ID |
Date |
Author |
Type |
Category |
Subject |
11673
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Thu Oct 8 14:14:50 2015 |
ericq | Update | LSC | DRFPMI Progress |
Quote: |
Please clarify: I wonder if you were at the zero offset for CARM and DARM or not.
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Yes, this was at the full DRFPMI resonance. |
11674
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Thu Oct 8 16:48:23 2015 |
Koji | Update | LSC | DRFPMI Progress | Awesome |
11675
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Thu Oct 8 21:35:49 2015 |
rana | Update | LSC | DRFPMI Progress | Give us a lockloss or other kind of time series plot so we can bask in the glory. |
11676
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Fri Oct 9 09:22:38 2015 |
ericq | Update | LSC | DRFPMI Progress | 
Look upon this three second lock, ye Mighty, and rejoice! |
Attachment 1: oct8_allRF.pdf
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11677
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Fri Oct 9 11:24:06 2015 |
Jenne | Update | LSC | DRFPMI Progress | I hope the grappa was already cold, and ready to drink! |
11725
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Mon Nov 2 17:39:01 2015 |
Koji | Frogs | General | DRFPMI celebration | やったー!Yatta! |
Attachment 1: yatta.jpg
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8179
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Wed Feb 27 02:44:39 2013 |
Jenne | Update | Locking | DRFPMI flashes | Before Yuta left, I asked him to restore all optics to last saved values, to avoid hysteresis.
Some interesting modes appear at ETMYT and ETMXT. The cavities aren't super well aligned right now, especially since we have been seeing this input pointing drift, but it's cool to see our first DRFPMI flashes. SRM, in particular, hasn't been aligned since before pumpdown. If I misalign SRM, the mode content at the trans cameras improves somewhat, but it still isn't all low-order modes.
Here is the note that I wrote on youtube describing the video:
DRFPMI Flashing
Upper left is AS, upper right is POP
lower left is Xarm Trans (ETMXT), lower right is Yarm Trans (ETMYT)
Arms were last aligned several hours ago, and we know input pointing drifts, so at least some of the higher order modes in the arm transmissions are due to poor input pointing. All optics are "restored" to their last saved values, including SRM, which has not been aligned since before pumpdown.
TRX DC PD values are flashing to as high as 10
TRY DC PD values are flashing to as high as 7
Since uploading the video, I have seen TRY flash (once) to 45. Yes, forty five!!! Both arms are usually flashing to ~3ish, with an occasional medium flash (5-10), and then a few rare TRY flashes above 20.
We may have officially lost the bet of having arms locked by 9am Monday, but I think Team Grad Student / Postdoc still deserves some beer from Team Faculty / Staff. |
8191
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Wed Feb 27 20:10:43 2013 |
rana | Update | Locking | DRFPMI flashes |
If its true that there have been large flashes, then there indeed might be beer. But first I'd have to see a calibrated plot. And make sure that the flashes are not overamplified due to a whitening filter imbalance.
Is it the readout of a PD with no whitening/antiwhitening? IF so, its much easier to believe. |
675
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Tue Jul 15 12:44:08 2008 |
John | Summary | Locking | DRFPMI with DC readout | Rob, John
Last night, despite suspect alignment, we were again able to reduce the CARM offset to zero using
the RF signal.We were also able to transfer to dc readout taking calibrated spectra in both states.
DC readout shows a marked improvement over RF above ~1kHz but introduces some noise around 100Hz.
Broadband sensitivity appears to be more than ten times worse than previously. The calibration
being used remains to be confirmed.
Engaging the ETMY dewhitening caused lock to be lost. We'll check this today. The OMC alignment loops
may also need some attention.
We looked at REFL_166 as a candidate for CARM, at present POX still looks better.
The DARM filters were modified to reduce excess noise around 3Hz. Updating filter coefficients does
not cause loss of lock. |
11718
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Tue Oct 27 03:56:52 2015 |
ericq | Update | LSC | DRFPMI work | A handful of DRFPMI locks tonight, longest one was ~7 minutes.
EPICS/network latency has been a huge pain tonight. The locking script may hang between commands at an unstable place, or fail to execute commands altogether because it can't find the EPICS channel. This prevented or broke a number of locks.
I made some CARM OLG and crossover measurements, and found the AO gain for the right crossover freq (~100Hz) to be ~8dB different than what's in the PRFPMI script, which is weird. Right now, the CARM bandwidth / ability to turn on boosts is limited by the gain peaking in the IMC CLG due to the high-ish PC/PZT crossover frequency we're using.
Gautam turned on some sensing excitations during the last couple of locks, but they weren't on for very long before the lock loss. Hopefully I can pull out at least some angles from the data.
I'm also more convinced that the PRC angular FF needs retuning; there is more residual motion on the cameras than I'm used to seeing. I've taken more data that I'll use to recalculate a wiener filter tomorrow.
The PMC, ALSX beat and ITMX oplev all needed a reasonable pitch realignment tonight. |
11722
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Thu Oct 29 03:25:49 2015 |
ericq | Update | LSC | DRFPMI work | [ericq, Gautam]
The length of DRFPMI lock did not increase much tonight, but we got a ~80 second sensing matrix measurement, and got the CARM bandwidth up to 10k with two boosts on.
NB: I did not measure the CARM loop gain at its excitation frequency, so the plotted sensing element is supressed by the CARM loop. However, this is still useful for gauging the size of the PRCL signal vs. the residual CARM fluctuations. The excitations are fairly closely spaced between 309 and 316 Hz.
For comparison, I'm also re-plotting the DRMI sensing measurement from a few weeks back taken at CARM offset of -4. We can see some change in the PRCL sensing, likely due to the CARM-coupled path. MICH/PRCL sadly looks pretty degenerate, but REFL55 looks more reasonable.

I think the main limitation tonight was SRC stability. Even before bringing CARM to zero offset, we would see occasional sharp dives in AS110 power. One lockloss happened soon after such an occurance, but I checked the values, and it was not sufficient to trigger the Schmitt trigger down; instead it may have been a real optical loss of signal. The SRCL OLTF looks sensible.
Random notes:
- Aux X laser was glitching yet again, twiddled laser current to 1.90A from the 1.95A that I twiddled it to on Monday from the nominal 2.0A.
- When aligning the PRMI, I saw both ITMs' oplevs shift by a few urad in both pitch and yaw when engaing/breaking the lock, but this was not repeatable.
- I reduced the AS110 whitening gain by 9dB, since the DC values were a few thousands, and I wanted to make sure there were no stray ADC saturations. This didn't change lock stability though.
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Attachment 1: DRFPMI.pdf
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Attachment 2: DRMIarms.pdf
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11726
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Tue Nov 3 03:12:46 2015 |
ericq | Update | LSC | DRFPMI work | Tonight was kind of a wash.
We spent some time retaking single arm scans with Gautam's frequency counting code to confirm the linewidths he measured before his most recent round of code improvements. During this, ETMX was being its old fussy self, costing us gentle realignment time. For the time being, we started actuating on ITMX for single arm locks. Also, out of superstition, I changed the static position offset that had been at +1k for the last N months to -1k.
ETMX broke us out of a few DRFPMI lock trials as well, as did poor SRM alignment. I finally set up dither alignement settings for SRM in DRMI though, which helped (even in the arms-held-off-resonance situation). I still prefer doing the PRM/BS dither alignment in a carrier PRMI lock, because I think the SNR should be better than DRMI.
We know that the ETMX excursions can happen without length drive exciting them, but also that length drives certainly can excite them. For future locks, I'm going to try out avoiding ETMX drive altogether; the sites use a single ETM for their DARM actuation and let the CARM loop take care of the resultant cross coupling, so hopefully we can do the same without angering the mode cleaner.
Anyways, we didn't really ever make it far enough to do anything interested with the DRFPMI tonight  |
10700
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Wed Nov 12 01:30:39 2014 |
ericq | Update | LSC | DRFPMI, PRFPMI HOM resonances | I did some simulations to see if we are susceptible to HOM resonances as we reduce the CARM offset. I restricted my search to HG modes of the Carrier+[-55,-11,0,+11,+55]MHz fields with n+m<6, and used all the real physical parameters I could get ahold of.
In short, as I change the CARM offset, I don't see any stray resonances within 2nm of zero, either in PRFPMI or DRFPMI.
Now, the mode matching in my simulation is not the real mode matching our real interferometer has. Thus, it can't tell us how much power we may see in a given mode, but it can tell us about our susceptibility to different modes. I.e. if we were to have some power in a certain mode coming out of the IMC, or present in the vertex, we can see what it would do in the arms.
Since my simulation has some random amounts of power in each HOM coming into the interferometer, I simply swept the CARM offset and looked for peaks in the power of each mode. Many of the fields exhibited gentle slopes over the range, and we know we ok from 3nm->~100pm, so I made the selection rule that a "peak" must be at least 10 times as big as the minimum value over the whole range, in order to see fields that really do have CARM dependence.
