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Reports until 23:48, Sunday 20 November 2016
H1 SUS (SUS)
cheryl.vorvick@LIGO.ORG - posted 23:48, Sunday 20 November 2016 - last comment - 16:03, Monday 21 November 2016(31675)
ITMY appears to be swinging in pitch at 0.55Hz thoughout H1 locks

Maybe this is known, but I didn't find an alog showing this feature of ITMY.

Plot 1: ITMY

OSEMs LF and RT have a peak at 0.55Hz throughout the long lock yesterday, T0 = 11/19, 16:00UTC, 750 averages

The peak in the LF and RT OSEMs seems to suggest the optic is swinging at 0.55Hz in pitch all the time, and that that swinging gets kicked up at lock loss.

Plot 2: ITMY, ITMX, ETMY, ETMX, OSEMs LF and RT, all optics

The peak at 0.55Hz in OSEMs LF and RT is unique to ITMY.

Images attached to this report
Comments related to this report
jeffrey.kissel@LIGO.ORG - 09:21, Monday 21 November 2016 (31680)OpsInfo
It's not really helpful, because we don't yet have a solution, but here's the aLOG where this problem has been explored: LHO aLOG 31404. I have no suggestions as of yet on how to fix it, other than re-designing the loops to add more gain (read: *any* gain) at this frequency.

Hugh is studying how far back in time this problem has persisted (it's been a problem since at *least* Oct 28), in hopes to find some sort of coincident hardware/electronics activity to blame. But so far, no dice.
sheila.dwyer@LIGO.ORG - 16:03, Monday 21 November 2016 (31701)OpsInfo

Jeff K, Sheila, Jenne, Evan

While we were having an EQ, we took a quick look at what is wrong with ITMY.  

Since Cheryl pointed out that this motion is seen in LF and RT, we became suspicous of a problem with top mass V and R damping.  Indeed, there was a "bounce" filter engaged in ITMY top mass V damping which must have been a mistake.  Once we turned this off the OLTF of the vertical damping looks verry similar between ITMX and ITMY.  With this filter on ITMY damping was garbage.  

I accepted the change in SDF. We also noticed while doing this that the top mass actuator state for ITMX was 1, while the rest of the quads were in state 2, so we switched that.  The large peak at 0.55 Hz that Cheryl aloged is gone now, and hopefully we won't have the problem with long long ringdowns on ITMY. 

Images attached to this comment
H1 CAL
kiwamu.izumi@LIGO.ORG - posted 18:52, Sunday 20 November 2016 - last comment - 15:27, Monday 21 November 2016(31671)
Preparation work for updating CALCS with ER10/O2 model

Jeff, Darkhan, Kiwamu,

This is a quick report; some more details will be reported tomorrow.

We started a preparation work to update the CAL CS front end model. We have created a new version of the matlab script that populates the actuator functions (21322). The new script can be found at

/ligo/svncommon/CalSVN/aligocalibration/trunk/Runs/ER10/H1/Scripts/CALCS/quack_eyresponse_into_calcs.m

We made some tunings to get the script running without making autoquack unhappy. We didn't update the actual foton filters for ETMY today although we made changes on the ITMY CALCS filters as tests. The attached is a first glance at the actuation functions in comparison to the O1 actuation functions. No surprise so far, except that the L3 stage had a different sign now. This will be followed up.

Images attached to this report
Comments related to this report
kiwamu.izumi@LIGO.ORG - 12:51, Monday 21 November 2016 (31687)

Here is a summary of the activities including yesterday's and today's.

We have ...

  • Adopted some matlab scripts as reported above and also below.
  • Made the actual changes on the foton file namely H1CALCS.txt
  • Loaded the new filters this morning at Nov. 21 18:24 UTC

This means that we have completed the update of the new suspension filters in CALCS.


[The new  CALCS actuator functions]

  • It now uses the latest suspension tag model that Jeff updated 10 days ago (31432).
    • The latest includes the oplev damping.
    • Also, as shown in the attached screenshot in the above entry, the latest have slight difference around 1 Hz and some difference above 100 Hz.

More explicitly, the suspensions are extracted from the tagged model,

/ligo/svncommon/CalSVN/aligocalibration/trunk/Common/externals/SUSdynamModelTags/quadmodelproduction-rev8274_ssmake4pv2eMB5f_fiber-rev3601_h1etmy-rev7915_released-2016-11-11.mat

which is specified in H1's parameter file at:

/ligo/svncommon/CalSVN/aligocalibration/trunk/Runs/ER10/H1/params/H1params.conf

The DC values for the suspensions came a bit different than what Darkhan reported (31677) by a subpercent level. The matlab code reported the following values.

Ku  = 8.1642e-08 N/ct

Kp  = 6.8412e-10 N/ct

Kt  = -4.3891e-12 N/ct

We will double check with Darkhan to see what actually affected these values even thought the discrepancies aren't significant.

 

[Adjustment for quacking the filters]

When running the matlab script

/ligo/svncommon/CalSVN/aligocalibration/trunk/Runs/ER10/H1/Scripts/CALCS/quack_eyresponse_into_calcs.m

to update the actuator functions in CALCS, we ran into some problems for which we spent almost a day. This is a summary of what we encountered and how we mitigated.

  • Issue 1: too many SOS sections in the TST stage
    • The TST stage ended up with too many SOS sections when using the latest tag model.
    • We relaxed the tolerance for minreal from 6e-5 to 1e-3 as a mitigation.
  • Issue 2: violins not compatible with biquad form
    • Depending on the cut off frequency for excluding fine structures, quackcheck often reported a 0-gain error.
    • It turned out that this happens when the SOS filter coefficients don't have a b0i. We could not come up with a good mitigation.
    • We decided to set the cut off frequencies individually so that we can let all of them survive. The good values we found were: UIM cutoff = 1600 Hz and PUM cutoff = 2000 Hz.
  • Issue 3: autoquack occasionally runs into a steady failure mode
    • Autoquack occasionally enters a situation where it keeps reporting BAD filter implementation for some reason.
    • We empirically found that we can get out of the situation by manually installing a simple and fake zpk filter once (e.g. zpk([], [], 19, "n") or similar ) at the filter module having the issue.
  • Issue 4: c2d and minreal return some bad filters
    • c2d and minreal occasionally returned filters that are bad for quack (such as the number of zeros exceeding the number of poles).
    • This, for some reason, can be mitigated by running the script again.

