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Reports until 17:39, Friday 31 August 2012
H2 ISC
daniel.sigg@LIGO.ORG - posted 17:39, Friday 31 August 2012 (4061)
picomotor interference
Using the picomotors interferes with cavity locking and seems to introduce glitches which are clearly visible in the cavity power (see circled regions in the attachment).
Images attached to this report
H1 IOO
giacomo.ciani@LIGO.ORG - posted 17:16, Friday 31 August 2012 (4034)
HAUX: proper testing started

[Alex, Cheryl, Deepak, Giacomo]

Yesterday morning we couldn't work to the suspensions due to drilling going on in the LVEA. We used the morning to debug the binary IO: now it is working properly and both the LP status and the Coil Output can be enabled and disabled from the front-end as expected.

In the afternoon we carried a large HxTS barrel from the staging building, changed the disposition of HAUX and cover all of them with the barrel, to ease the effect of air turbulence when taking transfer functions and PSDs. The suspensions were left covered and undamped (and no ECD)for the night. Note that we found the position of many of the OSEMs to be offset by couple hundreds um (or more), while they were initially set to be centered better (sometimes much better) than 100 um. Later investigation (this afternoon) suggested that this was due to a combination of:

- the table not being completely leveled (or flat), so that when you move the suspensions around the position of the optics slightly changes

- the frames being unevenly clamped (we only used 3 clamps yesterday as we didn't know where to find others...)

- the OSEM being not very well tightened, so some of them may have moved during handling of the cables and the suspensions to fit them under the barrel.

We also found that leaving the uninstalled ECD close to the base (instead of putting them further away) did not noticeably affect the position of the optic, as initially suspected (however, installing the ECD does change the pitch, as observed before).

 

Today we adjusted the pitch of all suspensions to 0+-0.5 mrad (assuming the table levelled to this precision, that we were unable to check) using an optical lever (actually IM4 should be adjusted to +4.1 mrad, but since all the suspensions will need to be balanced again once we put he ECD in, we didn't bother).

We centered the OSEMs (intial centering was well within +- 50 um, but after moving them around it degraded to a little better than +-80), cleaned the setup a bit, clamped the suspensions with 4 clamps each and left them under the barrel.

I took TF of Y, P and L (attached), applying small actuation offsets to make the OSEM work around the central position. The transfer functions show no sign of problems, although the peaks are not exactly all in the same place (as already observed at LLO and expected, as the HAUX design does not include any mechanism to fine tune the resonances' position).

At about 22:05 I left the suspensions quiet and with damping off for the night, so tomorrow we can retrieve data for PSDs.

Images attached to this report
H2 TCS
thomas.vo@LIGO.ORG - posted 17:07, Friday 31 August 2012 (4060)
H2 ETMY/ITMY RH Measurements
Thomas V

I measured the output voltage out of the RH drivers for both ITMY and ETMY for different values of input currents (ranging from 0 to 1 amp).  Attached is a spreadsheet of my measurements. Analysis soon to come, along with calibration parameters.
Non-image files attached to this report
LHO General
jeffrey.garcia@LIGO.ORG - posted 16:02, Friday 31 August 2012 (4059)
Ops Log
Eric A. - feedthrough protection install on HAM chambers
Thomas V. at End-Y
Keita at End-Y
man-lift work in LVEA.  completed by 10:30am
Bubba running crane in LVEA ~2:00pm
QUAD L2-stage coil output filter modifications in the morning hours before noon.
H2 SUS
jeffrey.garcia@LIGO.ORG - posted 16:00, Friday 31 August 2012 (4057)
H2 SUS QUAD L2 coiloutf changes
Updates to the QUAD L2 coiloutf filter modules were installed today on both ITMy and ETMy.  The previous filter files were modified via foton and saved to the usual directory.  The files were committed to the "cds_user_apps" SVN locally under:

'/opt/rtcds/userapps/release/sus/h2/filterfiles/H2SUS*TMY.txt'.

The following is the excerpt from the "H2SUSITMY.txt" file where the L2_COILOUTF_* filters are coded.  The changes were to the FMs 5,6, & 7 for all four coils on ITMY and ETMY.  The filter coefficients for both user models were loaded via the GDS medm for each suspension.  The attached pdf is a transfer function of the filter modules with the original and updated pole/zero pairs.