In the following plots, normalized IFO power is plotted and the locations of HOM peaks are indicated with circles; their actual heights are arbitrary, since I don't know our real mode content. However, I'm not really too concerned, since all I see is some -11MHz modes between 2-3nm of full resonance, where we have no problem controlling things... Also, all of the carrier HOMs effectively co-resonate with the 00 mode, which isn't too surprising, and I didn't include these modes in the plots.
 
Finally, I visually inspected the traces for all of the modes, and didn't really find anything else peeking out.
Code, plots attached. |
Attachment 1: HOMs.zip
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10705
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Wed Nov 12 21:18:32 2014 |
ericq | Update | LSC | DRFPMI, PRFPMI HOM resonances | So, with my last entry, I was guilty of just throwing stuff into the simulation and not thinking about physics... so I retreated to Siegman for some algebraic calculations of the additional Guoy phase accumulated by the HOMs in the arms -> their resonant frequencies -> the arm length offset where they should resonate. Really, this isn't completely precise, as I treated the arms independently, with slightly differing ETM radii of curvature, but I would expect the "CARM Arm" to behave as a sort of average of the two arm cavities in this regard. (EDIT: Also, I didn't really consider the effect of the coupled vertex cavities... so there's more to be done)
The basic idea I used was:
- Assume ITMs are effectively flat, infinite Rc
- Use 40mwiki values for ETM curvatures
- Each additional HG order adds arccos(sqrt(1 - Larm/Rc)) of Guoy phase for a one way trip down the cavity (Eqn 19.19 in Sigman)
- For each HOM order up to 5 of the carrier and first order sidebands, add the appropriate phase shift
- fold it onto +-FSR/2 of the carrier 00 resonance, convert to m
In practice, I threw together a python script to do this all and print out a table. I've highlighted the values within 10nm, but the closet one is 3.8nm
Results:
########## X Arm HOM Resonance Locations in nm ##########
Mode Order: 0 , 1 , 2 , 3 , 4 , 5
Carrier : +0, +156.21, -219.58, -63.376, +92.832, +249.04
LSB 11 : +59.563, +215.77, -160.02, -3.8126, +152.4, -223.4
USB 11 : -59.563, +96.645, +252.85, -122.94, +33.269, +189.48
LSB 55 : -234.18, -77.975, +78.233, +234.44, -141.35, +14.857
USB 55 : +234.18, -141.61, +14.6, +170.81, -204.98, -48.776
########## Y Arm HOM Resonance Locations in nm ##########
Mode Order: 0 , 1 , 2 , 3 , 4 , 5
Carrier : +0, +154.82, -222.35, -67.531, +87.292, +242.11
LSB 11 : +59.313, +214.14, -163.04, -8.218, +146.6, -230.57
USB 11 : -59.313, +95.51, +250.33, -126.84, +27.978, +182.8
LSB 55 : -235.43, -80.611, +74.212, +229.04, -148.14, +6.6809
USB 55 : +235.43, -141.74, +13.08, +167.9, -209.27, -54.452
Code is attached. Hopefully no glaring mistakes!
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Attachment 1: HOMlist.py.zip
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1670
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Fri Jun 12 02:01:03 2009 |
rob | Update | Computer Scripts / Programs | DRM matrix diagonalization | I started two scripts, senseDRM and loadDRMImatrixData.m, which Peter will bang on until they're correct. They're in the $SCRIPTS/LSC directory. The first is a perl script which uses TDS tools to drive the DRM optics and measure the response at the double demod photo-detectors, and write these results to a series of files loadable by matlab. The second loads the output from the first script, inverts the resulting sensing matrix to get an input matrix, and spits out a tdswrite command which can be copied and pasted into a terminal to load the new input matrix values.
What's left is mainly in figuring out how to do the matrix inversion properly. Right now the script does not account for the output matrix, the gains in the feedback filters at the measurement frequency, or the fact that we'll likely want the UGF of our loops to be less than the measurement frequency. Peter's going to hash out these details. |
11637
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Wed Sep 23 03:08:50 2015 |
ericq | Update | LSC | DRMI + ALS Arms | [ericq, Gautam]
We can reliably lock the DRMI with the arms held off on ALS. 
I have not been able to hold it at zero CARM offset; but this is probably just a matter of setting up the right loop shapes with enough phase margin to handle the CARM fluctuations ( or figuring out high bandwidth ALS...)
Right now, it's the most stable at CARM offsets larger (in magnitude) than -1. Positive CARM offsets don't work well for some reason.
The key to getting this to work was to futz around, starting from the misaligned arms DRMI settings, until brief locks were seen (triggering all 3 DRMI DoFs on POP22, since the correct AS110 sign was amiguous). I could tell from how the control signals responded to gain changes that REFL165Q, which was being used as the MICH error signal, was seeing significant cross coupling from both PRCL and SRCL, suggesting the demod angle of REFL165 had to be adjusted. I randomly tweaked the REFL165 demod angle until a 20 second lock was achieved, with excitations running. Then, I downloaded that data and analyzed the sensing matrix. This showed me that the REFL33 demod angle was ok, and the PRCL-from-SRCL subtraction factor determined with the arms misaligned was still valid. The main difference was indeed the SRCL angle in REFL165.
With the REFL165 demod angle properly adjusted, the DRMI would briefly lock, but the DRMI had become somewhat misaligned at this point, and the SRC could be seen to mode hop. Interestingly, the higer order modes had an opposite sign in AS110, with respect to the TM00. At that point, I went back to PRMI on carrier to dither-align the BS and PRM.
With alignment set, the DRMI would lock on TM00 readily, still only triggering on POP22. I set the AS110 angle, and moved SRCL triggering over to that, which sped up acquisition even more. The input matrix and FM gains from no-arms DRMI still work for acquistion; UGF servos were used to adjust overall gains a bit.
At CARM offsets larger in magnitude than -1, the DRMI lock seems indefinite. I just broke it to see how fast it would acquire; 3 seconds. 
Lastly, here is the sensing matrix at CARM offset of -4, measured over five minutes. REFL11 is the only degenerate looking PD. Thus, I feel like controlling the DRMI of the DRFPMI should be more managable than I had feared.

(I didn't include/excite CARM or DARM, because I'm not sure it would really mean anything at such a large CARM offset) |
Attachment 1: DRMIarms.pdf
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11638
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Wed Sep 23 10:31:49 2015 |
ericq | Update | LSC | DRMI + ALS Arms | Looking good. How many meters of CARM is '-1 counts'? |
11639
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Wed Sep 23 12:51:03 2015 |
Jenne | Update | LSC | DRMI + ALS Arms | Nice!! |
9049
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Thu Aug 22 02:40:12 2013 |
Jenne | Update | LSC | DRMI Locked for 1+ minute!!!!!! | [Jenne, Koji]
The DRMI has been locked!! And at least one time, it was for more than one minute!!

We are not 100% sure yet that it's correctly sideband locked. The test of this was to put a 50% BS in front of the AS camera (so after the beam has gone to AS55), and send the light over to a PDA10CF Thorlabs PD. I locked the Michelson on carrier for the alignment of this diode. Then I strung a cable to the control room, and plugged it into the RF spectrum analyzer. (First, I had turned off the green beat PD power, so there wasn't any RF stuff on the line that I unplugged). It's hard to watch the screen and a tv / dataviewer at the same time, so I've taken a video, so that we can see the nicely locked round DRMI beam on the AS camera, and the spectrum analyzer. My phone is working very hard at uploading the video, but we may have to wait until tomorrow for that. However, I think that we're locked on the 55MHz sideband. (Also, maybe I'm too tired or excited or something, but how do you make the real cameras take video??)
EDIT: Video uploaded. Pause the video at 10 seconds, and you'll see that we've got a strong 110MHz peak!! Hoooray! The TV in the upper right side of the video is AS. You can see as we flash, the peaks go up and down. When there's no resonance, the 110 peak goes away. (Ex., when I'm PRMI locked on the sideband, there isn't a visible peak).
Alignment procedure was as normal: Lock and align the arms. Misalign ETMs. Check that MICH fringes look good (ASS does a nice enough job that I don't actually lock and align the Michelson anymore). Restore the PRM. Lock PRMI. Tweak PRM alignment to maximize POP110I. At this point, Koji and I played a little with the PRMI, but when we finished with that, we restored the SRM, and tweaked its alignment by making nice overlap on the AS camera.
Then, we tried some DRMI settings, started seeing some locks, and played a bit with trying to optmize the settings that we have.
DETAILS:
PRMI settings:
PRCL ASC is on (with loop triggering). MICH gain = -0.8, PRCL gain = +0.05. FM4, FM5 always on, FM2 triggered. Loop and filter module triggering on POP22I. No power normalization. MICH and PRCL locked on REFL55 I&Q, with 1's in the LSC input matrix. PRCL actuating on PRM with +1, MICH actuating on BS with +0.5, PRM with -0.267.
