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Reports until 16:01, Monday 05 June 2017
H1 General
travis.sadecki@LIGO.ORG - posted 16:01, Monday 05 June 2017 (36665)
Ops Day Shift Summary

TITLE: 06/05 Day Shift: 15:00-23:00 UTC (08:00-16:00 PST), all times posted in UTC
STATE of H1: Planned Engineering
INCOMING OPERATOR: Jim
SHIFT SUMMARY:  Commissioning all day hunting down ALS issues and inability to proceed past PREP_TR_CARM.
LOG: 

22:52 Jenne and Sheila to LVEA ISCT racks to look at electronics.

H1 SEI
jim.warner@LIGO.ORG - posted 14:52, Monday 05 June 2017 (36664)
Z tilt decoupling on HAM ISI's

Similar to the work done on the BSC-ISI's, I've been working on tilt decoupling on the HAMs. So far I have most of the measurements needed for the the output HAMs, I just need a couple more measurements on the input HAMs to finiish. The first attached plot is the Z to X/Y coupling for HAM6. For this data, I took the Z tf at the isolation bank input with the ISI isolated with high blends (some measurements had sensor correction on, some off, it doesn't seem to matter much, off is probably best though). I then inverted the gs13 response (to get the units to nm/s), converted to nm and then divided by -g/w^2 to get the effective tilt. Doing this let me calculate the magnitude and sign decoupling element by getting the average of the Z to X/Y tf where the phase was either 0 or 180, usually over 10 to 80-100 mhz. I was also able to avoid getting the RX/RY tfs as I done for the BSCs by thinking a bit about the RX/RY to Y/X tfs. These transfer functions go as -g/w^2, so their signs are also possible to figure out, and after some thinking I realized I could model them by using (essentially) a +1 for the RX to Y tf and -1 for RY to X tf (something Jeff mentions in his eligo era log here). The second attached plot shows the improvements I was able to get for HAM6 Z to RX/RY decoupling.

It's interesting that while the Z tilt decoupling clearly needed to be done, the X/Y to RX/RY coupling does not seem so bad. I have taken several X or Y tfs, but all of the coefficients are pretty small (on order of .1%). In fact the coefficients are small enough that the X to RY or Y to RX coupling is hard to seen. The third attached plot is the HAM4 Y to RX/RY measurement. The blue trace is the Y to X tf and gives a coefficient of about .0015 for the Y to RY element. The red trace is the Y to Y tf and is dominated by the Y to Y closed loop tf. The first couple of frequency points around 5 mhz indicated a Y to RX coefficient of something like .00005. I don't fee like waiting around for a measurement long enough to resolve that any better. This seems to be typical of the "beam-line" coefficients for the HAMs.

So far the elements I've installed are:

HAM 4     Z        Y

    RX     .01    .0015

    RY    -.01

HAM 6     Z   

    RX     -.0181

    RY      .0178

I have a few more calculated coefficients, but I'm going to wait for a chance to do a before/after measurement to make sure I actually make things better.

 

 

Images attached to this report
H1 CAL (CAL)
travis.sadecki@LIGO.ORG - posted 13:22, Monday 05 June 2017 (36663)
End Y PCal PD output step

JeffK, TravisS

We noticed a DIAG_MAIN message reporting that the EY PCal RX PD was more than 1% out of normal.  We had this warning put in place to indicate if clipping we have seen previously at EY returns.  This time, however, it turned out not to be clipping, which is a good thing, but rather that something had happened that railed the OFS loop.  Trending the TX, RX, and OFS PDs showed that they all railed at the same time (of course) on June 2.  Talking to Sheila and looking at Ed's OPS shift summary from that day, there was a lot of electronics work done at EY earlier in the day.  Not conclusive that the two things are related, but definitely possible.

Hopefully this doesn't happen very often, but if it does, the fix is very easy.  Open the PCal screen for the end station of concern (from the CAL tab on the Sitemap), click Shutter 'OFF' button circled in the attached screenshot, then click the Shutter 'ON' button.  This should fix the issue.  If it does not, please contact your friendly neighborhood PCal person.

Images attached to this report
H1 ISC
peter.king@LIGO.ORG - posted 12:40, Monday 05 June 2017 (36661)
Old ALS-X laser
I measured the output power as a function of laser crystal temperature for the ALS laser that was at EndX
up until recently (InnoLight Prometheus S/N 2011B).