OLD:  
# DESIGN   ITMY_L2_COILOUTF_LL 5 zpk([13],[129.973],1,"n")
# DESIGN   ITMY_L2_COILOUTF_LL 6 zpk([1],[99.9877],1,"n")
# DESIGN   ITMY_L2_COILOUTF_LL 7 zpk([0.5;249.809],[5;19.9999],1,"n")


NEW:
# DESIGN   ETMY_L2_COILOUTF_LL 5 zpk([12],[110],1,"n")
# DESIGN   ETMY_L2_COILOUTF_LL 6 zpk([1.35],[80.5],1,"n")
# DESIGN   ETMY_L2_COILOUTF_LL 7 zpk([0.5;250],[6;20],1,"n")


-------------------------------------------------------------------------------------------------------
################################################################################
### ITMY_L2_COILOUTF_LL                                                      ###
################################################################################
# DESIGN   ITMY_L2_COILOUTF_LL 0 zpk([129.973],[13],1,"n")
# DESIGN   ITMY_L2_COILOUTF_LL 1 zpk([99.9877],[1],1,"n")
# DESIGN   ITMY_L2_COILOUTF_LL 2 zpk([5;19.9999],[0.5;249.809],1,"n")
# DESIGN   ITMY_L2_COILOUTF_LL 5 zpk([12],[110],1,"n")
# DESIGN   ITMY_L2_COILOUTF_LL 6 zpk([1.35],[80.5],1,"n")
# DESIGN   ITMY_L2_COILOUTF_LL 7 zpk([0.5;250],[6;20],1,"n")
###                                                                          ###
ITMY_L2_COILOUTF_LL 0 21 1      0      0 SimAcqOffL2        0.1022381444281  -0.9950269485578308   0.0000000000000000  -0.9513581602053965   0.0000000000000000
ITMY_L2_COILOUTF_LL 1 21 1      0      0 SimAcqOnL2    0.01018979855460631  -0.9996165783185160   0.0000000000000000  -0.9623720057438665   0.0000000000000000
ITMY_L2_COILOUTF_LL 2 21 1      0      0 SimLPL2         1.198428225279573  -1.9083200482101859   0.9083375891754886  -1.9904437581736589   0.9904583948159983
ITMY_L2_COILOUTF_LL 5 21 1      0      0 AntiAcqOffL2      8.999262730598492  -0.9586809127066087   0.0000000000000000  -0.9954086141798147   0.0000000000000000
ITMY_L2_COILOUTF_LL 6 21 1      0      0 AntiAcqOnL2      58.74299131244113  -0.9695955355155262   0.0000000000000000  -0.9994824154540793   0.0000000000000000
ITMY_L2_COILOUTF_LL 7 21 1      0      0 AntiLPL2        1.000393883340034  -1.9900610320883918   0.9900785927850526  -1.9082531975983987   0.9082707513809170
Non-image files attached to this report
X1 SEI
hugo.paris@LIGO.ORG - posted 14:52, Friday 31 August 2012 (4058)
eLIGO HAM6-ISI - GS13s received and huddle Tested

Greg, Jim, Hugo,

We huddle tested the GS13s intended to retro-fit eLIGO HAM6-ISI. Test results are attached.

Non-image files attached to this report
X1 SEI
corey.gray@LIGO.ORG - posted 11:22, Friday 31 August 2012 (4052)
Final LHO-Built HAM Boxed Up

(corey, greg, jim, justin, mitchell)

This morning we boxed up HAMISI#7 (destined for HAM#4).  This took about 2-2.5hrs.

H1 AOS
thomas.vo@LIGO.ORG - posted 09:54, Friday 31 August 2012 (4051)
H1 Optical Levers Drilling
Eric J, Thomas V, Apollo


The holes to set pylons and giraffes are drilled on the input side of H1, this includes the HAM2 and HAM3 optical lever transceivers as well as the PR3 transmitter and receiver(giraffe).  We also set the dwarf pylons down on the anchor bolts and are currently looking to have viewports placed in before installing more delicate components.

The H1 output side is being laid out and drilled today as well.

H1 SEI
corey.gray@LIGO.ORG - posted 09:00, Friday 31 August 2012 (4049)
Another Early Morning Quake Trips A Few SEI Watchdogs

Mag 7.6 earthquake (or an aftershock) in the Phillipines tripped the BSC8 HEPI & ISI and BSC6 HEPI.

