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Reports until 12:52, Tuesday 29 January 2013
H1 CDS
david.barker@LIGO.ORG - posted 12:52, Tuesday 29 January 2013 (5300)
CDS maintenance

A big maintenance day today. While the DC power to the front end IO Chassis was being worked on, we shutdown all the CDS frontends with the exception of h1pemmx.

We then reconfigured the fibrer optics ports of the timing system. The MSR master, the two H1CER fanouts and the EY fanout were recofigured to the standard as agreed between LHO and LLO. The temporary fanout in the LVEA for the test stands and the MX fanout were not changed.

All the front end machines were powered down for this work. The MSR front ends were powered up in the order:

h1psl0

h1seib1,h16,h23

h1susauxh2

h1susb123,h2a,h2b,h34

h1lsc0,h1asc0, h1oaf0

EY front ends

LVEA Test Stand Front Ends

Some problem with h1pemey IO Chassis timing, moving the tcs SFP over to the pem IO Chassis fixed this.

All system should now be burt restored and switch on.

H1 SEI
hugh.radkins@LIGO.ORG - posted 12:19, Tuesday 29 January 2013 (5299)
WBSC1 HEPI Actuators all Attached
Completed the last three attachments.  No real problems encountered.

Post attachment Dial Indicator readings suggests only a little bit of shift:

Level/Tilt--The West and South sides dropped down ~0.1mm; how this actually translates into the suspended ISI tilting is difficult to deduce but I'd say the effect is less.  If it does fully tilt the Optical Table, using my level observations of the ISI table Thursday 24 January, we are still in spec; runout of 0.2mm.  It may possibly cause some grief to SUS though, SEI's condolences.

Horizontal position--I see about 0.1mm of maximum translation with most readings 1/2 or even less than that.  I would forecast a maximum rotation of 50urad CCW.

So all & all pretty good; thanks to Randy Thompson.

There is one issue with this system though.  The South Crossbeam is only about 1mm away from the HEPI Housing on the SE Corner.  This is enough room for nominal operation but over time if the system walks North for what ever reason, we may have to address that.  Attached is a photo.
Images attached to this report
H1 PSL
michael.rodruck@LIGO.ORG - posted 10:26, Tuesday 29 January 2013 - last comment - 16:33, Tuesday 29 January 2013(5297)
PSL tripped

The laser shut down earlier today due to a communication failure between the control boxes and the Beckhoff computer. What I think happened is the power to the ethernet to fiber converter for the LVEA control box was lost - this is plugged into an AC outlet and the prongs were barely in, so it probably got bumped. I'll wait until the CDS work is done to bring the laser back up.

Comments related to this report
michael.rodruck@LIGO.ORG - 16:33, Tuesday 29 January 2013 (5307)

Restarted the laser. I had noticed that the diode chiller flow level was slowly decreasing over the past two months, and thought it might be due to clogged filters. I swapped both filters out from the diode chiller but the flow was less than it was before. I increased the flow as high as I could, to 22 lpm, but it has continued to decrease, although it looks like it is slowly settling down.

I included a 60 day trend of the flow rate, which shows that something happened at the end of December which decreased the flow and hasn't stopped. I don't believe it is due to anything we have done, as this occured over holiday.

Images attached to this comment
LHO General
patrick.thomas@LIGO.ORG - posted 19:48, Monday 28 January 2013 (5296)
plots of dust counts
Attached are plots of dust counts > .3 microns and > .5 microns in particles per cubic foot requested from 5 PM Jan. 27 to 5 PM Jan. 28. Also attached are plots of the modes to show when they were running/acquiring data. Dust monitor 10 in the H1 PSL enclosure is still indicating a calibration failure.

The data was taken from h1nds0.
1260 seconds worth of data was unavailable on this server
1440.0 minutes of trend displayed
Non-image files attached to this report
H1 SEI
vincent.lhuillier@LIGO.ORG - posted 18:03, Monday 28 January 2013 (5295)
TF - BS - T240s (corners 2-3) not working right

Transfer functions were measured during the week-end. Stage 1 and stage 2 look good (cf TF_L4C & TF_GS13). On the other hand, the TFs from stage 1 actuators to T240s in corner 2 and corner 3 don't look right (gain and resonance). These 2 instruments don't seem to work properly.