Otherwise, we didn't change the code and therefore it did the processes that are describd in detail at 21322.

 

[Accuracy of the actuation functions in CALCS]

The first attachment is a plot showing the discrepancy between the desired and installed filters. UIM is the one who has the largest discrepancy in 10-100 Hz about a few % in magnitude and a few degrees in phase. Nevertheless, this shouldn't pose an issue for the resulting accuracy of DETAL_EXTERNAL as the UIM affects very weakly above 1 Hz due to the actuation authority. The second attached is another comparison plot showing the desired (full ss) and installed (discrete) filters. Finally the third attachment shows the installed susnorm filters which are forced to be flat at high frequencies.

 

[Copying the digital filter settings for ETMY]

This was done by running the existing code,

/ligo/svncommon/CalSVN/aligocalibration/trunk/Runs/ER8/H1/Scripts/CALCS/copySus2Cal.py

Non-image files attached to this comment
kiwamu.izumi@LIGO.ORG - 15:27, Monday 21 November 2016 (31699)

Darkhan, Kiwamu,

Taking a further look at the K values, we came to the conclusion that the discrepancies are due to rounding error of the N/A values written in H1params.conf. As described above, this will not cause appreciable effects at the precision level we usually talk about (~1 % level). We left them as they are.

H1 General
jim.warner@LIGO.ORG - posted 16:04, Sunday 20 November 2016 - last comment - 23:39, Sunday 20 November 2016(31669)
Shift Summary

TITLE: 11/20 Day Shift: 16:00-24:00 UTC

STATE of H1: Observing

SHIFT SUMMARY:  Lost a 30 hour lock from an earthquake. Jeff, Kiwamu and Darkhan were here doing calibration stuff. Having problems relocking, can't get past noise-tunings. ITMY swing continues to annoy after lock losses.

20:00 Jeff and crew start calibration measurements

21:00 6.4 earthquake in Argentina breaks lock

21:30 Corey brings a tour through

22:00 Robert in and out of LVEA, setting up PEM injections

Comments related to this report
kiwamu.izumi@LIGO.ORG - 19:26, Sunday 20 November 2016 (31672)

Cheryl, Kiwamu,

Executing each line of NOISE_TUNINGS, we spotted typo in which MICH FF and SRCL FF1 were selecting a wrong set of digital filters. In particular, MICHFF was the worst -- it didn't use the AC coupling filter, resulting in a jolt to ITMs. We set them to the ones that had been used in the previous 30 hour lock stretch (31653). Cheryl will test this to see if the situation is better.

sheila.dwyer@LIGO.ORG - 23:39, Sunday 20 November 2016 (31674)
Sorry that was my mistake.
H1 CAL
jeffrey.kissel@LIGO.ORG - posted 12:14, Sunday 20 November 2016 (31665)
Process Sensing Functions from Calibration Sweeps To-Date: Optical Gain & Cavity Pole Frequency Consistent; Detuning Spring Frequency *is* Mobile
D. Tuyenbayev, J. Kissel

Darkhan and I have processed the measurements of the IFO's sensing function that we've made over the course of ER10 thus far. The measurements are compared against a model for the interferometer's optical plant, (a. la. T1600278, and G1601599)
      dS (f)     K exp(-2*pi*i*f*tau)               f^2
      ------  =  -------------------  * ---------------------------
      dL            1 + i*(f/f_cc)      f^2 + (f_s)^2 - i*(f*f_s/Q)
where 
      dS / dL = DARM_ERR error signal counts per differntial displacement of the test masses dL in [ct/m]
      K       = optical gain in [ct/m], though fundamental units are [A/m]
      f_cc    = DARM /RSE /coupled cavity pole frequency in [Hz]
      f_s     = detuned signal recycling cavity (SRC) "optical spring" frequency
      Q       = quality factor of said spring
      tau     = residual delay, after accounting for computational, light travel time, and FSR response delays

The resulting plots of model compared against measurement are attached. I also summarize the numerical values for the results in tabular form below for ease of comparison.

                                 [Units]  value(95% c.i.)

Meas Date                 2016            Nov 8         Nov 11        Nov 12        Nov 15        Nov 16        Nov 18  
IFO Input Power                  [W]      23.5          24.8          29.5          30.7          31.1          31.9
SRC1 Loop Status                          ON            ON            ON            OFF           ON            ON

Optical Gain              x 1e6  [ct/m]   1.15 (0.002)  1.15 (0.002)  1.15 (0.003)  1.12 (0.004)  1.14 (0.003)  1.12 (0.002)
DARM/RSE Cav. Pole Freq.         [Hz]     343.1(3.8)    351.1(3.1)    346.7(4.1)    342.0(5.9)    344.7(3.8)    348.4(5.1)
Detuned SRC Optical Spring Freq. [Hz]     5.5  (0.3)    4.9  (0.2)    7.4  (0.3)    7.8  (0.4)    8.1  (0.3)    8.5  (0.3)
Optical Spring Q-Factor (1/Q)    []       0.03 (0.01)   0.04 (0.01)   0.05 (0.01)   0.07 (0.01)   0.05 (0.01)   0.07 (0.01)
Residual Time Delay              [us]     -2.6 (3.4)    -1.7 (3.7)    2.3  (3.4)    2.8  (5.3)    0.6  (3.3)    5.1  (4.7)
 
aLOG                                      31303         31403         31433         31508         31527         31601


