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ID Date Author Type Categoryup Subject
  12480   Fri Sep 9 17:50:02 2016 gautamUpdateSUSHeavy doors on BS-PRM, ETMY chambers

[steve, teng, johannes, lydia, gautam]

  • we set about doing some final checks on the Y arm while Johannes and Lydia worked on the X arm alignment
  • locked IMC, turned on Oplev HeNes for ITMY, SRM, PRM, BS and ETMY
  • I first went into the BS-PRM chamber. Traced Oplev paths for PRM and BS, checked that the beam is approximately centered on all the steering mirrors, and traced the beam with a clean beam card to make sure there was no clipping. The beams make it out of the vacuum onto the PDs, but are not centered
  • I also checked the Y arm green - the beam isn't quite centered on the periscope mirrors but I guess this has always been the case and I didn't venture to make any changes
  • Checked new PRM foil hats were secure
  • Checked the main IR beam out of the IMC, and also the IPANG beam - Steve suggested we keep track of the way this moves during pumpdown. However, I didn't quite think this through and we put the heavy door on the BS-PRM chamber before checking where the IPANG beam was on ETMY table (we later found that the beam was a tad too high. Anyways, this isn't critical, wouldve been nice to have this reference though
  • Checked that there were no tools lying around inside the chamber, and proceeded to put the heavy door on
  • Moved to ETMY table, and did much of the same as above - Oplev beam makes it successfully out off the ETM, OSEM cables aren't a risk to clipping the green input beam
  • Proceeded to put the heavy door on ETMY chamber
  • I would have liked to put the heavy door on the ITMY chamber today evening too, but while freeing the SRM from its EQ stops, I noticed that the LL and LR OSEM PD readouts are approximately 60 and 75 % of their saturation values. I think this warrants fixing (I also checked against the frame files from our last DRFPMI lock in march and the PD signals are significantly different) so we should do this before putting the heavy door on. It would also be a good idea to check the table leveling
  • The Oplev beams for ITMY and SRM make it cleanly out of the chamber so all looks good on that front
  • IR and green beams are well clear of any OSEM cables

Depending on how the X arm situation is, we will finish putting back all the heavy doors on Monday and start the pumpdown

GV Edit 11.30pm: 

  • We succeeded in locking the X arm as well, although the transmission peaked at 0.1 (but this is the high gain PD and not the QPD, and also, unlike the Y arm, the 50-50 BS splitting the transmitted light between the QPD and the high gain PD is still in place, so can't really compare with the Y arm value of 0.6)
  • To get the lock going, we had to change a bunch of things like the POX DC offset, demod phase, sign of the gain etc. It is unclear whether we are locking on the TEM00 mode, but we judged it is sufficient to close doors and pump down
  • Johannes and I centered the ETMX and ITMX OL spots on their respective QPDs. Earlier today, Johannes and Lydia had checked ITMX and ETMX OL paths, everything looks decent
  • JE piggyback edit : We also tied the upper ITMX OSEM cables to the suspension cage side using copper wire since particularly UR looked like it could slip and possibly fall down into the beam path
  • JE piggyback edit: While leveling the ITMX table, Gautam and I found that some of the screws that secure the weights were not vented. None of these were put in during this vent. We replaced them all with vented screws.
  • Rana also checked PRM and SRM alignment, all looks okay on that front - the OSEM problem I had alluded to earlier isn't really a problem, once the SRM is aligned, all the OSEMs are reasonably close to 50% of their saturation value.

Looks like on Monday, we will look to put the heavy doors on ITMY, ITMX and ETMX chambers, and begin the pumpdown

  12484   Mon Sep 12 20:15:22 2016 LydiaUpdateSUSDiagonalization in air

[Lydia, Teng]

We ran the scripts to diagonalize the damping matrices using the free swinging data from staurday night/sunday morning. The actual entries used for damping have not been changed. However, we did generate updated matrices for all the main optics (not including the mode cleaner optics, which were not free swinging over the weekend).

  • The scripts appear to be mostly working as intended, with a couple of issues:
    • The plots made by makeSUSSpectra claim to be showing spectra of the individual OSEM readings, but are actually dofs calculated using the ideal input matrix.
    • The existing parameters file (for the peak finding) was only fitting the lorentz peaks to a very narrow band of data, close to the bandwidth of the spectrum. Too narrow a band means that the initial guess must be very close, and also means there are not enough points to fit to.
      • We modified a copy of the paramters file to use a wider band (~.1 Hz) for fitting, and also use updated estimates of the mode frequencies.
      • This was largely successful, but the ITMY POS peak is very close to the SIDE peak, and POS is also stringly coupled to SIDE, so the wider bandwidth fitting can't separate the peaks. (See attachment 1)
      • A longer time series, plus more accurate initial guesses for the resonance frequencies, would allow us to fit to a smaller (~.03 Hz) band without encountering the stated issues.
      • A better way than manually examining plots to choose an initial frequency guess would be to automatically start at the overall maximum point in the spectrum between 0.4 and 1.5 Hz
  • Most of the diagonalization results seem good: "Badness" numbers of 4-6 and secondary peaks very supressed or absent on spectra plotted in dof basis (See attachment 2). ITMY, perhaps beacuse of a related issue, has phase problems with the matrix elements that result in messages like "osem/dof 2/1 is imaginary."
Attachment 1: ITMY_fit.jpg
ITMY_fit.jpg
Attachment 2: BS_diag.jpg
BS_diag.jpg
  12486   Tue Sep 13 11:00:59 2016 LydiaUpdateSUSETMY UL glitch returned

 

Quote:

For the ITMY, I squished together the cables which are in the 'Cable Interface Board' which lives in the rack. This thing takes the 64 pin IDC from the satellite module and converts it into 2 D-sub connectors to go to the PD whitening board and the coil driver board. Lets see if the ITMY OSEM glitches change character overnight.

Last night from 8:30 pm to 8:30 am PDT, ETMY UL signal was glitchy again. As of now it seems to have quieted back down, but we pushed on the cables on the board at the Y end to hopefully prevent it from coming back. After doing so it still seems to be behaving well.

  12490   Tue Sep 13 19:18:43 2016 LydiaUpdateSUSDiagonalization in air

[Lydia, Teng]

We continued to work on the diagonalization scripts today and devised a way of choosing starting parameters that seems to work much better, and is easier to use, than tuning up to 15 parameters by hand per optic.

  • As before, the spectrum for each dof is estimated by using the "ideal" input matrix.
  • The starting guess for the peak frequency for each dof is the bin which achieves the maximum value of the spectrum between 0.4 and 1.5 Hz.
  • If another dof has a higher value at that frequency, the next highest peak is used. (Sometimes, for example, the peak in PIT at the POS frequency is stronger than the real POS peak!)
  • The peak height is initially guessed to be the spectrum value at the initial frequncy guess.
  • The width paramter Q can still be read from a file, but for all the times we tried, the peaks were found successfully if Q was initially guessed to be 300, so there might be no need to do this.
  • Spectra should still be examined to make sure the results make sense, and once we look at free swinging data in vacuum, we should compare the frequency results to the wiki values.
  • Reasonably good matrix values are saved to peakFit/inMats/1157630417. We got good diagonalization results for all but ITMY (see below). The values used for damping have not been overwritten.