Images attached to this report
H1 IOO
keita.kawabe@LIGO.ORG - posted 17:23, Monday 28 January 2013 (5294)
IMC MC2 M2-M3 cross-over, rehash

Matt, Keita

As noted in entry 5279 we had some trouble with changing MC2 acuation after the MC2 model change/restart.  It is not clear if the state before the change was the "right" one, and no explanation for the change was found (all MC2 coil driver bits were flipped, with no apparent change).  This should be looked at again with a model of the system in hand so that the measurements can be compared with expectations.  Since the "new" MC2_M2 TFs make the L1 filters stable, I am inclined to guess that we have returned to the "right" state.

In this state I changed the M2 stability filter to be very simple (zero at 2Hz, pole at 8Hz).  This gives the M2 cross-over resonable phase margin for all UGFs below 10Hz.  The attached images show the MC2 TFs with the M2 gain set to zero (no M2 actuation), M2 gain set to 0.03 (generally enough, and good for locking), and M2 gain of 0.1 (good for ISI work or high seismic times).  The maximum "good" value of the M2 gain is about 0.2, more than 0.3 is unstable.

Note that in the TFs involving MC2_M3, this system is working with heirachical control, so the measurement includes M3 and M2 (e.g., the whole MC2 actuation, or combine MC2 M2 and M3 actuator).  These TFs show that the M3 gain has about 8dB of gain margin, so gains more than about -2000 are likely to cause problems (-1000 is the nominal value).

Images attached to this report
H1 SUS
arnaud.pele@LIGO.ORG - posted 17:20, Monday 28 January 2013 (5293)
Modification of plot****_dtttfs.m
Mark suggested to modify the "plot****_dtttfs.m" scripts for QUAD HLTS HSTS HAUX and BSFM. 
From now, it will automatically create a Results folder in the right path (if it is not already existing) to save the pdf figures.

For example .../SusSVN/sus/trunk/HAUX/Common/MatlabTools/plotHAUX_dtttfs.m 
line 108 to 113 :

DIR=exist(resultsDir,'dir');
if DIR==7
else
    system(['mkdir -p ' resultsDir])
end
H1 SEI
hugh.radkins@LIGO.ORG - posted 16:33, Monday 28 January 2013 (5292)
WBSC1 HEPI Actuators 5/8 Attached
We (Randy & I) got the 4 Vertical Actuators attached along with the SE Horizontal.  Hopefully we'll wrap this up mid-day tomorrow.
LHO VE
kyle.ryan@LIGO.ORG - posted 16:26, Monday 28 January 2013 (5291)
Closed GV18, started purge air skid and rotating pumps at Y-end
Ready to vent Y-end

LHO VE
kyle.ryan@LIGO.ORG - posted 16:25, Monday 28 January 2013 (5290)
Finished roughing X-end -> Switched over to Turbo (MTP)


			
			
H1 General
justin.bergman@LIGO.ORG - posted 15:47, Monday 28 January 2013 (5287)
Ops Summary
LVEA laser safe all day

1030 Dave B restarting  PEMs and DAQ
1030 Cheryl and Kiwamu working in HI PSL enclosure
1040 Kyle to Y-end to prep for venting
1100 Corey G to LVEA then Y-end looking for "stuff and things"
1200-1245 Cheryl doing viewport work on HAM2, PSL shutter closed (see other aLog entry)
1240 RDO tractor onsite dropping repaired John Deere
1415 Jim B working in H1 EE room
1500 GV18 closed