I took transfer functions between REFL55 I&Q and REFL11 I&Q, to determine the relative gains and signs. REFL11I's gain should be -18dB relative to REFL55I, with the opposite sign. We tried PRMI locking with MICH = 1*REFL55Q and PRCL = -0.125*REFL11I for the input matrix. Still no power normalization (we haven't used power norm at all today, so I'll quit writing that).
I took transfer functions between REFL55 I&Q and REFL33 I&Q. REFL33I's gain is -8dB relative to REFL55I, but they have the same sign. We tried locking PRMI with MICH = 1*REFL55Q and PRCL = +0.6*REFL33I. Success.
Next up, some Optickle simulations, to help us go in the right direction for DRMI locking. I checked the signs of the error signals REFL55I (PRM sweep), REFL11I (PRM sweep) and REFL55Q (MICH sweep) in both PRMI and DRMI configurations. For all of these cases, the signs were the same (i.e. no sign flips needed to happen for DRMI locking, relative to PRMI locking). I checked the sensing matrices for DRMI and PRMI for those same signals, and took the ratios of the sensing matrix elements. This gave me the ratio of optical gains for each error signal, in the DRMI case vs. PRMI case, so any servo gain changes should be the inverse of these numbers. These numbers are all DRMI/PRMI: REFL55I PRCL response = 0.76, REFL11I PRCL response = 0.99, REFL55Q MICH response = 18. So, when trying to lock the DRMI, we wanted to keep the gains for PRCL about the same, reduce the servo gain for MICH by a factor of ~20, but keep the same signs for everything.
In doing that, we started seeing some short DRMI locks, so we twiddled some parameters (mostly the elements in the LSC input matrix) a bit. We eventually settled on: PRCL = -0.125*REFL11I, MICH = 0.1*REFL55Q, and SRCL = 1.0 * REFL55I. The output matrix was the same (MICH pushing on BS and PRM, PRCL on PRM), with the addition of a +1 in the SRCL -> SRM element. For all 3 degrees of freedom (PRCL, MICH, SRCL), FMs 4 and 5 were always on. For PRCL, FMs 2,3,6 were triggered to come on after 0.5 seconds of delay. The PRCL FM triggers helped enormously. I tried several other things, including changing the MICH input matrix element up and down in value, changing the SRCL input matrix element up and down in value, and engaging triggering for a few different filters in the MICH and SRCL degrees of freedom. However, none of these made things better, and several made things worse. Most notably, for SRCL, engaging triggering for FMs 2 and 3 kicked the cavities out of lock, which implies that perhaps our gain isn't high enough yet (and thus our UGF isn't very high yet). I changed FM1 of SRCL to be +3dB of gain (from +10dB), and it would live through that coming on (trigger delayed by 1 sec, then ramping up over 1 second), but within a second after the filter finishing coming on, the cavity would fall out of lock (not violently kicked, just not locked anymore).
At this point, we were trying to figure out a way to confirm what kind of lock we had. I checked Optickle again, and we do not expect to see a significant change in POP110I between the PRMI and DRMI cases, so that isn't a useful check. We dreamed of having our AS110 demod board, or the AS OSA set up, but neither of those was going to happen tonight. Instead, Koji suggested hooking up the PD, and looking directly at the output.
To-do: Set up the AS OSA. Also, perhaps temporarily borrow the 110 demod board from POP. We were triggering on POP22 tonight, and that seemed to work okay.
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9050
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Thu Aug 22 07:57:57 2013 |
Lisa | Update | LSC | DRMI Locked for 1+ minute!!!!!! | Very nice!! I was wondering, shouldn't the driving matrix be such that MICH pushes on SRM as well? |
9051
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Thu Aug 22 10:20:32 2013 |
kiwamu | Update | LSC | DRMI Locked for 1+ minute!!!!!! | Wonderful ! I like the video -- the spatial mode looks pretty clean and much cleaner than what I observed in the old days.
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9052
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Thu Aug 22 13:03:40 2013 |
Jenne | Update | LSC | DRMI Locked for 1+ minute!!!!!! |
Quote: |
Very nice!! I was wondering, shouldn't the driving matrix be such that MICH pushes on SRM as well?
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Hmmm, yes, that's a very good point. I think you're right, and I'll give that a try today. |
9053
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Thu Aug 22 13:20:54 2013 |
Koji | Update | LSC | DRMI Locked for 1+ minute!!!!!! | Don't go for a hacky solution. We want to climb a staircase step by step.
Prepare an independent 110MHz demod ports.
Quote: |
To-do: Set up the AS OSA. Also, perhaps temporarily borrow the 110 demod board from POP. We were triggering on POP22 tonight, and that seemed to work okay.
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9060
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Sat Aug 24 00:11:07 2013 |
Koji | Update | LSC | DRMI Locked with improved lock streatches | Friday night locking
Much more stable DRMI lock was achieved, partly thanks to the Friday-night quiet seismic,
and partly because of the improved servo gain and LF boosts
55MHz thru-put
I wanted to confirm the enhancement of the 110MHz signal at the AS port.
As the AS110 PD is placed in the CCD path, there is nothing visible with PRMI.
The Thorlabs PD was moved to the main AS path. Now the AS110 PD is receiving 50% of the power.
With PRMI 110MHz peak was -30dBm (As it was fluctuating, anything more precise number did not make sense)
When the DRMI was locked, the peak was enhanced to 0dBm.
The 2f signal comes from the beat between the sidebands.
Thus the amplitude of the intensity is proportional to the power of the sidebands (assuming the +1 and -1 order sidebands have the same amplitude)
-30dBm -> 0dBm means 31.6 times amplitude of the intensity. Therefore the amplitude transmission of the sidebands is 5.6 times more. (Is this true?)
According to the wiki, the AS port thru-put (i.e. power transmission) for the 55MHz sideband is 0.0026 and 0.43 for PRMI and DRMI respectively.
This corresponds to the amplitude difference of ~13. So we still have only half of the sidebands leaking out from the IFO. This could be attributed
to both the smaller PR gain and SR gain.
Locking setup
Same as the one Jenne used the other day. Later I engaged several additional triggers.
The following is the trigger setting I used
MICH: Delay 2 sec, FM1/FM2/FM3/FM6/FM7
PRCL: Delay 0.5 sec, FM2/FM3/FM6
SRCL: Delay 5 sec, FM1/FM2/FM3/FM6
SRCL FM1 was modified from +3dB to +6dB
Lock stability
Once lock is acquired, it lasts tens of minutes. (see the attached striptool chart.)
Even the lock is lost, it reacquires quickly.
The videos to show the lock acquisition and the in-lock stability are attached below.
The AS port beam is very round. It is not so shaky, but some yaw motion is visible.
The mode at the AS port is defined by the SRM, putting a QPD at the AS port would help to
stabilize the spot.
IFO state upon leaving
I left the 40m with the arms aligned, PRM and SRM slightly misaligned, and LSC setting is for the DRMI locking.
TO DO
- AS110I/Q for triggering
- PRCL/MICH/SRCL normalization
- We should resurrect the IFO config scripts.
- Remove BS->SRCL actuation coupling
- Handing off to 3f signals (preparation for the full lock)
- Improve ALS stability
- SRM ASC: AS QPD for SRM control
Lock Acquisition Video
UL (REFL) / UR (POP)
LL (AS) / LR (PRM Face)
In-lock video
UL (REFL) / UR (POP)
LL (AS) / LR (PRM Face)
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Attachment 1: Screenshot-Untitled_Window.png
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9061
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Sun Aug 25 06:07:11 2013 |
rana | Update | LSC | DRMI Locked with improved lock streatches | We're ready for using the auto configure.
We can put our scripts for the MICH, PRMI, and DRMI into the IFO CONFIGURE screens for now and then it should be easy to get them into the Guardian once Jamie has the bugs worked out.
This screen can also be used to setup and start the dither alignment for each configuration (once we have one working for DRMI / SRM).
Also, now that the notches/bandstop filters for the violin modes have been move from the SUS into the LSC, we should fix the triggering to engage them a few seconds after the boosts. |
13367
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Mon Oct 9 01:29:26 2017 |
gautam | Update | LSC | DRMI Nosie Budget v3.0 | Summary:
I spent this weekend doing a more careful investigation of the DRMI noise. I think I have some new information/insights. Attachment #1 is the noise budget (png attached because pdf takes forever to upload, probably some ImageMagick problem. The last attachment is a tarball of the PDF). Long elog, so here are the Highlights:
- Coil de-whitening does result in small improvement in noise in the 60-200Hz band.
- Above 200Hz, we seem to be limited by "Dark" noise. More on this below.