We still noticed phase problems with ITMY, which appear to be preventing good diagonalization (See Attachment 1). Almost every degree of freedom has a significant imaginary part in the sensing matrix. We looked at the phases of the cross spectra in DDT and saw that indeed, the OSEM signals do not have the appropriate relative phases at the peak frequencies, especially in PIT and YAW (see Attachment 2: the phase at the peak is about 30 degrees when it should be 180). These phases are different for data takes ~24 hours apart, but are still wrong. We also looked at this information for ETMY and saw the correct behavior. We temporarily moved the pitch and yaw sliders for ITMY and looked at the OSEM response on a striptool, and the signals moved in the expected way. Can anyone suggest a reason why this would be happening? Is there another stretch of data (besides this past weekend) which would be good to compare to?

 

Attachment 1: ITMY_diag.jpg
ITMY_diag.jpg
Attachment 2: 38.png
38.png
  12495   Wed Sep 14 20:27:03 2016 LydiaUpdateSUSDiagonalization

Today the main optics were free swinging for several hours, so I attempted diagonalization in vacuum.

  • ITMY still has bad phases. I looked at the spectra for this and other optics, and it looks like the other optics have the 60Hz line notched out for all coils while ITMY only has it notched on the side coil. (Using C1:SUS-ITMY_SENSOR channels). Where is this controlled from, and could it be the source of the issue? 
    • I tried using a different coil as the "standard," with the other coils compared against it in tfestimate. Default is UL, I tried UR and LL. The phase problems were still present for ITMY, but the script was still working fine for other optics.
    • The phase difference between coils is different for different start times.
    • A short segment of the time series for ITMY shows significantly more high frequency noise than for other optics at the same time.
  • The ETMY matrix for vacuum has the wrong sign for UL coupling to pitch! The diagonalization results look OK on the graph, but the butterfly mode still has small peaks (See attachment 1). When the individual coil spectra are plotted, the angular degrees of freedom show very weak coupling for UL to pitch, and LL to yaw. We initially replaced the matrix on the MEDM screen with the one generated by the script. After realizing this, the PIT row was changed to 1 1 -1 -1 0, but the effectiveness of the damping on the locked transmission fluctuations was about the same both ways.
Attachment 1: ETMY_diag.png
ETMY_diag.png
  12497   Thu Sep 15 18:37:20 2016 LydiaUpdateSUSDiagonalization

[Teng, Lydia]

  • We fixed the 60Hz filter on ITMY. This improved the phase problems somewhat but one coil (UL) is still about 12 degrees out of phase compared to the others for all the dofs. Is there some other place where a filter coule be applied to just one coil sensor? I pressed the "Load coefficients" button for UL, so maybe that will have helped.
  • We want to interpret the coil signals to have an accurate measurement of each dof. This means what the input matrix should describe is the dependence of each dof on the OSEM signals, which is found by inverting the matrix which describes the sensitivity of each OSEM to changes in that degree of freedom.
    • We looked at the spectra of the individual coils for ITMY and ETMY (See attachment 1 & 2). The coupling between some coils and applicable resonance peaks is very weak (~0.1 times the sensitivity of the other coils).
    • However, when a certain degree of freedom, e.g. pitch, is deliberately driven using awggui, the response of the ITMY coils is clear on the StripTool and is about the same magnitude for all of the face OSEMS. So, it seems like the diagonalization script does not always succeed at measuring the relative sensitivity of the OSEMs to the degrees of freedom.
    • This may be because the fundamental swing modes experienced by the free swinging pendulum are not the same as what we measure as pitch, yaw, etc. This could be possible if the wire tension is not the same on both sides. For ITMY, the spectra imply that the funamdental frequencies are actually at some linear combinations of pitch and yaw, swinging about a diagonal axis that results in a much weaker response for some of the OSEMS. Calling these peaks pitch and yaw may be inaccurate. Certainly they do not indicate the true relative sensitivity of the coils.
    • We propose an alternate approach to measuring this sensitivity: drive one dof at a time with awggui, take a spectrum (less resolution is ok because we already know the drive frequency), and measure the sensing matrix values for that dof the same way as before, but using a spectral peak that decribes motion that we know is purely pitch. Repeat this for all 4 dofs that we can actuate on, then compile these results into a sensing matrix and take the inverse.
Attachment 1: ETMY_osemspec.png
ETMY_osemspec.png
Attachment 2: ITMY_osemspec.png
ITMY_osemspec.png
  12499   Fri Sep 16 19:14:27 2016 LydiaUpdateSUSDiagonalization

[Lydia, Teng]

We built matrices for ITMY and ETMY by driving one degree of freedom at a time with awggui, while the damping was on. These have been applied to the damping loops.

  • Each segment of data is 1000s long and each dof was driven at 0.25 Hz.
  • These matrices are much closer to the ideal matrix and have no wrong signs. We believe they represent the relative sensitivity of the OSEMs to the degrees of freedom much more accurately. This is because the free swinging modes are not actually pitch, yaw, etc, but some linear combination of these. However, the damping actuates on pitch, yaw, etc. So we should isolate the degrees of freedom by driving them one at a time instead of just looking at free swinging peaks.
    • Attachment 1: An example of the dof spectra, calculated using the default input matrix, when ETMY YAW was driven at 0.25 Hz.
    • Attachment 2: The same OSEM sensor data, with the dofs calculated using the matrix found from this data. There is still a significant peak in pitch, but the other dofs are significantly suppressed.
    • Attahcment 3: The same data again, but the dofs are measured with the input matrix calculated by the free swinging data. This achieves much less suppression than the new matrix. Obviously this is not exactly a fair comparison because the new matrix was generated with this data, but the method of measuring OSEM responses by driving peaks has a much close relationship between what it measured (the OSEM response), and how the matrix is used (by damping loops which drive the coils in much the same way as awggui).
  • The phase problems seem to be mostly solved. Both Y arm test masses have some phase warnings, but they mostly occur with side. This can happen because the ideal matrix elements are 0, so the real parts are small. If there is no strong coupling then there is no reason to expect the background spectrum to be in phase with the peak. Other phase differences are small; most less than 5 degrees, a couple between 5 and 10 degrees. This may still merit further investiagtion.
  • Comparing the damping results for ITMY with the old (based on free swinging data) and new (based on driven data), we see the 1Hz peak suppressed by ~35% and the noise above 1Hz generally suppressed by ~25-30% . There is, however, significantly more movement between 0.5 and 1 Hz, maybe because the fundamental physical modes are not being directly measured and suppressed. Overall this seems like an improvement.

GPS times:

ITMY

Pitch:1158085097 Yaw: 1158086537 Pos: 1158089237 Side: 1158087977

ETMY

Pitch: 1158095897 Yaw: 1158097577 Pos: 1158099377 Side: 1158100817

Attachment 1: ETMY_yawdrivedefault.png
ETMY_yawdrivedefault.png
Attachment 2: ETMY_yawdrivenew.png
ETMY_yawdrivenew.png
Attachment 3: ETMY_yawdriveold.png
ETMY_yawdriveold.png
Attachment 4: 57.png
57.png
  12501   Sat Sep 17 02:00:23 2016 ranaUpdateSUSAlignment status

All is not lost. I've stuck and unstuck optics around a half dozen times. Can you please post the zoomed in time series (not trend) from around the time it got stuck? Sometimes the bias sliders have to be toggles to make the bias correct. From the OSEM trend it seems like it got a large Yaw bias. May also try to reseat the satellite box cables and the cable from the coil driver to the cable breakout board in the back of the rack.