Ongoing:
-No horseplay around Doug Cook's transit parked near termination slab of YBM. Marked with caution tape.
-ITMY watchdogs tripped all day. Optic seeing motion as a result of SEI actuator work on adjacent chambers.
X1 SUS
jeffrey.bartlett@LIGO.ORG - posted 15:44, Monday 28 January 2013 (5289)
Phase 1b Testing of I1-SR3
   We have completed taking Phase 1b transfer functions and spectra testing data for the India HLTS SR3. The results data looks positive. The data files are posted below. We will wait for the review of the results by Jeff K and Stuart A before doing anything more to I1-SR3.   
Non-image files attached to this report
H1 IOO
cheryl.vorvick@LIGO.ORG - posted 13:35, Monday 28 January 2013 - last comment - 15:38, Monday 28 January 2013(5286)
HAM2 IFO REFL Beam baffle now has a camera view in the Control Room - alignment of REFL has begun:
- Cheryl, Kiwamu, Slim and Mark (Apollo)

A camera was installed on the REFL beam viewport where the REFL beam will exit the vacuum system through a baffle and viewport.  The camera view is available in the Control Room, and the IOT2L IMC REFL beam camera view was replaced by the IFO REFL camera view.  The hope is that the IFO REFL beam view will allow us to align the REFL beam through the baffle.  I got the beam to clip on the edge of the baffle aperture, and currently Kiwamu is working to improve this alignment.
Comments related to this report
kiwamu.izumi@LIGO.ORG - 15:38, Monday 28 January 2013 (5288)

I was trying to establish nicer alignment such that we can see a bright beam spot on the camera view, but no luck this time. I tweaked only IM3 and IM4 for aligning the beam. Right now the settings of IM3 and IM4 are back to how they used to be when I started (at around 14:00).

LHO VE
kyle.ryan@LIGO.ORG - posted 11:35, Monday 28 January 2013 (5281)
HAM4-BSC2 septum annulus passes leak test
Unassisted nominal ion pump current on-scale for the past three days -> OK
H1 CDS
david.barker@LIGO.ORG - posted 10:47, Monday 28 January 2013 (5280)
New PEM models installed, DAQ restarted

I have installed the latest PEM models into h1pemey, h1peml0 and h1pemmx. There were some naming errors and the MAG BLRMS channels which were mistakenly added have been removed. The DAQ was then restarted.

H1 SEI
hugo.paris@LIGO.ORG - posted 10:44, Monday 28 January 2013 - last comment - 12:45, Monday 28 January 2013(5268)
HEPI commissioning work - HAM2 HAM3

The DAC and ADC numbers for the simulink models of HAM2-HEPI and HAM3-HEPI  were adjusted. Models are re-compiled and commited to the SVN.

The ground STS that will help evaluating SEI controls performance on the IMC was wired in these models (STS A). Its readouts initially looked like the sensor was railed. We re-cetered the sensor's test mass by pushing the centering button of its interface. Readouts make more sense now. 

We measured a spectrum of the ground motion with this STS and compared it with the same measurement performed with the STS that is set on the ground at EY. Spectra have similar shape but different amplitude which make sense since the perturbation level is higher in the LVEA during work day (Friday, early afternoon), than it is at EY.

Folder arborscence was adjusted for HAM2-HEPI commissioning. HAM2-HEPI comissioning scripts were created from ETMY templates and added to these folder. Input filters and coordinate transform matrices are loaded. Same operations will be performed for HAM3-HEPI. 

Images attached to this report
Non-image files attached to this report
Comments related to this report
vincent.lhuillier@LIGO.ORG - 11:37, Monday 28 January 2013 (5282)

Why recentering the STS? It was centered already. Railing during the day is normal.

vincent.lhuillier@LIGO.ORG - 11:37, Monday 28 January 2013 (5283)

Why recentering the STS? It was centered already. Railing during the day is normal.

hugo.paris@LIGO.ORG - 12:15, Monday 28 January 2013 (5284)

This ground STS is not railing now and has not been re-centered since last week. So, I would not say railing is the normal state of this sensor, even during the day.

This sensor does not rail at LLO.

vincent.lhuillier@LIGO.ORG - 12:45, Monday 28 January 2013 (5285)

Trends of the last 10 days. Last week was a 4-day week.

Images attached to this comment
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