H1 SEI
greg.grabeel@LIGO.ORG - posted 08:42, Friday 31 August 2012 (4048)
Unit 3 HAM purge
Unit 3 HAM had its cabling and pods removed on the 28th and was resealed in a storage container. A purge was started shortly thereafter. Interestingly the time it took to drop below -25 td°C was very similar to Unit 6 which had cabling and viton. 
Images attached to this report
LHO General
patrick.thomas@LIGO.ORG - posted 18:41, Thursday 30 August 2012 (4046)
plots of dust counts
Attached are plots of dust counts > .5 microns in particles per cubic foot.
Non-image files attached to this report
LHO VE
kyle.ryan@LIGO.ORG - posted 17:01, Thursday 30 August 2012 (4045)
West Crane out-of-service -> postponing BSC1 16.5" feedthrough flange work


			
			
H2 ISC
alberto.stochino@LIGO.ORG - posted 16:42, Thursday 30 August 2012 (4044)
WFS sensing matrix still not good

With the arm cavity locked I tried to measure again the WFS sensing matrix. It still looks almost degenerate in both PIT and YAW.

These are the measurements:

sensP =
   1.0e-03 *
   -0.2374    0.2929
   -0.1506    0.1611
sensY =
   1.0e-03 *
    0.0133   -0.1897
    0.0177   -0.2023

And these are inverted matrices:

iP =
   1.0e+04 *
    2.7373   -4.9782
    2.5596   -4.0341
iY =
   1.0e+05 *
   -2.9772    2.7915
   -0.2610    0.1953

The measuremetns are at about 4 Hz.

They look quite bad. I won't even try to impelment them.

H2 ISC
alberto.stochino@LIGO.ORG - posted 16:38, Thursday 30 August 2012 (4043)
Arm cavity stably locked

The arm cavity is stably locked since 23:15 UTC.

There is only damping enabled on the ISI. We turned the isolation off because it was causing the oscilaltions at few tens of mHz on the reflected power.

H1 PSL
michael.rodruck@LIGO.ORG - posted 16:15, Thursday 30 August 2012 (4040)
PMC mode matching

This is a summary of fine tuning the mode matching into the PMC for the 35W laser. The attached spreadsheet lists the power of each mode looking at ISS_PDA_DC hooked into an oscilloscope. The position of the lenses L2 and L3 is measured from the lens's block's edge facing HAM1. After moving a lens the alignment peak was minimized to below 10mV and was not included in this spreadsheet. Mode power is measured in mV and going to the 'right' of the 00 mode. The strongest peak is the last one (first to the 'left') and looks similar to a 11 Laguerre-gaussian mode. I believe the second mode listed is the 02 mode, however most are too faint to see clearly.

The best position appears to be

L2: 368mm

L3: 738mm

Note that this is very different for the 200W laser. For the 200W laser, the lenses are at:

L2: 310mm

L3: 728mm

I do not have other numbers for the 200W laser.

Images attached to this report
Non-image files attached to this report
LHO General
corey.gray@LIGO.ORG - posted 16:14, Thursday 30 August 2012 (4032)
Morning OPS Summary

One-Arm Test yielded morning to "noisy" activities; goal was to have some cavity locking & Wavefront Sensor work later.

Apollo drilling for oplev piers in morning (and a little in the afternoon)

Giacamo/Cheryl:  SUS AUX assembly work in LVEA (after lunch)

Hugh going to check BSC6 to look at HEPI (morning)

Alex going to EY optics lab to inventory TMS (morning)

Bubba squaring up main crane by hitting bumpers, but this activity ended up tripping/deactivating the crane.  Will be investigated in the morning (manlift required)

Scotty doing some quick drilling (1:50-2:10)

Eric doing feedthru protection work (avoiding HAM3 due to OAT)

Keita at EY lab (left at 3:30)

H2 CDS
david.barker@LIGO.ORG - posted 17:42, Tuesday 28 August 2012 - last comment - 12:40, Friday 31 August 2012(4019)
H2 maintenance day

About 50% of the H2 front ends were upgraded to RCG 2.5.1 last week, this week I cleanly rebuilt and restarted all H2 frontends against 2.5.1 in conjuction with the timing change.

All of H2's timing signals were moved from the old h2 timing master to the new h1 timing master. The old h2 timing master is being decommissioned.

errors in the burt restore of the safe.snap files were seen on h2peml0, h2tcsitmy and h2pemey (my problem, I'll fix these).