- The coupling from SRCL->MICH is the other limiting noise in the 60-200Hz band now.
Sensing Matrix Measurement:
- I rotated the AS55 demod phase from -42 degrees to -82 degrees, the idea being to get more of the MICH error signal in AS55_Q.
- Consequently, the MICH servo gain has been lowered from -0.035 to -0.021. Settings have been updated in the snap file used by the locking script.
- Seems to have worked.
- Attachment #2 is the measured sensing elements.
- One major source of uncertainty in these sensing element numbers is the actuator gains for PRM, SRM and BS. The coil driver electronics for the latter two have been modified recently, and for them, I am using numbers from this elog scaled by the expected factor as a result of removing the x3 gain in the de-whitening boards for SRM and BS.
MICH OLTF
- Measurement was done in lock using the usual IN1/IN2 method.
- Model made by loading the FOTON filters + assumed models for the BS pendulum and AA/AI filters in Matlab, and fitting to an overall gain + delay.
- Attachment #3 shows the agreement between measurement and model.
- The model was exported and used to invert in-loop signals to their out-of-loop counterparts in the noise budget.
DAC Noise
- I had claimed that turning on the coil de-whitening did not improve the MICH noise.
- This was not exactly true - I had only compared MICH noise with the BS de-whitening turned ON/OFF, while the ITM de-whitening was always on.
- Turns out that there is in fact a small improvement - see Attachment #4 (DTT crashes everytime I try to print a pdf, so png screenshot will have to do for now).
- I have also changed the way in which DAC noise is plotted in the Noise Budget code:
- I used to directly convert the measured voltage noise (multiplied by appropriate scalar to account for quadrature sum of 4 coils each in 3 optics) to displacement noise using the sensing measurement cts/m values.
- Now I convert the measured voltage noise first to current noise (knowing the series resistance), then to force noise (using the number 0.016 N/A per coil), then to displacement noise (assuming a mirror mas of 250g).
- Quadrature sum is again taken for 4 coils on 3 optics.
- I've also added the option to plot the DAC noise with the de-whitening filter TF applied (taking care that the maximum of filtered DAC noise / coil driver electronics noise is used at each frequency).
- So the major source of uncertainty in the calculated DAC noise is the assumed actuator gain of 0.016 N/A.
The DAC noise is not limiting us anywhere when the coil de-whitening is switched on.
Dark Noise
I think this is the major find.
- The dark noise spectrum is measured with:
- the PSL shutter closed
- the AS55 I and Q analog whitening filters (and corresponding digital de-whitening filters) engaged, to mimic the operating conditions under which the in-lock error signal is acquired.
- Comparing the blue and black traces, it is clear that turning on the analog whitening is having some effect on the dark noise.
- However, the analog whitening filters should suppress the ADC noise by ~30dB @ 100Hz - so assuming 1uV/rtHz, this would be ~30nV/rtHz @100Hz.
- But the measured noise seems to be ~5x higher, with 4*10^-4 cts/rtHz translating to roughly 120nV/rtHz.
- The photodiode dark noise is only 15nV/rtHz according to the wiki. Where is this measured?
So I don't understand the measured Dark Noise level, and it is limiting us at frequencies > 200Hz. Some busted electronics in the input signal chain? Or can the LSC demod daughter board gain of ~5 explain the observed noise?
Shot noise
- The DC power on AS55 photodiode was measured to be ~13mW with the SRM misaligned.
- This corresponds to ~100cts peak amplitude on the ASDC channel (derived from AS55 photodiode).
- In the DRMI lock, the ASDC level is ~200cts.
- I used these numbers, and equation 2.17 in Tobin's thesis, to calculate this curve.
Edit 1730 9 Oct: I had missed out the factor of 5 gain in the demod board in calculating the shot noise curve. Attachment #7 shows the corrected shot noise level. Explicitly:
, where is to convert shot noise in W to displacement units.
AUX coupling
This is the other find.
- While chatting with Gabriele, he suggested measuring the SRCL->MICH and PRCL->MICH cross couplings.
- I injected a signal in SRCL servo EXC channel, and adjusted amplitude till coherence in MICH_IN1 was good.
- The actual TF measured was MICH_IN1 / SRCL_IN1 (so units of cts/ct).
- My multiplying the in-lock PRCL and SRCL IN1 signals by these coupling coefficients (assumed flat in frequency for now, note that measurement was only made between 100Hz and 1kHz), I get the trace labelled "AUX coupling" in Attachment #1 (this is the quadrature sum for SRCL and PRCL couplings).
- Also repeated for PRCL -> MICH coupling in the same way.
- Measurements of these TFs and coherence are shown in Attachment #5 (again png screenshot because of DTT).
- However, there is no significant coherence in MICH/SRCL or MICH/PRCL in this frequency range.
This seems to be limiting us from saturating the dark noise once the coil de-whitening is engaged. But lack of coherence means the mechanism is not re-injection of SRCL/PRCL sensing noise? Need to think about what this means / how we can mitigate it.
OL A2L coupling
- I didn't measure these
- These couplings would have changed because I modified the Oplev loop shapes to allow engaging of coil de-whitening filters.
- But anyways, their effect will only be below 100Hz because I made the roll-offs steeper.
Still to measure (but not likely to be limiting us anywhere in the current state):
- Laser intensity noise -> MICH coupling (using AOM).
- Laser frequency noise -> MICH coupling (using CM board IN2).
- Oscillator noise (amplitude + phase) -> MICH coupling (using AM/FM input of Marconi).
I've also made several changes to the NB code - will push to git once I finish cleaning stuff up, but it is now much faster to make these plots and see what's what. |
Attachment 1: DRMI_NB.png
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Attachment 2: DRMI1f_Oct8.pdf
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Attachment 3: MICH_OLTF_model.pdf
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Attachment 4: MICH_noises.png
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Attachment 5: AUX_couplings.png
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Attachment 6: C1NB_disp_40m_MICH_NB_2017-10-08.pdf.tar.gz
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Attachment 7: MICH_NB_corrected.png
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Mon Oct 9 11:55:01 2017 |
Koji | Update | LSC | DRMI Nosie Budget v3.0 | My last characterization of the AS55 PD was on Feb 2013. ELOG 8100
There I said the dark noise at the PD output was 16nV/rtHz. I don't have the measurement of the Voltage noise at the output of the demod board.
Note that the PD can only be limited by shot noise when the DC current is larger then 4mA. |
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Tue Nov 7 17:45:05 2017 |
gautam | Update | LSC | DRMI Nosie Budget v3.1 | Some days ago, I had tried to measure the SRCL->MICH and PRCL->MICH cross couplings using broadband noise injected between 120-180 Hz, a frequency band chosen arbitrarily, in hindsight, I could have done a more broadband test. I've spent some time including the infrastructure to calculate "White-Noise TFs" in the noise budgeting code, where a transfer function is estimated by injecting a "broadband" excitation into a channel of interest, and looking at the resulting response in MICH. I figured this would be useful to estimate other couplings as well, e.g. laser intensity nosie, oscillator noise etc.
I estimate the transfer function of the coupling using the relation (MICH is the median ASD of the MICH error signal in the below expression, and similarly for PRCL)

Attachments #1 and #2 show the spectra of the MICH, PRCL and SRCL signals during 'quiet' times and during the injection, while Attachment #3 shows the calculated coupling TFs using the above relation. These are significantly different (more than 10dB lower) than the numbers I reported in elog 13367, where the measurement was made using swept sine. As can be seen in the attached plots, the injected broadband excitation is visible above the nominal noise level, and I calculated the white noise TFs using ~5mins of data which should be plenty, so I'm not sure atm what to make of the answers from swept-sine and broadband injections being so different.
Attachment #4 shows the noise budget from the October 8 DRMI lock with the updated SRCL->MICH and PRCL->MICH couplings (assumed flat, extrapolated from Attachment #2 in the 120-180Hz band). If these updated coupling numbers are to be believed, then there is still some unexplained noise around 100Hz before we hit the PD dark noise. To be investigated. But if Attachment #4 is to be believed, it is not surprising that there isn't significant coherence between SRCL/PRCL and MICH around 100Hz.
Nov 8 1600: Updating NB to inculde estimated Oplev A2L.
Quote: |
AUX coupling
This is the other find.
- While chatting with Gabriele, he suggested measuring the SRCL->MICH and PRCL->MICH cross couplings.
- I injected a signal in SRCL servo EXC channel, and adjusted amplitude till coherence in MICH_IN1 was good.
- The actual TF measured was MICH_IN1 / SRCL_IN1 (so units of cts/ct).
- My multiplying the in-lock PRCL and SRCL IN1 signals by these coupling coefficients (assumed flat in frequency for now, note that measurement was only made between 100Hz and 1kHz), I get the trace labelled "AUX coupling" in Attachment #1 (this is the quadrature sum for SRCL and PRCL couplings).
