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Reports until 17:01, Wednesday 05 March 2014
H1 SEI
hugh.radkins@LIGO.ORG - posted 17:01, Wednesday 05 March 2014 (10567)
WHAM4 SEI HEPI Progress/Status

One more pair of WHAM4 HEPI Actuators attached--NE(corner 4.)  Sure and steady's the word.

H1 ISC
jaclyn.sanders@LIGO.ORG - posted 16:32, Wednesday 05 March 2014 (10563)
BIO IP changes at EY

The BIO chassis that controls the ISC Whitening was shifted over from H2 without having its IP addresses shifted over, so it couldn't communicate with the rest of the slow controls system. Since we like being able to use the slow controls to control things, I changed the IP addresses from the H2 10.80.xx.xx convention to the H1 10.40.xx.xx convention. 

H1 AOS (SEI)
mitchell.robinson@LIGO.ORG - posted 16:27, Wednesday 05 March 2014 (10565)
Staging building, 3IFO BSC (unit 1) progress
Greg, Mitchell,
Greg and I were able to attach the lift hook receiver onto the first 3IFO BSC. This is in preparation to transplant the ISI into it's long term storage home. 
H1 SUS
jeffrey.bartlett@LIGO.ORG - posted 16:27, Wednesday 05 March 2014 (10564)
Install Glass in H1-SR3
Betsy & Jeff

   The glass optic was installed in H1-SR3. There were no problems or issues during the installation.
H1 INS (SEI)
jim.warner@LIGO.ORG - posted 16:19, Wednesday 05 March 2014 (10561)
ETMY ISI rebalanced, measurments starting tonight

It was realized yesterday that TMS still had some "head-banger" hardware left from the cartridge install. This was removed today, which necessitated a rebalancing of St2. While working on this, I also looked at a CPS that was acting like it was broken. I poked around the cable for the CPS and it fixed itself, so I'm hoping it was just a loose connection. I'll look at this again tomorrow, but at this point it looks like the in-air cable MAY be bad. For now, I will be running TF's tonight. from OPSWS5.

H1 SUS (ISC)
jeffrey.kissel@LIGO.ORG - posted 16:14, Wednesday 05 March 2014 - last comment - 16:34, Wednesday 05 March 2014(10552)
H1 SUS ETMX UIM/L1 Coils Balanced
J. Kissel

Following the same procedure outlined in LHO aLOGs 9453 and 9079, and similar to results from LHO aLOG 10493, with virtually the same demod parameters (only the amplitude was decreased from 1.25e5 to 1.2e5 [ct]) I balanced the coils on the UIM stage of H1 SUS ETMX. The final balanced gains in the L1_COILOUTF bank are
H1 SUS ETMX L1
Channel     Balanced COILOUTF Gain
 UL            -0.966
 LL            +1.004
 UR            +0.996
 LR            -1.034

The precision is still within +/- 0.5%; the ground motion while tuning the gains was not much better than yesterday, even though I tried several configurations of the ISI. See details of balanced vs. unbalanced signal SNR in comments below.

This balancing has reduced the L3 P and Y caused by a L1 pringle excitation at 4 [Hz] by
   DOF                  Reduction Factor @ 4.0 [Hz]
    P                          > 11.9      (peak below the noise, and totally incoherent)
    Y                          > 57.6      (peak below the noise, and totally incoherent)
The attachment shows the result from which these values were obtained, comparing the optical lever ASD at 4 [Hz] driven from L2 at the same amplitude for both balanced and unbalanced configurations.

Important note -- I found and was foiled by finding the L1_COILOUTF_UR gain sign set to
       Found   Expected
L1 UL    -        -
L1 LL    +        +
L1 UR    -        +
L1 LR    -        -
where expected comes from T1200015, and E1000617. Note these signs are exactly opposite from the PUM, because the UIM uses BOSEMs and the PUM uses AOSEMs, whose coils are wound in a different direction. Thus, the same magnet polarities are compensated by opposite signs.

I did a cursory check on the other three QUADs, and the same mistake is there too. This might just be a systematic, copy and paste error that we've propagated every where, and didn't notice until now because we haven't needed to use the UIM.
Non-image files attached to this report
Comments related to this report
jeffrey.kissel@LIGO.ORG - 16:34, Wednesday 05 March 2014 (10562)
Measurement Details
-------------------

Coil Driver Configuration:
State = 1
I was able to get plenty of SNR leaving the coil driver in the state I found it. 

