Kyle, Gerardo Vented X-end (DP < -45 C)-> Vented Y-end (DP < -35 C) -> Installed NEG assembly on BSC6 -> Installed TMDS reducing nipple+valve+elbow on BSC10 Kyle, Gerardo, Bubba Removed BSC9 West door at X-end -> Removed BSC10 North door at Y-end Bubba Connected TMDS 100 psi line to purge-air skid
(Keita, Kiwamu, Corey)
After the Vacuum crew removed the door, and Jim Warner locked up the ISI (& removed the Contamination Control plates), we started TMS work. Summaries of the TMS activities are below:
1) Green Clipping
The ETMx Bias were:
In order to center the beam on the ISCT-EX REFL_PD, the ETMx was steered to the following biases:
After this Keita entered the chamber and looked for clipping. He started with the first steering mirror on the TMS, the one that showed very bright scattering back in Feb., and no clipping was observed this time though the beam was somewhat low, and there was some ghost beam hitting the top right edge.
Keita checked downstream optics and no clipping was observed either. No changes were made to the TMS optics alignment.
2) Strain Relief of QPDs
Ran into a problem with attaching the Strain Relief Parts (D1101911 & D1002110) to the QPDs. The problem was attaching the Strain Relief Clamp (D1101911) to the main QPD Housing. Unfortunately, the 1/4-20 hole in the housing had bad threads for two of the four QPDs. It's a thru-hole and screw could only go in a thread or two. My guess is the machinist tapped the holes from the backside with a tapered tap & didn't tap all the way through. So some of the threads at the entrance of the hole aren't cut completely.
Keita & Kiwamu went ahead and installed the Strain Relief Assy on the two QPDs which were fine.
As for the remaining two, we might use thinner 10-32 or 10-24 screws, long enough to go through the QPD base and the strain relief combined, and use a nut and two washers if such things are found. Otherwise we'll leave them without strain relief, as there's more than 1/4" of space between the cable collar and the metal part of the QPD support structure.
3) Krytox Beam Diverter
Corey went into the chamber, loosened the screw that attaches the shaft collar to the axle, slid the axle and the jewel bearing out on one side, applied Krytox, did the same to the other side, rebalanced the diverter by attaching 5 1/4" and one #8 vented washers as a counter mass, and assembled everything together.
This was done all in situ. Tested opening/closing via MEDM several times and it worked fine.
I modified ASC_MASTER today to give us the option of using AS 45 Q Yaw signals to damp roll, because yesterday we saw that this was needed for ETMX. The model is committed, and I added an medm screen that is linked from the ASC overview and the small bounce roll monitor screen for the matrix. The ASC model changes were done today because Adam at LLO will also work on this library part tomorow durring maintence.
I also added log scale monitors to the oaf model, but made two typos in doing this. I've fixed the mistakes and recompiled the model, we will wait to do a make install until the normal maintence time tomorow.
Modified installed Matlab 2010a system libraries to point to Ubuntu12 system libraries to allow awgstream to run. This is an unusual request, as the control room is set up to run Matlab 2012b by default, but one user had a script which runs with Matlab2010a (but not 2012b).
All times in UTC
15:00 It Seems the NPRO trippedhttps://alog.ligo-wa.caltech.edu/aLOG/index.php?callRep=19141. GRB alert/alarm is sounding so I'm getting my first look at where thing are regarding this. LASER is back up and Peter i working on getting it back into nominal operating condition. End Station LASER status is BUILDING SAFE for vent work. This means all viewports are secured, ISC tables are locked and safety signs have been transitioned.
15:31 Cleaning crew done second cleaning at EX and goin to EY
15:44 Peter to Transistion the LVEA to LASER SAFE
15:46 Turned of both CO2 LASERS.
15:57 Gary ad Danny to EX
16:00 LVEA transitioned to LASER SAFE.
16:02 Picomotors disabled at EX, EY and HAM6
16:09 Bartlett to cleaning area.
