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Reports until 21:41, Wednesday 06 January 2016
H1 ISC (OpsInfo)
jenne.driggers@LIGO.ORG - posted 21:41, Wednesday 06 January 2016 - last comment - 12:42, Thursday 07 January 2016(24733)
ASC woes

[Jenne, Kiwamu, Sheila, JeffK]

Today, the interferometer decided that it didn't want to go from ASC_PART2 to ASC_PART3 without some hand-tuning each lock.  However, after some investigation, it's still not entirely clear what the right thing to do is :(

The things we were playing with were the offsets in the CSOFT and DSOFT pitch filter banks (can only be tweaked *after* the loops are on, since there's an integrator always on in each of those filter banks) and the transmon qpds' ASC-[x,y]_TR_[a,b]_[pit,yaw]_OFFSETs.  These things are kind of the same, but you need to adjust the transmon offsets if you want to do some adjusting before the loops are closed, and you need to adjust the CSOFT and DSOFT offsets if you want to do some adjusting after the loops are closed.

We've had locks where we didn't survive if we didn't re-zero the qpd offsets before going to part3, and we've had locks where we didn't survive part3 if we didn't adjust the CSOFT and DSOFT offsets.  But, we've also had locks where the opposite was true.

Anyhow, at this point, I think our advice is to try going through the guardian like normal (no by-hand offsetting), and if that fails one or more times, call a commissioner (it's me for now, so please call).  For example, the last lock, I re-set the qpd offsets during asc part 2, but forgot to engage the CSOFT and DSOFT offsets, and we seemed to be just fine.  So, it's not totally clear yet what the final prescription should be.

Comments related to this report
sheila.dwyer@LIGO.ORG - 00:35, Thursday 07 January 2016 (24737)

Tonight we had one OK lock with the offsets as Jenne aloged above, which we lost because of an EQ (see Cheryl's shift summary).  On relocking without changing the offsets or doing anything special, we lost lock due to the CSOFT pitch instability that has plauged us when we have changed the TMS QPD offsets in the past. (There was a small EQ that arrived on site shortly after this lockloss, but clearly we lost lock because of the pit instability before it arrived). After this, Cheryl and I let the IFO lock and engage ASC with the offsets that Jenne had found this afternoon, then once the soft loops were closed very slowly reverted to the old offsets (see Cheryl's alog) at 2 Watts. Our recycling gain was around 41 when we started, and although it dropped as we reverted the offsets it returned to 41-42 once they were all reverted.  We powered up slowly and the recycling gain stayed above 40.  After about 20 minutes I thought that things seemed better than they have in several days, so I suggested we offload the full lock ASC.  Sadly this broke the lock. 

Since this situation is very similar to what happened Dec 3rd -4th, I re-ran the script I used then to look at build ups (23959), for the past 10 days.  The results are very similar, the drop off in the POP DC trace is very similar to the drop off in the arm transmissions (ratio of arm transmissions to POP DC is shown in the middle panel, and is changing by at worst 1% while the powers drop by nearly 15%. )

One explanation we considered in December was that the OMC was becoming misaligned, causing the DARM offset to change.  The second attachment shows the OMC ASC control signals and the QPDs, which are out of loop.  You can see that they move around even in locks where the recycling gain is stable and don't seem to be any worse in the last few days, so it seems like this is not our problem.  

 

Images attached to this comment
sheila.dwyer@LIGO.ORG - 01:06, Thursday 07 January 2016 (24740)

Jim has just relocked with a recycling gain of 41, which has been stable for nearly 20 minutes, so this is looking more promising.  One thing that we did is edit lscparams so that the guardian will go to 10 Watts in the increase power state instead of the normal set point of 23 W.  

Until this is reverted the steps to follow for power up are:

1) request INCREASE_POWER (it is important to change the PSL power only in this state, this state automatically takes care of gain scalings for you).

wait until the power reaches approximately 10 watts, and the recycling gain seems stable.  We have been waiting a few minutes here to make sure it stays stable, that should not normally be necessary.

2) open the PSL rotation stage medm screen (from site map under IOO on the top right hand side, Rotation Stage).

3) type 23 in the requested power dialog box and hit go to power

4) only once the rotation stage has finished moving is it safe to leave the INCREASE_POWER state.

kiwamu.izumi@LIGO.ORG - 09:22, Thursday 07 January 2016 (24746)

For the record, I give you another similar example that Nutsinee and I had experienced back in October (alog 22575 and comments). At that time, we conluded that it was due to subopitimal alignment in TMSY.

thomas.shaffer@LIGO.ORG - 12:42, Thursday 07 January 2016 (24750)

Opened FRS ticket

Fault Report 4186 - Trouble advancing past Guardian state ENGAGE_ASC_PART2

(This was done as "for-real" practice with R. Oram)

H1 General
cheryl.vorvick@LIGO.ORG - posted 18:24, Wednesday 06 January 2016 (24735)
GRB alert at 01:37:28UTC

GRB alert arrived at 01:37:28UTC, and it's currently 2:22UTC.

H1 was locked before the GRB arrived, and is still locked.