- Also repeated for PRCL -> MICH coupling in the same way.
- Measurements of these TFs and coherence are shown in Attachment #5 (again png screenshot because of DTT).
- However, there is no significant coherence in MICH/SRCL or MICH/PRCL in this frequency range.
This seems to be limiting us from saturating the dark noise once the coil de-whitening is engaged. But lack of coherence means the mechanism is not re-injection of SRCL/PRCL sensing noise? Need to think about what this means / how we can mitigate it.
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Attachment 1: SRCL_MICH_whitenoise_tf.pdf
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Attachment 2: PRCL_MICH_whitenoise_tf.pdf
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Attachment 3: MICH_aux.pdf
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Attachment 4: C1NB_disp_40m_MICH_NB_2017-10-08.pdf
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Wed Nov 8 09:37:45 2017 |
rana | Update | LSC | DRMI Nosie Budget v3.1 | why no oplev trace in the NB ?
#4 shows the noise budget from the October 8 DRMI lock with the updated SRCL->MICH and PRCL->MICH couplings (assumed flat, extrapolated from Attachment #2 in the 120-180Hz band). If these updated coupling numbers are to be believed, then there is still some unexplained noise around 100Hz before we hit the PD dark noise. To be investigated. But if Attachment #4 is to be believed, it is not surprising that there isn't significant coherence between SRCL/PRCL and MICH around 100Hz
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also, this method would work better if we had a median averaging python PSD instead of mean averaging as in Welch's method. |
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Wed Nov 8 09:59:12 2017 |
gautam | Update | LSC | DRMI Nosie Budget v3.1 | The Oplev trace is missing for now, as I have not re-measured the A2L coupling since modifying the Oplev loop shape (specifically the low pass filter and overall gain) to allow engageing the coil de-whitening.
The averaging for the white noise TFs plotted is computed using median averaging - I have used a python transcription of Sujan's matlab code. I use scipy.signal.spectrogram to compute the fft bins (I've set some defaults like 8s fft length and a tukey window), and then take the median average using np.median(). I've also incorporated the ln(2) correction factor.
It seems like GwPy has some in-built capability to compute median (and indeed various other percentile) averages, but since we aren't using it, I just coded this up.
Quote: |
why no oplev trace in the NB ?
also, this method would work better if we had a median averaging python PSD instead of mean averaging as in Welch's method.
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Mon Feb 9 16:05:01 2009 |
Yoichi | Update | LSC | DRMI OK | After the ISS work, I aligned the IFO and confirmed that DRMI locks with good SPOB and AS166 values. |
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Fri Sep 14 00:56:13 2012 |
Jenne | Update | General | DRMI aligned | [Rana, Jenne]
We aligned the DRMI, and have concluded that it looks good enough that we should close up and pump down soon. We still need to use the camera to check things, and get all pickoff beams out of the chambers, so don't get too excited yet.
We looked at the mode matching telescope's calculated beam propagation, and since we're using spherical telescope mirrors at non-zero degree incidence angle, we expect an astigmatism about like what we are seeing on the AS camera. This matches up with the measurements that Mike posted from his and Q's measurements earlier today. We think that it has 'always' been this way, and someone just picked a camera position such that the beam used to look more round than it does now.
We aren't entirely sure what's up with the SRM - it almost looks like the pitch and yaw are coupled, but it was pretty easy to align the PRMI. We don't see any evidence of the crazy, crappy beam that we did before the vent. This means we have fixed most of the bad clipping problems we were seeing over the last ~year.
In the process of aligning the DRMI, we fixed up the input beam alignment - we were not hitting the exact centers of the MMT mirrors (in pitch, mostly), so we fixed that, and propagated the alignment fix through the chain. In all, we touched the knobs on PZT1, MMT1, MMT2, PZT2. The beam then went through the SRM, and we touched a few of the output steering mirrors to get the beam centered on all mirrors.
I remeasured the MC spot positions, and they're a little worse than they have been. Some of the spots seem to be off by 1.75mm (or less) on MC 1 and 3. The numbers, MC1,2,3 pitch, then MC1,2,3 yaw are: 1.749759 9.744013 1.025681 -0.791683 -1.338786 -1.779958
A question to consider before doing the final-final alignment checking is: do we need to get the MC spots centered better than this, especially in light of the potential PMC axis having moved? |
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Wed Sep 19 01:08:48 2012 |
Jenne | Update | General | DRMI aligned again | The DRMI was aligned once again tonight.
Here's a video: http://youtu.be/Cy8nHL9yMeM (Can someone please tell me / remind me how to make the elog embed videos?!?)
Description of video:
Video capture of AS camera.
NOTE: The beam is a few centimeters above ETMY with this alignment, so it will not be final.
Beginning is ITMY only.
ITMX is realigned to form MICH.
PRM is realigned to form PRMI.
SRM is realigned to form DRMI.
PRM is misaligned to form SRMI.
ITMX is misaligned to form SRY.
With this alignment, I opened up the ETMY door to find the beam there. The beam is ~half on, ~half off of the top of the glass baffle. Not the top of the hole, but the top of the piece of glass. This means that it's many centimeters too high at ETMY. This helps explain why, while swinging PZT2 around the other day, I could not see any beam on the cage. It did, however, look pretty close (within a centimeter....I didn't look closer than that since it was so off in pitch) to centered yaw-wise.
Tomorrow I'd like a Clean assistant to help tweak PZT2 to hit the center of ETMY. We'll need to put the 45 degree target back on to make sure that we don't end up pointing funny down the arm. Then I'll realign the DRMI one more time.
Tonight, I can't check the full AS path, or any of the REFL path once it diverges from the main path. Steve's new contraption (which is awesome!) doesn't have doors/windows yet, so I can't open it to get an IR card anywhere near any optics in the IOO or OMC chambers. I waved PRM around a bit, but I can't find the beam on the REFL camera, so I definitely need to check that whole path again before we close up.
So, we're not closing up tomorrow, but progress has been made, and we're getting closer.
Note to self: These are the ITMX, ITMY, PRM, BS, SRM biases with this DRMI alignment. The DRMI is good, but the arms aren't, so these won't be final. The saved alignments are still those with (for the Yarm) the beam bouncing several times between ITMY and ETMY. BS was aligned at the time to hit the center of ETMX, and PRM and SRM should be retro reflecting in that alignment. So, it's possible, that aligning PZT2 to hit the center of ETMY and restoring all of the optics will get me close to being back to DRMI aligned, but in a condition that the arms are align-able too. |
Attachment 1: DRMI_aligned_19Sept2012_ETMYwasHighNeedToFix.png
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Thu Sep 20 01:28:14 2012 |
Jenne | Update | General | DRMI aligned again, but with good arms | [Jenne, Manasa]
Using the alignment of the PZTs and BS from pre-dinner, where the beam was hitting the center of both ETMs, we aligned the DRMI. The beam was off on the SRM in yaw by ~half a beam diameter, so I undid Koji's movement of SR2 from a week ago. I loosened the SR2 dog clamps, touched it gently on the base to do a little bit of angle, then re-clamped it. Once again, Steve's new brass centering target was awesome, since it was on the SRM while I was moving SR2.
We approximately recentered the beam on the AS camera, although it didn't need much once we got the beam out of the vacuum, by centering it on all of the output AS path mirrors.
We also got IPPOS out of the vacuum. Manasa was in the process of centering the QPD when the laptop died from too long being unplugged, so we leave that for tomorrow.
Left to do:
REFL path. REFL is not coming out of the vacuum, and with the light access connector I can't reach any of the REFL steering mirrors, since they're in the center of the IOO table.
IPANG. Should be easy.
POP, POX, POY. Need to the the camera-on-a-stick back down to the corner (from ETMY) and point it at the pickoff mirrors to ensure that beam is getting out of the vacuum. |
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Thu Sep 20 08:34:46 2012 |
Manasa | Update | General | DRMI aligned again, but with good arms |
Quote: |
[Jenne, Manasa]
Using the alignment of the PZTs and BS from pre-dinner, where the beam was hitting the center of both ETMs, we aligned the DRMI. The beam was off on the SRM in yaw by ~half a beam diameter, so I undid Koji's movement of SR2 from a week ago. I loosened the SR2 dog clamps, touched it gently on the base to do a little bit of angle, then re-clamped it. Once again, Steve's new brass centering target was awesome, since it was on the SRM while I was moving SR2.
We approximately recentered the beam on the AS camera, although it didn't need much once we got the beam out of the vacuum, by centering it on all of the output AS path mirrors.
We also got IPPOS out of the vacuum. Manasa was in the process of centering the QPD when the laptop died from too long being unplugged, so we leave that for tomorrow.
Left to do:
REFL path. REFL is not coming out of the vacuum, and with the light access connector I can't reach any of the REFL steering mirrors, since they're in the center of the IOO table.