Conclusions: 
(1) We see a clear *decrease* in IFO optical gain between 25 [W] and 30 [W], but it may be a function of alignment not input power. We expect and *increase* as a function of power. This may be evidence for power/alignment dependent losses. It would interesting to compare these data sets to the spot-position measurements that we've been taking.
(2) The DARM /RSE /coupled cavity pole frequency (f_cc) is consistently 345.9(3.5) [Hz], regardless of input power or alignment.
(3) We continue to see the effects of a detuned SRC cavity, characterized/approximated by a pair of poles at spring frequency (f_s) and quality factor (Q), unlike LLO.
(3) The f_s shows statistically significant changes over the course of these measurements, unlike LLO. Difficult at best to tell if its correlated with any of the parameters we've tracked here, but it will be very interesting to use the 7.92 Hz PCAL line to confirm this in the future. This characteristic frequency will be another interesting thing to compare against spot positions.
(4) Though we only have one data point, having SRC1 loops OFF does not significantly change f_cc, and the trend in f_s seems unrelated. (However I still highly recommend that we run with them ON if at all possible)
(5) The residual time delay is consistent with zero. This is great -- it means we really have a handle on the high-frequency response of the IFO.

We'll take one more of these measurements to set the front-end calibration all within the same lock stretch, to make sure the time-dependent tracking for the relative optical gain and cavity pole frequency are as close to 1.0 and 346 [Hz] as possible.

Details:

CalSVN repo root: [~] = /ligo/svncommon/CalSVN/aligocalibration/

Analysis produced by running:
[~]/trunk/Runs/ER10/H1/Scripts/PCAL/fitDataToC_20161116.m          Revision: 3815
on each of the measurement config files listed below.

Model Config Files:
[~]/trunk/Runs/ER10/Common/params/IFOindepParams.conf              Revision: 3776
[~]/trunk/Runs/ER10/H1/params/H1params.conf                        Revision: 3811
[~]/trunk/Runs/ER10/H1/params/2016-11-12/H1params_2016-11-12.conf  Revision: 3800

Measurement Config Files:
[~]/trunk/Runs/ER10/H1/params/2016-11-07/measurements_2016-11-07_sensing.conf   Revision: 3800
[~]/trunk/Runs/ER10/H1/params/2016-11-10/measurements_2016-11-10_sensing.conf   Revision: 3800
[~]/trunk/Runs/ER10/H1/params/2016-11-12/measurements_2016-11-12_sensing.conf   Revision: 3800
[~]/trunk/Runs/ER10/H1/params/2016-11-15/measurements_2016-11-15_sensing.conf   Revision: 3800
[~]/trunk/Runs/ER10/H1/params/2016-11-16/measurements_2016-11-16_sensing.conf   Revision: 3800
[~]/trunk/Runs/ER10/H1/params/2016-11-17/measurements_2016-11-17_sensing.conf   Revision: 3800
Non-image files attached to this report
H1 CAL (DetChar)
jeffrey.kissel@LIGO.ORG - posted 09:10, Sunday 20 November 2016 (31664)
PCALX Roaming Calibration Line Frequency Changed from 4501.3 to 4801.3 Hz
J. Kissel for S. Karki

More high duty cycle gives Sudarshan way more data than he needs! We're coming to a close on having an entire sweep, but we'll likely start over at the low end so that all the data is at ~30 [W] under the same alignment configuration. From data he's processed thus far, there's a significant and confusing amount of scatter between model and measurement (aLOG pending).

Current Schedule Status:
Frequency    Planned Amplitude        Planned Duration      Actual Amplitude    Start Time                 Stop Time                    Achieved Duration
(Hz)         (ct)                     (hh:mm)                   (ct)               (UTC)                    (UTC)                         (hh:mm)
---------------------------------------------------------------------------------------------------------------------------------------------------------
1001.3       35k                      02:00                   39322.0           Nov 11 2016 21:37:50 UTC    Nov 12 2016 03:28:21 UTC      ~several hours @ 25 W
1501.3       35k                      02:00                   39322.0           Oct 24 2016 15:26:57 UTC    Oct 31 2016 15:44:29 UTC      ~week @ 25 W
2001.3       35k                      02:00                   39322.0           Oct 17 2016 21:22:03 UTC    Oct 24 2016 15:26:57 UTC      several days (at both 50W and 25 W)
2501.3       35k                      05:00                   39322.0           Oct 12 2016 03:20:41 UTC    Oct 17 2016 21:22:03 UTC      days     @ 50 W
3001.3       35k                      05:00                   39322.0           Oct 06 2016 18:39:26 UTC    Oct 12 2016 03:20:41 UTC      days     @ 50 W
3501.3       35k                      05:00                   39322.0           Jul 06 2016 18:56:13 UTC    Oct 06 2016 18:39:26 UTC      months   @ 50 W
4001.3       40k                      10:00                   39322.0           Nov 12 2016 03:28:21 UTC    Nov 16 2016 22:17:29 UTC      days     @ 30 W (see LHO aLOG 31546 for caveats)
4301.3       40k                      10:00                   39322.0           Nov 16 2016 22:17:29 UTC    Nov 18 2016 17:08:49 UTC      days     @ 30 W          
4501.3       40k                      10:00                   39322.0           Nov 18 2016 17:08:49 UTC    Nov 20 2016 16:54:32 UTC      days     @ 30 W (see LHO aLOG 31610 for caveats)   
4801.3       40k                      10:00                   39222.0           Nov 20 2016 16:54:32 UTC                                  
5001.3       40k                      10:00
Images attached to this report
H1 General
nutsinee.kijbunchoo@LIGO.ORG - posted 08:16, Sunday 20 November 2016 (31662)
Ops Owl Shift Summary

TITLE: 11/20 Owl Shift: 08:00-16:00 UTC (00:00-08:00 PST), all times posted in UTC

STATE of H1: Observing

INCOMING OPERATOR: Jim

SHIFT SUMMARY: Locked for 25 hours and counting. Dust monitor alarm has been going off.

LOG:

13:24 Noticed low freq noise floor raised between 10-20Hz. Out of Observing to run a2l.

13:29 Back to Observe.