  12502   Sat Sep 17 16:51:01 2016 LydiaUpdateSUSAlignment status

Here's the timeseries plots. I've zoomed in to right after the problem- did you want before? We pretty much know what happened: c1susaux was restarted from the crate but the damping was on, so as soon as the machine came back online the damping loops sent a huge signal to the coils. (Also, it seems to be down again. Now we know what to do first before keying the crate.) It seems like both right side magnets are stuck, and this could probably be fixed by moving the yaw slider. Steve advised that we wait for an experienced hand to do so. 

Quote:

All is not lost. I've stuck and unstuck optics around a half dozen times. Can you please post the zoomed in time series (not trend) from around the time it got stuck? Sometimes the bias sliders have to be toggles to make the bias correct. From the OSEM trend it seems like it got a large Yaw bias. May also try to reseat the satellite box cables and the cable from the coil driver to the cable breakout board in the back of the rack.

 

Attachment 1: Screenshot_from_2016-09-17_16-45-00.png
Screenshot_from_2016-09-17_16-45-00.png
  12503   Sun Sep 18 16:18:05 2016 ranaUpdateSUSAlignment status

susaux is responsible for turning on/off the inputs to the coil driver, but not the actual damping loops. So rebooting susaux only does the same as turning the watchdogs on/off so it shouldn't be a big issue.

Both before and after would be good. We want to see how much bias and how much voltage from the front ends were applied. l1susaux could have put in a huge bias, but NOT a huge force from the damping loops. But I've never seen it put in a huge bias and there's no way to prevent this anyway without disconnecting cables.

I think its much more likely that its a little stuck due to static charge on the rubber EQ stop tips and that we can shake it lose with the damping loops.

  12504   Mon Sep 19 11:11:43 2016 ericqUpdateSUSAlignment status

[ericq, Steve]

ITMX is free, OSEM signals all rougly centered. 


This was accomplished by rocking the static alignment (i.e. slow controls) pitch and yaw offsets until the optic broke free. This took a few volts back and forth. At this point, I tried to find a point where the optic seemed to freely swing, and hopefully have signals in all 5 OSEMS. It seemed to be free sometimes but mostly settling into two different stationary states. I realized that it was becoming torqued enough in pitch to be leaning on the top-front or top-back EQ stops. So, I slowly adjusted the pitch from one of these states until it seemed to be swinging a bit on the camera, and three OSEM signals were showing real motion. Then, I slowly adjusted the pitch and yaw alignments to get all OSEMS signals roughly centered at half of their max voltage.

  12516   Fri Sep 23 01:09:04 2016 ericqUpdateSUSETMX hysteresis test

I had hoped to do some ALS work, but I realized too late that we loaned our HP analyzer to Andrew. I decided instead to do some ETMX testing. 

I have a script running that'll misalign both ETMs and back by about 0.5mrad with half hour rests in between. It'll be done around 6AM.

  12517   Sat Sep 24 11:04:00 2016 ericqUpdateSUSETMX hysteresis test

Seems like the angular position was fairly stable, though there is some change in the ETMX pitch that could be hysterisis or normal drift. I didn't mention it explicity in the previous log, but the misalignment was purely in pitch. I'll give it another shot with a bigger misalginment, and maybe a mix of pitch and yaw.

  12518   Mon Sep 26 19:48:09 2016 LydiaUpdateSUSITMX stuck again, ITMY whitening issue

This afternoon around 2:45, ITMX started ringing up at ~.9Hz for about a minute and then got stuck again. When I noticed this evening, I tried to free it with the alignment sliders but was unable to see any signal on UL or UR. It also looks like the damping for ITMY was turned off at the same time ITMX got stuck (not at the start of its ring up). SRM also has a spike in its motion at this time, and another one minute later that ended up with the LR OSEM at a much higher level, though the mirror does not appear to be stuck. We didn't see any strange behavior from any of the other optics.

Teng and I were working on diagnosing a problem with the ITMY UL whitening, but by the time we disconnected any applicable cables, the damping for ITMY was already off. Later we unplugged the ITMX PD whitening cables after verifying that the ITMX damping was also already off. This problem may have occured earlier, while Teng, Eric, and I were examining and pushing in the cables at 1X5 without unplugging anything.

We found that the reason for the bad phase on the ITMY free swing data is because the whitening filter for UL is not being properly turned on. We are in the process of investigating the source of this problem. Right now all the cables to the PD whitening boxes in 1X5 are switched between ITMY and ITMX.
 

Attachment 1: 44.png
44.png
Attachment 2: 26.png
26.png
  12519   Tue Sep 27 08:49:47 2016 SteveUpdateSUSseismic activity is up

The earth quake shook ITMX free for a  short while.

 

Attachment 1: 4.3mSaltonSee.png
4.3mSaltonSee.png
Attachment 2: ITMXstuck.png
ITMXstuck.png
  12520   Tue Sep 27 18:04:50 2016 LydiaUpdateSUSITMX slow channels down, ITMY diagonalization update

[Teng, Lydia]

When we plugged in the back cables yesterday on the whitening boxes after switching them, two of the ITMX PDMon channels (UR and LR) got stuck at 0. This caused me to believe ITMX was still stuck even when it was freed. However, it was left in a stuck state overnight and freed again today after this issue was discovered. The alignment sliders have been set to 0 as a safety net to keep ITMX from getting stuck again if c1susaux is restarted again. We switched the cables back and the problem was still there.

The ITMY UL whitening filter problem, which the cables were originally switched to diagnose, was also still there. Ericq suggested we turn off all the whitening filters in order to get diagonalization data that would not show a phase difference between coils. We ran the diagonalization again with all the dewhitening filters off and got much cleaner results, with no visible cross-coupling peaks remaining between the degrees of freedom (see attachemnt 1). We did not apply this matrix to the damping, however, because there are elements which have the wrong sign compared to the ideal matrix. Significant adjustments to the output matrix will probably need to be made if this result is to be used. We also verified that the phase problem had been solved in DTT, where we saw the same sign discrepancies as in the matrix below. 

Damping can be turned back on, using the old, non-diagonalized matrix currently in effect. There is enough free swing data to diagonalize ITMY now, so feel free to mess with it. 

Matrix (wrong signs red, suspiciously small elements orange):

           pit     yaw     pos         side    butt
UL    1.633   0.138   1.224   0.136   0.984  
UR   -0.202  -1.768   1.179   0.132  -1.028  
LR   -2.000   0.094   0.776   0.107   1.001  
LL   -0.165   2.000   0.821   0.111  -0.987  
SD    0.900   1.131  -1.708   1.000  -0.107  

 

Attachment 1: ITMY_diagsuccess.pdf
ITMY_diagsuccess.pdf
  12523   Thu Sep 29 16:19:29 2016 LydiaUpdateSUSFree swing eigenmodes

[Lydia, Teng]

Motivated by the strange pitch/yaw coupling behavior we ran into while doing diagonalization, we looked at the oplev pitch and yaw free swing spectra for all 4 test masses (see attachment 1). We saw the same behavior there: At the peak frequencies for the angular degress of freedom, the oplevs saw significant contributions from both pitch and yaw. We also examined the phase between pitch and yaw at these peaks and found that consistently, pitch and yaw were in phase at one of the resonance frequencies and out of phase at the other (ignoring the pos and side peaks). 