Demodulator filters used:
SIG band pass: BP4.0Hz = butter("BandPass",2,3.5,4.0)
DEMOD I & Q low-pass: CLP50mHz = cheby1("LowPass",2,3,0.05)

Demodulator Drive Parameters
 Freq [Hz]     Amp [ct]     Sin [ct]    Cos [ct]
 4.0          120000         10000     10000
 4.0          120000         10000     10000

SEI Configuration:
HPI: Level 1 Isolation, "Pos" position sensor only blend filters
ST1: Level 2 Isolation, "TCrappy" blend filters (in all DOFs)
ST2: Level 2 Isolation, "TCrappy" blend filters (in all DOFs)
Note -- Sebastien had informed us that the Level 3 isolation filters and ST1-ST2 Sensor Correction are unstable for the time being, so I stuck with the above configuration.

Resulting Demod Phases:
Measured using a 200 second average (shorter than yesterday) of the demodulated signals, i.e.
tdsavg 200 H1:SUS-ETMX_LKIN_P_DEMOD_I_OUT H1:SUS-ETMX_LKIN_P_DEMOD_Q_OUT H1:SUS-ETMX_LKIN_Y_DEMOD_I_OUT H1:SUS-ETMX_LKIN_Y_DEMOD_Q_OUT
H1 ETMX L2
     Demod Phase [deg]          Unbalanced Value [ct]    Balanced Value [ct]
P       79            I         +1.933 pm ~0.75           -0.103 pm ~0.75
                      Q         -0.072 pm ~0.75           -0.060 pm ~0.75
Y       78            I         +5.181 pm ~0.75           -0.012 pm ~0.75
                      Q          0.148 pm ~0.75            0.078 pm ~0.75
note that the quote pm values are the by-eye, peak-to-peak amplitude of the demodulated signal which oscillates with a ~25 sec period. I qoute values to a much higher precision because I'm averaging over 200 seconds.

To perturb the PIT or YAW balancing by 1%:
/ligo/svncommon/SusSVN/sus/trunk/Common/PythonTools/perturbcoilbalance_fourosem.py H1 ETMX L2 [PIT/YAW] 0.01

Exact balanced values:
Measured using a simple command line caget, i.e.
caget H1:SUS-ETMX_L2_COILOUTF_UL_GAIN H1:SUS-ETMX_L2_COILOUTF_LL_GAIN H1:SUS-ETMX_L2_COILOUTF_UR_GAIN H1:SUS-ETMX_L2_COILOUTF_LR_GAIN
H1 ETMX L1
 Coil     COILOUTF Gain
UL         -0.965868
LL         +1.003680
UR         +0.995864
LR         -1.003386
Of course, these values are set at arbitrary precession, they're rounded to the values quoted in the main entry (a) because the measurement uncertainty is no better than 0.5%, and (b) the MEDM screen does not display out to higher precession, so further precision would not be visible.
H1 ISC
stefan.ballmer@LIGO.ORG - posted 16:11, Wednesday 05 March 2014 (10559)
PRMI locked with ballanced BS/PRM feed-back for MICH
Kiwamu, Yuta, Stefan

We finished installing the inverse plant filters for PRM and BS. Compared to yesterday, we lowered the Q of the <1Hz to 5. This effectively adds some boost at the main pendulum resonance, bud hardly affects the cancellation above 2Hz.

Locking with the new filters required some reshuffling of limiters and boost filters. See snapchot.

We then added PRM feed-back to the MICH loop, driving it at 99 Hz and cancelling its signature in REFL_45_I.
We rescaled the BS gain (divided it by 16) to make the MICH output matrix the correct one from theory (1,-0.5). 
An updated all-included-snapshot is attached.

New OLG measurements are also included.

Attached are a screen shot of all relevant MEDM screens, as well as PRCL and MICH OLG measurements.

The LSC Guardian was updated to reflect these changes.

