Displaying reports 73701-73720 of 83002.Go to page Start 3682 3683 3684 3685 3686 3687 3688 3689 3690 End
Reports until 22:20, Monday 27 January 2014
H1 IOO
paul.fulda@LIGO.ORG - posted 22:20, Monday 27 January 2014 - last comment - 19:27, Tuesday 28 January 2014(9586)
IMC calibrated length / frequency path housekeeping

[Jeff, Paul]

I had a look through the calibrated length and frequency paths for the IMC (IMC-X and IMC-F respectively) to check that the calibration is still in order. A description of all the filters in the IMC-X and IMC-F paths can be found in Giacomo's entry 5945.

In fact, some things were amiss in the IMC_X path:

IMC-X_M1 path:

Filters that were engaged: to_m

Filters that are now engaged: dc_cal, wresg1, wresg2, to_m

MC2 M1 feedback is not currently engaged, so this may not matter right now. However, I've engaged the filters that calibrate the IMC-X_M1 signal to M3 motion. wresg1 and wresg2 model the suspension TF from M1 actuation to M3 actuation with the resg damping filters engaged (as they are currently). If and when M1 stage feedback is applied, the corresponding IMC-X channel should be calibrated now.

IMC-X_M2 path:

Filters that were engaged: dc_cal, white, sus_d1, sus_d2, to_m

Filters that are now engaged: dc_cal, wresg, to_m

The sus_d1 and sus_d2 filters are used to model the suspension TF without the resg filter in the M1 L damping path turned on. Because we are now using the resg damping I have switched the sus_d1 and sus_d2 filters off and engaged the wresg filter, which is used to model the suspension TF with the resg filter in the M1 L damping path. The white filter is a filter which was implemented in L1 in an attempt to avoid digitization noise above 50Hz (since the signal is so small there). I don't think we want to have this filter engaged, since it has to be accounted for later in data analysis, and I think we can ignore IMC_X so far above the L to F crossover. I've therefore disengaged this filter. This isn't the first time this one has come back to haunt us: see e.g 5311 or 5452.

IMC-X_M3 path:

Filters that were engaged: dc_cal, white, sus_d, to_m

Filters that are now engaged: dc_cal, wresg, to_m

Same story as for the M2 path.

I took a snapshot of all IMC-X filter banks.

IMC-F path:

Filters that were engaged: cts2V, InvGenFilt, VCO, FtoL

Filters that are now engaged: cts2V, InvGenFilt, VCO, FtoL

The only filter that changed since Giacomo's entry 5945 is the FtoL filter being engaged now instead of the tokHz filter. This means that the IMC_F signal is now calibrated in meters, presumably for ease of comparison with IMC_X. I checked the VCO gain filter: it is still the 536,604 Hz/V value, agreeing with Kiwamu's number from entry 5556 after accounting for the double pass of the AOM.

Comments related to this report
laura.nuttall@LIGO.ORG - 17:59, Tuesday 28 January 2014 (9616)
I had at four separate times (first plot) after these changes were made to see how H1:IMC-X_DQ looked after it didn't appear comparable to LLO last week (see alog 9373). I've also attached a more recent plot of the same channel at LLO (second plot). The same channel still looks quite different between sites and H1:IMC-X_DQ still seems quite featureless in comparison to LLO. A rather naive question...are they meant to look similar?
Images attached to this comment
paul.fulda@LIGO.ORG - 19:27, Tuesday 28 January 2014 (9618)

As Laura pointed out, the calibrations for L1 and H1 data for these two paths were quite different. I've now gone ahead and changed the H1 calibration path to match the L1 settings.

IMC-X

M1 filters: dc_cal, white, wresg1, wresg2, to_um

M2 filters: dc_cal, white, wresg, to_um

M3 filters: dc_cal, white, wresg, to_um

This means that the IMC-X path is now calibrated in micrometers and it does have the whitening filter engaged. This means the whitening filter (two zeros at 0.2Hz and two poles at 1kHz) should be accounted for in post-processing.

IMC-F

Filters: cts2V, InvGenFilt, VCO, tokHz

This means that the IMC-F path is now calibrated in kHz.

I've saved a snapshot of all 4 filter bank states.

H1 SEI
sebastien.biscans@LIGO.ORG - posted 20:07, Monday 27 January 2014 - last comment - 08:50, Tuesday 28 January 2014(9585)
BSC-ITMX 0.5Hz investigation part2

Arnaud, Sebastien

We've kept investigatiing on the 0.5Hz resonance issue that we've been having on ISI-ITMX (see first alog here). Reminder: we see a  peak at 0.5Hz on all the sensors of the ISI when it is controlled.