This corresponds physically to angular motion about some axis that is diagonal, ie not perfectly vertical or horizontal. If we trust the oplev calibration, and Eric says that we do, then the angle of this axis of rotation with the horizontal (pitch axis) is

 \theta = \arctan \frac{Y\left ( f_{peak} \right )}{P\left ( f_{peak} \right )}  

Where Y and P are yaw and pitch ASD values. This will always give an angle between 0 and 90 degrees; which quadrant the axis of rotation occupies can be dermined by looking at the phase between pitch and yaw at the same frequencies. 0 phase means that the axis of rotation lies somewhere less than 90 degrees counterclockwise from the horizontal as viewed from the AR face of the optic, and a phase of 180 degrees means the axis is clockwise from horizontal (see attachment 2). Qualitatively, these features show up the same way for segments of data taken at different times. In order to get some quantitative sense of the error in these angles, we found them using spectrogram values with a bandwidth of 0.02 Hz averaged over 4000 seconds. 

Results (all numbers in degrees unless otherwise specified):

ITMY
peak 1 ( 0.692  Hz):
mean: 24.991
std: 1.23576
ptich/yaw phase: -179.181
peak 2 ( 0.736  Hz):
mean: 21.7593
std: 0.575193
pitch/yaw phase: 0.0123677

 

ITMX
peak 1 ( 0.502  Hz):
mean: 17.4542
std: 0.745867
ptich/yaw phase: -179.471
peak 2 ( 0.688  Hz):
mean: 74.822
std: 0.455678
pitch/yaw phase: -0.43991

 

ETMX
peak 1 ( 0.73  Hz):
mean: 43.1952
std: 1.54336
ptich/yaw phase: -0.227034
peak 2 ( 0.85  Hz):
mean: 60.7117
std: 0.29474
pitch/yaw phase: -179.856

ETMY
peak 1 ( 0.724  Hz):
mean: 78.2868
std: 2.18966
ptich/yaw phase: 6.03312
peak 2 ( 0.844  Hz):
mean: 26.0415
std: 2.10249
pitch/yaw phase: -176.838

ETMY and ITMX both show a more significant (~4x) contribution from pitch on one peak, and from yaw on the other. This is reflected in the fact that they each have one angle somewhat close to 0 (below 30 degrees) and one close to 90 (above 60 degrees). The other two test masses don't follow this rule, meaning that the 2 angular frequency peaks do not correspond to pitch and yaw straightforwardly. 

Also, besides ITMX, the axes of rotation are at least several degrees away from being perpendicular to each other. 

 

Attachment 1: 05.png
05.png
Attachment 2: SUS_eigenmodes.png
SUS_eigenmodes.png
  12536   Thu Oct 6 15:42:51 2016 LydiaUpdateSUSOutput matrix diagonalization

Summary: At the 40m meeting yesterday, Eric Q. gave the suggestion that we accept the input matrix weirdness and adjust the output matrix by driving each coil individually so that it refers to the same degrees of freedom. After testing this strategy, I don't think it will work. 

Yesterday evening I tested this idea by driving one ITMY coil at a time, and measuring the response of each of the free swing modes at the drive frequency. I followed more or less the same procedure as the standard diagonalization: responses to each of the possible stimuli are compared to build a matrix, which is inverted to describe the responses given the stimuli. For the input matrix, the sensor readings are the responses and the free swing peaks are the stimuli. For the output matrix, the sensors transformed by the diagonalized input matrix as the responses of the dofs which are compared, and the drive frequency peak associated with a coil output is the stimulus. However, the normalization still happens to each dof independently, not to each coil independently. 

The output matrix I got had good agreement with the ITMY input matrix in the previous elog: for each dof/osem the elements had the same sign in both input and output matrices, so there are no positive feedback loops. The relative magnitude of the elements also corresponded well within rows of the input matrix. So the input and output matrices, while radically different from the ideal, were consistent with each other and referred to the same dof basis. So, I applied these new matrices (both input and output) to the damping loops to test whether this approach would work. 

drive-generated output matrix: 

      UL      UR      LR       LL      SD
pit    1.701  -0.188  -2.000  -0.111   0.452  
yaw    0.219  -1.424   0.356   2.000   0.370  
pos    1.260   1.097   0.740   0.903  -0.763  
sid    0.348   0.511   0.416   0.252   1.000  
but    0.988  -1.052   0.978  -0.981   0.060

However, when Gautam attempted to lock the Y arm, we noticed that this change significantly impacted alignment. The alignment biases were adjusted accordingly and the arm was locking. But when the dither was run, the lock was consistently destroyed. This indicates that the dither alignment signals pass through the SUS screen output matrix. If the output matrix pitch and yaw columns refer instead to the free swing eigenmodes, anything that uses the output matrix and attempts to align pitch and yaw will fail. So, the ITMY matrices were restored to their previous values: a close to ideal input matrix and naive output matrix. We could try to change everything that is affected by the output matrices to be independent of a transformation to the free swing dof basis, and then implement this strategy. But to me, that seems like an unneccessary amount of changes with unpredictable consequences in order to fix something that isn't really broken. The damping works fine, maybe even better, when the input matrix is set by the output matrix: we define pitch, for example, to be "The mode of motion produced by a signal to the coils proportional to the pitch row of the naieve output matrix," and the same for the other dofs. Then you can drive one of these "idealized" dofs at a time and measure the sensor responses to find the input matrix. (That is how the input matrix currently in use for ITMY was found, and it seems to work well.) 

 

  12540   Fri Oct 7 20:56:15 2016 KojiUpdateSUSOutput matrix diagonalization

I wanted to see what is the reason to have such large coupling between pitch and yaw motions.

The first test was to check orthogonality of the bias sliders. It was done by monitoring the suspension motion using the green beam.
The Y arm cavity was aligned to the green. The damping of ITMY was all turned off except for SD.
Then ITMY was misaligned by the bias sliders. The ITMY face CCD view shows that the beam is reasonably orthogonally responding to the pitch and yaw sliders.
I also confirmed that the OPLEV signals also showed reasonablly orthogonal responce to the pitch and yaw misalignment.

=> My intuition was that the coils (including the gain balance) are OK for a first approximation.

Then, I started to excite the resonant modes. I agree that it is difficult to excite a pure picth motion with the resonance.


So I wanted to see how the mixing is frequency dependent.

The transfer functions between ITMY_ASCPIT/YAW_EXC to ITMY_OPLEV_PERROR/YERROR were measured.

The attached PDFs basically shows that the transfer functions are basically orthogonal (i.e. pitch exc goes to pitch, yaw exc goes to yaw) except at the resonant frequency.