Problems with a large ADC input on h2hpietmy is being tracked to a HEPI pump issue at EY.

The 24MHz RF amplifier at EY is showing a timing problem on the fanout, and its fpga led is blinking red sometimes.

Comments related to this report
daniel.sigg@LIGO.ORG - 12:40, Friday 31 August 2012 (4056)
Fixed timing synchronization of the EY RF source by power cycling the unit.
H2 SUS
keita.kawabe@LIGO.ORG - posted 13:25, Tuesday 28 August 2012 - last comment - 12:00, Friday 31 August 2012(4007)
ETMY POS to cavity length and oplev measurements from yesterday

We measured the transfer functions to the cavity length from M0 POS, L1 POS and L2 POS, when the cavity was locked and only M0 was damped.

At the same time we also measured the transfer functions from the same actuation points to the OPLEV signals.

Two main goals of this were:

1. To see if L2 stage (penultimate mass) drive was working fine. There has been speculations but no definitive answer.

2. To provide a set of measured data for SUS so hierarchical control effort could be accelerated.

 

Anyway, if you're only interested in the plots see attached. Frequency points are kind of sparse and not even (the former is constrained by time, the latter is by the fact that I'm throwing away low coherence data).

Plots as well as data files etc. are all under /ligo/home/controls/keita.kawabe/OAT_2012/ETM_M0_L1_and_L2_POS_to_L3

Everything was checked into svn: /ligo/svncommon/SusSVN/sus/trunk/QUAD/H2/ETMY/Common/Data/2012-08-27_H2SUSETMY_M0_L1_L2_POS_to_L3

[Update 13:30-ish 28/Aug/2012]

The plots are now normalized by the L2L element of the drivealign matrix, as that was 1 for M0 and L2 (as it should be) but 10 for L1 for whatever reason.

Non-image files attached to this report
Comments related to this report
keita.kawabe@LIGO.ORG - 13:30, Tuesday 28 August 2012 (4009)

Two things that are obvious from the plots:

(Updated 13:30-ish Pacific, 28/Aug/2012) 1. L2 drive is working. It is about a factor of 120 or so weaker than L1, and L1 is about a factor of 6 weaker than M0 (see page 1).

1. L2 drive is working. It is about a factor of 12 or so weaker than L1, and L1 is about a factor of 60 weaker than M0 (see page 1).

2. Cavity length to angle coupling could be problematic at resonances (see page 4). At DC for M0, it seems to be 0.1rad/m in a ball park, and and even if we feed back 1um RMS this is 0.1urad RMS, which sounds OK.

keita.kawabe@LIGO.ORG - 10:59, Tuesday 28 August 2012 (4010)

One thing that is not obvious from the plot:

For L2 drive, I had to use a ridiculously large excitation (+-120000 counts, half about a quarter of the range of 18bit DAC considering the output matrix of 0.25) with ridiculously long integration time (e.g. 160 seconds) to get a good coherence for f>1Hz. The background noise is too large.

This practically means that, as others pointed out, L2 is going to be railing if the ALS signal is fed back to L2 with a UGF of 1 Hz.

0.1Hz might be possible, but 1Hz, not likely.

keita.kawabe@LIGO.ORG - 13:32, Tuesday 28 August 2012 (4012)

Other things:

When the measurement was done, L2 stage driver FM2/3/5/6/7 were on while FM1 was off.

EUL2OSEM output matrix elements for M0 (for two lower face coils F2 and F3) were (0.5, 0.5).

EUL2OSEM output matrix elements for L1 and L2 (for all four coils) were both 0.25*(1, 1, 1, 1).

keita.kawabe@LIGO.ORG - 06:57, Friday 31 August 2012 (4047)

Update Aug/31/2012

In the above entry,

"When the measurement was done, L2 stage driver FM2/3/5/6/7 were on while FM1 was off."

this was  incorrect but I cannot edit it any more, it seems. It should read

 

" L2 stage driver FM2/3/6/7/8 were on while FM1 was off." 

jeffrey.kissel@LIGO.ORG - 12:00, Friday 31 August 2012 (4053)
J. Kissel, B. Shapiro

I attached plots comparing Keita's transfer functions to what I expect from the model. Executive summary: 5 of the 9 transfer functions measured match my model exquisitely -- All L to L TFs, and the TOP to TST, and PUM to TST L to P TFs. Of the remaining TFs: I don't expect the model to predict the L to Y coupling well at all, but I'm still baffled as to why the UIM to TST L to P transfer function doesn't match up. 

