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Reports until 16:55, Wednesday 11 October 2017
H1 SUS
betsy.weaver@LIGO.ORG - posted 16:55, Wednesday 11 October 2017 (38992)
ITM stat today

Today, Travis and I put the ITMx main and reaction chains back together and bolted them up.  This process included reseating the UIM and PUM magnet flag assemblies to their proper controls configuration and reattaching them to their 8 respective locations.  We also had to apply First Contact to the CP-HR side and peal it and the ITM-AR sheet prior to pushing the structures togetehr to their nominal 5 mm separation.  The unit is still sitting just outside of the chamber, waiting for install later this week.

GariLynn and I also spent some time installing the AUX alignment system she procured for us in the ITMy chamber.  It is currently installed/clamped to the in-chamber stool pointing toward HAM4/5/6.  We'll continue alignment of various targets tomorrw.

 

Images attached to this report
H1 SQZ (CDS, DAQ)
david.barker@LIGO.ORG - posted 16:34, Wednesday 11 October 2017 (38991)
renamed h1sqzwfs model running on h1asc0, added to DAQ

Daniel, Sheila, Dave:

we opted to rename the model h1sqzwfs to resolve an EPICS channel naming duplication while preserving the correct fast channel names.

Because the original model had already been installed, I hand edited the rtsystab, H1.ipc and testpoint.par files to correct the name. The new model was added to the DAQ and to the CDS overview MEDM.

DAQ was restarted at 16:27 PDT to acquire h1sqzwfs

H1 General
edmond.merilh@LIGO.ORG - posted 15:56, Wednesday 11 October 2017 (38983)
Shift Summary - Day

TITLE: 10/11 Day Shift: 15:00-23:00 UTC (08:00-16:00 PST), all times posted in UTC
STATE of H1: Planned Engineering
INCOMING OPERATOR: None
SHIFT SUMMARY:
LOG:

16:05 Gerardo out to VPW

16:15 Betsy and Garilynn out to biergarten

17:27 Fil to MX to look for PEM test equipment

17:31 Gerardo out to HAM5

17:43 TJ out to HAM5

17:45 Jeff K and Sheila out to squeezer area

18:36 Jeff and Peter out of the PSL

19:10 Richard into CER

19:41 Fil to LVEA

20:15 Richard back into the CER

20:26 Jeff and Peter back into the PSL to check for water leaks

21:08 Travis and Betsy out to biergarten

21:31 Norna and Gerardo out to HAM5

 

 

 

 

 

 

 

 

 

 

 

 

H1 PSL
peter.king@LIGO.ORG - posted 12:02, Wednesday 11 October 2017 - last comment - 16:58, Wednesday 11 October 2017(38990)
Noise eater
There was some ambiguity as to whether the NPRO noise eater was on or off because the MEDM screen
did not change.

    Attached is a plot of the NPRO output as seen by the photodetector inside the front end laser
with the noise eater toggled on and off.  Clearly the switch on the power supply works.  However
the status indicator did not change.  The output voltage of the photodetector was 0.210 V and the
number of counts on the MEDM screen was ~ -335.  Blocking the light to the photodiode resulted in
the status indicator changing and an increase in the number of counts to ~ -5000.  We know that
the change in status occurs around ~ -1792 counts.

    I do not recall when this problem first manifested itself.
Images attached to this report
Comments related to this report
peter.king@LIGO.ORG - 16:58, Wednesday 11 October 2017 (38993)
From the trend data, it looks like the noise eater signal started misbehaving about a week ago.  The photodetector monitoring
the output power of the NPRO seems to be still working.  I would be inclined to check the field box that the
H1:PSL-MIS_NPRO_RRO_OUTPUT is attached too, as there maybe a large DC offset in that monitor signal's output.
H1 SQZ (CDS, DAQ)
david.barker@LIGO.ORG - posted 11:02, Wednesday 11 October 2017 (38989)
new h1sqzasc model running on h1asc0. Working channel naming issues

Sheila, Dave:

the first version of the h1sqzasc model was started on h1asc0 yesterday. We noticed an EPICS channel was a duplicate of h1asc (H1:ASC-DCU_ID), caused by top naming an ASC block in h1sqzasc. We are working this issue. Until it is resolved I'll not add this model to DAQ.