We are about 10 minutes from completing the stand-down time.

H1 General
travis.sadecki@LIGO.ORG - posted 16:01, Wednesday 06 January 2016 (24731)
OPS Day Shift Summary

Title: 1/6 Shift 16:00-24:00 UTC (8:00-16:00 PST).  All times in UTC.

State of H1: Locking/Commissioning

Shift Summary: We have been struggling to acquire lock all day due to issues with ASC loops.  Commissioners are working on it and hopefully we are nearing success.  Microseism is trending up and is currently at 0.6 um/s.  Wind is calm.

Incoming operator: Cheryl

Activity log:

19:00 Kyle and Gerardo to Mid Y

19:54 Kyle and Gerardo back

23:34 Kyle to Mid Y

23:54 Kyle back

H1 INJ (INJ)
cregg.yancey@LIGO.ORG - posted 15:10, Wednesday 06 January 2016 (24730)
HWInjReport 1132272017 - 1133039434

HWInjReport 1132272017 - 1133039434

Performed a run spanning the time period from 1132272017 (Nov 23 2015 00:00:00 UTC) to 1133039434 (Dec 01 2015 21:10:17 UTC)

Parameters

The following parameters were used for this run:

Scheduled Injections

There were no injections scheduled to occur within this time period.

Network and IFO Injections

Only a single CAL-INJ reset in L1 was found to occur within this time period

This was, of course, UNSCHEDULED.

Discussion of Anomalies

No anomalies of interest were found.

Non-image files attached to this report
H1 INJ (INJ)
cregg.yancey@LIGO.ORG - posted 14:55, Wednesday 06 January 2016 (24729)
HWInjReport 1132084817 - 1132350679

HWInjReport 1132084817 - 1132350679

Performed a run spanning the time period from 1132084817 (Nov 20 2015 20:00:00 UTC) to 1132350679 (Nov 23 2015 21:51:02 UTC)

Parameters

The following parameters were used for this run:

Scheduled Injections

There were no injections found to be scheduled during this time period.

Network and IFO Injections

There were no injections found to occur during this time period.

Discussion of Anomalies

No anomalies found during this time period.

Non-image files attached to this report
H1 CAL (CAL)
darkhan.tuyenbayev@LIGO.ORG - posted 11:59, Wednesday 06 January 2016 - last comment - 15:23, Friday 08 January 2016(24726)
LHO Pcal EndX calibration measurements were taken

RickS, Darkhan,

Yesterday, Jan 5, 2016, we took Pcal end-station calibration measurements at EX using WS1 calibration standard. The measurement procedure is described in T1500063.

Rough numbers from dataviewer and GPS times were noted in the attached scan (blank form is taken from T1500062).

A generated report (comparison with previous measurements) was uploaded to DCC T1500129-v3.

At first when we started the measurements we found out that laser power in PcalX is modulated through Pcal hardware injection channels H1:CAL-PINJX_*, we had to restart the measurements after tuning off these excitations.

Non-image files attached to this report
Comments related to this report
darkhan.tuyenbayev@LIGO.ORG - 12:20, Wednesday 06 January 2016 (24727)

At first we used CAL_INJ_CONTROL medm screen to turn off injections.

When we found out that some injections are still going into PCALX, we looked into H1:CAL-PINJX_* filters using auto-generated medm screens in

/opt/rtcds/lho/h1/medm/h1calex/H1CALEX_PINJX_*.adl

We switched off outputs from these filters before taking our measurements and put them back on afterwards.

darkhan.tuyenbayev@LIGO.ORG - 15:23, Friday 08 January 2016 (24777)

Jeff pointed out that going to /opt/rtcds/lho/h1/medm/h1calex/H1CALEX_PINJX_*.adl  is not necessary, there's a MEDM screen under Sitemap -> CAL -> PINJX that gives an access to Pcal hardware injection switches.

H1 CDS (DAQ)
david.barker@LIGO.ORG - posted 11:28, Wednesday 06 January 2016 (24724)
CDS model and DAQ restart report Sunday-Tuesday 3rd-5th January 2016

O1 days 108-110

No restarts reported on any of these days. No CDS front end or DAQ maintenance Tues 5th.

H1 SEI
hugh.radkins@LIGO.ORG - posted 10:49, Wednesday 06 January 2016 (24723)
A look at the STS2-B after Mass Centering

Bottom line: I don't see this mass centering made any difference.  Although I did get the mass within spec, and it remains so, it was difficult as in it took many attempts.  This may still indicate that the machine is not well enough leveled or still something more difficult to fix.

Attached are spectra of the STS2-B (ITMY) and STS2-C (HAM5) and coherences between them early Tuesday and Wednesday morning to compare them before and after the centering done yesterday, I adjusted the times to avoid an EQ Tuesday am.   STS2-A remains rotated out of position so is not included in this comparison.

The attached spectra and coherences don't reveal any great improvement from the centering.  The reference traces are after and the current traces are before the centering.  The coherence and ASD continues to show that the Y channel looks pretty good and the X and Z channels much less so.  If you look at the STS2 channel/axis orientations (see second attachment,) you'll see that the Y channel does not use the U axis sensor, and, the centering of the U axis was the problem axis.  This is why I want to play with the level of the U axis and continue this examination.