After more tests, we realized that this peak appears on all the sensors only when the T240s are in the blend (see plot attached).

Plus, by looking at the T240-X signal, you can clearly see this peak at 0.5Hz. It is even more obvious when the noise floor is reduced (ISI controlled).

 

Thus the issue seems to come from the T240s. We'll continue the investigation tomorrow and find which T240 is bad and how to fix it.

Images attached to this report
Comments related to this report
daniel.sigg@LIGO.ORG - 21:46, Monday 27 January 2014 (9587)

The last plot seems to show harmonics at 1Hz, 1.5HZ(?) and 2Hz. Is this 0.5Hz sharp? If so, this could indicate a problem with the DAQ timing.

sebastien.biscans@LIGO.ORG - 23:04, Monday 27 January 2014 (9588)

Good point Daniel. We have to double check how the other sensors behave. We'll check that tomorrow.

keita.kawabe@LIGO.ORG - 08:50, Tuesday 28 January 2014 (9596)
Exactly 0.5Hz (and its harmonics).
Images attached to this comment
H1 ISC
stefan.ballmer@LIGO.ORG - posted 19:57, Monday 27 January 2014 (9584)
PR2 M3 pitch drivealign done
Jeff, Stefan

We did the PR2 M3 pitch L2P decoupling today.

Plot 1:  transfer functions:
 - blue:   measured L2P TF
 - green:  measured P2P TF
 - red:    L2P/P2P (from measured data)
 - black:  fit (note that we paid more attention to the frequencies below 1Hz, because they matter almost 2 orders of magnitude more (see L2P)
 - Purple: fitted filter times measured P2P.


Plot 2: 3e5cts drive to H1:SUS-PR2_M3_LOCK_L_EXC, first at 0.75Hz, then at 0.95Hz. At both frequecies we get about 1 order of magnitude suppression.
Images attached to this report
H1 SEI (INS, SEI)
jim.warner@LIGO.ORG - posted 16:50, Monday 27 January 2014 - last comment - 09:44, Tuesday 28 January 2014(9581)
HAM4 DTT tf's versus Matlab

Still no resolutions to the problems with HAM4 ISI transfer functions. I took more DTT tf's today, and they all look a little better than the Matlab tf's. The attached plot shows the 3 vertical pods. The 3 thinner lines are the Matlab tf's (which, though not shown, have been repeated 3 times, all 3 times look pretty similar) and the 3 thicker lines (red, green and blue) are the same sensors with a DTT whitenoise tf.

Images attached to this report
Comments related to this report
jim.warner@LIGO.ORG - 09:44, Tuesday 28 January 2014 (9601)INS, SEI

I should add that the H3 GS-13 looks bad, no matter what. It's just hard to see against the general awfulness of the vertical GS-13's.  The first attached image shows the DTT tf in the .5 hz to 5 hz range on the H3 GS13. There should be a taller, pointier peak at ~1hz, which is now kind of squashed. Second image is the power spectra for all GS13s, H3 doesn't look exactly the same as the others at higher frequencies, but not bad. All the other sensors look okay.

Images attached to this comment
H1 SUS (SUS)
travis.sadecki@LIGO.ORG - posted 16:31, Monday 27 January 2014 (9580)
ETMy resuspended

T. Sadecki, B. Weaver

The now final (?) monolithic ETMy Quad has had both chains fully suspended.  Electronics were hooked up and troubleshot for all stages.  OLVs were taken for all stages and MEDM screens updated.  We are satisfied with the current alignment enough that we are ready for the first IAS rough alignment look tomorrow.  We have some rather gross yaw work to do on the main chain, but would like a preliminary look at the overall position on the table so we can take care of any gross, whole structure moves before continuing with finer alignments. 