I think the problem is that the two modes are almost degenerate but not completely. This elog shows that the resonant freq of the ITMY modes are particularly close compared to the other suspensions.
If they are completely degenerate, the motion just obeys our excitation. However, they are slightly split. Therefore, we suffer from the coupled modes of P and Y at the resonant freq.
However, the mirror motion obeys the exitation at the off resonance as these two modes are similar enough.

This means that the problem exists only at the resonant frequencies. If the damping servos have 1/f slope around the resonant freqs (that's the usual case), the antiresonance due to the mode coupling does not cause servo instability thank to the sufficient phase margin.

In conclusion, unfortunately we can't diagnalize the sensors and actuators using the natural modes because our assumption of the mode purity is not valid.
We can leave the pitch/yaw modes undiagnalized or just believe the oplevs as a relatively reliable reference of pitch and yaw and set the output matrix accordingly.

 

The figures will be rotated later.

Attachment 1: 161007_P.pdf
161007_P.pdf
Attachment 2: 161007_Y.pdf
161007_Y.pdf
  12541   Mon Oct 10 09:31:25 2016 SteveUpdateSUSPRM damping restored

Local earth quake 3.7 mag  trips PRM

ETMY_UL glitch

What about the MC?

 

Attachment 1: 3.7mLomaLinda.png
3.7mLomaLinda.png
Attachment 2: ETMY_UL_glitch.png
ETMY_UL_glitch.png
Attachment 3: MC_glitcing?.png
MC_glitcing?.png
  12546   Tue Oct 11 00:43:50 2016 ericqUpdateSUSPRM LR problematic again

Tonight, and during last week's locking, we noticed something intermittently kicking the PRM. I've determined that PRM's LR OSEM is problematic again. The signal is coming in and out, which kicks the OSEM damping loops. I've had the watchdog tripped for a little bit, and here's the last ten minutes of the free swinging OSEM signal:

Here's the hour trend of the PRM OSEMS over the last 7 days a plot of just LR since the fix on the 9th of September.

It looks like it started misbehaving again on the evening of the 5th, which was right when we were trying to lock... Did we somehow jostle the suspension hard enough to knock the foil cap back into a bad spot?

  12549   Tue Oct 11 10:15:04 2016 SteveUpdateSUSPRM LR problematic again

It started here

 

Attachment 1: PRMalfoiled.png
PRMalfoiled.png
  12550   Tue Oct 11 10:38:51 2016 SteveUpdateSUS wire standoffs update

100 Sapphire prizms arrived.

 

Attachment 1: A028_-_20161010_170319.jpg
A028_-_20161010_170319.jpg
Attachment 2: A027_-_20161010_170202.jpg
A027_-_20161010_170202.jpg
  12551   Tue Oct 11 13:30:49 2016 gautamUpdateSUSPRM LR problematic again

Perhaps the problem is electrical? The attached plot shows a downward trend for the LR sensor output over the past 20 days that is not visible in any of the other 4 sensor signals. The Al foil was shorting the electrical contacts for nearly 2 months, so perhaps some part of the driver circuit needs to be replaced? If so a Satellite Box swap should tell us more, I will switch the PRM and SRM satellite boxes. It could also be a dying LED on the OSEM itself I suppose. If we are accessing the chamber, we should come up with a more robust insulating cap solution for the OSEMs rather than this hacky Al foil + kapton arrangement.

The PRM and SRM Satellite boxes have been switched for the time being. I had to adjust some of the damping loop gains for both PRM and SRM and also the PRM input matrix to achieve stable damping as the PRM Satellite box has a Side sensor which reads out 0-10V as opposed to the 0-2V that is usually the case. Furthermore, the output of the LR sensor going into the input matrix has been turned off.

 

  12552   Wed Oct 12 13:34:28 2016 gautamUpdateSUSPRM LR problematic again

Looks like what were PRM problems are now seen in the SRM channels, while PRM itself seems well behaved. This supports the hypothesis that the satellite box is problematic, rather than any in-vacuum shenanigans.

Eric noted in this elog that when this problem was first noticed, switching Satellite boxes didn't seem to fix the problem. I think that the original problem was that the Al foil shorted the contacts on the back of the OSEM. Presumably, running the current driver with (close to) 0 load over 2 months damaged that part of the Satellite box circuitry, which lead to the subsequent observations of glitchy behaviour after the pumpdown. Which begs the question - what is the quick fix? Do we try swapping out the LM6321 in the LR LED current driver stage? 

GV Edit Nov 2 2016: According to Rana, the load of the high speed current buffer LM6321 is 20 ohms (13 from the coil, and 7 from the wires between the Sat. Box and the coil). So, while the Al foil was shorting the coil, the buffer would still have seen at least 7 ohms of load resistance, not quite a short circuit. Moreover, the schematic suggests that that the kind of overvoltage protection scheme suggested in page 6 on the LM6321 datasheet has been employed. So it is becoming harder to believe that the problem lies with the output buffer. In any case, we have procured 20 of these discontinued ICs for debugging should we need them, and Steve is looking to buy some more. Ben Abbot will come by later in the afternoon to try and help us debug.

  12553   Wed Oct 12 15:01:22 2016 steveUpdateSUSSOS ITM baffles plates are ready

The two 40 mm apeture baffles at the ends were replaced by 50 mm one. ITM baffles with 50 mm apeture are baked ready for installation.

Quote:

 Green welding glass 7" x 9"   shade #14 with 40 mm hole and mounting fixtures are ready to reduce scatter light on SOS

PEEK 450CA shims and U-shaped clips  will keep these plates damped.

 

 

Attachment 1: baffle7x9_1.5.jpg
baffle7x9_1.5.jpg
Attachment 2: baffle_holder.jpg
baffle_holder.jpg
Attachment 3: baffle_top_view.jpg
baffle_top_view.jpg
  12569   Wed Oct 19 08:28:11 2016 SteveUpdateSUSITMY_UL

Everybody is happy, except ITMY_UL or satalite box.

Gautam shows perfect form in the OMC chamber.

Attachment 1: 12hrs.png
12hrs.png
Attachment 2: vent79.jpg
vent79.jpg
  12590   Tue Nov 1 09:03:08 2016 SteveUpdateSUSseismic activity is up

Salton See is shaking again.

 

Attachment 1: seismicActivity.png
seismicActivity.png
  12598   Thu Nov 3 16:30:42 2016 LydiaConfigurationSUSETMX to coil matrix expanded

[ericq, lydia]

Background: 

We believe the optimal OSEM damping would use an input matrix diagonalized to the free swing modes of the optic, and an output matrix which drives the coils appropriately to damp these free swing modes. As was discovered, a free swinging optic does not necessarily have eigenmodes that match up perfectly with pitch and yaw, however in the current state the "TO_COIL"  output matrix that determines the drive signals in response to the diagonlized sensor output also controls the drive signals for the oplevs, LSC/ASC, and alignment biases. So attempts to diagonalize the output matrix to agree with the input matrix have resulted in problems elsewhere. (See previous elog). So, we want to expand the "TO_COIL" matrices to treat the OSEM sensor inputs separately from the others.