16:25 Bartlett came out and went back in to prepare HAM6 area for Vent
16:26 Cleaning crew done with second cleaning at EX.
16:33 ISS is stable now and the REFSIGNAL is set to -2.12 for 6.5% AOM diff power
16:36 GV20 (EX) closed. (not sure what time). Gary and Danny to EY to meet Kyle. GV18 Not closed yet.
16:57 Closed Green Beam ISC table shutters
17:15 Arnaud testing a script to test MC1 suspensinon actuators
17:22 Danny and Travis at EX
18:00 Betsy, Travis, Danny and Gary to EY
18:06 Bartlett to EY
18:10 Karen and Christina into LVEA for cleaning
18:14 J Worden and co. dropping a ditch digger of at the turnaround next to VPW.
18:21 Jeff leaving EY
18:24 Ditch machine dropped off and Truck is moving to MX to pick up a scissor lift
18:28 Gary and Danny back from EY
18:46 Betsy and Travis back from EY
18:48 Hugh back from EX
18:57 GV18(EY) closed
19:12 Corey into LVEA
19:15 Betsy into the LVEA w Bay
19:30 Betsy out nd going to EX
19:38 Sheila informed me of a not so distant DAQ restart.
20:00 Danny and Travis to EY
20:16 Jim is at EX and garbing. He will lock the ISI in about 20-30 min.
20:44 Keita, Kiwamu and Corey to EX to start TMS investigation.
21:03 DAQ restart
21:15 Kate and Calum on site. They will be here for a couple of weeks.
22:18 Hugh into the LVEA to install 2 STS2 seismometers in the BG
22:32 Hugh out of the LVEA
22:42 Betsy out to HAM6 to have a look
Generated Xilinx iMPACT configuration archives (.iaf) for most recent timing firmware and uploaded them to the DCC pages corresponding to their respective device firmware: 1PPS Locking Firmware: https://dcc.ligo.org/LIGO-E1200033 Comparator Firmware: https://dcc.ligo.org/LIGO-E1200034 IRIG-B Firmware: https://dcc.ligo.org/LIGO-E1200035 DuoTone Firmware: https://dcc.ligo.org/LIGO-E1200036 The links for these .iaf files on the FPGA code page of the Timing Wiki (https://awiki.ligo-wa.caltech.edu/aLIGO/TimingFpgaCode) are now functioning.
To correct problems with the Simulink web view of models (accessible from https://lhocds.ligo-wa.caltech.edu/simulink/) several models have been changed to be saved at the top level of the model. If this isn't done, the top level of the model is not generated for the web view. The models which were changed are: h1iscex h1iscey h1isietmx h1pemcs h1pemex h1pemey h1pemmx h1pemmy h1susauxb123 h1susauxh34 h1susetmx h1susim There are still a few models that need to be changed.
This appears to be correctable without modifying model files by adding parameters to the slwebview() call in the matlab script. I'll make the change in time for the 18:00 hour model web view to see if it works.
Attached is a noise budget for the DARM spectrum from 2015-06-07 00:00:00Z–02:00:00Z. Notes:
Conclusions:
Attached are the MICH and SRCL coupling TFs into OMC-DCPD_SUM.
Restarted the data concentrator because of changes to the h1asc and h1oaf models.
model restarts logged for Sun 14/Jun/2015
2015_06_14 00:04 h1fw1*
2015_06_14 15:31 h1fw1*
* = unintentional restart. Last day of ER7.
Have locked HEPI at X End.
The rotational DOFs are within ~100nrads of the closed loop running position. The Translational DOFs were let go as the Rots were dialed in: X -5um, Y +67um, Z +108um. These are the deltas from the nominally servo'd position.
The PSL is back up. PMC is locked @ 23.2W w/2.4W in refl. This is slightly over the 10% that is consideredthe high range of optimal.
The ISS is stabilized at 7.2%diffracted power.
The FSS TPD is showing 1.34V
Frontened watchdog not reset (RED) output power @ HPO is 28.9W
HPO (not used) watchdog is RED.