 

Commissioners: Do we still want to run a2l very hour? No one's been doing it during the past two shifts so I wasn't sure.

Images attached to this report
LHO VE
kyle.ryan@LIGO.ORG - posted 08:01, Sunday 20 November 2016 - last comment - 19:44, Sunday 20 November 2016(31661)
Annulus ion pump out of range
Can't id exact unit remotely or from memory but think this is on the Diagonal Volume.  I think that all AIPs on the diagonal are low hour so hopefully this will be an easy electronics swap? 

Comments related to this report
john.worden@LIGO.ORG - 09:31, Sunday 20 November 2016 (31663)

This one is labeled IBM AIP 192 (also LY-IBM)  - perhaps the 2K input MC tube?? Did we mislabel these?

The other red one is HAM12 on the 2K volume.

Images attached to this comment
chandra.romel@LIGO.ORG - 19:44, Sunday 20 November 2016 (31673)

The one labeled IBM is on 2K volume, but there is no pump connected to annulus volume right now, which is why it's been red on vacuum GUI. That volume was pumped down and capped off at a valve. HAM 12 on vacuum GUI is actually HAM 11 (same with HAM7/8). We should fix wiring so they read right.

H1 General
nutsinee.kijbunchoo@LIGO.ORG - posted 05:14, Sunday 20 November 2016 (31660)
Ops OWL mid-shift summary

Still locked! 22 hours and counting.

H1 General
nutsinee.kijbunchoo@LIGO.ORG - posted 01:05, Sunday 20 November 2016 (31659)
Owl Shift Transition

TITLE: 11/20 Owl Shift: 08:00-16:00 UTC (00:00-08:00 PST), all times posted in UTC

STATE of H1: Observing

OUTGOING OPERATOR: Cheryl

QUICK SUMMARY: Been locked for 17 hours and counting.

H1 General
cheryl.vorvick@LIGO.ORG - posted 00:01, Sunday 20 November 2016 (31658)
Ops Eve Summary:

State of H1: locked 16+ hours

Commissioners: Sheila

Activities:

Note from Sheila:

Gains:

H1 General
cheryl.vorvick@LIGO.ORG - posted 21:38, Saturday 19 November 2016 (31657)
EY saturation, out of Observe to damp it's violin modes

At handoff from Jim he mentioned he'd had to damp ETMY's violins in a long lock recently, so when I got an E_Y saturation I trended it's violin modes 1 and 7 which had been climbing steadily.  I looked at the peak in DARM, and it was big, so I went out of Observe to damp the modes. 

Images attached to this report
H1 General
cheryl.vorvick@LIGO.ORG - posted 19:03, Saturday 19 November 2016 (31654)
H1 in Observe

3:01UTC

H1 CDS (CDS, DetChar)
sheila.dwyer@LIGO.ORG - posted 17:57, Saturday 19 November 2016 - last comment - 12:28, Wednesday 23 November 2016(31651)
RF incident?

It looks like we had another incident of the POP90 power changing, (circled in the striptool screenshot) similar to what Stefan described in 31181.  Is this still a problem with the demod as RIchard found the first time?  If its only an intermittent problem with the POPAIR 90 demod, we probably don't need to worry about fixing it before O2 because that is jiust a monitor and won't be used if we are able to close the beam diverters for the run.  

Detchar question: 

Did we have RF45 glitches around these times?  The times are roughly 16:26, 16:30, 16:36 and 16:42 Nov 19th local time, which is 0:26, 0:30, ect Nov 20th UTC time.  

Images attached to this report
Comments related to this report
richard.mccarthy@LIGO.ORG - 11:46, Sunday 20 November 2016 (31666)
We were able to fix some obvious problems with this but the problem with the shield was not changed as we did not test it after the fact.  Though this problem should only appear if someone was in the rack.  
Would be interesting to see if anything is on 9,or 45MHz
laura.nuttall@LIGO.ORG - 11:18, Monday 21 November 2016 (31686)

I took at look at the auiliary channels we used to create DQ flags monitoring RF45 noise in O1, namely H1:LSC-MOD_RF45_AM_CTRL_OUT_DQ and H1:ASC-AS_B_RF36_I_YAW_OUT_DQ. I created BLRMS of these channels in the same way we did in O1 to threshold on. In all of these plots we see a steady BLRMS over 21 hours from 20th Nov 00:00 - 21:00 UTC, indicating that these channels do not see any form of RF45 noise we are used to:

* Plot 1 - BLRMS of H1:LSC-MOD_RF45_AM_CTRL_OUT_DQ between 10-100Hz in 60 seconds strides
* Plot 2 - BLRMS of H1:LSC-MOD_RF45_AM_CTRL_OUT_DQ between 10-100Hz in 1 second strides
* Plot 3 - BLRMS of H1:ASC-AS_B_RF36_I_YAW_OUT_DQ between 30-170Hz in 1 second strides

Hveto for this day indicated that H1:ASC-AS_A_RF45_Q_PIT_OUT_DQ was a good channel to veto noise with on Sunday. I therefore did a BLRMS of this channel:

* Plot 4 - BLRMS of H1:ASC-AS_A_RF45_Q_PIT_OUT_DQ between 5-100 Hz in 1 second strides

This channel does show excess noise at certain times of the day. If we were to threshold on this BLRMS using the 99.5% BLRMS value during this time period, we would capture the times Sheila mentions and also veto 8/10 top ten pycbc live triggers for this day. 

Not conclusive that this noise is RF45 noise similar to what we saw in O1, investigating further...

Images attached to this comment
evan.hall@LIGO.ORG - 12:28, Wednesday 23 November 2016 (31786)

Seemingly another incident: circa 2016-11-23 20:25:30 Z.

H1 CAL (CSWG, DetChar, ISC, SUS)
jeffrey.kissel@LIGO.ORG - posted 15:11, Friday 18 November 2016 - last comment - 16:22, Wednesday 05 July 2017(31603)
H1 SUS ETMY High-Frequency Actuation UIM/L1
J. Kissel, D. Tuyenbayev

Analyzing the high-frequency data for the UIM that we took last night (LHO aLOG 31601), we find -- as previously suspected -- there is lots of dynamical resonant features in the UIM / L1 actuation stage; it definitely does NOT fall as f^6 to infinity as one might naively suspect. 