LHO General
justin.bergman@LIGO.ORG - posted 16:03, Monday 27 January 2014 - last comment - 16:24, Monday 27 January 2014(9578)
ops

Monday 27 JAN 2014

-LVEA laser safe

-Diode room dust monitor needs investigating; false readings all day for 0.03um

920 -1100, 1120 -1200 Mitchell working on ACB in LVEA test stand area

1000- Betsy and Travis at EY

1120 Sheila, Alexa to EX

1155-1215 Richard to EY working with Betsy and Travis

1225 Kiwamu is transitioning the H1 PSL from commissioning to science mode.

1237 Kiwamu working ISCT1 inside the NHZ (LVEA remains laser safe)

1300-1600 Mitch and Scott (Apollo) working on ACB

1404 Hugh to LVEA for ITMX-CPS investigation

1454 - 1547 - Thomas and Aidan to LVEA for parts search

1457-1505 - Corey to LVEA ACB area for brief period

1533 - Sheila and Alexa to EX to toggle noise eater, etc

Comments related to this report
alexan.staley@LIGO.ORG - 16:24, Monday 27 January 2014 (9579)

16:23 -- Alexa and Sheila returned from EX

H1 SEI
hugh.radkins@LIGO.ORG - posted 15:07, Monday 27 January 2014 (9577)
ETMx ISI Alignment changed

St1 Before

St1 After St2 Before St2 After
X 6959nm 41458 -9643 2702
Y 8935nm 9155 253 478
Z -22709nm -22563 -10660 -10743
Rx 39467nrad 39195 10198 10083
Ry -7904nrad -5523 5845 7101
Rz 19481nrad 20104 4123 4482

To help make the isolation of the ETMx less troublesome, this morning I reset the ETMX ISI position loop alignment targets to the tilted location.  This way the ISI will not drive back to the untilted position putting larger outputs on the ISI and reliably running up the trilliums, tripping the WDs.  If the local to cart matrices are somewhat correct, the position/alignment change is small & so far OK.  Adding theStage1 & Stage2 cart position changes gives a 46um position shift of the ISI Optical Table with <4urads on the Ry.  All the other dofs combine to 1um or 1 urad or less.  Sheila did spend some time realigning but the ITM wasn't in nominal isolation either so that might have been hampering efforts there.  Once the ITM was Isolated properly, the green locked much better.

So above is the before and afters.

H1 SEI
hugh.radkins@LIGO.ORG - posted 14:44, Monday 27 January 2014 (9576)
Wiggling cables at ITMx CPS

From ~1400 to 1440--moving ladders, wiggling cables, general trouble making.

H1 SUS
mark.barton@LIGO.ORG - posted 14:34, Monday 27 January 2014 - last comment - 10:47, Friday 07 February 2014(9575)
ETMy OL values

Betsy swapped all the BOSEMs and AOSEMs on ETMy and left them retracted for open light measurements. The resulting values with gains and offsets are:

prettyOSEMgains('H1','ETMY')

M0F1 30218 0.993 -15109
M0F2 29922 1.003 -14961
M0F3 29480 1.018 -14740
M0LF 31134 0.964 -15567
M0RT 30792 0.974 -15396
M0SD 31110 0.964 -15555
R0F1 31059 0.966 -15529
R0F2 30058 0.998 -15029
R0F3 29953 1.002 -14977
R0LF 30794 0.974 -15397
R0RT 31050 0.966 -15525
R0SD 30282 0.991 -15141
L1UL 29222 1.027 -14611
L1LL 30117 0.996 -15059
L1UR 25735 1.166 -12868
L1LR 22721 1.320 -11361
L2UL 21334 1.406 -10667
L2LL 24582 1.220 -12291
L2UR 21223 1.414 -10612
L2LR 20325 1.476 -10163

I entered the gains, checked that all the outputs were right (should be 15000*0.023333=350) and redid the safe.snap.

 

prettyOSEMgains('H1','ETMY')
 
data =
 
   1.0e+04 *
 
    3.0218
    2.9922
    2.9480
    3.1134
    3.0792
    3.1111
    3.1059
    3.0058
    2.9953
    3.0793
    3.1050
    3.0282
    2.9221
    3.0117
    2.5735
    2.2721
    2.1334
    2.4582
    2.1223
    2.0325
 
 
ans =
 
M0F1 30218 0.993 -15109
M0F2 29922 1.003 -14961
M0F3 29480 1.018 -14740
M0LF 31134 0.964 -15567
M0RT 30792 0.974 -15396
M0SD 31110 0.964 -15555
R0F1 31059 0.966 -15529
R0F2 30058 0.998 -15029
R0F3 29953 1.002 -14977
R0LF 30794 0.974 -15397
R0RT 31050 0.966 -15525
R0SD 30282 0.991 -15141
L1UL 29222 1.027 -14611
L1LL 30117 0.996 -15059
L1UR 25735 1.166 -12868
L1LR 22721 1.320 -11361
L2UL 21334 1.406 -10667
L2LL 24582 1.220 -12291
L2UR 21223 1.414 -10612
L2LR 20325 1.476 -10163
prettyOSEMgains('H1','ETMY')
 