H1 SQZ (CDS, DAQ)
david.barker@LIGO.ORG - posted 10:57, Wednesday 11 October 2017 (38988)
h1susopo model change, DAQ restart

Jeff and Dave:

late entry from yesterday evening. Jeff made a model change to h1susopo (binary IO) which required a DAQ restart at 17:05 PDT Tuesday. I have just renamed the partial second trend frame file to permit NDS1 to provide date when spanning the gap.

LHO VE
chandra.romel@LIGO.ORG - posted 10:37, Wednesday 11 October 2017 (38987)
CP2 Dewar bottom fill valve issue

Kyle, Chandra

CP2's bottom fill valve (V1) had an obstuction and was allowing LN2 to sneak past and pressurize and frost the line that truck deliveries use to fill the Dewar. Both top and bottom fill valves felt closed, but Kyle opened and reseated both. Fixed.

H1 SEI
edmond.merilh@LIGO.ORG - posted 09:58, Wednesday 11 October 2017 (38986)
H1 ISI CPS Sensor Noise Spectra Check - Weekly FAMIS #6919

Elevated HF in plots is clearly due to work being done in-chambers.

Images attached to this report
H1 General
edmond.merilh@LIGO.ORG - posted 08:32, Wednesday 11 October 2017 (38982)
Shift Transition - Day

TITLE: 10/11 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: 3mph Gusts, 1mph 5min avg
    Primary useism: 0.02 μm/s
    Secondary useism: 0.22 μm/s
QUICK SUMMARY:

15:30 Travis out to biergarten with Fil

H1 SUS
travis.sadecki@LIGO.ORG - posted 16:34, Tuesday 10 October 2017 - last comment - 16:42, Tuesday 10 October 2017(38979)
ITMx and ITMy progress today

ITMx:

The first half of the day was spent packing up welding and IAS equipment and converting the space from a laser enclosure welding area to a install/assembly area.  I then replaced the middle wire segment (from top mass to UIM) that was broken during the extraction of the lower structure.  I also added the UIM non-magnetic blade dampers (NMBDs) to the blades of the main chain and removed the unused copper ECD blocks as per E1600011.  We then called Fil in to start looking into an FRS 4509 (ringheater RTD sensor non-functional).  Fil will continue this work tomorrow.

ITMy:

With Fil working on RH issues on ITMx and Garilynn visiting this week to commission the new baffle alignment equipment, we redirected our effort to ITMy.  We got as far as swinging back the ACB (Note: we had to un-swing-away the ITMx ACB since we only have one wedge, but will hopefully have another arrive in the mail from LLO shortly) and putting on optic face shields.  It is NOT locked yet. 

Comments related to this report
travis.sadecki@LIGO.ORG - 16:42, Tuesday 10 October 2017 (38980)

NMBDs installed on ITMx are serial numbers 015 and 016.

LHO VE
chandra.romel@LIGO.ORG - posted 16:18, Tuesday 10 October 2017 (38978)
Leaving pump run overnight in ME shop

Pumping on shroud prototype in mech. shop - leaving scroll pump run overnight. Pump is relatively quiet.

LHO General
corey.gray@LIGO.ORG - posted 16:15, Tuesday 10 October 2017 - last comment - 09:47, Wednesday 11 October 2017(38962)
DAY Operator Summary

I'm covering for Cheryl.  Ed covered for me from 8:50 - 10:50.  Cheryl covered 12:30- ?.  Patrick covered from ?-2:30.  And now I'm back to cover while Cheryl heads out to HAM2.

Had "Noise Eater out of range" verbal alarm this morning.  Ed mentioned filing an FRS for this on behalf of Jason.

Day's Log Of Activities

As of 23:12UTC: (completed by Cheryl)

Comments related to this report
patrick.thomas@LIGO.ORG - 09:47, Wednesday 11 October 2017 (38984)
Patrick rebooting ISC at EX: Actually h1ecatx1 EPICS IOC (alog 38970).
H1 IOO (IOO)
corey.gray@LIGO.ORG - posted 15:36, Tuesday 10 October 2017 - last comment - 15:56, Tuesday 10 October 2017(38975)
IO Items Removed From HAM2 Today + Checking/Tightening IM3 Assembly Screws

(Cheryl, Corey, Ed, Keita)

Items Removed 

The following assemblies/items were removed today & bagged/tagged:

ROM RH4:  

ROM RH5:

NOTE:  The 2" HR ("M-38-UNP-53") & Black Glass dump for this one was installed on ROM RH4

ROM RH6:

ROM LH2:

NOTE:  A V-Black Glass Dump was installed on the post for LH2.