Inverse plant filters:
BS:
zpk([0.0382738+i*1.57475;0.0382738-i*1.57475;0.0647002+i*1.13667;0.0647002-i*1.13667;
    0.0420175+i*0.418069;0.0420175-i*0.418069],[0.0163157+i*1.54679;0.0163157-i*1.54679],1,"n")
zpk([],[0.5+i*0.866025;0.5-i*0.866025],1,"n")zpk([],[1250+i*4841.23;1250-i*4841.23],1,"n")

PRM:
zpk([0.130304+i*2.84281;0.130304-i*2.84281;0.092145+i*1.61388;0.092145-i*1.61388;
    0.0683932+i*0.680504;0.0683932-i*0.680504;37.2961],
    [0.139329+i*2.35023;0.139329-i*2.35023;9.53503+i*13.2475;9.53503-i*13.2475;3.58083;
    0.5+i*0.866025;0.5-i*0.866025],1,"n")


MICH roll-off filter (to avoid BS saturation):
zpk([-0+i*120;-0-i*120],[25+i*43.3013;25-i*43.3013;50+i*86.6025;50-i*86.6025;400],1,"n")
Images attached to this report
LHO General
patrick.thomas@LIGO.ORG - posted 15:49, Wednesday 05 March 2014 (10557)
Jax to end Y to change IP address for modbus in Beckhoff chassis


			
			
H1 SEI
patrick.thomas@LIGO.ORG - posted 14:10, Wednesday 05 March 2014 - last comment - 16:59, Wednesday 05 March 2014(10556)
Hugh to HAM4 to work on HEPI


			
			
Comments related to this report
hugh.radkins@LIGO.ORG - 16:59, Wednesday 05 March 2014 (10566)

Exited LVEA 1630pst.

H1 SUS
patrick.thomas@LIGO.ORG - posted 13:30, Wednesday 05 March 2014 - last comment - 15:58, Wednesday 05 March 2014(10555)
Betsy to LVEA
Jeff and Betsy will swap the glass optic into the SR3 suspension when Jeff gets back from end Y.
Comments related to this report
patrick.thomas@LIGO.ORG - 15:50, Wednesday 05 March 2014 (10558)
Betsy out of LVEA.
patrick.thomas@LIGO.ORG - 15:58, Wednesday 05 March 2014 (10560)
Work is done.
H1 PEM
patrick.thomas@LIGO.ORG - posted 13:27, Wednesday 05 March 2014 (10553)
Jeff B. to end Y
Swapping cable on dust monitor.
LHO General
patrick.thomas@LIGO.ORG - posted 12:50, Wednesday 05 March 2014 (10548)
Karen to end Y


			
			
H1 General
patrick.thomas@LIGO.ORG - posted 11:16, Wednesday 05 March 2014 - last comment - 13:00, Wednesday 05 March 2014(10536)
Keita to end X lab for parts and then to end Y to help with TMS


			
			
Comments related to this report
patrick.thomas@LIGO.ORG - 12:04, Wednesday 05 March 2014 (10541)
Back from end X.
patrick.thomas@LIGO.ORG - 12:33, Wednesday 05 March 2014 (10545)
going to end Y.
patrick.thomas@LIGO.ORG - 13:00, Wednesday 05 March 2014 (10550)
Done
H1 ISC
sheila.dwyer@LIGO.ORG - posted 00:32, Wednesday 05 March 2014 - last comment - 12:56, Wednesday 05 March 2014(10514)
ETMX ISI

We had a lot of trouble early in the evening isolating ETMX, we kept tripping the watchdog on stage 2.  We tried reseting the CPS offsets, and eventually were able to get it to isolate with Tcrappy and level 2 controllers, but the motion was rather large (~ten fringes per second).  We left stage 2 with damping only. 

Comments related to this report
jeffrey.kissel@LIGO.ORG - 09:02, Wednesday 05 March 2014 (10518)SEI
Were you sending any particularly large locking transients to the ETM, to the top mass in particular? What did the input motion look like? Did it trip on actuators, or some sensor? 
sheila.dwyer@LIGO.ORG - 12:56, Wednesday 05 March 2014 (10549)

We haven't been using feedback to HEPI, and turned off the feedback to the top mass when we started having trouble.  there were acutator trips, GS13 trips, and T240 trips (I frogot to disable the T240 watchdog once).  

