in my MEDM hunting, please advise. 

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jenne.driggers@LIGO.ORG - 13:57, Wednesday 07 October 2015 (22307)

Josh -

The beam diverter was closed in between lock stretches.  Because it is mounted on the suspended TMS, moving the diverter moves the TMS, which requires realignment of the interferometer. 

It was open through the lock stretch that ended ~14:00 UTC on 6 Oct 2015, and was closed before the beginning of the lock stretch that started ~00:30 UTC on 7 Oct 2015.

sheila.dwyer@LIGO.ORG - 14:32, Wednesday 07 October 2015 (22309)

The beam diverter readback channels are:

 H1:SYS-MOTION_X_BDIV_A_POSITION (similar for Y) 1 is closed.  

joshua.smith@LIGO.ORG - 17:06, Wednesday 07 October 2015 (22313)DetChar

Thanks Sheila and Jenne, the 78, 640, and 1278Hz stuff was all there at the end of the last lock when the X BDIV was zero (open). They were all gone on the first lock when X BDIV was 1 (closed). 

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sheila.dwyer@LIGO.ORG - 06:02, Thursday 08 October 2015 (22333)

Just to note, I got a chance to make a few excitations on ETMX ISI last night (WP5528 again)  and it seems that there is still a bilinear coupling from ETMX ISI motion to DARM which is much larger than the linear coupling from ETMY ISI motion; that this coupling at 75 Hz hasn't changed much with the beam divereter closed; and that noise from this is not neglibigle in the DARM noise budget over a broad range of frequencies from about 50-90 Hz.

H1 SYS (ISC, SEI)
sheila.dwyer@LIGO.ORG - posted 09:57, Tuesday 06 October 2015 - last comment - 15:24, Wednesday 07 October 2015(22211)
duty cycle sept 17th to Oct 2nd, downtime Oct2-3rd

Motivated by our locking difficulties at the end of last week, I downloaded guardian state data for the last two weeks to look into our locklosses durring the CARM offset reduction.

To start with the good news, the script that I use to do this automatically makes a few figures that tell us about our duty cycle, and we are doing well overall. As usual, I am only looking at the guardian state, and not considering any intent bits.  My reaasoning is that the hardest part is getting and keeping the IFO locked, and that is currently the important limit to our duty cycle. 

The main weakness in our lock acquistion sequence now seems to be the early steps of CARM offset reduction, as we saw yesterday. 

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sheila.dwyer@LIGO.ORG - 22:12, Tuesday 06 October 2015 (22294)

As requested, I've made a few plots which bettter show how individual locks contribute to our total low noise time.  The first attached plot is a repeat of the histogram of lock times from above, with the lower panel sshowing the sum of the low noise time accumlated in all the locks in that bin of the histogram.  The second attached plot shows the accumlated low noise time, theere is a point for each lock stretch with the length of the lock on the horizontal axis and the cumulative low noise time on the vertical axis.  

The message of both plots is that we accumulate a lot of our time durring a small number of long locks.  The secondd plot shows that in the 3 longest locks (out of 33 total) we accumlated 133 hours of low noise time out of 312 total hours.

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sheila.dwyer@LIGO.ORG - 15:24, Wednesday 07 October 2015 (22310)

I also had a look at relocking times for this period based on a request from Keita. 

The minimum relocking time was 20 minutes (this is measured from the time of lockloss to the time that the guardian arrives in nominal low noise), the median was 53 and the maximum was 6 hours and 20 minutes (long stretch of downtime on the evening of Oct 2nd is not included here).

A histogram is attached.

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