Misc:

Tightening IM3 Assembly Screws

Here is a note Ed wanted me to take while Keita tightens:

1)  Tightened screws on top of IM3, and had this:

2) Tightened 1/4-20 bolts (on sides, OSEM plates, etc.), and had this:

 

Comments related to this report
edmond.merilh@LIGO.ORG - 15:56, Tuesday 10 October 2017 (38977)
  • IMG-2655 shows overhead view of the black glass beam dump that was added (9:00 position in photo)
  • IMG-2656 shows the HR optic w/black glass which replaced the 90/10 BS that was there before
  • IMG-2658 shows the vacant space where there were two HR mirrors (one of which resides where the BS used to)
  • IMG-2659 is a close up of the mirror that replaced the BS
Images attached to this comment
H1 TCS
thomas.shaffer@LIGO.ORG - posted 17:12, Monday 09 October 2017 - last comment - 17:23, Tuesday 17 October 2017(38956)
Installed SR3 RoC Heater

Betsy, Hugh, TJ

Last week Betsy put the heater on the table and today Hugh checked it's vertical center with an auto-level. Some washers were added to get it as close to center as possible, which ended up around 0.4mm high. Betsy and I then had to wiggle the assembly into place, and rotate the entire gold ceramic holder to allow the screws on the outside to clear the OSEM brackets. The heater is currently sitting ~6mm away from the back of the SR3 optic and it is plugged into the feed through.

Picture attached.

Images attached to this report
Comments related to this report
betsy.weaver@LIGO.ORG - 17:24, Monday 09 October 2017 (38957)

Here are a few more pics.  As TJ notes, the ROC front face is 5-6mm from the SR3 AR surface.  It is locked down in this location. 

 

Note, we followed a few hints from LLO's install:

https://alog.ligo-la.caltech.edu/aLOG/index.php?callRep=25831

 

Continuity checks at the feedthru still need to be made.  Will solicit EE for their help.

Images attached to this comment
filiberto.clara@LIGO.ORG - 12:42, Tuesday 10 October 2017 (38969)

Initial continuity test failed. Found issues with in-vacuum cable, power pins not pushed in completely. Pins were pushed in until a locking click was heard.

Reading are:
Larger Outer Pins, Heater: 66.9Ω
Inner pair (left most looking at connector from air side), thermacouple: 105Ω

hugh.radkins@LIGO.ORG - 15:24, Tuesday 10 October 2017 (38974)

Found center of SR3(-X Scribe) to be 230.2mm above optical table.  By siting the top and bottom of RoC Heater, found center to be at 231.4mm. Removed available shim to put center of RoC Heater at 229.6 for 230.2-229.6=0.6mm below perfect.

thomas.shaffer@LIGO.ORG - 08:27, Wednesday 11 October 2017 (38981)

Hugh's comment reminded me that to get the heater to fit, Betsy and I added a 1mm washer to raise the height of the assembly. In total we have 4mm of washers (2x1.5mm & 1x1mm).

stephen.appert@LIGO.ORG - 17:23, Tuesday 17 October 2017 (39058)TCS
I conducted measurement of quantity 6 of [D1600104 SR3 ROC Actuator, Ceramic Heater Assy] at CIT on 4 March 2016. Dirty state before baking.
The serial number of the heater assy installed in LHO HAM5 is S1600180 - see https://ics-redux.ligo-la.caltech.edu/JIRA/browse/ASSY-D1500258-002
S1600180 Resistance = 66.8 Ohms on 4 March 2016.
There is good agreement between the as-installed and pre-bake measurements.
H1 SEI (SUS)
sam.cooper@LIGO.ORG - posted 12:46, Monday 09 October 2017 - last comment - 15:55, Wednesday 11 October 2017(38919)
What should we do during large earthquakes?

J Warner, S Dwyer, S Cooper

We've been looking at what we should do during large earthquakes. The attached plots show the state of both the SEI Guardian (State N), and the L2 watchdog (L2 WDMON) channel, the L3 Oplev and the HEPI L4C's (as the ground STS's saturated) for the 8.1 magnitude Mexico earthquake (GPS: 1188881718), alog 38570, for the chambers ITMX,ITMY,ETMX,ETMY. During the earthquake, all the ISI's tripped as well as the ITMX suspension watchdog. From these plots we think that the decrease in amplitude of the Oplev signal is due to the reduction in ground motion around this time, rather than damping of the ISI, as both the damping and the reduction in ground motion occurred at similar times.