    The laser crystal temperature was varied by ~7 degC, which corresponds to about 42 GHz of frequency
tuning.  At the time of the measurements, the laser settings were:
diode 1 temperature             21.00 degC
diode 2 temperature             20.30 degC
diode current                   1.837 A
doubling crystal temperature    32.9 degC

    The laser was set to the following in order to put it into the middle of the mode hop free region
laser crystal temperature       26.11 degC
doubling crystal temperature    33.09 degC

    The output power of the laser was 1.600 +/- 0.002 W at 1064 nm and 48.1 mW at 532 nm with these
settings.
Images attached to this report
LHO VE
logbook/robot/script0.cds.ligo-wa.caltech.edu@LIGO.ORG - posted 12:10, Monday 05 June 2017 - last comment - 15:46, Monday 05 June 2017(36660)
CP3, CP4 Autofill 2017_06_05
CP4 Fill completed in 244 seconds. Starting CP4 fill. LLCV enabled. LLCV set to manual control. LLCV set to 70% open. Fill completed in 244 seconds. TC B did not register fill. LLCV set back to 41.0% open.
Images attached to this report
Comments related to this report
david.barker@LIGO.ORG - 12:50, Monday 05 June 2017 (36662)

WP7016, removed reporting of CP3 autofill since this no longer runs. Noticed I've left CP3 in the alog title.

david.barker@LIGO.ORG - 15:46, Monday 05 June 2017 (36666)

CP4 autofill ran late today, at 11:16 PDT instead of 11:02. Turns out checking the code into svn changed its permissions (became non executable). I set the executable prop-tag on this file to fix this. The script was ran (by crontab) at 11:16 for today, and was reset to 11:02 for tomorrow.

LHO General
kyle.ryan@LIGO.ORG - posted 11:40, Monday 05 June 2017 (36659)
~1828 hrs. UTC -> Removed ladder which had been leaned against OMC tube and SR3 optical lever laser enclosure
My bad!  I had neglected to remove this ladder from having used it to access IP3 and IP4 following the recovery of the ITMx incursion a few weeks ago.  It was also in contact with the "Thermos" cooler (laser enclosure?) located at the base of the "giraffe" pier on the South side of the OMC tube near HAM4.
H1 SEI (CDS, SEI, SUS)
jeffrey.kissel@LIGO.ORG - posted 11:33, Monday 05 June 2017 (36658)
H1SUSOMC USER Watchdog Connected to ISI HAM6
J. Kissel
II 4705
WP 7010

After recent review of open FRS/Integration Issue tickets, I've found and remembered that we haven't yet connected the OMC SUS's USER Watchdog to the ISI HAM6 (and hasn't been since before the OMC SUS was initially installed before O1). 

A while back, when we re-remembered this we'd argued that, if/because the OMC SUS OSEMs are covered in the IOP / Independent Software Watchdog (SWWD), that we need not both connecting the USER watchdog. However, I think now (a) since LLO has their's connected, and (b) if we're going to rely soley on the SWWD, this should be done for all chambers, not just HAM6, and it should be raised to a more general review of watchdog philosophy / ECR / integration issue, that is more work than we want to do today.

So, in prep for making the change, I've connected the USER watchdog at the top-level model of 
   /opt/rtcds/userapps/release/sus/h1/models/h1susomc.mdl. 

We'll restart the model if/when convenient today or if not tomorrow during maintenance. This will not require a DAQ restart.

See attached before vs. after comparison of the simple change in the lower right-hand corner.
Images attached to this report
H1 PSL
jim.warner@LIGO.ORG - posted 11:17, Monday 05 June 2017 (36657)
PSL Weekly- FAMIS 7441

Laser Status:
SysStat is good
Front End Power is 34.06W (should be around 30 W)
HPO Output Power is 158.5W
Front End Watch is GREEN
HPO Watch is GREEN

PMC:
It has been locked 3 days, 19 hr 9 minutes (should be days/weeks)
Reflected power = 16.11Watts
Transmitted power = 59.46Watts
PowerSum = 75.57Watts.