Today:

  • We modified the ETMX suspension model (c1scx) to use a modified copy of the sus_single_control block (sus_single_control_mod) that has 3 additional input columns. These are for the sensing modes determined by the input matrix, and are labeled "MODAL POS", "MODAL PIT", and "MODAL YAW." 
    • The regular POS, PIT, and YAW columns no longer include the diagonalized OSEM sensor signals for ETMX.
    • The suspension screen now out of date; it doesn't show the new columns under Output Filters and the summed values displayed for each damping loop do not incluse the OSEM damping.
  • The new matrix can be acessed at /opt/rtcds/caltech/c1/medm/c1scx/C1SUS_ETMX_TO_COIL.adl (see Attachment 1). For now, it has the naive values in the new columns so the damping behavior is the same. 
  • In trying to get a properly generated MEDM screen for the larger matrix, we discovered that the Simulink block for TO_COIL specifies in its description a custom template for the medm autogeneration. We made a new verion of that template with extra columns and new labels, which can be reused for the other suspensions. These templates are in /opt/rtcds/userapps/release/sus/c1/medm/templates, the new one is SUS_TO_COIL_MTRX_EXTRA.adl
  • I will be setting the new column values to ones that represent the diagonlized free swing modes given by the input matrix. Hopefully this will improve OSEM damping without getting in the way of anything else. If this works well, the other SUS models can be changed the same way. 
Attachment 1: 01.png
01.png
  12601   Mon Nov 7 08:00:11 2016 SteveUpdateSUSSRM -PRM sat. amp swap

I just realized that Gautam set this test up and turned damping off......He will explane the details

 

Attachment 1: SRM.jpg
SRM.jpg
Attachment 2: SRM-UR_OK.png
SRM-UR_OK.png
  12602   Mon Nov 7 16:05:55 2016 gautamUpdateSUSPRM Sat. Box. Debugging

Short summary of my Sat. Box. debugging activities over the last few days. Recall that the SRM Sat. Box has been plugged into the PRM suspension for a while now, while the SRM has just been hanging out with no electrical connections to its OSEMs.

As Steve mentioned, I had plugged in Ben's extremely useful tester box (I have added these to the 40m Electronics document sub-tree on the DCC) into the PRM Sat. Box and connected it to the CDS system over the weekend for observation. The problematic channel is LR.  Judging by Steve's 2 day summary plots, LR looks fine. There is some unexplained behavior in the UR channel - but this is different from the glitchy behaviour we have seen in the LR channel in the past. Moreover, subsequent debugging activities did not suggest anything obviously wrong with this channel. So no changes were made to UR. I then pulled out the PRM sat.box for further diagnostics, and also, for comparison, the SRM sat. box which has been hooked up to the PRM suspension as we know this has been working without any issues. 

Tracing out the voltages through the LED current driver circuit for the individual channels, and comparing the performance between PRM and SRM sat. boxes, I narrowed the problem down to a fault in either the LT1125CSW Quad Op-Amp IC or the LM6321M current driver IC in the LR channel. Specifically, I suspected the output of U3A (see Attachment #1) to be saturated, while all the other channels were fine. Looking at the spectrum at various points in the circuit with an SR785, I could not find significant difference between channels, or indeed, between the PRM/SRM boxes (up to 100kHz). So I decided to swap out both these ICs. Just replacing the OpAmp IC did not have any effect on the performance. But after swapping out the current buffer as well, the outputs of U3A and U11 matched those of the other channels. It is not clear to me what the mode of failure was, or if the problem is really fixed. I also checked to make sure that it was indeed the ICs that had failed, and not the various resistors/capacitors in the signal path. I have plugged in the PRM sat. box + tester box setup back into our CDS data acquisition for observation over a couple of days, but hopefully this does the job... I will update further details over the coming days.

I have restored control to PRM suspensions via the working SRM sat. box. The PRM Sat. Box and tester box are sitting near the BS/PRM chamber in the same configuration as Steve posted in his earlier elog for further diagnostics...


GV Edit 2230 hrs 7Nov2016: The signs from the last 6 hours has been good - see the attached minute trend plot. Usually, the glitches tend to show up in this sort of time frame. I am not quite ready to call the problem solved just yet, but I have restored the connections to the SRM suspension (the PRM and SRM Sat. Boxes are still switched). I've also briefly checked the SRM alignment, and am able to lock the DRMI, but the lock doesn't hold for more than a few seconds. I am leaving further investigations for tomorrow, let's see how the Sat. Box does overnight.

Attachment 1: D961289-B2.pdf
D961289-B2.pdf
Attachment 2: PRMSatBoxtest.png
PRMSatBoxtest.png
  12606   Tue Nov 8 11:54:38 2016 gautamUpdateSUSPRM Sat. Box. looks to be fixed

Looks like the PRM Sat. Box is now okay, no evidence of the kind of glitchy behaviour we are used to seeing in any of the 5 channels.

Quote:
 
GV Edit 2230 hrs 7Nov2016: The signs from the last 6 hours has been good - see the attached minute trend plot. Usually, the glitches tend to show up in this sort of time frame. I am not quite ready to call the problem solved just yet, but I have restored the connections to the SRM suspension (the PRM and SRM Sat. Boxes are still switched). I've also briefly checked the SRM alignment, and am able to lock the DRMI, but the lock doesn't hold for more than a few seconds. I am leaving further investigations for tomorrow, let's see how the Sat. Box does overnight.

 

  12612   Sun Nov 13 23:42:43 2016 LydiaUpdateSUSETMX output matrix data

I took data of the ETMX SUSPOS, SUSPIT and SUSYAW channels while driving each of the 4 face coils. I manually turned off all the damping except the side. 

Excitation: I used white noise bandpassed from 0.4 to 5 Hz in order to examine the responses around the resonance frequencies. To avoid ringing things up too much, I started with a very weak drive signal and gradually increased it until it seemed to have an effect on the mirror motion by looking at the oplev signals/sensor RMS values on the SUS screen; it's possible I'll need to do it again with a stronger signal if there's not enough coherence in the data. 

Finding the matrix: The plan is to estimate the transfer function of the coil drive signal with the sensed degrees of freedom (specified by the already diagonalized input matrix). This transfer function can be averaged around the resonance peak for each dof to find the elements of the matrix that converts signals to dof responses, (the "response matrix", which is the inverse of the output matrix). Each column of the response matrix gets normalized so that the degrees of freedom influence the drive signals in the right ratio. 

Other notes: 

  • I had some trouble getting the awg python library to work: I had to manually edit a CDLL statement to use the absolute path of an .so file. I wasn't sure what environment variable to set to make it look in the right folder automatically.
  • The awg ArbitraryLoop object seems to be affected by cds getdata calls (The EXC signal stopes early and then stop() hangs) so I ended up doing the excitation and data reading in 2 separate scripts. 
  • Reminder that the watchdogs must be on "Normal" for the EXC signal to make it to the coils, so the damping must be turned off manually with the watchdogs still on if you want to drive without damping. 
  12643   Mon Nov 28 10:27:13 2016 gautamUpdateSUSITMY UL glitches are back

I left the tester box plugged in from Thursday night to Sunday afternoon, and in this period, the glitches still appeared in (and only in) the UL channel.