Images attached to this report
H1 General
jim.warner@LIGO.ORG - posted 08:19, Wednesday 06 January 2016 (24722)
Shift Summary

Ops Owl Summary: 8:00-16:00UTC

State of H1: unlocked

Commissioners: Jenne, Sheila (fellow), JeffK

Shift Summary:

9:00 Lock and Observing finally

11:45 I realize the LVEA lights were still on, LLO is still down, so briefly out of Observe and I go turn them off, back to Observing right as LLO comes back up

13:45 An earthquake in Mexico knocks us out

14:15 Start trying to lock

15:00 Richard arrives and starts spreading sand around parking lot

15:00 I start initial alignment, high microseism is making locking difficult

H1 General
jim.warner@LIGO.ORG - posted 05:20, Wednesday 06 January 2016 (24721)
Mid shift summary

Currently in observing at about 75 Mpc. So far everything looks better than last night. Sheila did some ASC tweeking before she left and it seems to have prevented the POP decay so far. Microseism is high-ish, wind is low. EX ISI is occasionally ringing up but I think the microseism is maybe to high to switch to higher blends.

H1 General
sheila.dwyer@LIGO.ORG - posted 00:30, Wednesday 06 January 2016 - last comment - 01:12, Wednesday 06 January 2016(24719)
Attempt to improve recycling gain

Sheila, Cheryl, Jenne

When Cheryl locked the interferometer after maintence day and calibration work was done this afternoon, the recycling gain was again low, (POP_A_LF around 15500 cnts), around the level we have started at in locks where the recycling gain degraded until loosing the lock over the last few days.  (When the recyclcing gain is stable this is normally around 16500 cnts).  Since LLO was not locked, we took some time to open the refl beam diverter and look at the camera for a msalignement. 

We then opened the PRC1 ASC loops (POP A to PRM, slow loop) and moved PRM by hand, very slowly so that the CHARD and CSOFT loops had time to catch up.  We moved PRMI pit alignment slider from -1419 to -1405 urad, and yaw from 518 to 537 urad.  This increased POP A by about 400 counts.  At the slightly better recycling gain the offsets on POP A were -0.35 for Yaw and -0.3 for pitch.  As Cheryl mentioned in her alog, we lost the lock for reasons I don't really understand while adjusting pitch.  There didn't seem to be any environmental problem, so it would seem likely that it was my PRM pitch adjustment that is to blame, but I was not doing anything different from what I had been doing for the previous half hour. 

We may want to try these QPD offsets as a new set point for the PRC1 loop, depending on what the reccyling gain looks like when Jim finishes locking. 

Cheryl and I also spent some time debugging the PRMI branch, which has had some bugs in it for a while that have probably been causing problems. 

Images attached to this report
Comments related to this report
sheila.dwyer@LIGO.ORG - 01:12, Wednesday 06 January 2016 (24720)

This lock also started with low recycling gain, and Jim and I decided to try changing the soft loop offsets instead of repeating the PRM expiriment.  I added offsets to DSOFT P and CSOFT P (the normal offsets are still in the TMS QPDs, I have not touched those.)

The current offset in DSOFT P is 0.04, while CSOFT P has an offset of -0.02.  It seems like we could probably keep moving CSOFT to more negative offsets and keep improving the recycling gain, but we decided just to go to observing and see what happens over the course of the lock.  POP A LF is now at around 15600 counts.  

If anyone wants to revert this in the morning, just set H1:ASC-DSOFT_PIT_OFFSET and H1:ASC-CSOFT_PIT_OFFSET to zero.

H1 General
cheryl.vorvick@LIGO.ORG - posted 00:12, Wednesday 06 January 2016 (24718)
Ops Eve Summary:

Ops Eve Summary: 00:00-08:00UTC, 16:00-23:59PT

State of H1: unlocked

Commissioners: Jenne, Sheila (fellow), JeffK

Incoming Operator: JimW

Shift Summary:

H1 CAL (SUS)
jeffrey.kissel@LIGO.ORG - posted 18:45, Tuesday 05 January 2016 - last comment - 10:27, Thursday 07 January 2016(24716)
EY SUS Coil Driver Measurements Complete
J. Kissel

In efforts to finally nail down the mysterious "zero" around 50 [Hz] in the UIM (see LHO aLOG 24296), I've measured the TOP, UIM, and PUM driver using three different measurement configurations. The hope is that, with this "matrix" of differences, we can find out what's going on with the UIM to see if its something specific to the driver, or specific to the OSEM chain upstream of the driver. From what I've seen watching the measurements go by on the SR785, both the TOP and PUM stage show similar zero-like behavior as the UIM, though the TOP mass has a pole-like behavior above the zero and eventually rolls off. Both the PUM and the UIM look as though they are rolling up to "infinity" by 10 [kHz], without even a phase shift indicating their might be a pole "soon" in frequency.  More detailed analysis and plots to come.