Also, at one point last night I turned on the sensor correction with the blend filters still on Start, this was obviously bad although nothing tripped.  Maybe this is only intended to be used with T240s, or only with Tcrappy blends. 

H1 ISC
sheila.dwyer@LIGO.ORG - posted 00:29, Wednesday 05 March 2014 - last comment - 13:38, Wednesday 05 March 2014(10511)
measurement of IR noise with COMM locked

Alexa, Daniel, Sheila

We normalized the refl PDH error signal, and saw that we can stay in the linear range of this signal with only ALS COMM locked. 

We first normalized LSC-X_TR_A_LF by adding a gain of 0.000154 so that the tranmission peak is at roughly 1.  We set LSC-REFLBIAS to  REFL_A_RF9_I over the transmitted power (LSC-X_TR_A_LF).  The first screen shot is the PDH, the transmitted power, and the normalized error signal as we move the COMM VCO set frequency.  In the red trace we moved the frequency by 2kHz; meanwhile, in the blue trace we moved half as fast over 1kHz.  We used Alexa's equation from alog 7054  to roughly calibrate the signal: 80Hz cavity pole/150 counts pp of the PDH signal=0.533Hz/count.

We put this gain into the REFL_BIAS filter, we will do a more carefull calculation in the morning. With this calibrated error signal we were able to measure an out of loop spectrum of the noise between the arm cavity and the PSL.  Attached are some of the spectra that we took. In the top panel the green trace is a reference with the cleanroom over HAM1 on, in the red trace we turned the cleanroom off and Alexa tried to tune up the arm cavity alignment by maximizing the green transmitted power.  This realingment clearly helped at low frequecies, and reduced the coherence with the ETMX PIT oplev. 

The RMS we measured is completely dominated by low frequency noise that changed, probably because the alignment was drifting.  The RMS down to 0.1 Hz varied from 30Hz-70Hz, we also measured an RMS of 58Hz down to 0.01 Hz.

We saw coherence with the end station PDH reflected signal above 1kHz,  coherence with the PIT oplevs (mostly ETMX, which currently has level 2 controlers on Stage 1 and damping only on stage 2) around the PIT resonances (0.4-0.5 Hz), and coherence with YAW OpLevs from 0.04-0.5 Hz.  We also looked for coherence with some of Robert's PEM sensors, we have coherence from the periscope on ISCT1 from about 50-100Hz, as we kind of expected.

Tonight the noise is much worse than it was on saturday, the transmitted power was not stable at all over time.  This might be because we don't have as good of an alignment, or be because the arm cavity motion is larger because of the problems with ETMX ISI.  We also measured the spectrum with higher and lower gains in the COMM board, higher gain did not seem to help, which is different from the situation on saturday alog 10439

Images attached to this report
Comments related to this report
peter.fritschel@LIGO.ORG - 06:44, Wednesday 05 March 2014 (10516)

Did you have the ALS WFS servos running for these measurements?

jeffrey.kissel@LIGO.ORG - 09:07, Wednesday 05 March 2014 (10520)
Note, this same measurement at LLO looks strikingly similar: see LLO aLOG 11265!
sheila.dwyer@LIGO.ORG - 13:15, Wednesday 05 March 2014 (10551)

No WFS, dither alignment, or longitudnal feedback to the test mass was on for any of these measurements. 

daniel.sigg@LIGO.ORG - 13:38, Wednesday 05 March 2014 (10554)

When comparing this spectrum to the LLO one has to undo the red cavity pole in the above spectra. It is a little bit more complicated, since we are dividing by the red transmitted power which itself can carry noise. With this correction both spectra are referenced to the input laser frequency and look more or less identical.

When comparing this spectrum to the HIFO-Y spectrum in T1300688, the story at mid frequencies is more or less the same:

  • There is large periscope peak around 70Hz with no evidence that the crossfire beam propagation solution helped at all.
  • Between 100Hz and 1kHz we are limited by acoustic noise from the corner.
  • At frequencies of a 1kHz and above we see the laser noise from the end station. Due to the much lower green finesse, it shows up an order of magnitude stronger.
  • At frequencies below 10Hz we now see a strong angular coupling, again due to the lower green finesse. The wavefront sensors were not engaged during the above measurement, and the excess is about two orders of magnitude over the HIFO-Y baseline.
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