So yesterday evening, I pulled the Sat. Box. out and checked the DC voltages at various points in the circuit using a DMM, including the output of the high current buffer that supplies the drive current to the shadow sensor LEDs. When we had similar behaviour in the PRM box, this kind of analysis immediately identified the faulty component as the high current buffer IC (LM6321M) in the bad channel, but everything seems in order for the ITMY box. 

I then checked the Satellite Amplifier Termination Board, which basically just adds 100ohm series resistors to the output of the PD readout, and all the resistors seem fine, the piece of insulating material affixed to the bottom of this board is also intact. I then used the SR785 in AC coupled mode to look at the high frequency spectrum at the same points I checked the DC voltages with the DMM (namely the drive voltage to the LEDs, and the PD readout voltages on the PCB as well as on the pins of the connector on the outside of the box after the termination board (leading to the DAQ), and nothing sticks out here in the UL channel either. Of course it could be that the glitches are intermittent, and during my tests they just weren't there...

I am hesitant to start pulling out ICs and replacing them without any obvious signs of failure from them, but I am out of debugging ideas...


One possibility is that the problem lies upstream of the Sat. Box - perhaps the UL channel in the Suspension PD Whitening and Interface Board is faulty. To test, I have now hooked up ITMY Sat. Box. + tester box to the signal chain of ETMY. If I can get the other tester box back from Ben, I will plug in the ETMY sat. box. + tester to the ITMY signal chain. This should tell us something...

Attachment 1: ITMY_satboxSpectra.pdf
ITMY_satboxSpectra.pdf
  12650   Wed Nov 30 14:53:56 2016 SteveUpdateSUSnew sus wire stored in N2 filled dessicator

The new SOS sus wire finally is stored in a nitrogen filled dessicator. This was recommended by Ca. Fine Wire to minimize the aging - oxidation.

The dessicator was pumped down with " aux-drypump " to 1 Torr and than filled up with N2 to 760 Torr. This was repeated 2x and the dessicator was sealed off.

Attachment 1: dessicatorC.jpg
dessicatorC.jpg
Attachment 2: wireN2c.jpg
wireN2c.jpg
  12720   Sat Jan 14 22:39:30 2017 ranaSummarySUSITMY is drifting ?

https://nodus.ligo.caltech.edu:30889/detcharsummary/day/20170114/sus/susdrift/

ITMY is not like the others. Real or just OSEM madness?

  12722   Mon Jan 16 18:54:01 2017 ranaUpdateSUSBS: whitening re-engaged

Found that the BS whitening was off. Gautam says that "it has always been that way" and "there's nothing in the elog about this" and "I have no special relationship with Putin".

I looked at DV and DTT while turning the OSEM whitening back on. As expected, the sensor noise improved by 10x above 10 Hz. The time series shows no problems - its just less fuzzy now.

All OSEM spectra after the switch show on upper panel of plot. Lower panel shows comparison of BS UL before/after. To rotate the DTT PDF landscape output I typed this:

pdftk BS-white.pdf cat 1N output BSwhite.pdf

"if you see something, do something"

Attachment 1: BSwhite.pdf
BSwhite.pdf
  12725   Mon Jan 16 23:25:07 2017 gautamUpdateSUSMC1 SUS electronics investigation

[rana,gautam]

Summary:

  • MC1 glitchy behaviour is back
  • Found a broken LEMO cable, left unplugged for the night -> to be repaired tomorrow
  • Further diagnosis to follow

During the course of Rana's inspection of the general state of the IFO, he commented that there seemed to be several seismic-related IMC lock losses in the time that he had been observing it. This issue looked suspiciously like the the MC1 glitches I had noticed sometime late last year, especially since each time the IMC would unlock, we could see significant amounts of motion on MC REFL. To diagnose, we did the following:

  1. Closed PSL shutter
  2. Ramped down the gains of the MC1 damping loops by factor of 1000 in ~4 secs using z step
  3. Shut down the watchdog for MC1
  4. Observed dataviewer traces for glitches

Sure enough, there were several glitches that occurred in all 5 sensor channels. These glitches varied in size from a few counts (the smaller ones) to 60-70counts for the bigger ones. In the past, squishing the LEMO connector on the front of the PD whitening board (D000210) had apparently made the glitching go away. So tonight, for starters, we squished everything else - Sat. Box connectors, the breakout board from Sat. Box to whitening board on the back of 1X6, and the DB connector on the front of the whitening board. This had no effect - the glitching remained consistent.

Next, Rana pulled out two of the three 4pin LEMOs, and left only those coresponding to UL/LL plugged in - but the glitching persisted in these two channels. We then pulled out the board. It was installed in 1998, but has a sticker on it that says "fixed in 2003". Not sure what the fix was. Visual inspection of the circuit didn't show anything obviously faulty, but it did look like the two MAX333A quad switches (these control whether the whitening is bypassed or not) had been replaced at some point. There are other undesirable features, such as the use of thick film resistors, but nothing that would explain the glitchy behaviour.

Next, we re-inserted the whitening board back into its original slot in the Eurocrate, but switched the cables (both D sub and LEMO, but only on the whitening board end) between the boards for MC1 and MC3 (i.e. MC1 cables were routed through the whitening board that was originally used for MC3, and vice-versa). But the glitches remained consistent on the MC1 channels. So it looks like the board is not a likely culprit.

Finally, we went in and squished all the cables from the PD whitening board to the ADC (via an AA filter board). For some of the LEMO cables from the whitening board, the LEMO backshells were not properly tightened. Rana fixed these before putting them back in. Some of the connectors were also not pushed in tightly enough, Rana heard the click when he pushed them in. The cables from the adaptor board to the ADC itself looked fine, it was screwed on at both ends, and all these connections looked snug enough. In the interest of completeness, Rana also pushed in the backplane connectors on the Eurocrate (these supply the signals from the BIO cards to switch the whitening ON/OFF). The one corresponding to MC1 was indeed a little loose.

Coming back to the control room, we saw that the MC1 LR sensor was dead. After some investigation, Rana found that on the AA filter board end, one of the 4pin LEMOs from the whitening board had one of its wires come unstuck from where it was soldered (this presumably happened while we were squishing cables tonight, as the LR channel was fine before that). Also, there was no heat shrink used on any of the solder joints. Could this explain the glitchy behaviour? Perhaps, but the glitches remained in the 3 channels that were connected. Anyways, I will repair this cable tomorrow, and we can see if this has fixed the problem or not..


Some misc points:

  1. Regarding the adaptor boards that take the PD signals from the satellite box and route it to the whitening board, there are some clamps that hold the IDE connectors in place for MC1, MC2 and MC3 boards, but not for the others (see attached picture). Steve, can we install clamps for all of the boards? [taken care of, see here]
  2. The whitening boards are not screwed in place into the Eurocrate. This should be rectified.

PSL shutter is closed, MC1 watchdog is shutdown for the night.

Attachment 1: 20170116_231625.png
20170116_231625.png
Attachment 2: IMG_7175.JPG
IMG_7175.JPG
Attachment 3: IMG_7174.JPG
IMG_7174.JPG
  12728   Tue Jan 17 21:29:52 2017 gautamUpdateSUSMC1 SUS electronics investigation

 

Quote:
 

After some investigation, Rana found that on the AA filter board end, one of the 4pin LEMOs from the whitening board had one of its wires come unstuck from where it was soldered (this presumably happened while we were squishing cables tonight, as the LR channel was fine before that). Also, there was no heat shrink used on any of the solder joints.