The data has been committed to the repo here:
/ligo/svncommon/CalSVN/aligocalibration/trunk/Runs/PostO1/H1/Measurements/Electronics/
EYPUMDriver/2016-01-05/TFSR785*.txt
EYTOPDriver/2016-01-05/TFSR785*.txt
EYUIMDriver/2016-01-05/TFSR785*.txt
where the key to each driver's measurement set is in the log files,
/ligo/svncommon/CalSVN/aligocalibration/trunk/Runs/PostO1/H1/Measurements/Electronics/
EYPUMDriver/2016-01-05/2016-01-05_EYTOP_Measurement_log.txt
EYTOPDriver/2016-01-05/2016-01-05_EYUIM_Measurement_log.txt
EYUIMDriver/2016-01-05/2016-01-05_EYPUM_Measurement_log.txt

I also attach a white board sketch that indicates each of the measurement configurations.
   (0) [Not shown] The "reference" measurement is identical to the reference setup shown in page 2 of the 2nd attachment in 18518, which is divided out of every transfer function to get rid of the response of the differential driver.
   (1) This is measuring the response of the coil driver as it is typically measured on the bench by CDS. It uses a differential to single-ended receiver and the 40 [ohm] internal load (as I only found out later, the documentation on this box, D1000931 leaves something to be desired), so the response differs from configuration (2) only by a scale factor of 2.
   (2) This is measuring the response of the coil driver as is typically done in the field when the OSEM and/or satellite amplifier is not available. The box (D1100278) is, as far as the coil chain is concerned, only a two 20 [ohm] (for a total of 40 [Ohm]) resistor load.
   (3) This is the "real life" scenario, where we measure the response of the driver with the full SatAmp and OSEM included as a load on the output of the driver. It is in this configuration is where the magic happens, apparently.
Images attached to this report
Comments related to this report
jeffrey.kissel@LIGO.ORG - 11:43, Wednesday 06 January 2016 (24725)
Since the IFO has decided to give up on Calibration Week, I've put together some .graffle diagrams of what I show in the whiteboard picture above such that a future user and/or LLO can more clearly replicate my results, if need be (or they don't trust what Evan G's is about to post).

Also note for future me, the source code for these diagrams lives in
/ligo/svncommon/CalSVN/aligocalibration/trunk/Runs/PostO1/H1/Measurements/Electronics/EYTOPDriver/2016-01-05/
CoilDriverChassisSetup_BenchTestSetup.graffle
CoilDriverChassisSetup_DummyOsemChain.graffle
CoilDriverChassisSetup_RealOsemChain.graffle
Non-image files attached to this comment
evan.goetz@LIGO.ORG - 10:27, Thursday 07 January 2016 (24734)

Summary:
I plotted the results of Jeff's measurements for the H1 End Y driver electronics for the top, UIM, and PUM masses. All show odd behavior at high frequencies that we cannot model as an ideal inductor.

  1. The top mass BOSEMs have an odd behavior, approximately f^(1/4) dependence, but can't be fit to a simple pole-zero pair, nor more complicated 2 pole/1 zero, or 2-complex-pole/1 zero models.
  2. The UIM BOSEMs show an f^(3/4) dependence and also have 180-degree phase flip with respect to the top mass BOSEMs.
  3. The PUM AOSEMs in state 1 and 3 show an odd high frequency behavior something like f^(3/4) dependence, especially with the phase turn-over at 60 degrees and we cannot fit a 2-complex-pole/1 zero to this.
  4. AOSEMs in state 2 and 4 have the complicated aquire electronics that change the Bode plots but we ignore these issues as they are expected

Details:
For each measurement of a given mass' driver electronics (TOP, UIM, or PUM), I divided the measured BOSEM (for TOP/UIM) or AOSEM (for PUM) transfer functions (normalized) by the corresponding transfer function for when there is a dummy 40 ohm resistor terminating the output of the drive electronics (also normalized). In addition to plotting the results of the measurements, I also investigated the high frequency behavior. Nominally, we expect to observe the inductance of the BOSEMs or AOSEMs as a simple zero--the high frequency dependence goes as f. Instead, we observe different dependences for the BOSEMs of the top and UIM masses and the AOSEMs of the UIM (state 1 and 3). We attempted to fit by hand some zero-pole models to these Bode plots but were unsuccessful to replicate the high frequency dependence.

  1. For the top mass, it appears like there is a pole-zero pair, but we are unable to replicate the transfer function behavior with simple pole-zero or more complicated 2 pole/1 zero and 2-complex-pole/1 zero. In the 1 kHz region, the frequency dependence is approx. f^(1/4). For all top mass BOSEMs, in both states, we observe the same issue.
  2. For the UIM, It definitely appears that the BOSEM frequency dependence is f^(3/4) from the measurements above 1 kHz for all UIM BOSEMs and all states.
  3. The PUM AOSEMs in states 1 and 3 show an interesting ~f^(3/4) dependence and phase turn over at 60 degrees. We were unable to fit this to zero-pole pair.
  4. State 2 and 4 in the PUM AOSEMs show the complicated acquire electronics that we do not attept to model here.
Non-image files attached to this comment
LHO VE (VE)
gerardo.moreno@LIGO.ORG - posted 16:41, Tuesday 05 January 2016 (24715)
CP3 Manual Overfill @ 00:08 UTC

After notifying the operator I drove past the CS @ 00:02 and arrived at Y-Mid station @ 00:07.
Started filling CP3 @ 00:08, opened the exhaust check valve bypass valve, then opened LLCV bypass valve 1/2 turn, started to notice flow @ 00:18. and closed the LLCV bypass valve @ 00:19.
5 minutes later I closed the exhaust check valve bypass valve.