FSS:
It has been locked for 0 days 0 hr and 45 min (should be days/weeks)
TPD[V] = 3.415V (min 0.9V)

ISS:
The diffracted power is around 3.2% (should be 3-5%)
Last saturation event was 3 days 19 hours and 9 minutes ago (should be days/weeks)

Possible Issues:
Head 1-4 flow error, see SYSSTAT.adl

 

H1 SEI
edmond.merilh@LIGO.ORG - posted 10:49, Monday 05 June 2017 (36656)
Monthly Seismometer Mass Check - FAMIS #6087

Averaging Mass Centering channels for 10 [sec] ...
2017-06-05 10:43:01.360996


There are 5 T240 proof masses out of range ( > 0.3 [V] )!
ETMX T240 2 DOF X/U = -1.017 [V]
ETMX T240 2 DOF Y/V = -0.987 [V]
ETMX T240 2 DOF Z/W = -0.743 [V]
ITMX T240 1 DOF X/U = -0.664 [V]
ITMX T240 3 DOF X/U = -0.685 [V]


All other proof masses are within range ( < 0.3 [V] ):
ETMX T240 1 DOF X/U = -0.064 [V]
ETMX T240 1 DOF Y/V = -0.03 [V]
ETMX T240 1 DOF Z/W = -0.008 [V]
ETMX T240 3 DOF X/U = -0.05 [V]
ETMX T240 3 DOF Y/V = -0.161 [V]
ETMX T240 3 DOF Z/W = -0.052 [V]
ETMY T240 1 DOF X/U = -0.008 [V]
ETMY T240 1 DOF Y/V = 0.18 [V]
ETMY T240 1 DOF Z/W = -0.224 [V]
ETMY T240 2 DOF X/U = 0.147 [V]
ETMY T240 2 DOF Y/V = -0.231 [V]
ETMY T240 2 DOF Z/W = 0.032 [V]
ETMY T240 3 DOF X/U = -0.244 [V]
ETMY T240 3 DOF Y/V = -0.019 [V]
ETMY T240 3 DOF Z/W = 0.271 [V]
ITMX T240 1 DOF Y/V = -0.213 [V]
ITMX T240 1 DOF Z/W = -0.15 [V]
ITMX T240 2 DOF X/U = -0.162 [V]
ITMX T240 2 DOF Y/V = -0.135 [V]
ITMX T240 2 DOF Z/W = -0.182 [V]
ITMX T240 3 DOF Y/V = -0.131 [V]
ITMX T240 3 DOF Z/W = -0.075 [V]
ITMY T240 1 DOF X/U = -0.024 [V]
ITMY T240 1 DOF Y/V = -0.046 [V]
ITMY T240 1 DOF Z/W = -0.058 [V]
ITMY T240 2 DOF X/U = 0.125 [V]
ITMY T240 2 DOF Y/V = 0.138 [V]
ITMY T240 2 DOF Z/W = 0.008 [V]
ITMY T240 3 DOF X/U = -0.248 [V]
ITMY T240 3 DOF Y/V = 0.053 [V]
ITMY T240 3 DOF Z/W = -0.263 [V]
BS T240 1 DOF X/U = -0.166 [V]
BS T240 1 DOF Y/V = -0.03 [V]
BS T240 1 DOF Z/W = 0.219 [V]
BS T240 2 DOF X/U = 0.067 [V]
BS T240 2 DOF Y/V = 0.195 [V]
BS T240 2 DOF Z/W = 0.007 [V]
BS T240 3 DOF X/U = 0.028 [V]
BS T240 3 DOF Y/V = -0.068 [V]
BS T240 3 DOF Z/W = -0.118 [V]


Assessment complete.

 

2017-06-05 10:45:39.355333
All STSs prrof masses that within healthy range (< 2.0 [V]). Great!


Here's a list of how they're doing just in case you care:
STS A DOF X/U = -0.609 [V]
STS A DOF Y/V = 0.203 [V]
STS A DOF Z/W = -0.448 [V]
STS B DOF X/U = 0.492 [V]
STS B DOF Y/V = 0.314 [V]
STS B DOF Z/W = -0.307 [V]
STS C DOF X/U = -0.37 [V]
STS C DOF Y/V = -0.661 [V]
STS C DOF Z/W = 0.497 [V]
STS EX DOF X/U = 0.018 [V]
STS EX DOF Y/V = 0.624 [V]
STS EX DOF Z/W = -0.01 [V]
STS EY DOF X/U = 0.002 [V]
STS EY DOF Y/V = 0.213 [V]
STS EY DOF Z/W = 0.443 [V]


Assessment complete.