There are even more features than the (now anticipated; LHO aLOG 31432) broad impacts of the violin modes of the Sus Point-to-TOP wires (~311 Hz), and UIM-to-PUM wires (~420 Hz). We had seen hints of these features previously (LHO aLOG 24917), but here they are fully characterized out to 500 Hz with a combination of swept-sine (SS) and broad-band (BB) transfer function ratios (the calibration standard measurements of PCAL2DARM = C / (1+G) and iEXC2DARM = C A_i / (1+G)). The measurements yield the actuation strength of the UIM stage, in terms [m] of test mass displacement per [ct] of drive from the L1_TEST_L bank, which is the Euler-basis equivalent to DAC [ct]. To scale to [m/N], is a mere scale factor, measured to be 
     20/2^18 [V/ct] 0.62e-3 [A/V]* 1.7082 [N/A] = 8.08e-8 [N/ct] (see LHO aLOG 31344).


Via private communication in January this year, Norna suspects that 111 Hz feature is the first internal mode of the UIM blades, backed by a bench test of the blades at CIT which revealed a resonance at 109 Hz. No ideas on the 167 Hz mode though.

These high frequency dynamics continue to plague the estimate of the UIM actuation strength at DC using the traditional frequency-dependent sweep method, because these high frequency dynamics begin to affect the actuation strength at as low a frequency as ~30 Hz (LHO aLOG 31427), and any model fitting code gets totally distracted by these features. 

A challenge to the CSWG team: fit this transfer function above 20 Hz and create a set of zeros and poles that can be used as a "correction" filter to a model that falls off as f^6. This filter need not perfectly resolve the details of all of the high-Q features, but it must track the overall frequency dependence over the 20 - 500 Hz region well. I attach all of the measurements compressed onto one (discontinuous) frequency vector as an ascii in the standard DTT form of [freq re(TF) im(TF)]. To use: 
    >> foo = load('2016-11-17_H1SUSETMY_L1_Actuation_HighFreqChar_asciidump.txt')
    >> figure; loglog(foo(:,1), abs( foo(:,2)+1i*foo(:,3) ))
This data is also committed to the CalSVN repo here:
    /ligo/svncommon/CalSVN/aligocalibration/trunk/Runs/ER10/H1/Results/Actuation/2016-11-17_H1SUSETMY_L1_Actuation_HighFreqChar_asciidump.txt
Kiwamu has already tried to create such a filter from the previous data (LHO aLOG 28206), but was limited by  that measurement's high-frequency bound falling between the 111, 137, and 167 Hz features. 

Details:

Analysis code:
    /ligo/svncommon/CalSVN/aligocalibration/trunk/Runs/ER10/H1/Scripts/FullIFOActuatorTFs/process_H1SUSETMY_L1_HFDynamicsTest_20161117.m

Config files:
    IFOindepPars = '../../../Common/params/IFOindepParams.conf';
    IFOdepPars   = {'../../params/H1params.conf'};
    IFOmeasPars  = {'../../params/2016-11-12/H1params_2016-11-12.conf'};
    PCALPars = {'../../params/2016-11-12/measurements_2016-11-12_ETMY_L1_actuator.conf'};

Model:
    /ligo/svncommon/CalSVN/aligocalibration/trunk/Runs/O2/DARMmodel/src/computeDARM.m

Will post the data for the fitting challenge later this afternoon.
Images attached to this report
Non-image files attached to this report
Comments related to this report
brett.shapiro@LIGO.ORG - 19:42, Saturday 19 November 2016 (31656)DetChar, ISC, SUS

I made an update to the quad matlab model to account for these mystery features. See CSWG log 11197.

dennis.coyne@LIGO.ORG - 23:13, Wednesday 08 March 2017 (34688)

I describe my use of the Frequency Domain System Identification toolbox (FDIDENT) to fit this transfer function in CSWG elog #11205. FDIDENT is a third party Matlab toolbox which provides tools for identifying linear dynamic single-input/single-output (SISO) systems from time response or frequency response measurements. The toolbox is free for non-profit use.

https://www.mathworks.com/products/connections/product_detail/product_35570.html

http://home.mit.bme.hu/~kollar/fdident/

A stable, but non-minimum phase, model without delay – compatible with a Linear Time Invariant (LTI) representation -- results in a best fit for a 22 order numerator and 28 order denominator model, m2228. The model is compared to the measurement data in the attached bode plot.

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jeffrey.kissel@LIGO.ORG - 16:22, Wednesday 05 July 2017 (37338)
I attach several new parts of this high frequency characterization in order to facilitate incorporating the uncertainty in any future transfer function fitting. 

I attach three new text files:
    "..._tf.txt" -- a copy of the originally attached text file, columns are 
        [freq re(A) im(A)]
    "..._coh.txt" -- an export of the (prefiltered) coherence, columns are 
        [freq iEXCCoh PCALCoh]
    "..._relunc.txt" -- an export of the combined relative uncertainty on the transfer function, columns are 
        [freq sigma_A]

Computing the uncertainty on this actuation strength was a bit of a challenge. 
Remember, the above measure of the actuation strength of the UIM stage, A, is a combination of two transfer functions, as described in P1500248, Section V. In this aLOG they're referred to as "PCAL2DARM" where we use the photon calibrator as a reference actuator, and "iEXC2DARM" where the suspension stage under test is used as the actuator. Typically, the iEXC2DARM transfer function has the lowest coherence. 
Even worse, I've combined many data sets of both transfer functions covering different frequency regions each with a different number of averages.
Thus form the uncertainty, I've taken each frequency region's data set, and 
    - Filtered both iEXC and PCAL transfer functions for data points in which the iEXC TF has coherence greater than 0.95,
    - Created a relative uncertainty vector for each iEXC and PCAL transfer functions using the standard B&P equation,
        sigma_TF(f) / TF = sqrt( (1-C(f)) / (2 N C(f)) )
    where C(f) is the coherence, and N is the number of averages (N was 10 for swept sine TFs, 25 for broad band TFs)
    - Concatenated the data sets to form the overall transfer function, A,
    - Combined the two uncertainty vectors in the standard way,
        sigma_A / A = sqrt((sigma_iEXC / iEXC)^2 + (sigma_PCAL / PCAL)^2)
    - Sorted the collection of 
        [frequency complextf iexccoh pcalcoh sigma_A]
    by frequency.
    - Exported the uncertainty.