IPANG. Should be easy.
POP, POX, POY. Need to the the camera-on-a-stick back down to the corner (from ETMY) and point it at the pickoff mirrors to ensure that beam is getting out of the vacuum.
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Steve!! The light access connector got more ripped during the work last night ...we've just taped it back. We might need to figure out a better way to do this than just cutting through the cover. |
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Thu Sep 20 11:39:40 2012 |
Manasa | Update | General | DRMI aligned again, but with good arms |
QPD at IPPOS has been centered by removing the filter at the QPD.
So we need to remember to check back on AS camera path and the IPPOS as well in addition to the usual MCrefl path.
P.S. We would be happy to have a new laptop in the lab to replace "Belladonna"! |
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Sat Apr 7 06:58:34 2012 |
kiwamu | Update | LSC | DRMI lock : lost good alignment | Somehow I lost the good alignment, where the lock can be frequently acquired and hence I didn't go further ahead.
I will try locking the DRMI during the weekend again. My goal is to take time series when the DRMI is being locked and sensing matrix.
Quote from #6506 |
Currently SRM is slightly misaligned such that the MICH optical gain at AS55Q doesn't increase so much with the presence of SRM.
With this condition I was able to acquire the lock more frequently than how it used to be on the Wednesday.
The next step is to gradually align SRM, to optimize the controls and to repeat this process several times until SRM is fully aligned.
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Wed Aug 20 13:23:32 2008 |
rob | Update | Locking | DRMI locked |
I was able to lock the DRMI this afternoon. All the optical levers have been centered. |
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Sat Nov 1 16:06:32 2014 |
Koji | Configuration | LSC | DRMI locked | Continued from ELOG 10659
DRMI locking
Following Jenne's elog entry in Aug 2013 (9049), DRMI was configured and locked. The lock was stable, indefinite, and repeatitive.
- DRMI Configuration
Demod phases has not been changed from PRMI
REFL11: WTN 0dB PHASE 21deg, REFL11I x0.1 -> PRCL
REFL55: WTN 21dB PHASE 25deg, REFL55Q x1 -> MICH, REFL55I x1 -> SRCL
AS110 phase was adjusted to maximize Q during the lock: +1deg (AS110Q_ERR was +4400 ~ +5500)
PRCL: GAIN -0.05 FM4/5 ON, Triggered FM 2/3/6/9, Servo trigger: POP22I 20up 10down, No Normaization.
MICH: GAIN +1 FM4/5 ON, Triggered FM 2/3/6/9, Servo trigger: POP22I 20up 10down, No Normaization.
SRCL: GAIN +2 FM4/5 ON, Triggered FM2/3/6/8/9, Servo trigger: AS110Q up 500 down 5, No Normaization.
(FM8 was set to be x2.5 flat gain such that the gain is increased after the lock)
MICH actuation is still BS+PRM and does not include SRCL decoupling yet.
This should be fixed ASAP.
DRMI Calibration
Let's use these entries
SRM: http://nodus.ligo.caltech.edu:8080/40m/10664
SRM = (19.0 +/- 0.7) x 10 -9/ f2
PRM: http://nodus.ligo.caltech.edu:8080/40m/8255
PRM: (19.6 +/- 0.3) x 10 -9 / f2 m/counts
BS/ITMs http://nodus.ligo.caltech.edu:8080/40m/8242
BS = (20.7 +/- 0.1) x 10 -9 / f2 m/counts
ITMX = (4.70 +/- 0.02) x 10 -9/ f2 m/counts
ITMY = (4.66 +/- 0.02) x 10 -9/ f2 m/counts
- PRCL Calibration
Lock-in oscillator module 675.13Hz 100 -> +1 PRM
Measurement bandwidth 0.1Hz -> Signal power BW 0.471232 (FLATTOP window)
C1:SUS-PRM_LSC_IN1: 97.45 cnt/rtHz => 4.19 pm/rtHz
REFL11I: 12.55 cnt/rtHz => 3.00e12 cnt/m
REFL11Q: 0.197 cnt/rtHz => 4.70e10 cnt/m
=> 0.90 deg rotated! (GOOD)
REFL33I: 1.63 cnt/rtHz => 3.89e11 cnt/m
REFL33Q: 0.196 cnt/rtHz => 4.68e10 cnt/m
=> 8.32 deg rotated!
REFL55I: 0.0495 cnt/rtHz => 1.18e10 cnt/m
REFL55Q: 0.548 cnt/rtHz => 1.31e11 cnt/m
=> 84.8 deg rotated! (WHAT!)
REFL165I: 1.20 cnt/rtHz => 2.86e11 cnt/m
REFL165Q: 0.458 cnt/rtHz => 1.09e11 cnt/m
=> 20.9 deg rotated!
- MICH Calibration
Lock-in oscillator module 675.13Hz 100 -> -1 ITMX +1 ITMY
Measurement bandwidth 0.1Hz -> Signal power BW 0.471232 (FLATTOP window)
C1:SUS-ITMX_LSC_IN1: 121.79 cnt/rtHz => 1.26pm/rtHz
C1:SUS-ITMY_LSC_IN1: 121.79 cnt/rtHz => 1.25pm/rtHz
AS55Q: 12.45 cnt/rtHz => 4.96e12 cnt/m (STRONG)
REFL11I: 0.0703 cnt/rtHz => 2.80e10 cnt/m
REFL11Q: 0.0142 cnt/rtHz => 5.66e09 cnt/m => 78.5 deg rotated! (WHAT!)
REFL33I: 0.0473 cnt/rtHz => 1.88e10 cnt/m
REFL33Q: 0.0291 cnt/rtHz => 1.16e10 cnt/m => 58.4 deg rotated!
REFL55I: 0.00668cnt/rtHz => 2.66e09 cnt/m
REFL55Q: 0.0261 cnt/rtHz => 1.04e10 cnt/m => 14.4 deg rotated! (OK)
REFL165I: 0.0233 cnt/rtHz => 9.28e09 cnt/m
REFL165Q: 0.0512 cnt/rtHz => 2.04e10 cnt/m => 24.5 deg rotated! (GOOD)
- SRCL Calibration
Lock-in oscillator module 675.13Hz 100 -> SRM
Measurement bandwidth 0.1Hz -> Signal power BW 0.471232 (FLATTOP window)
C1:SUS-SRM_LSC_IN1: 121.77 cnt/rtHz => 5.08pm/rtHz
AS55I: 0.256 cnt/rtHz => 5.05e10 cnt/m
AS55Q: 0.3498 cnt/rtHz => 6.90e10 cnt/m
REFL11I: 0.00624 cnt/rtHz => 1.23e09 cnt/m
REFL11Q: 0.00204 cnt/rtHz => 4.02e08 cnt/m
REFL33I: 0.00835 cnt/rtHz => 1.65e09 cnt/m
REFL33Q: 0.0659 cnt/rtHz => 1.30e10 cnt/m
REFL55I: 0.0201 cnt/rtHz => 3.97e09 cnt/m
REFL55Q: 0.01505 cnt/rtHz => 2.97e09 cnt/m
REFL165I: 0.0238 cnt/rtHz => 4.69e09 cnt/m
REFL165Q: 0.0247 cnt/rtHz => 4.87e09 cnt/m
DRMI Openloop measurements
Servo filter TF measurements
The UGFs were ~250Hz for PRCL and ~100Hz for MICH, and ~250Hz for SRCL, respectively.
MICH showed (presumably) crosscoupling related peak ~350Hz. SRCL had small deviation from the model.
This may also be related to the cross couplig.
The OLTF was modelled by the servo and violin filters TF from foton, estimated TF of the AA/AI filters, and the constant time delay.
Displacement spectra measurement
- PRCL
The OLTF compensation was not actually succesfull at 300Hz, but otherwise the situation is very similar to the one with PRMI.
- MICH
Again the servo compensation at 300Hz was not successful. If we believe that AS55Q is the best MICH sensor, the out-of-loop
noise level of MICH was quite similar to the one in PRMI. We should try to use AS55Q for DRMI MICH for investigation purpose
to see which REFL signal has the best MICH quality. REFL165 seems to be iproved in the signal amplitude. Can we use this
for locking now?
- SRCL
It is in fact difficult to tell what is the correct out-of-loop noise level. AS55I has too much contamination from MICH and is not indicating
useful info. This measurement should be tried once the sensor diagonalization is done.
REFL55I is not seeing anything real abobe 30Hz. We should be able to reduce the UGF and the servo gain.
The absolute motion level of SRCL is something similar to PRCL, rather than MICH.