Comments / questions / concerns welcome. I really haven't yet been able to get a warm and fuzzy feeling about a lot of this data. So, take it with a grain of salt.

You'll notice that among the series of plots is the predicted maximum range for each stage. Please don't read too much into these numbers, I haven't yet verified them against Norna's numbers (see T1100595), taking into to account the differences between her numbers and mine (mostly the maximum range of the coil driver, updated to use the real, recently measured, transconductance of the coil drivers times the 10 [V] DAC range.) BUT I know that frequency response is accurate, because it uses the latest and greatest measured responses. 

Notes / Details:
- There are fudge factors that I don't yet understand. They're explicitly called out in the legend, but they're summarized here:

                  %L  P  Y
driveAlignGain = [-1 -1 -1;... % M0
                  -5 -5 -5;... % L1
                   1  1  1];   % L2
meas(iStage,iDOF).tf = meas(iStage,iDOF).tf / driveAlignGain(iStage,iDOF);
 
As Keita mentions, I expect the L1/UIM fudge factor to be 10 not 5, from the driveAlign gain. 
I'm NOT really that surprised that we got the sign wrong on M0 and L1, but I don't know yet where it lies.

- The modeled M0-only damping loops are not *exactly* representative of what Matt tuned a month or 3 ago, but they should be close enough. I expect the overall gain to be different, and I expect the low frequency bump filters to be different, but otherwise they should match pretty well.
Non-image files attached to this comment
H2 ISC
matthew.evans@LIGO.ORG - posted 00:16, Thursday 19 July 2012 - last comment - 15:17, Thursday 30 August 2012(3490)
OAT - first dither alignment

It is a long way from being robust, and it is quite slow, but the cavity dither alignment worked this evening.  The commands are:

YAW
./tdsdither 1.9 30 4 0 300 H2:SUS-ITMY_M0_TEST_Y_EXC H2:ISC-ALS_EY_REFL_PWR_MON_OUT H2:SUS-ITMY_M0_OFFSET_Y 10 5
./tdsdither 2.3 50 5 0 300 H2:SUS-ETMY_M0_TEST_Y_EXC H2:ISC-ALS_EY_REFL_PWR_MON_OUT H2:SUS-ETMY_M0_OFFSET_Y 10 5

PIT
./tdsdither 1.9 30 4 90 300 H2:SUS-ITMY_M0_TEST_P_EXC H2:ISC-ALS_EY_REFL_PWR_MON_OUT H2:SUS-ITMY_M0_OFFSET_P 10 5
./tdsdither 2.3 50 5 30 300 H2:SUS-ETMY_M0_TEST_P_EXC H2:ISC-ALS_EY_REFL_PWR_MON_OUT H2:SUS-ETMY_M0_OFFSET_P -10 5
 

The new tdsdither is a perl script replacement for the malfunctioning ezcademod which currently lives in userapps/trunk/isc/common/scripts.  The attached image shows the power increase as the ITM and ETM alignment are dithered.

Images attached to this report
Comments related to this report
alberto.stochino@LIGO.ORG - 15:17, Thursday 30 August 2012 (4042)

With the new channels names the commands are:

PIT

./tdsdither 1.9 30 4 90 300 H2:SUS-ITMY_M0_TEST_P_EXC H2:ALS-Y_REFL_B_PWR_OUT H2:SUS-ITMY_M0_OFFSET_P 10 5

./tdsdither 1.9 30 4 90 300 H2:SUS-ETMY_M0_TEST_P_EXC H2:ALS-Y_REFL_B_PWR_OUT H2:SUS-ETMY_M0_OFFSET_P -10 5

 

YAW

./tdsdither 1.9 30 4 90 300 H2:SUS-ITMY_M0_TEST_Y_EXC H2:ALS-Y_REFL_B_PWR_OUT H2:SUS-ITMY_M0_OFFSET_Y 10 5
./tdsdither 1.9 30 4 90 300 H2:SUS-ETMY_M0_TEST_Y_EXC H2:ALS-Y_REFL_B_PWR_OUT H2:SUS-ETMY_M0_OFFSET_Y 10 5

Displaying reports 82381-82400 of 86325.Go to page Start 4116 4117 4118 4119 4120 4121 4122 4123 4124 End