I'm told this was intentional. I wasn't informed.
This was actually completely accidental. Peter and I went out to see if we could pull a log off of the NPRO UPS as part of our investigation into this morning's NPRO trip. Turns out that when you plug in a DB9 cable to the back of the UPS, the UPS shuts off. We did not know this. Now we do. Note to self...
In other news we were not able to establish communication between the laptop and the UPS, not sure why. Will continue to investigate.
That make me feel much better about not having gone out there alone to try it!
ISS is stable now and the REFSIGNAL is set to -2.12 for 6.5% AOM diff power
Visitors: Arnaud, Katie (SURF student), Ivan (STAR program) Gary T. and Danny S., Stefan from Columbia U(timing system), Curtis Rau (SURF Student)
SEI: General maintanance. Also supporting the Vent activities.
VAC: Kyle preparing for End Station vents. Doors should be off by this afternoon. ALS LASERS will need to be turned off.
SUS: Danny S and Gary T on site to assist with discharging tests masses and working on EX pitch issues.
FAC: Clean Rooms and Dust Monitors are running - second cleaning of End Sytations in progress. Beam Tube cleaning is on ongoing.
I think that's it?
This is a minor update to those discussed in log 18987. In addition to importing live damping filters from the sites into the model (with a 5 min delay), you can now request damping filters from a specific gps time. So svn up ../SusSVN/sus/trunk/QUAD/Common/MatlabTools/QuadModel_Production.
The requirements are the same for reading live damping filters: you must have nds2 and various corners of the noise budget svn on your computer. See the notes at the bottom of this log.
The model script, generate_QUAD_Model_Production, has instructions on how to run the model with all the various features. An example of generating a model with damping filters from a specific gps time is show here:
quadModel = generate_QUAD_Model_Production(frequency_vector,'h1etmy',[],0,true,'gps1118413940h1etmy',0,0,true,8);
* frequency_vector is some frequency vector you specify.
* 'h1etmy' is the customized H1 ETMY parameter file ('quadopt_fiber' is the general quad file). All other quads have parameter files now too, but h1etmy is the only unique one at this point.
* true (the first one) says you want damping
* 'gps1118413940h1etmy' says you want the damping filters from H1 ETMY that were running at gps time 1118413940. The 'gps' prefix is what triggers the flag to read from the given gps time.
* true (the second one) says you want violin modes
* 8 says you want the first 8 violin modes in the model (2 is the default if not specified)
I am not sure how this does foton file version control when reading the filters. It claims it is loading the foton file from the given gps time, but for all I know it is actually loading the current foton file and simply displaying the gps time you gave it. One of the noise budget experts may know more about this (the site filter reading code is adapted from the noise budget stuff, courtesy of Chris Wipf).
In general, let me know if any of these new feature do not work properly, or should be modified in any way. They have been tested on my laptop, but there could be something I have missed.
The generate script has instructions for setting up your computer to get the running damping filters from the sites (either live or from a gps time). This text is copied here:
> Follow noise budget SVN checkout instructions here
https://awiki.ligo-wa.caltech.edu/aLIGO/NoiseBudget
Checkout the following addpath paths:
svnDir = '../NbSVN/aligonoisebudget/trunk/' (the '..' must be the same as for the SusSVN, e.g. /ligo/svncommon/)
addpath(genpath([svnDir 'Externals/SimulinkNb/']))
addpath([svnDir 'Common/Utils/NoiseModel/'])
addpath([svnDir 'Common/Utils/'])
> Follow NDS2 install instructions here
https://wiki.ligo.org/viewauth/RemoteAccess
Matlab should be pointed to this version of liveparts.m:
../NbSVN/aligonoisebudget/trunk/Externals/SimulinkNb/SimulinkNb/liveParts.m
Jeff and Greg found the necessary screws, washers and nuts, so we'll do the rest of QPD strain reliefs the first thing in the morning, then rebalance TMS. We'll be done by noon-ish.
EX station is left in laser hazard.