Note that one only needs one column of uncertainty, for the absolute uncertainty in magnitude is just
    |sigma_A| = abs(A) * (sigma_A / A)
and the absolute uncertainty in phase is
    /_ sigma  = 180/pi * (sigma_A / A)

I attach a plot of the magnitude and its uncertainty for demonstrative purposes, so that when the files are used, you can compare your plots of this against mine to be sure you're using the data right. Note that I've multiplied the uncertainty by a factor of 10 for plotting only so that it's visible.

I've updated and committed the function that's used to process this data, and it can be found here:
    /ligo/svncommon/CalSVN/aligocalibration/trunk/Runs/ER10/H1/Scripts/FullIFOActuatorTFs/
    process_H1SUSETMY_L1_HFDynamicsTest_20161117.m
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H1 CAL (CAL)
jeffrey.kissel@LIGO.ORG - posted 11:06, Friday 18 November 2016 - last comment - 03:46, Monday 21 November 2016(31601)
Fourth Round of ER10 Calibration Measurements Complete -- Second at 30 W
J. Kissel, D. Tuyenbayev

Darkhan and I was able to get another round of calibration sweeps in last night, just after Sheila finished up her alignment test (LHO aLOG 31599). This set is at 31.92 W, with SRC1 Loops Closed -- and the second set of data with the anticipated O2 configuration.

Datasets live here: 
Sensing Function:
/ligo/svncommon/CalSVN/aligocalibration/trunk/Runs/ER10/H1/Measurements/DARMOLGTFs
2016-11-17_H1_DARM_OLGTF_4to1200Hz_fasttemplate.xml
/ligo/svncommon/CalSVN/aligocalibration/trunk/Runs/ER10/H1/Measurements/PCAL
2016-11-17_H1_PCAL2DARMTF_4to1200Hz_fasttemplate.xml

Actuation Functions
2016-11-17_H1SUSETMY_L1_iEXC2DARM.xml
2016-11-17_H1SUSETMY_L1_PCAL2DARM.xml
2016-11-17_H1SUSETMY_L2_iEXC2DARM.xml
2016-11-17_H1SUSETMY_L2_PCAL2DARM.xml
2016-11-17_H1SUSETMY_L3_iEXC2DARM.xml
2016-11-17_H1SUSETMY_L3_PCAL2DARM.xml


I'd found that I'd stored the wrong channels in my new templates for the exploration of the UIM/L1 high frequency actuation on 2016-11-12 (LHO aLOG 31433), so I repeated those measurements as well storing the right channels this time:
2016-11-17_H1SUSETMY_L1_iEXC2DARM_HFDynamicsTest_100-250Hz.xml
2016-11-17_H1SUSETMY_L1_iEXC2DARM_HFDynamicsTest_250-350Hz.xml
2016-11-17_H1SUSETMY_L1_iEXC2DARM_HFDynamicsTest_300-500Hz.xml
2016-11-17_H1SUSETMY_L1_iEXC2DARM_HFDynamicsTest_90-400Hz_SweptSine.xml
2016-11-17_H1SUSETMY_L1_PCAL2DARM_HFDynamicsTest_100-250Hz.xml
2016-11-17_H1SUSETMY_L1_PCAL2DARM_HFDynamicsTest_250-350Hz.xml
2016-11-17_H1SUSETMY_L1_PCAL2DARM_HFDynamicsTest_300-500Hz.xml
2016-11-17_H1SUSETMY_L1_PCAL2DARM_HFDynamicsTest_90-400Hz_SweptSine.xml

Analysis will be posted today (it's finished, we now just need to document it all), and we plan on updating the DARM model and front-end calibration by Monday.
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jeffrey.kissel@LIGO.ORG - 12:50, Friday 18 November 2016 (31609)CAL, CSWG, DetChar, SUS
The high-frequency dynamics measurements quoted in this aLOG have been analyzed. See results in LHO aLOG 31603.
darkhan.tuyenbayev@LIGO.ORG - 18:14, Saturday 19 November 2016 (31649)CAL

J. Kissel, K. Izumi, D. Tuyenbayev,

Overview

Actuation strengths [N/ct] for all three stages have been calculated with MCMC method. In In this analysis we used data from last set of measurements taken on Nov 17 (see above), together with measurements from Nov 7, 8, 10 and 12 (see LHO alogs 31303, 31371, 31403, 31433). The calculated actuation coefficients are:

KU = 8.1648-8 N/ct

KP = 6.844-10 N/ct

KT = 4.395-12 N/ct

The H1DARM model parameters were updated using these values, particularty:

UIM_NpA = 1.739; [N/A]
PUM_NpA = 0.0334; [N/A]
TST_NpV2_y = 1.612e-10; [N/V^2]

We will double check the overall DARM loop model, with the updated sensing and actuation, by comparing it to DARM loop TF measurements.

Notice that TST actuation coef came out as a negative quantity, we believe that there is a "-1" missing in the model of this stage.