Images attached to this report
Comments related to this report
jim.warner@LIGO.ORG - 14:42, Monday 09 October 2017 (38946)

We've also talked about seismic watchdogs a bit and why the ISIs trip after the isolation loops are shut off by the guardian. Both ETMs are in damped right now so we set the T240 threshold to 100 counts, and sure enough, the T240s started counting saturations, but did not trip the watchdog. Attached plot shows the T240 saturation counts, threshold and ST1 WD mon state. The dip on the top left plot is where we reduced the threshold, the spike on the bottom left is where the model started counting T240 saturations, and the flat line bottom right shows the watchdog didn't trip. This is as it should be.

However, what I think I've seen during ISI trips before, is the ST1 T240s saturate, ST1 trips and ST2 runs for a little bit then trips. This results in ST1 getting whacked pretty hard. I'll try to see if that's what happened with this earthquake.

Images attached to this comment
jeffrey.kissel@LIGO.ORG - 15:23, Monday 09 October 2017 (38948)SEI
J. Kissel, inspired by conversation from S. Cooper, S. Dwyer, J. Warner

I'll remind folks that this collective SEI/ SUS watchdog system has been built up sporadically over ~10 years in fits and spurts as reactionary and quick solutions to various problems by several generations of engineers and scientists. Also, the watchdog system is almost entirely designed only to protect the hardware from a software failure, and never designed to combat this latest suggestion -- protecting the hardware from the earth. So I apologize on behalf of that history at how clunking and confusing things are when discussing what to do in that situation. 

Also, I'll remind people that there are three "areas" of watchdogs: 
    (1) in software, inside the user model -- typically defined by the subsystem experts
    (2) in software, inside the upper level iop model -- typically defined by CDS software group, with input from subsystem experts
    (3) in hardware, either in the AA/AI chassis, or built into the analog coil drivers -- typically defined during initial aLIGO design phase

In my reply here, I'll only be referring to (1) & (2), though I still have an ECR pending approval regarding (3) -- see E1600270 and/or FRS Ticket 6100.

With all that primer done, here's what we should do with the suspension user watchdogs (1), and not necessarily just for earthquakes:
    (a) Remove all connection between SUS and the ISIs user watchdogs. The independent software watchdogs (2) should cover us in any bad scenarios that that connection was designed to protect against.
    (b) Update the RMS system to be *actually* an RMS, and especially, one that we can define a time-constant. The RMS system that is currently installed is some frankenstein brought alive before bugs in the RCG were appreciated (namely LHO aLOG 19658), and before I understood how to use the RCG's RMS function in general. The independent software's watchdog (2) is a good role model for this
    (c) We should rip out all USER MODEL usage of the DACKILL part. The way the DACKILL used across suspension types and platforms with many payloads is confusing and inconsistent. Any originally designed intent of this part is now covered by the independent software watchdog.
    (d) Once (b) is complete, we should tailor the lower the time-constants and the band-passing to better match the digital usage of the stage. For example, the worst that can happen to a PUM stage is getting sent junk ASC and Violin Mode Damping control feedback signals when the IFO has lost lock, but the guardian has not figured it out and switched off control.
    (e part 1) Upon watchdog trip, we should consider leaving the alignment offsets alone. Suddenly turning off alignment offsets often causes just as much of a kick to the system as what had originally set off the watchdog. HEPI has successfully implemented such a system.
    (e part 2) We should re-think the interaction between the remaining USER watchdog system and the Guardian. Currently, after a watchdog trip the guardian state immediately jumps to "TRIPPED" and begins to shut off all outputs and bringing the digital control system to "SAFE." 
    (f) Add a "bypass" feature to the watchdog such that a user can request the "at all costs, continue to try damping to top mass" in the case of earthquakes.
jim.warner@LIGO.ORG - 15:55, Wednesday 11 October 2017 (38985)

I'm attaching some more plots of what happened to the ISIs during this earthquake. The first plot is the saturation count time series for all seismometers and actuators for the test mass ISIs. All of the chambers saturated on the Stage 2 actuators first, this is the first green spike. This tripped the high gain DC-coupled isolation loops, and probably cause Stage 2 to hit it's lockers. The watchdog stopped counting all saturations for 3 seconds (by design), then immediately tripped damping loops on the saturated L4Cs or T240s. I'm not sure why the GS13s don't show up here.

