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Reports until 15:47, Monday 28 January 2013
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
H1 IOO
giacomo.ciani@LIGO.ORG - posted 20:09, Friday 25 January 2013 (5279)
IMC status

Yesteday, after the MC2 model was replaced, recompiled and burt restored to the settings of the preceeding night, we noticed a change of behaviour of the locking loop. It would no more lock easily with the usual settings, and with the higher gain settings it would trigger an oscillation at 21 Hz that we didn;t observe before. Today Matt worked at re-measuring the cross-over frequencies and re-tuning the filters and we'll write an entry about the changes he made and the new suggested operating settings.

 

In the meanwhile, I'm leaving the IMC locked for the weekend with mild gains, so to increase the chances of a spontaneous re-lock should an un-lock occour:

- common mode board: common gain at -5 db, compensation enabled, boost disabled, fast gain to -2 (as always)

- MC2: MC3_LOCK filters 5 and 8 engaged, gain to -1000; MC2_LOCK filters 2, 3 and 4 engaged, gain 0.03.

H1 IOO
giacomo.ciani@LIGO.ORG - posted 19:59, Friday 25 January 2013 (5278)
IMC commissioning miscellanea

[Cheryl, Giacomo]

A couple of IMC activities were started today and not completed:

 

- the setup for the measurement of the cavity pole was prepared: using an SR785 signal analyzer, a  swept sine is injected in the "inner loop transfer function input" on the PSL ISS front end on the field rack. The output of one of the ISS PD (A or B, we used the one that is not used int he loop in loop) is taken from the same field rack and sent to one of the channels. A Thorlabs PDA100A photodiode sits on the IOT1 table and is connected to the other channel fo the signal analyzer using one the the (unfortunately currently available) WFS RF cable. The PDA100A is put in the REFL path with the IMC both unlocked and misaligned to measure the relative TF of the two PD. Then it is moved to the TRANS path, the IMC locked, and the measurement repeated. The ratio of the two TF should give the IMC transfer fucntion. A quick measure was taken late this evening, but it still needs to be analyzied (and checked for errors).

 

- with the goal of computing a power budget, we checked if all the beams were coming out pretty much in the expected positions:

  - the forawrd and backward beams were coming out from their (common) viewport pretty much in the expected positions (they pretty much covnerge at maybe 20 inches from the viewport).

  - the parking beam was not visible, and it seemed to be clipping on the baffle right in front of IM4.

  - IM3 and IM4 also showed to have drifted during pumpdown in pitch and yaw, much more thean IM1 and IM2. Note that bringing them back to the "in-air" positions (as read by the OSEMs) did not make the parking beam reach its target, and apparently spoiled the position of the IM4 forward and backward transmitted beams (they were still coming out of the viewport, but convergin much farther away)

We played with the IM suspensions to try to reroute the parking beam to its intended location, but we started late due to other activities going on and we only got to the point in which the beam is badly clipped by the parking baffle (but at least is visible!). We are not far, but not quiete there yet. We'll resume next week.

H1 ISC
lisa.barsotti@LIGO.ORG - posted 17:12, Friday 25 January 2013 (5277)
RF signal chain of the IMC LSC RFPD checked
Matt, Lisa

With the fixed laser calibrator head we could finally make a measurement of the RF signal chain of the IMC LSC RFPD (24.078 MHz, S/N: S1203396).

- Laser Head: 4 mW @ 980 nm;
- Laser Head RF input calibration: 13e-3 W/V;
- LSC RFPD DC Transimpedance = 200 Ohm;
- LSC RFPD RF Transimpedance = 476 Ohm;

 Calibration using the DC response 

* Measured REFL_DC = 480 counts

=> Resp = 480/(1638 [counts/V] * 200 [V/A] * 4e-3 [W]) = 0.37 [A/W] 

 RF Signal chain 

- RF input modulation to the Laser Head Calibrator: 0.1 Vptp sine @ 24.078473 MHz;

=> Expected RF to the demod board = 476 [V/A] x 0.37 [A/W] x 13e-3 [W/V] x 0.1 [Vptp] = 230 mVptp

* Measured RF_in to the demod board: 240 mVptp

=> Expected I/Q monitor of the demod board = 10 (demod board gain) x 1/2 (mixer) x 240 [mV] = 1.2 Vptp  @ 100 Hz

* Measured I/Q monitors of the demod board: 1.3 Vptp
* Measured TEST1 input of the common board: 1.3 Vptp


The measured values are withing 10% of what we expected.



H1 SEI
hugh.radkins@LIGO.ORG - posted 16:25, Friday 25 January 2013 (5276)
BSC1-ITMY North Side Dial Indictors reset
Mostly important only to me.  Needed to move the DI mounting points on the North side to make room for the Pier Pod modules.  This just means that I needed to record the before and after numbers cause they are no longer the same.
H1 SEI
jim.warner@LIGO.ORG - posted 16:17, Friday 25 January 2013 (5275)
BSC2 CPS issues...resolved?
A few weeks ago, Vincent reported some of BSC2's St2 cps-es were "weird". With no changes to the system, some were reading ~ +/-15000 cts. Today, in preparation for fixing the system, Vincent and I checked the sensors again and they were back to normal. Grounding issues are suspected, and a better connection to ground was added this afternoon. Hopefully, the sensors are now fixed, but power spectra still show some noise in some of the sensors. Vincent will be taking TF's over the weekend, in preparation for the impending BS glass install.
H1 ISC
sheila.dwyer@LIGO.ORG - posted 15:52, Friday 25 January 2013 (5273)
IMC WFS whitening slow controls
The slow controls are working now for the IMC WFS whitening filters.  
LHO VE
kyle.ryan@LIGO.ORG - posted 15:52, Friday 25 January 2013 (5272)
Pumped X-end for a few hours -> will resume on Monday
Kyle 
Removed bellows tie-rods from spool connecting BSC9 to BSC5 -> Started pumping X-end -> Noticed that BSC5 gauge pair was missing and a that the filter connection installed for the X-mid to X-end move of BSC5 was still connected to the gauge pair port -> Stopped pumping X-end -> Vented X-end -> Removed filter connection and installed conflat blank -> Restarted pumping of X-end 

1530 hrs. local -> Valved-out pump from X-end -> will resume pumping on Monday (Rough pumping must be attended)
LHO VE
kyle.ryan@LIGO.ORG - posted 15:45, Friday 25 January 2013 (5271)
HAM6 bellows leak testing -> Retested NE bellows -> OK
Observed a delayed signal response initially this morning when retesting the NE bellows -> Pumped annulus volume and applied instrument air to external leak test ports closest to NE bellows -> Retested -> OK  

HAM6 bellows pass leak testing.
H1 SUS
arnaud.pele@LIGO.ORG - posted 13:21, Friday 25 January 2013 - last comment - 15:57, Friday 25 January 2013(5265)
ITMY Transfer functions
Arnaud P and Mark B.

Starting a round of tfs after the alignement of suspensions
Comments related to this report
arnaud.pele@LIGO.ORG - 15:57, Friday 25 January 2013 (5274)
Done with the measurements that can be found here : 

/ligo/svncommon/SusSVN/sus/trunk/QUAD/H1/ITMY/SAGM0/Data/2013-01-25_1300_H1SUSITMY_M0_*_WhiteNoise.xml
/ligo/svncommon/SusSVN/sus/trunk/QUAD/H1/ITMY/SAGM0/Data/2013-01-25_1300_H1SUSITMY_R0_*_WhiteNoise.xml

Everything looks great except T dof that is a bit noisy between 2Hz and 3Hz as yesterday

Non-image files attached to this comment
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