Started driving back from Y-Mid @ 00:26, arrived at the CS @ 00:30.

H1 SUS (ISC)
brett.shapiro@LIGO.ORG - posted 22:38, Friday 01 January 2016 - last comment - 19:36, Tuesday 05 January 2016(24625)
Additional Updates to the quad Matlab model

svn up at .../SusSVN/sus/trunk/QUAD/Common/MatlabTools/QuadModel_Production

All current model features are summarized in a table in G1401132.

Update to existing features

The main change in existing features is that the top mass damping now sees both the suspension and the cage, as in real life because we use OSEMs. Consequently, if you input seismic noise to a damped suspension it will enter both mechanically as usual, as well as through the damping loops. See Seismic_Noise_Propagation_2016_01_01.pdf. Page 1 shows longitudinal transfer functions from seismic noise to the test mass with and without the OSEMs seeing the cage. The second page shows the ratio of these transfer functions. Note that the ratio is greater than a factor of 2 at 4.5 Hz. Beyond 10 Hz the maximum is about 20% at about 10.5 Hz.

 

Two new features 

1. Additional inputs and outputs added to reflect the relative nature of the OSEMs - i.e. they measure relative displacements and actuate between two points

2. Suspension point reaction forces

The discussion above is one consequence of the first new feature. Another is that you can now make transfer functions between seismic noise and the top mass OSEMs, which is dramatically different from the seismic noise to top mass transfer function. See Seismic_to_Top_OSEMs_2016_01_01-2.pdf. These are obtainable in the model with the new 'toposem' field in the 'out' structure given by the generate_QUAD_Model_Production function.

The second new feature is that there are now outputs for the suspension point reaction forces on the ISI. These are obtainable in the model with the new 'suspoint' field in the 'out' structure given by the generate_QUAD_Model_Production function. These reaction forces allow us to dynamically couple the quad model to the ISI model. Thus, if we wanted, we can make one big ISI-SUS model.

 

Under-the-hood updates

This update includes significant under-the-hood modifications to how the pieces of the model are put together. Essentially, Simulink files now define the connections and signal flow, where previously this was all done with append/connect commands in the generate script. The motivation for this change is to make the model more extensible and maintanable by humans. The append/connect commands had become virtually unreadable with the dozens of inputs and outputs now in the model. Now someone can look at a more intuitive graphical representation in a simulink file to read or modify how the model is layed out.

There are 4 simulink files defining the 4 possible layouts of the quad model:

1) A single undamped chain - generate_QUAD_SingleChainUndamped_Simulink.slx
2) A single damped chain - generate_QUAD_SingleChainDamped_Simulink.slx
3) Two undamped chains - generate_QUAD_BothChainsUndamped_Simulink.slx
4) Two damped chains - generate_QUAD_BothChainsDamped_Simulink.slx

 

For reference, this is a summary of the history of model revisions in the svn:

generate_QUAD_Model_Production.m

rev 7359: now reads foton files for main chain and reaction damping

rev 7436: Changed hard coded DAMP gains to get the correct values for LHO ETMX specifically.

rev 7508: Restored damping filter choice for P to level 2.1 filters as opposed to Keita's modification. Cleaned up error checking code on foton filter files, and allowed handling of filter archive files and files with the full path.

rev 7639: renaming lho etmy parameter file

rev 7642: Adding custom parameter file for each quad. Each one is a copy of h1etmy at this point, since that one has the most available data.

rev 7646: added ability to read live filters from sites, and ability to load custom parameter files for each suspension

rev 7652: updated to allow damping filters from sites from a specific gps time (in addition to the live reading option)

planned future revision - seismic noise will progate through the damping filters as in real life. i.e the OSEMs are relative sensors and measure the displacement between the cage and the suspension.

rev 7920: big update - added sus point reaction forces, top OSEMs act between cage and sus, replaced append/connect command with simulink files

ssmake4pv2eMB5f_fiber.m

no recent (at least 4 years) functional changes have been made to this file.

* quadopt_fiber.m

- rev 2731: name of file changed to quadopt_fiber.m, removing the date to avoid confusion with Mark Barton's Mathametica files.

- rev 6374: updated based on H1ETM fit in 10089.

- rev 7392: updated pend.ln to provide as-built CM heights according to T1500046

- rev 7912: the update described in this log, where the solidworks values for the inertias of the test mass and pum were put into the model, and the model was then refit.  Same as h1etmy.m.

* h1etmy.m

- rev 7640: created the H1ETMY parameter file based on the fit discussed in 10089.