Details

For this analysis we took each actuation stage to DARM TF and PCALY to DARM TF measurements at the same frequency vector and used only data points with coherences above 0.9, we adopted a Matlab script used at LLO for this part of the analysis (see EvanG's LLO alog 29438). For each actuation stage i, the test point excitation to DARM TF is

iEXC2DARM = Ai,meas * C / (1 + G)

and PCALY to DARM is

PCALY2DARM = C / (1 + G)

The ratio of the two gives:

iEXC2DARM / PCALY2DARM = Ai,meas

Then we divided this my the model of the given stage without the N/ct coefficient, Ai,model / Ki,model = Fi,model, gives measurement of the frequency-independent N/ct coefficient:

Ai,meas / Fi,model = Ki,meas

Then, we used GWMCMC library (https://github.com/grinsted/gwmcmc) for fitting amplitude and phase of the N/ct coefficient for each stage (if the frequency dependent part of the model is correct, then the phase should be 0 deg). The log likelihood function used for fitting is

logLike = log( ∏( 1 / sqrt(2πσi2) exp( - (Ki,meas - Kfit)2/(2σi2) ) )

Fit results for magnitudes are given above and the phases are at the order of 10-3 deg.

The KU, KP and KT coefficients calculated from multiple-frequency transfer function measurements differ from earlier estimations from single line (LHO alog 31344) by 1.7%, 5.3% and 3.1% for UIM, PUM and TST stages. Possibly some unaccounted systematics in the frequency reponses of the DARM model near 35 Hz (the previous analysis was done with the DARM model for ER9).

Non-image files attached to this comment
darkhan.tuyenbayev@LIGO.ORG - 17:47, Sunday 20 November 2016 (31668)CAL

Izumi K, Kissel J, Tuyenbayev D,

We used ER10 model to re-run an earlier actuation strength analysis using calibrartion line data from Nov 3 - Nov 8 (LHO alog 31344). The original analysis was done with the DARM model in which the positive N/ct sign was used for TST stage actuation, the correct KT sign must have been negative. Below we list the updated results from this single-line analysis, the values are taken from GPS time interval [1162369920 1162413500]:

KU = 8.613 × 10-8 ± 3.204 × 10-10 N/ct
KP = 6.802 × 10-10 ± 2.254 × 10-12 N/ct
KT = -4.341 × 10-12 ± 1.339 × 10-14 N/ct

Notice this analysis is used as an additional check of the multiple-frequency analysis (see above). The DARM model parameters for ER10/O2 will be based on the multiple-frequency analysis results (refined numbers and comparison results are coming soon).

Non-image files attached to this comment
darkhan.tuyenbayev@LIGO.ORG - 03:46, Monday 21 November 2016 (31677)CAL

Izumi K, Kissel J, Tuyenbayev D,

Overview

We calculated the actuation coefficients for the H1 DARM reference time model. For UIM (L1) and PUM (L2) stages the N/ct coefficients were fit based on actuation TF measurements on Nov 7, 8, 10, 12 and 15. These numbers have been reported earlier (see above). The TST actuation strength will have a trend over long time period due to charge accumulation, thus for TST stage it is better to estimate the coefficient based on measurements taken within a short period of time. Since we set the reference sensing function parameters based on measurements taken on Nov 12, for estimation of the TST (L3) stage actuation we decided to use measurements around that date, particularly measurements from Nov 10 and 12.

Contributions from each of the actuation stages to the overall DARM response drops as 1/f6, 1/f4 and 1/f2, for this reason MCMC (and LSQ) fitting were restricted to [0 10] Hz, [0 200] Hz and [0, 200] Hz for UIM, PUM and TST stages respectively.

Below are the resulting N/ct values, these values:

KU = 8.1648 × 10-8 N/ct (±  0.074% 1-σ)
KP = 6.844 × 10-10 N/ct (± 0.018% 1-σ)
KT = -4.389 × 10-12 N/ct (± 0.031% 1-σ)

And the H1DARM model were updated in the following way (only the N/V2 for TST stage is different from LHO alog 31649):

UIM_NpA = 1.739;         % [N/A]
PUM_NpA = 0.0334;        % [N/A]
TST_NpV2_y = 1.6097e-10; % [N/V^2]

New EPICS values used for DARM time-dependent parameters have been calculated with the updated H1 DARM model for ER10/O2 (see attachment 1).

Comparisons

MCMC and LSQ methods gave consistent results, fractional discrepancies between the two were at the order of 10-5 (LSQ fit was done only for magnitude).

Discrepancies between the new values and the ones currently installed in the CAL-CS front-end model are:

UIM: 0.05% (compared 8.1689 × 10-8 N/ct, the currently installed, old value)
PUM: 0.05% (compared to 6.8407 × 10-10 N/ct)
TST: 3.42% (compared to 4.239 × 10-12 N/ct)

Discrepancies between these values and an updated single-line analysis results (see LHO alog 31668 above) are 5.5% (UIM), 0.6% (PUM) and 1.4% (TST). A larger discrepancy between MCMC and the single-line analysis for UIM, we believe, is mostly due to 5-10% systematic errors in the UIM suspension model at ~36 Hz (see a residual plot attached to Kiwamu's LHO alog 31427).*

Although, the TST stage coefficient was calculated based on Nov 10th and 12th measurements, discrepancies between the values estimated for each of the 5 measurements (Nov 7 - 17), are within 0.5% (see attachment 2).

*Check out Jeff's LHO alog 31603 for more UIM HF investigations.

Details

TST stage fitting plots are attached below (see attachments 3 and 4). UIM and PUM fitting results did not change (see previous report above, LHO alog 31609).