 

 

 

H1 PSL
edmond.merilh@LIGO.ORG - posted 09:32, Monday 05 June 2017 (36654)
PSL Weekly Report - 10 Day Trends FAMIS #6151

Ed, Jason

Everything looks normal. The ever degrading HPO diode box 1 is causing a strange anomalous increase in the DC output power due to the changing thermal lens in head 1 resulting in an operating point which is, ironically,  actually better for the laser.

Images attached to this report
H1 General
travis.sadecki@LIGO.ORG - posted 08:40, Monday 05 June 2017 (36651)
Ops Day Shift Transition

TITLE: 06/05 Day Shift: 15:00-23:00 UTC (08:00-16:00 PST), all times posted in UTC
STATE of H1: Planned Engineering
OUTGOING OPERATOR: None
CURRENT ENVIRONMENT:
    Wind: 2mph Gusts, 1mph 5min avg
    Primary useism: 0.01 μm/s
    Secondary useism: 0.11 μm/s
QUICK SUMMARY:  Arrived to find the arms locked in green (they have been locked in green for ~12 hours according to trends).  Will consult with commissioners as to how to proceed today.

 

H1 PSL (PSL)
jeffrey.bartlett@LIGO.ORG - posted 07:43, Monday 05 June 2017 - last comment - 07:44, Monday 05 June 2017(36648)
Monthly PSL Chiller Filter Check (FAMIS #8297)
   Perform monthly PSL Chiller Filter Checks. No debris or air found in either filter. There is some yellowing of the filter pleats but this is normal. All is normal with both the Crystal or Diode chiller filters. 

   Closing FAMIS task #8297.
Comments related to this report
jeffrey.bartlett@LIGO.ORG - 07:44, Monday 05 June 2017 (36649)
Water levels for both chillers are good. 
H1 ISC
sheila.dwyer@LIGO.ORG - posted 18:43, Sunday 04 June 2017 - last comment - 16:10, Monday 05 June 2017(36645)
ALS work today

Summary: 

After swapping a few electronics that we broke while investigating the ALS glitches at EY, the glitches are still there, but not nearly as bad as they were.  We have had these glitches go away on their own before when nothing was done, so that might be what is happening.  Now they are at End X, and about as bad as they were at End Y for most of the week.  ALS still will not lock for longer than 10 minutes.  It might be that this problem will go away on its own, but will probably come back again.  

Things that are not the cause of glitches at EX:

From PLL bypass test:

Other things that are not the problem:

Things that we haven't checked:

I recommend that the first thing in the morning operators take the ISC lock guardian to locking arms green, wait there for 10-20 minutes, and look at second trends of the arm transmissions.  You can compare them to the screenshot I've attached here, if the glitches are gone or much smaller it would be worth doing an initial alignment and trying to lock to DC readout, if the glitches are still there it is not worth trying. 

Images attached to this report
Comments related to this report
daniel.sigg@LIGO.ORG - 08:24, Monday 05 June 2017 (36650)

A surprising number of the small glitches in Y align with bigger glitches in X. We should take a look at the fiber distribution.

keita.kawabe@LIGO.ORG - 09:07, Monday 05 June 2017 (36652)

zooming in you really can see that some of them are aligned.

Images attached to this comment
keita.kawabe@LIGO.ORG - 09:19, Monday 05 June 2017 (36653)

Fibers including ALS fiber with flapping tag. The fan of the network equipment is blowing directly on it.

Daniel pinged this and both arms unlocked. It's not clear this is the problem but it's not good anyway and will be fixed. (WP7015)

Images attached to this comment
keita.kawabe@LIGO.ORG - 10:24, Monday 05 June 2017 (36655)

Richard's solution was a yellow tubing around the fibers. A stuffed bag as a wind barrier is probably Daniel's thing.

After that the glitches seem to have been gone. We'll see if ALS survives longer than 10 minutes.

Images attached to this comment
david.barker@LIGO.ORG - 16:10, Monday 05 June 2017 (36667)

perhaps we can put the side panel on the networking rack. I suspect we left it off since the Cisco core switch is sideways venting.

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