data =
 
   1.0e+04 *
 
    3.0218
    2.9922
    2.9480
    3.1134
    3.0792
    3.1111
    3.1059
    3.0058
    2.9953
    3.0793
    3.1050
    3.0282
    2.9221
    3.0117
    2.5735
    2.2721
    2.1334
    2.4582
    2.1223
    2.0325
 
 
ans =
 
M0F1 30218 0.993 -15109
M0F2 29922 1.003 -14961
M0F3 29480 1.018 -14740
M0LF 31134 0.964 -15567
M0RT 30792 0.974 -15396
M0SD 31110 0.964 -15555
R0F1 31059 0.966 -15529
R0F2 30058 0.998 -15029
R0F3 29953 1.002 -14977
R0LF 30794 0.974 -15397
R0RT 31050 0.966 -15525
R0SD 30282 0.991 -15141
L1UL 29222 1.027 -14611
L1LL 30117 0.996 -15059
L1UR 25735 1.166 -12868
L1LR 22721 1.320 -11361
L2UL 21334 1.406 -10667
L2LL 24582 1.220 -12291
L2UR 21223 1.414 -10612
L2LR 20325 1.476 -10163
Comments related to this report
travis.sadecki@LIGO.ORG - 10:47, Friday 07 February 2014 (9910)

Corresponding serial numbers as follows:


M0F1 094
M0F2 588
M0F3 266
M0LF 058
M0RT 041
M0SD 095
R0F1 050
R0F2 186
R0F3 422
R0LF 180
R0RT 056
R0SD 083
L1UL 477
L1LL 493
L1UR 485
L1LR 022
L2UL 473
L2LL 428
L2UR 332
L2LR 321

H1 ISC
alexan.staley@LIGO.ORG - posted 13:53, Monday 27 January 2014 - last comment - 19:15, Monday 27 January 2014(9574)
EX PDH Measurements

(Sheila, Alexa)

We made a few measurements at EX under the following configuration:

PLL Servo Board

PDH Servo Board

  1. PDH open loop transfer function (EX_PDH_OpenLoopTF_mag/phase.TXT)
  2. To calculate the arm cavity length we zoomed in around the FSR resonance (~37MHz) and took the open loop TF (EX_PDH_OpenLoopTF_mag/phase_zoom.TXT). We found FSR ~ 37.752 kHz, which gives a crude estimate of L~3970.6m for the arm cavity length.
  3. PDH error signal power spectrum (EX_PDH_Noise.TXT, EX_PDH_Noise_High.TXT, EX_PDH_Noise_Low.TXT). When plotting the power spectrum at full span we noticed a lot of variation in the measurement (we tried to collect the high and low spectrum in this variation). This variation is due to an unstable cavity lock which causes a variation in the optical gain.
  4. PDH shot noise (EX_PDH_ShotNoise.TXT)
Non-image files attached to this report
Comments related to this report
alexan.staley@LIGO.ORG - 18:37, Monday 27 January 2014 (9582)

(Sheila, Alexa)

 

With the above servo board configurations and the HEPA fans off we measured the shot and dark noise again (in a previous alog I mentioned we didnt take the correct frequency ranges for the dark noise which is why we took it again). I have attached a plot of the power spectrum of the PDH error signal, the shot noise w. the fans off and on, and the dark noise with the fan off. All these spectra's were measured out of IMON. There is a considerable difference at low frequency of the shot noise with the fan off and on. The beam size might be too large on the BBPD? Another possibilty is fringe wraping. It is also suspicious that the shot noise is not flat and seems to drift if there is movement around the table...Are we really measuring pure shot noise??

Non-image files attached to this comment
sheila.dwyer@LIGO.ORG - 19:15, Monday 27 January 2014 (9583)

Keita, Alexa, Sheila

Some of the excess noise on the ALS end refl PD is due to fringe wrapping. We looked at spectra of REFL B from the control room while the ITM was misalinged, ( so we should have been looking at the RIN on our green beam returning from the chamber).  This is motivated by seeing that the niose at Imon with the ITM mislainged is accoustic, and seems to have a fringe wrapping shelf when the HEPA filters are on. By driving the ETM longitudnaly, we see a fringe wrapping peak on the DC PD.  We tried misalinging the reaction chain, and don't see any difference.  At some point we need to go bow on optics on the table and try to find the scattering path. 