The faulty cable has been re-soldered (with heat shrink) and replaced. All 5 sensor signals appear normal on dataviewer now. I am leaving things in this state for the night, let us see if the glitches return overnight.

PSL shutter remains closed

  12731   Wed Jan 18 11:40:54 2017 gautamUpdateSUSMC1 SUS electronics investigation

After the repair of the faulty LEMO cable, I left MC1 with it's watchdog off overnight. Unfortunately, it looks like the problem still persists. The first attachment shows a second trend plot for the past 15 hours. Towards the left end of the plot, you can see where I re-connected the LEMO cable for the LR/UR channels.

A couple of months ago, I added a BLRMS block for the IMC optics that calculates BLRMS for the shadow sensor output as well as the coil output. Looking at this trend overnight, I noticed that the glitches appear in the coil outputs as well, as shown in the plot below, which is for a 1 hour stretch last night (I used the full data from a 16Hz coil output channel and not the BLRMS, I am not sure if there is a DQ'ed version of the coil outputs?).

Zooming in further to one of these glitches, we can see that the glitches in the coil and shadow sensor signals are in fact coincident.

But given that the watchdog was turned off all this time, the only voltage going to the coils should be the DC bias voltages. So does this not support the hypothesis that the problem lies in the part of the signal chain that supplies the bias voltage to the coils?

Never mind, the "coil output" channel isn't a true readback of the voltage to the coil, but is the calculated damping output (which is not sent to the coils when the watchdog is shutdown...

  12734   Wed Jan 18 14:23:47 2017 gautamUpdateSUSMC1 SUS electronics investigation

As part of the ongoing debugging, I've switched the MC1 and MC3 satellite boxes. Both MC1 and MC3 have their watchdogs shudown for the moment.

  12736   Wed Jan 18 18:44:53 2017 gautamUpdateSUSMC1 SUS electronics investigation
Quote:

As part of the ongoing debugging, I've switched the MC1 and MC3 satellite boxes. Both MC1 and MC3 have their watchdogs shudown for the moment.

In the last 3.5 hours, there has been nothing conclusive - no evidence of any glitching in either MC1 or MC3 sensor channels. I am going to hold off on doing the LEMO cable swap test for a few more hours, to see if we can rule out the satellite box.

  12737   Thu Jan 19 08:25:12 2017 SteveUpdateSUSMC1 SUS electronics investigation
Quote:
Quote:

As part of the ongoing debugging, I've switched the MC1 and MC3 satellite boxes. Both MC1 and MC3 have their watchdogs shudown for the moment.

In the last 3.5 hours, there has been nothing conclusive - no evidence of any glitching in either MC1 or MC3 sensor channels. I am going to hold off on doing the LEMO cable swap test for a few more hours, to see if we can rule out the satellite box.

No change.

Attachment 1: MC1_MC3_ITMY_ETMX_sensors.png
MC1_MC3_ITMY_ETMX_sensors.png
Attachment 2: sensors_UL.png
sensors_UL.png
  12739   Thu Jan 19 12:00:10 2017 gautamUpdateSUSMC1 SUS electronics investigation

Going through the last ~20 hours of data, the MC1 sensor channels look glitch free the entire period. However, there is a ~10min period around 1PM UTC today when there were a couple of glitches ~80 counts in size in all the MC3 sensor channels. The attached shows the full 2k data from all 10 channels (MC1 and MC3 sensors) around this time.

Is this sufficient evidence to conclude that the Satellite boxes are to blame? It's hard to explain why the glitches come and go in this fashion, and also the apparent difference in the length of time for which the glitches persist. Here, in almost 24 hours, there is one incidence of glitching, but in yesterday's trend plot, the glitching remains present over several hours... The amplitude of the glitches, and their coincidence in all 5 channels, seems consistent with what we have been seeing though...

 

  12741   Thu Jan 19 19:56:09 2017 ranaUpdateSUSMC1 SUS electronics investigation

Might be. Or it might be in the satellite box cabling. Hard to tell without a tester. I recommend you squish the cables on there and lock the MC and get back to the usual business. I'll check on sat. box with Ben.

Quote:

 

Is this sufficient evidence to conclude that the Satellite boxes are to blame? It's hard to explain why the glitches come and go in this fashion, and also the apparent difference in the length of time for which the glitches persist. Here, in almost 24 hours, there is one incidence of glitching, but in yesterday's trend plot, the glitching remains present over several hours... The amplitude of the glitches, and their coincidence in all 5 channels, seems consistent with what we have been seeing though...

 

  12742   Fri Jan 20 11:16:30 2017 gautamUpdateSUSMC1 SUS electronics investigation

Both suspensions have been relatively well behaved for the best part of the last two days, since I effected the Satellite Box swap. Today morning, I set about re-enabling the damping and locking the MC. Judging by the wall StripTool, it stayed locked for about 30 mins or so, after which the glitching returned.

Attached is a screenshot of the sensor signals from MC1 and MC3 (second trend), and also the highest band (>30Hz) BLRMS output for the same 10 channels (full data sampled at 16Hz). Note that MC1 and MC3 satellite boxes remain swapped. So the glitches now have migrated to the MC3 channels.

I need to think about whether this is just coincidence, or if me re-enabling the damping has something to do with the re-occurrence of the glitching...


Addendum 4.30pm: I've also re-aligned the Y arm. Its alignment has been stable over the last few hours, despite several mode cleaner lock losses in between, it recovers good IR transmission. The X arm has been re-aligned to green, but I can't get it locked to the IR - everytime I turn the LSC to ETMX on, there seems to be some large misalignment applied to it. c1iscaux was dead, I restarted it by keying the crate. I haven't had time to investigate the X arm locking in detail, I will continue to debug this.

  12745   Mon Jan 23 10:24:01 2017 SteveUpdateSUSMC1 SUS electronics investigation

Two day plot of glitching suspentions: MC3, ITMY and ETMX

Attachment 1: 3glitchingSUS.png
3glitchingSUS.png
  12753   Wed Jan 25 10:46:58 2017 steveSummarySUSoplev laser summary updated

                    Oct.  5, 2015              ETMY He/Ne replaced by 1103P, sr P919645,  made Dec 2014, after 2 years

                   Jan. 24, 2017              ETMY He/Ne replaced by 1103P,  sr P947049,  made Apr 2016,  after 477 hrs running hot

Attachment 1: oplev_sums.png
oplev_sums.png
  12760   Fri Jan 27 14:50:04 2017 SteveUpdateSUS wire standoffs update

The 3 pieces of Sapphire v-groove test cuts are back. They look good. The suspension wire 0.0017" ( 43 micron ) is show on some of the pictures.

  12761   Fri Jan 27 15:36:17 2017 KojiUpdateSUS wire standoffs update

Very nice! I got excited.

  • Don't you ask Calum and co to check the groove size with their microscopes? Just give the samples and the wire.
  • Do we want to make a simple "guitar" setup to measure the vibration Qs with Al piece, glass prism, ungrooved Sapphire, this grooved sapphire, grooved ruby, etc?
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