- rev 7911: the update described in this log, where the solidworks values for the inertias of the test mass and pum were put into the model, and the model was then refit. Same as quadopt_fiber.m.

Non-image files attached to this report
Comments related to this report
brett.shapiro@LIGO.ORG - 10:37, Saturday 02 January 2016 (24638)

The quad model was tagged on the SVN both before and after this update. The tagged models are at 

before this update:
/ligo/svncommon/SusSVN/sus/trunk/Common/SusModelTags/Matlab/quadmodelproduction-rev7652_ssmake4pv2eMB5f_fiber-rev3601_fiber-rev7913_released-2016-01-01.mat
This version reflects the model after the previous recent update discussed in log 24456, which updated the test mass and PUM inertias with solidworks values. No model features were changed in this update.

After this update
/ligo/svncommon/SusSVN/sus/trunk/Common/SusModelTags/Matlab/quadmodelproduction-rev7920_ssmake4pv2eMB5f_fiber-rev3601_fiber-rev7913_released-2016-01-01.mat

The tags were created using the following script:

/ligo/svncommon/SusSVN/sus/trunk/Common/MatlabTools/tagsusdynamicalmodel.m    rev 7923

jenne.driggers@LIGO.ORG - 16:32, Monday 04 January 2016 (24694)

Just as an FYI, I have done this svn update.

brett.shapiro@LIGO.ORG - 19:36, Tuesday 05 January 2016 (24717)

MInor updates and fixes:

1) The simulink files were generating warnings in Matlab 2012b because they were saved in 2013a. I resaved them in 2012b, recommited, and the problem has gone away. Matlab versions 2013a and 2015b are fine as well. No promises for versions earlier than 2012b.

2) While fixing the simulink diagrams, I added some extra inputs based on a disucssion with Brian Lantz. These are 'osem like' force inputs acting between the top mass and the cage for the purpose of testing the reaction force outputs on the ISI. These will not impact any prior features of the model.

H1 INJ (INJ)
cregg.yancey@LIGO.ORG - posted 15:01, Friday 20 November 2015 - last comment - 16:02, Wednesday 06 January 2016(23603)
HWInjReport 1129593617 - 1131828544

HWInjReport 1129593617 - 1131828544

Performed a run spanning the time period from 1129593617 (Oct 23 2015 00:00:00 UTC) to 1131828544 (Nov 17 2015 20:48:47 UTC)

Parameters

The following parameters were used for this run:

Scheduled Injections

Only two injections were found to be scheduled during this period:

However, neither of these injections were found to actually occur within the examined time period.

Network and IFO Injections

There were no normal injections that occurred within the examined period. There were a number CAL-INJ resets, all single-IFO with the same curious pattern to the frame flags as denoted in the immediately prior HWInj report (https://alog.ligo-wa.caltech.edu/aLOG/index.php?callRep=23485). There was a single-IFO burst injection in H1

BURST 1129673117.000 (H1)

with the only anomaly being that it is UNSCHEDULED. There was a single UNKNOWN injection in L1

UNKNOWN 1129673117.000 (L1)

This injection was confirmed to occur only within the CAL-INJ channel of RAW frames with the TRANSIENT bit indicating an injection but none of the specific injection-type bits, CBC, BURST, DETCHAR, or STOCHASTIC, indicating an injection. It was confirmed to not occur in ODC HOFT, ODC RDS, ODC RAW, or GDS HOFT frames.

Discussion of Anomalies

It is interesting that the single-IFO injections BURST 1129673117.000 (H1) and UNKNOWN 1129673117.000 (L1) are found to occur at the exact same time but within different IFOs. Even further, the fact the BURST injection in H1 is perfectly normal, other than being UNSCHEDULED, while the UNKNOWN injection in L1, in addition to being UNSCHEDULED, is inconsistent. HWInjReport currently does not check the HW bit or the CW bit in the CAL-INJ channel for RAW frames for the presence of injections; however, upon examining these bits directly, it was found that while the HW bit indicated an injection, along with the TRANSIENT bit, the CW bit did not indicate an injection (my first thought was that this may be a CW injection only occurring in L1). This means this was a truly UNKNOWN, UNSCHEDULED injection occurring only with L1. Given both injections occur at the exact same time and the L1 injection is a truly UNKNOWN type (practically a ghost injection, by the bits), it is likely this was intended to be a normal network injection; however either user-error or a catastrophic software error corrupted the proper setting of the bits.

Non-image files attached to this report
Comments related to this report
cregg.yancey@LIGO.ORG - 14:21, Monday 23 November 2015 (23670)

There was an additional UNKNOWN injection that occurred at 1131397646 in both H1 and L1 (as noted by Peter Shawhan) with a signature similar to the one reported here.  However, for some reason HWInjReport missed it.  I will have to investigate why HWInjReport missed that particular injection, but, unlike the last session of bug-fixing, I am not going to cease production of reports.  It is my estimation that HWInjReport is currently operating with reasonable confidence to find and report most true anomalies.  If reporting errors or omissions are found, then those errors should be correctable and a new report on the relevant time period can be generated.

christopher.biwer@LIGO.ORG - 13:54, Monday 14 December 2015 (24206)
I didn't see any follow-up on this but I did some checks:

The injection at 1129673117 is the stochastic hardware injection that Joe and Chris did. This was out of science mode.