Images attached to this comment
H1 PSL (PSL)
justin.bergman@LIGO.ORG - posted 12:23, Monday 27 January 2014 - last comment - 12:28, Monday 27 January 2014(9571)
PSL Change

Kiwamu is transitioning the H1 PSL from commissioning to science mode.

Comments related to this report
kiwamu.izumi@LIGO.ORG - 12:28, Monday 27 January 2014 (9573)

The transition is done at 12:27. Now it is is the science mode.

H1 SEI
hugh.radkins@LIGO.ORG - posted 12:04, Monday 27 January 2014 (9570)
ETMX ISI running fine.

Stefan logged yesterday that he was unable to get the ISI into operation state without tripping.

First time I did this today, I did Stage2 one dof at a time and had no problem.  The ETMx blends at 750mHz on both Stages all dofs.  Pretty sure this isn't as well as can be squeaked from the ISI.  I took this opportunity to take spectra as I brought other blend filters to bare.  Attached is the Stage2 GS-13 X In1 with various filter combos.

Ref3, red: As found 750mHz all dofs both Stages.

Ref7, blue: T(rilliums)750mHz all dofs Stage1, 750mHz Stage2---Maybe a factor of 2 improvement below 0.5Hz

Ref11, green: T250mHz all dofs Stage1, 750mHz Stage2---Much better above 0.5Hz but worse between ~.1 and 0.5Hz.

Ref15,thick brown: T100mHz.44NO Stage1 X Y & Rz else T250s, Stage2 750mHz---Big win below 1Hz to about 0.1Hz.

Ref18, pink:T100mHz.44NO Stage1 X Y & Rz else T250s, Stage2 250mHz---Better ~x2 or 4 above 0.8 but worse below especially 0.2Hz.

Ref23, aqua: T100mHz.44NO Stage1 X Y & Rz plus Notch X Y else T250s, Stage2 750mHz---Lost improvement above 0.8Hz but improves over brown between 0.8 and 0.2Hz.

Ref28, black: T100mHz.44NO Stage1 X Y & Rz plus Notch X Y else T750s, Stage2 750mHz---Some improvements below 0.2Hz and some above 1Hz.

I'm not sure this is exactly the best configuration such as maybe the T250 is better than the T750 for both Stages.  Certainly incrementally there were tradeoffs.  We need to combine the benefits in a better way.

So I have the ISI in this final arrangement. I took the ISI out of Isolation (it triggered then!)  I then reset the ISI targets to the unisolated postions.  The ISI was then able to go into Isolation with 'One Button'.  Green team is evaluating if they can live with this minor alignment change.

Images attached to this report
LHO General
justin.bergman@LIGO.ORG - posted 11:19, Monday 27 January 2014 - last comment - 12:24, Monday 27 January 2014(9568)
ops

Sheila to EX

Comments related to this report
justin.bergman@LIGO.ORG - 12:24, Monday 27 January 2014 (9572)

Sheila and Alexa return 1215

H1 SYS
daniel.sigg@LIGO.ORG - posted 11:11, Monday 27 January 2014 (9567)
Commissioning calendar for next 2 weeks

Here is the list of commissioning task for the next 7-14 days:

Green team:

  1. Measure difference between red and green locking offsets.
  2. Commission the common mode hand-off including the AO path.
  3. Make an exact measurement of the cavity length.
  4. Complete the noise model for ALS X by adding PDH and COMM servos.
  5. Commission a relief script for the angular offsets in the initial alignment controls.
  6. Commission the length feedback path to the ETM top suspension point to suppress microseism.
  7. Asses the status of the reference cavity temperature controls.

Red team:

  1. Angular decoupling optimization for PR2 and PRM.
  2. Lock the PRMI using 1f and 5f signals.
  3. Lock the PRMI using the 3f signals.
  4. Arm cavity alignment for the red beam.
  5. Mode matching measurements using ISCT1 and maybe IOT2R.
  6. Mode cleaner characterization: Absorption, heating and scattering.
  7. Track down the 0.5 Hz feature in the seismic isolation system.
  8. Investigate the REFLAIR45 whitening filter issue.

TMS:

  1. Repair and exchange the in-vacuum cable for the beam diverter.

ISCTEY (starting next week):

  1. Complete the feedthrough panels.
  2. Install the on table cabling.
  3. Prepare for move to the end station.
  4. Check out ALS electronics in EY.
Displaying reports 73701-73720 of 83002.Go to page Start 3682 3683 3684 3685 3686 3687 3688 3689 3690 End