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Attachment 1: DRMI_PRCL_OLTF.pdf
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Attachment 2: DRMI_MICH_OLTF.pdf
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Attachment 3: DRMI_SRCL_OLTF.pdf
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Attachment 4: DRMI_PRCL_SPE.pdf
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Attachment 5: DRMI_MICH_SPE.pdf
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Attachment 6: DRMI_SRCL_SPE.pdf
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Fri Oct 7 04:42:24 2011 |
kiwamu | Update | LSC | DRMI locked and some plans | DRMI has been locked using the same RFPD selection as the old days (i.e. AS55_I, AS55_Q and REFL_I).(#4760)
But remember : this is just a beginning of several measurements and tests to characterize the central part.
Here is a list of the measurements and actions :
- 3f locking related
+ Listing up the necessary RFPDs and their installations.
+ Calibration of the SRM actuator => this is necessary to convert the sensing matrix into unit of [counts/m] or [W/m].
+ Measurement of the sensing matrix => check the performance of 3f signals. Also diagonalization of the LSC sensing matrix
+ Diagonalization of the output matrix.
+ Noise characterization of 3f PDs => confirm the noise are low enough to keep the lock of the central part
- Power-recycling gain issue related (#5541)
+ Estimation of the mode matching efficiency => maybe we can use power-recycled ITMs to estimate it (?)
+ Implementation of auto alignment servos and scripts for MICH, PRCL and SRCL. => integrate it to the existing ASS model
+ Search for a possible loss factor |
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Fri Oct 7 11:53:47 2011 |
Koji | Update | LSC | DRMI locked and some plans | - REFL165 PD to be fixed (shows constant high voltage at the DC out)
- Make POP22/110 PD
- Install AS11? or use it as POX11?
- Install POP55 |
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Fri Sep 4 04:05:51 2015 |
ericq | Update | LSC | DRMI locked on 1F and 3F | Thanks to some expertly timed coffee from Ignacio, I have been able to achieve indefnite locks of the DRMI, first on a 1F/3F mix (P:REFL11, S: REFL165, M:AS55), and then purely on 3F (P:REFL33, S:REFL165, S:REFL165). MICH is currently actuated on the ITMs.
I saved a snapshot of the current settings so I don't lose my settings. I think one thing that prevented earlier recipies from working is that whitening gains may have changed, which we don't typically note down when reporting input matrix settings
My current settings for 3F locking:
REFL33:
+30dB whitening gain, +136 demod phase
PRCL = 9 x I - 200 counts
REFL165:
+24dB whitening gain, +3 demod phase
SRCL = 1 x I, MICH = 5 x Q - 1000counts
MICH: G=-0.03; Acq FM4/5; Trig 2/3/6/9
PRCL: G=-0.003; Acq FM4/5; Trig 1/2/6/9
SRCL: G=0.2; Acq FM4/5; Trig 2/3/6/9
I've injected excitations into the control filter outputs via the LSC-FFC FMS (and notched the frequencies in the control filters themselves), and noted GPS times for offline sensing analysis. (Namely the 10 minutes following 1125398900)
Handing off to pure 3F was a little finicky at first, I needed to use some pretty large offsets in the MICH_B and PRCL_B FMs. (-1000 and -200 counts respectively). Once these offsets were found, the DRMI can acquire on 3F. Alignment is pretty important, too. Acquiring is much faster when the loop gains are "too high." i.e. I see a fair amount of gain peaking at ~300Hz. Nevertheless, things are stable enough as is that I didn't feel like digging into reducing the gains to quieter values. |
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Fri Sep 4 20:06:23 2015 |
rana | Update | LSC | DRMI locked on 1F and 3F | Nice going. I think the LLO / LHO scheme is to acquire on 1F and then cdsutils avg to get the 3F offsets. The thinking is that that 1F signals have less intrinsic offset than the 3F signals, so we want to be use digital offsets for the 3F locks. |
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Wed Nov 16 03:10:01 2016 |
gautam | Update | LSC | DRMI locked on 1f and 3f signals | After much trial and error with whitening gains, demod phases and overall loop gains, I was finally able to lock the DRMI on both 1f and 3f signals! I went through things in the following order tonight:
- Lock the arms, dither align
- Lock the PRMI on carrier and dither align the PRM to get good alignment
- Tried to lock the DRMI on 1f signals - this took a while. I realized the reason I had little to no success with this over the last few days was because I did not turn off the automatic unwhitening filter triggering on the demod screens. I had to tweak the SRM alignment while looking at the AS camera, and also adjust the demod phases for AS55 (MICH is on AS55Q) and REFL55 (SRCL is on REFL55I). Once I was able to get locks of a few seconds, I used the UGF servos to set the overall loop gain for MICH, PRCL and SRCL, after which I was able to revert the filter triggering to the usual settings
- Once I adjusted the overall gains and demod phases, the DRMI locks were very stable - I left a lock alone for ~20mins, and then took loop shape measurements for all 3 loops
- Then I decided to try transfering to 3f signals - I first averaged the IN1s to the 'B' channels for the 3 vertex DOFs using cds avg while locked on the 1f signals. I then set a ramp time of 5 seconds and turned the gain of the 'A' channels to 0 and 'B' channels to 1. The transition wasn't smooth in that the lock was broken but was reacquired in a couple of seconds.
- The lock on 3f signals was also pretty stable, the current one has been going for >10 minutes and even when it loses lock, it is able to reacquire in a few seconds
I have noted all the settings I used tonight, I will post them tomorrow. I was planning to try a DRFPMI lock if I was successful with the DRMI earlier tonight, but I'm calling it a night for now. But I think the DRMI locking is now back to a reliable level, and we can push ahead with the full IFO lock...
It remains to update the auto-configure scripts to restore the optimized settings from tonight, I am leaving this to tomorrow as well...
Updated 16 Nov 2016 1130am
Settings used were as follows:
1f/3f |
DOF |
Error signal |
Whitening gain (dB) |
Demod phase (deg) |
Loop gain |
Trigger |
DRMI Locking 16 Nov 2016
1f |
MICH (A) |
AS55Q |
0 |
-42 |
-0.026 |
POP22I=1 |
1f |
PRCL (A) |
REFL11I |
18 |
18 |
-0.0029 |
POP22I=1 |
1f |
SRCL (A) |
REFL55I |
18 |
-175 |
-0.035 |
POP22I=10 |
3f |
MICH (B) |
REFL165Q |
24 |
-86 |
-0.026 |
POP22I=1 |
3f |
PRCL (B) |
REFL33I |
30 |
136 |
-0.0029 |
POP22I=1 |
3f |
SRCL (B) |
REFL165I and REFL33I |
- |
- |
-0.035 |
POP22I=10 |
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Wed Nov 16 08:14:43 2016 |
Steve | Update | LSC | DRMI locked on 1f and 3f signals | Nice job.
Quote: |
After much trial and error with whitening gains, demod phases and overall loop gains, I was finally able to lock the DRMI on both 1f and 3f signals! I went through things in the following order tonight:
- Lock the arms, dither align
- Lock the PRMI on carrier and dither align the PRM to get good alignment
- Tried to lock the DRMI on 1f signals - this took a while. I realized the reason I had little to no success with this over the last few days was because I did not turn off the automatic unwhitening filter triggering on the demod screens. I had to tweak the SRM alignment while looking at the AS camera, and also adjust the demod phases for AS55 (MICH is on AS55Q) and REFL55 (SRCL is on REFL55I). Once I was able to get locks of a few seconds, I used the UGF servos to set the overall loop gain for MICH, PRCL and SRCL, after which I was able to revert the filter triggering to the usual settings
- Once I adjusted the overall gains and demod phases, the DRMI locks were very stable - I left a lock alone for ~20mins, and then took loop shape measurements for all 3 loops
- Then I decided to try transfering to 3f signals - I first averaged the IN1s to the 'B' channels for the 3 vertex DOFs using cds avg while locked on the 1f signals. I then set a ramp time of 5 seconds and turned the gain of the 'A' channels to 0 and 'B' channels to 1. The transition wasn't smooth in that the lock was broken but was reacquired in a couple of seconds.
- The lock on 3f signals was also pretty stable, the current one has been going for >10 minutes and even when it loses lock, it is able to reacquire in a few seconds
I have noted all the settings I used tonight, I will post them tomorrow. I was planning to try a DRFPMI lock if I was successful with the DRMI earlier tonight, but I'm calling it a night for now. But I think the DRMI locking is now back to a reliable level, and we can push ahead with the full IFO lock...
It remains to update the auto-configure scripts to restore the optimized settings from tonight, I am leaving this to tomorrow as well...