The new EPICS values for DARM time-dependent parameters are committed to

${CalSVN}/Runs/ER10/H1/Scripts/CAL_EPICS/D20161120_H1_CAL_EPICS_VALUES.m

The up-to-date H1 DARM model parameters are commited to CalSVN:

${CalSVN}/Runs/ER10/Common/params/IFOindepParams.conf              r3752
${CalSVN}/Runs/ER10/H1/params/H1params.conf                        r3826
${CalSVN}/Runs/ER10/H1/params/2016-11-12/H1params_2016-11-12.conf  r3786

DARM model scripts (SRC detuning TF was modified to include Q-factor at r3814):

${CalSVN}/Runs/O2/DARMmodel/*  r3814

Actuation coefficient fitting script was uploaded to

${CalSVN}/Runs/ER10/H1/Scripts/FullIFOActuatorTFs/fitActCoefs_Npct.m  r3829

And the results are at

${CalSVN}/Runs/ER10/H1/Results/Actuation/2016-11-20_H1_SUSETMY_*.pdf

Non-image files attached to this comment
H1 CAL
jeffrey.kissel@LIGO.ORG - posted 13:59, Monday 07 November 2016 - last comment - 16:53, Sunday 20 November 2016(31289)
ETMY UIM and PUM CAL Lines Turn OFF
J. Kissel, D. Tuyenbayev

Following preliminary results from Darkhan on the individual actuation strength of the UIM and PUM stages for H1SUSETMY (see, thus far LHO aLOG 31275), and the current delightfully long lock stretch with them in place, I'm bringing this study to a close. I've turned off the temporary L1 and L2 calibration lines at 33.7 and 34.7 Hz, respectively. We do not intend on turning on these lines again for the duration of the run.

These lines were turned OFF at Nov 07 2016 21:21:49 UTC.
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darkhan.tuyenbayev@LIGO.ORG - 20:10, Tuesday 08 November 2016 (31344)CAL

Summary

A refined analysis of the L1, L2 and L3 stange actuation strenghts was done using the data from last several days that include several low-noise lock stretches. Actuation strength factors are:

KU = 8.020-8 +/- 2.983-10 N/ct   ( std(KU) / |KU| = 0.0037 )

KP = 6.482-10 +/- 2.748-12 N/ct   ( std(KP) / |KP| = 0.0033 )

KT = 4.260-12 +/- 1.313-14 N/ct   ( std(KT) / |KT| = 0.0031 )

Details

Following 4 lines were used to calculate the factors: UIM (L1) line at 33.7 Hz, PUM (L2) line at 34.7 Hz, TST (L3) line at 35.9 Hz and PcalY line at 36.7 Hz. The most recent DARM model parameters were used for this analysis. Also, values past Nov 5 were calculated with the updated DARM filters (see LHO alog 31201), not accounting for this would produce results biased by 1-2%.

Each data point is a quantity calculated from 10s FFTs. The outliers were removed in two steps:
- took the mean and the standard deviation of all data points in intervals when the IFO range was >=50 MPC, removed 3-sigma outliers;
- removed the 3-sigma outliers from the mean of the remaining data points.

The mean values and the standard devitaions noted above were taken from GPS time interval [1162369920 1162413500], ~11 hours of low-noise data (blue markers). Standard errors on the mean values, std(Ki) / sqrt(N), are orders of magnitude smaller compared to the Pcal and the DARM loop model uncertainties (number of data points in the seletected interval - N=4251).

For preliminary results from Nov 4 data and before see related reports: 31183, 31275.

Non-image files attached to this comment
jeffrey.kissel@LIGO.ORG - 12:27, Wednesday 09 November 2016 (31369)
Recall the ER8/O1 values for these coefficients were

    'Optic'      'Weighted Mean'    '1-sigma Uncertainty'    '1-sigma Uncertainty'
    'Stage'      '[N/ct]'           '[N/ct]'                 '%'                  
    'ETMY L1'    '8.17e-08'         '3.2e-09'                '3.9'                
    'ETMY L2'    '6.82e-10'         '5.2e-13'                '0.076'              
    'ETMY L3'    '4.24e-12'         '4.1e-15'                '0.096' 
from LHO aLOG 21280.

Comparing against numbers above,
    KU = 8.020-8 +/- 2.983-10 N/ct   ( std(KU) / |KU| = 0.0037 )
    KP = 6.482-10 +/- 2.748-12 N/ct   ( std(KP) / |KP| = 0.0033 )
    KT = 4.260-12 +/- 1.313-14 N/ct   ( std(KT) / |KT| = 0.0031 )

This means a change of
               (ER8 - ER10)/ER8 = 
    ETMY L1        0.0183
    ETMY L2        0.0495
    ETMY L3       -0.0047

We will compare these numbers against those determined by frequency-dependent transfer functions, e.g. the to-be processed data from LHO aLOG 31303, and update the low-latency/ calibration accordingly next week. It will also be interesting to re-cast the L1 and L2 numbers into a combined actuation strength change from ER10/O1, and compare it against the constantly calculated kappa_PU and check consistency there.
darkhan.tuyenbayev@LIGO.ORG - 10:16, Thursday 10 November 2016 (31391)CAL

Data points prior to DARM filter update mentioned in the report were analyzed with the help of following DARM model parameters:

ifoIndepFilename : ${CalSVN}/Runs/PreER10/Common/params/IFOindepParams.conf (r3519)
ifoDepFilename   : ${CalSVN}/Runs/PreER10/H1/params/H1params.conf (r3640)
ifoMeasParams    : ${CalSVN}/Runs/PreER10/H1/params/H1params_2016-10-13.conf (r3519)

and after the the DARM filters were updated (GPS 1162336667) the following configuration was used:

ifoIndepFilename : ${CalSVN}/Runs/PreER10/Common/params/IFOindepParams.conf (r3519)
ifoDepFilename   : ${CalSVN}/Runs/PreER10/H1/params/H1params_since_1162336667.conf (r3640)
ifoMeasParams    : ${CalSVN}/Runs/PreER10/H1/params/H1params_2016-10-13.conf (r3519)

Scripts were uploaded to CalSVN at

${CalSVN}/Runs/PreER10/H1/Scripts/Actuation/2016-11-08/

5 days SLM data (75 MB): ${CalSVN}/Runs/PreER10/H1/Measurements/Actuation/2016-11-08/

Plots: ${CalSVN}/Runs/PreER10/H1/Results/Actuation/2016-11-08_H1_UPT_act_strengths_*

darkhan.tuyenbayev@LIGO.ORG - 16:53, Sunday 20 November 2016 (31670)CAL

We discovered that in the single-line analysis we had an incorrect sign for TST stage actuation (we incorrectly set the sign of the N/ct coefficient).

The updated results have been posted in LHO alog 31668.

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