The second plot I attach shows how long the ETMX was saturating different sensors. The L4Cs were saturated for about 45 seconds, the T240s and GS13s were saturated for minutes. The L4Cs never had their analog gains switched, but the chamber guardian should have switched the GS13s automatically. For this reason, if we increase the pause time in the watchdog (between shutting off the isolation loops and full shutdown), I think this shows that for this earthquake the ride-thru time needs to be more than 45 seconds.

 

Images attached to this comment
H1 SEI
hugh.radkins@LIGO.ORG - posted 16:19, Friday 06 October 2017 - last comment - 15:51, Tuesday 10 October 2017(38922)
WHAM6 5-Way Cross Added to D4--ISI rerouted through

The image attached shows the 5 way cross installed.  The Fiber feedthru (currently blanks) are visible below the cross.  The five ISI cables are rerouted to FTs on the cross but the in-air cables have not been reconnected.  I'll do that after Kyle gives it all a look and touch; fingers cross for leak checks down the road.  The facing 25p has no cables but it was readily available, that is why it isn't a blank.

Images attached to this report
Comments related to this report
hugh.radkins@LIGO.ORG - 15:51, Tuesday 10 October 2017 (38976)

Here are a couple photos with the feedthru protection on and the cables secured.  Please be very cautious with the CPS cables going out to the left.  The ends of the cable are barely behind the shroud plane and I certainly worry about them.

Images attached to this comment
H1 SEI (OpsInfo)
jim.warner@LIGO.ORG - posted 16:18, Friday 06 October 2017 - last comment - 15:58, Tuesday 10 October 2017(38921)
Python code to transition SEI systems during very large earthquakes

I've added a button the ISI_CONFIG screen that transitions the seismic systems to a robust state to protect the suspensions during a verly large earhquake, like the infamous Montana earthquake or the recent Mexican earthquakes. It's the red button that says Very Large Earthquakes. This script requests the DAMPED state for all of the chambers with ISIs and switches the gains of the all the L4Cs and GS13s. This button is likely temporary, but is probably the state we want to leave the seismic systems in when no-one is on site in the future. The script lives at /opt/rtcds/userapps/release/isi/common/scripts, and is called SET_EQ.py .

Images attached to this report
Non-image files attached to this report
Comments related to this report
cheryl.vorvick@LIGO.ORG - 06:30, Monday 09 October 2017 (38929)OpsInfo

As I recall, being the operator on site for the Montana quake, one or two optics/chambers tripped, and I couldn't see any info on a website or even on the plot of our own siesmometers about an EQ, so at first I didn't know that there was an EQ, I thought it could have been some other kind of a failure, and I only knew it was an EQ when more things tripped.

I'm wondering if, given that scenario, you would recommend that in the next observing run Operators transition SEI if any chamber trips, as a precausion for big close EQs?

Would there be enough time for SEIs to transition before a big close EQ arrives?

If not, is there any down side to having an EQ arrive mid-transition?

jim.warner@LIGO.ORG - 15:58, Tuesday 10 October 2017 (38940)OpsInfo

The motivation for this code comes from the struggles commissioners had during the Mexican earthquake on Sept 8th, this year. The goal is to put the ISIs into a state where it is as easy as possible to keep the ISI damping loops on. It's a last ditch effort to protect the suspensions. So, even if the earthquake is already tripping platforms, it would be best to make the transition, anyway.

For an earthquake as close as the Montana quake, we won't get any advanced notice. I still would not advocate just switching to this configuration just because some chamber tripped. It takes about 45 seconds for a BSC to go from Fully Isolated to damped and about 2 minutes the other way, and there will still be settings to recover after (because the script switches the gains on ISI seismometers). You will also probably have to run an initial alignment. Some thought should be given to a wall FOM for the live ground seismometer signals to help identify if there is an earthquake arriving on site, unannounced. The low frequency blrms on the wall only update every minute, and are probably too slow to help, but all 3 seismometers seeing large, similar signals at the same time is a pretty good indication.

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