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Attachment 1: 5hrs.png
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Mon Nov 21 14:02:32 2016 |
gautam | Update | LSC | DRMI locked on 3f signals, arms held on ALS | Over the weekend, I was successful in locking the DRMI with the arms held on ALS. The locks were fairly robust, lasting order of minutes, and was able to reacquire by itself when it lost the lock in <1min. I had to tweak the demod phases and loop gains further compared to the 1f lock with no arms, but eventually I was able to run a sensing matrix measurement as well. A summary of the steps I had to follow:
- Lock on 1f signals, no arms, and run sensing lines, adjust REFL33 and REFL 165 demod phases to align PRCL, MICH and SRCL as best as possible to REFL33I, REFL165Q and REFL165I respectively
- I also set the offsets to the 'B' inputs at this stage
- Lock arms on ALS, engage DRMI locking on 3f signals (the restore script resets some values like the 'B' channel offsets, so I modified the restore script to set the offsets I most recently measured)
- I was able to achieve short locks on the settings from the locking with no arms - I set the loop gains using the UGF servos and ran some sensing lines to get an idea of what the final demod phases should be
- Adjusted the demod phases, locked the DRMI again (with CARM offset = -4.0), and took another sensing matrix measurement (~2mins). The data was analyzed using the set of scripts EricQ has made for this purpose, here is the result from a lock yesterday evening (the radial axis is meant to be demod board output volts per meter but the calibration I used may be wrong)

I've updated the appropriate fields in the restore script. Now that the DRMI locking is somewhat stable again, I think the next step towards the full lock would be to zero the CARM offset and turning on the AO path.
On the downside, I noticed yesterday that ITMY UL shadow sensor readback was glitching again - for the locking yesterday, I simply held the output of that channel to the input matrix, which worked fine. I had already done some debugging on the Sat. Box with the help of the tester box, but unlike the PRM sat. box, I did not find anything obviously wrong with the ITMY one... I also ran into a CDS issue when I tried to run the script that sets the phase tracker UGF - the script reported that the channels it was supposed to read (the I and Q outputs of the ALS signal, e.g. C1:ALS-BEATX_FINE_I_OUT) did not exist. The same channels worked on dataviever though, so I am not sure what the problem was. Some time later, the script worked fine too. Something to look out for in the future I guess.. |
Attachment 1: DRMIArms_Nov20.pdf
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Thu Apr 5 07:19:16 2012 |
kiwamu | Update | LSC | DRMI locking | I tried locking the DRMI to the signal-extraction condition with the new trigger by AS110.
A first thing I tried was : flipping the control sign of the SRCL while keeping the same control setups for the PRCL and MICH.
Occasionally the DRMI was "sort of" locked and hence I believe this setup must be a good starting point.
As a next step I will try some different gains and demodulation phase to make it more lockable.
(Time series)

The picture above is time series of some signals when the DRMI was barely locked.
The red arrows indicate the durations when the DRMI was sort of locked.
(Green curve) REFLDC becoming a high value state, which indicates that the carrier is anti-resonant.
(Red curve) ASDC becoming dark, which indicates the MICH is in the vicinity of the dark condition.
(Brown curve) AS110 becoming a high value state, which means the 55 MHz sidebands got amplified by the SRCL.
(Blue curve) POP22 becoming a high value state, which indicates that the 11 MHz sidebands are resonating in the PRC.
According to the measurement of AS110 when PRMI was locked ( #6488), the AS110 signal went up to ~ 1 counts or so.
On the other hand when the DRMI was locked the AS110 went to up more than 10 counts as shown in the plot above.
Therefore at least some kind of signal amplification is happening for the 55 MHz sidebands in the SRC.
Looking at the AS CCD, I found that the beam looked like a TEM01 mode (two beam spots at top and bottom) every time when the DRMI was locked.
(settings)
- REFL33I => PRCL G = -0.2
- AS55Q => MICH G = -6
- AS55I => SRCL G = 1 (G = -50 for the signal recycling condition)
- AS55 demod phase = 17 deg
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Fri Sep 12 00:40:23 2014 |
Jenne | Update | LSC | DRMI locking | Tonight I worked on DRMI locking.
I think the reason the May2014 DRMI recipe wasn't working for me is because I wasn't including the REFL11 -> SRCL element. I had left it out because (a) I didn't think we should need it and (b) REFL11 is going through the CM board.
Tonight, I flipped the switch on the CM screen so that OUT2 was seeing REFL11I, not REFLDC, so I had REFL11 in the usual place. I reset the demod phase, since we had left it at zero for CM stuff.
Setting demod phases for PRMI:
I locked PRMI on sideband, REFL 33 I&Q and drove PRM. REFL55 was at 55deg, and I changed it to 33deg to minimize the peak in the Q-phase. REFL11 was a 0deg, and I set it to 17deg. I also checked the AS55 phase in the MICH-only case, and changed it from 14.75deg to 24.75 deg.
The May 2014 recipe (elog 9968) calls for adding 25 degrees to the REFL55 phase, so I put REFL55 at 58deg for DRMI locking.
After that, using the parameters in the May2014 recipe, the DRMI just locked. Awesome!
I checked the demod phases with DRMI lock. REFL11 stays at 17 degrees. If I actuate the SRM, I get the largest peak in the I-phase of REFL55 with a phase of -143deg, but the acquisition is best with phase around 55deg. [Note, as Q points out, I wonder if SRCL is mostly locked with REFL11I for some magical reason, which is why it didn't matter so much that I put a sign flip into REFL55...I wonder if fixing our macroscopic length offset in SRCL will fix this]. I also changed the REFL165 phase from -155.5deg to +145deg.
By looking at transfer functions at an excitation frequency, I expected that I should be able to hold SRCL and MICH on REFL165, with matrix elements -0.085 for REFL165I->SRCL and -0.23 for REFL165Q->MICH. I was not able to acquire with these values, nor was I able to ramp the matrix elements while keeping lock.
So, I tried moving PRCL to REFL33I, which did work. I used 1.245*REFL33I->PRCL, but left SRCL and MICH on REFL55 I&Q, with the REFL11I->SRCL element also there. This is where I started trying to get rid of the REFL11I element, but couldn't maintain lock most times, and could never acquire lock without it.
Next up, checking the MICH->SRCL coupling due to the output matrix. I did as Koji did in elog 8816 , but first I copied the notches in FM10 of MICH over to PRCL and SRCL (old notch freqs were SRCL=566.1Hz, PRCL=675.1Hz, now they're all 475.1Hz). I drove BS, and checked that the PRM element minimized the peak in REFL33I, the PRCL error signal. I also added an SRM element to reduce the peak in REFL55I, the SRCL error signal. I ended up with 0.5*BS, -0.284*PRM, -1.5*SRM for MICH drive, and unity in the PRM and SRM elements for PRCL and SRCL, respectively.
I measured the SRCL open loop gain, and the UGF was pretty low, so I increased the SRCL gain from 0.2 to 0.5 to make the UGF be around 70Hz. I measured PRCL and MICH also, and they matched their references.
I worked a little bit on trying to remove REFL11 from the SRCL error signal, but didn't get anywhere. I'm leaving the IFO to Q for the rest of the night.
To sum up, here is the set of parameters that worked for DRMI locking. (These are saved as the template on the IFO Config screen.):
DEMOD PHASES:
REFL11: 17 deg
REFL33: 140.5 deg (not changed tonight)
REFL55: 58 deg (58deg for DRMI, 33deg for PRMI)
REFL165: 145 deg
AS55: 24.75 deg
INPUT MATRIX
MICH = 0.15 * REFL55Q
PRCL = 1.245 * REFL33I
SRCL = -0.09 * REFL11I + 1.0 * REFL55I
DOF Triggers
MICH, PRCL, SRCL all on POP22I, 50:10
GAINS
MICH = 1.0
PRCL = -0.02
SRCL = 0.5
FM triggers
MICH: 35:2, 2 sec delay, FM 2, 3, 6, 9
PRCL: 35:2, 0.5 sec delay, FM 2, 3, 6, 9
SRCL: 35:2, 5 sec delay, FM 3, 6, 9 (always lose lock trying to engage FM2).
OUTPUT MATRIX
MICH = 0.5 * BS + (-0.284)*PRM + (-1.5)*SRM
PRCL = 1*PRM
SRCL = 1*SRM |
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Fri Sep 12 11:25:42 2014 |
Koji | Update | LSC | DRMI locking | This is great.
And I got confused. Is REFL11 going through the CM board?
If so how the demod phase for REFL11 take an effect for the sensing?
Maybe I understood. CM SERVO SLOW has been connected to REFL11I? whitening.
Therefore using REFL11 in the CM SERVO gives us REFL11I at the usual channels.
And then how can we ensure the gain matching between I & Q?
Then is the next step 3f DRMI? How is REFL165 healthy?
I also wonder how the relative phase and modulation depths improves the sensing matrix. |
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Fri Sep 12 12:00:59 2014 |
ericq | Update | LSC | DRMI locking | REFL11 I, as seen in digital land, is connected to the slow output of the CM board. I tuned the demod angle of the REFL11 demodulator board by cable length back in ELOG 9850. It would be good to check that the phase is still good. If the CM board gains are at 0dB, we should be able to used the digital angle adjustment as normal. |
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