The injection at 1131397646 should be the injection in the schedule file from line: 1131397639 1 1.0 coherentbbh0_1126259455_

This CBC injection was not logged properly for the searches because tinj was setting CAL-INJ_TINJ_TYPE instead of CAL-PINJX_TINJ_TYPE. So I would guess that was the problem that you're seeing here. The issues have since been fixed though.
cregg.yancey@LIGO.ORG - 16:02, Wednesday 06 January 2016 (24732)INJ

Now that I finally have my diagnostic tool working (it's a ripped-down version of HWInjReport called HWInjCheck that simply returns raw output from FrBitmaskTransitions to allow rapid verification of anomalies found in HWInjReport), I re-examined the missing UNKNOWN injection at 1131397646.  Firstly, HWInjReport can only identify injections as UNKNOWN if they occur in the CAL-INJ.  This is because, as far as I can determine, only the CAL-INJ channel has an independent excitation bit that indicates whether a transient injection has occurred, regardless of type (as well as an independent HW bit indicating the occurrence of an injection of any type).  This does not seem to be true for ODC-MASTER and GDS-CALIB channels.  So, in CAL-INJ, if the TRANSIENT bit is "off" (indicating the presence of a transient injection) but the CBC, BURST, DETCHAR, and STOCHASTIC bits, which indicate the type of injection, are "on", then it is clear we have an UNKNOWN type transient injection occurring.  However, for ODC-MASTER and GDS-CALIB, if the type bits are not "off", there is nothing to indicate excitation of a transient injection with an unspecified type.  If 1131397646 occurs with an unspecified type in the ODC-MASTER or GDS-CALIB channel but not in the CAL-INJ channel, then HWInjReport will completely miss the injection as it won't show up at all in any of the bits and channels that HWInjReport checks.

Using HWInjCheck to check the output from FrBitmaskTransitions, I have not, yet, found any indication of the occurrence of 1131397646, that is, there is no indication of excitation in the excitation bits.  I will check again more carefully, but, at this point, it does seem HWInjReport is working properly; this is an expected missing injection.  To be clear, there may still have actually been an excitation, there just doesn't seem to be any record of it in the bits and channels that HWInjReport checks.

H1 ISC
kiwamu.izumi@LIGO.ORG - posted 15:09, Thursday 30 January 2014 - last comment - 00:30, Friday 15 January 2016(9630)
REFLAIR and POPAIR PD chain check

I have been silently checking the signal chain of the REFLAIR and POPAIR RFPDs using the AM laser (a.k.a. PD calibrator) to make sure that they are functional expectedly.

Summary

The RF frequency of the AM modulation was adjusted in each measurement such that the demodulated IF signal was below 50 Hz.


Calibration of the amplitude modulation depth

We recalibrated the AM laser.

The current setting of the laser was changed recently because we opened up the current driver when we thought the laser diode had been dead in the early December. Then the laser head and its current driver were sent to Rich at Caltech for his extensive testing although the laser magically fixed itself and he didn't find anything wrong. So this was the first time for us to use the AM laser which had been fixed. Because of that mysterious event, I wanted to recalibrate the laser. First of all, Yuta and I measured the power to be 2 mW with an Ophir Vega without the attenuation filter. Then we measured the modulation depth for the amplitude modulation by using a Newfocus 1611 as a reference.

The new calibration for the amplitude modulation is:

P_am =  5.13 mW x (P_dc / 1 mW) * (1 V / V_drive)

where P_dc is the laser power at DC and V_drive is the drive voltage when it is driven by a 50 Ohm source. For example, if one puts this laser to a PD which then shows a DC laser power of say 2 mW, the AM coefficient is now 5.13 mW x ( 2 mW / 1 mW) /V_drive = 10.26 mW/V_drive.


REFLAIR_A_RF9 (S1203919)

Remarks:

The signal chain is OK. The PD response is smaller by 15% for some reason.

It seems as if the transimpedance is smaller by 15% than what had been measured at Caltech (LIGO-S1203919). The cable loss from the RFPD to the rack was measured to be 0.47 dB. Be aware that the demod gain is half of the quad I/Q demodulator because this is a dual channel demod (see E1100044). The demod conversion gain is assumed to be 10.9 according to LIGO-F1100004-v4.


REFLAIR_A_RF45 (S1203919)

Remarks:

The signal chain is healthy.

Found cable loss of about 1.5 dB. The measurements excellently agree with the loss-included expectation.


POPAIR_A_RF9 (S1300521)

Remarks:

The signal chain is healthy.

The measurement suggests that there is loss of 1 dB somewhere. I didn't measure the cable loss this time.


POPAIR_A_RF45 (S1300521)

Remarks:

The signal chain is OK. Though loss sounds a bit too high.

The measurement suggests a possible loss of 2.6 dB somewhere. I didn't measure the cable loss.


REFLAIR_B_RF27 (S1200234)

Remarks:

The signal gain is bigger than the expectation by a factor of 2.3.


REFLAIR_B_RF135 (S1200234)

Remarks:

The signal gain is bigger than the expectation by a factor of 1.5


POPAIR_B_RF18 (S1200236)

Remarks:

The signal gain is bigger than the expectation by a factor of 2.3


POPAIR_B_RF90 (S1200236)

Remarks:

The signal gain matches with the expected value, but I don't believe this.

Comments related to this report
kiwamu.izumi@LIGO.ORG - 17:16, Thursday 30 January 2014 (9678)

There was a typo:

P_am =  5.13 mW x (P_dc / 1 mW) * (1 V / V_drive)

P_am = 5.13 mW x (P_dc / 1 mW) x (V_drive / 1 V)

koji.arai@LIGO.ORG - 18:38, Thursday 30 January 2014 (9686)

For 27MHz and 136.5MHz, the RF gains are +19.8dB and +50.7dB, respectively. S1400079

 

daniel.sigg@LIGO.ORG - 22:46, Thursday 30 January 2014 (9696)

The response of the BBPD isn't really flat over all frequencies. See D1002969.

koji.arai@LIGO.ORG - 12:59, Friday 31 January 2014 (9719)

The description in D1002969 is for the initial version. (The schematics seems up-to-date.)

The latest version has the rf performance as attached.

Non-image files attached to this comment
kiwamu.izumi@LIGO.ORG - 13:11, Wednesday 05 February 2014 (9845)

This is a follow up of the calibration measurements for REFLAIR_B and POPAIR_B.

I have updated the expected signal gain for these photo detector chains using more realistic gains which Koji gave (see his comments above). Now all the values make sense. Note I did not perform any new measurements.

In the following calculations, the quantity in red represent the updated parameters.

 


REFLAIR_B_RF27(S1200234)

Remarks:

The signal chain is healthy. There is loss of 0.92 dB somewhere.

  • Expected AM at 27 MHz = 5.13 mW x (1.045 mW / 1 mW) x 0.05 V_drivepp x 0.4 A/W x 2.1 kOhm = 225 mVpp
  • Expected ADC counts = 19.8dB (S1400079-v1) x 225 mVpp x 10.9 x 2^16/40 counts/V = 39294 counts pp
  • Measured ADC counts = 35431 counts pp
    • The signal is smaller by 0.92 dB than the expected.

REFLAIR_B_RF135(S1200234)

Remarks:

The signal chain is OK. There is loss of 3.9 dB somewhere.

  • Expected AM at 135 MHz = 5.13 mW x (1.045 mW / 1 mW) x 0.0014 V_drivepp x 0.4 A/W x 1 kOhm = 3 mVpp
  • Expected ADC counts = 50.7 dB (S1400079-v1) x 3 mVpp x 10.9 x 2^16/40 counts/V = 18377 counts pp
  • Measured ADC counts = 11689 counts pp
    • The signal is smaller by 3.9 dB than the expected.

POPAIR_B_RF18 (S1200236)

Remarks:

The signal chain is healthy. The signal was bigger by 9% than the expected.

  • Expected AM at 18 MHz = 5.13 mW x (0.93 mW / 1 mW) x 0.1 V_drivepp x 0.4 A/W x 2.1 kOhm = 401 mVpp
  • Expected ADC counts = 401 mVpp x 10.9 x 2^16/40 counts /V = 7157 counts pp
  • Measured ADC counts = 7803 counts pp
    • The signal is greater by 9 % than the expected.

POPAIR_B_RF90 (S1200236)

Remarks:

The signal chain is healthy. There is loss of 1.2 dB somewhere.

  • Expected AM at 90 MHz = 5.13 mW x (0.93 mW / 1 mW) x 0.1 V_drivepp x 0.4 A/W x 1.2 kOhm = 229 mVpp
  • Expected ADC counts = 229 mVpp x 10.9 x 2^16/40 counts/V = 4090 counts pp
  • Measured ADC counts = 3549 counts pp
    • This is smaller than the expected by 1.2 dB
evan.hall@LIGO.ORG - 14:08, Wednesday 06 January 2016 (24728)

From these measurements, we can use POPAIR to infer the calibration for POP.

I looked at a recent lock acquisition while the interferometer was trying to engage the outer ISS loop. The LSC is relatively stable during this time, and the POP beam diverter is still open.

After undoing whitening gain and digital gain (2 ct/ct for POPAIR9/45, and 32 ct/ct for POP9/45), we find the following TFs:

  • POP9I/POPAIR9I = 0.19 ct/ct
  • POP45Q/POPAIR45Q = 0.21 ct/ct

This implies calibrations of 1.7×106 ct/W for POP9 and 1.8×106 ct/W for POP45.

Images attached to this comment
evan.hall@LIGO.ORG - 00:30, Friday 15 January 2016 (24959)

There's a factor of 4 difference in power between POP and POPAIR (17 mW versus 68 mW with a PSL power of 23 W), so the values I gave above are off by a factor of 4. The demod gains should be 6.4×106 ct/W for POP9 and 7.2×106 ct/W for POP45.

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