Sheila, Alexa, Kiwamu
Even though we swapped the oplev laser for BS recently. The BS optical level laser power started showing another power modulation, which resulted in kicks on BS through the damping loops.
For now, we recentered the beam on the QPD to reduce the intensity coupling.
The power modulation looks more like a step which randomly shows up as a function time as shown in the attached screenshot. The modulation depth is roughly 1%. This was actually big enough to cause BS angle agitation which was visible at the dark port digital camera. The coupling seemed bigger in the horizontal direction presumably due to a bigger off-centering in the horizontal direction on the QPD. After the re-center, the coupling seemed to have become lesser, but it is still kicking BS in its angle. This needs to be fixed.
Alexa, Kiwamu ( a report from this past Friday)
We started checking out the REFL WFSs again. The misssion of the day is to engage the DC centering servos and check out the demod phases.
(REFL WFS DC centering servos)
We applied some modifications on the DC centering servo so that the servo basis REFL_A and REFL_B QPD signals. This had been adjusted to be some other basis (alog 9966), but we wanted a simpler basis. The attached is a screenshot of the new centering servo configuration. The input matrices are simple diagonal matrices so that the servo basis is simply REFL_A and REFL_B. In order to actuate on those basis through RM1 and RM2, we did some algebra based on the number reported in the previous alog (alog 9966). After the adjustment, we tuned up the gains to have a few second impulse repose time scale in every servo loop. Also, the sign of the output matrix were chosen such that all the servo gain consistently has negative sign.
(REFL_A_RF9 looked not great)
While we could easily re-adjust the demodulation phases on REFL_B_RF9, we could not perfectly adjut the demod phase on segment 1 of REFL_A_RF9. In addition, segment 4 of REFL_A_RF9 showed no reliable signals. This looked as if a cable was unplugged or something. Indeed the noise floor of segment 4 was lower than everyone else. We need to check REFL_A_RF9 at some point.
We did not check RF45 because we ran out the commissioning time.
With installation ramping down, Vern will be chairing the morning meeting for the Detector Group. Meetings will be on Monday, Wednesday, and Friday, starting at 08:30. OpLevs – Need laser safe to continue work on HAM5. Ongoing alignment and problem resolution work at ITMX and ITMY. Glitches with the BS OpLev laser are being looked into. Seismic – Continuing work on ITMX control loops stability. Commissioning on the various HAM HEPIs. Electrical – Pulling cables and power distribution configuration in the LVEA. Work on the Chiller 3 tripping problem. Reconnecting Staging Building fire system to the alarm distribution panel in the OSB
Some features in TF we'd like to confirm are SUS peaks. Will desist if needed.
model restarts logged for Sun 07/Sep/2014
2014_09_07 12:28 h1fw1
unexpected restart of h1fw1
no restarts reported
The matrices described in 13703 were installed. This caused a noticable improvement in the shape of the QPD alignment OLGs. They are now more clearly a clean 1/f shape.
I also tuned the OMC LSC demod phase and set the gain for a 80Hz UGF. (This was done by opening the LSC loop and sitting on the side of a resonance and tuning the phase until the Q signal was 0)
I suppose the matrices Nic used are the ones described in T1400585
There is some factor adjustment from the one in ALOG 13703 such that we now have the servo inputs calibrated in um and urad for POS and ANG.
Nic, Jamie, Lisa With the QPD alignment engaged, we did a scan of the OMC in ITMY single bounce configuration. Data are being sent to Koji right now for a careful analysis, but our rough estimate is that indeed the matching to the OMC is around 90%, so slightly better than for ITMX, as expected. Scan data: Sep 9, 2014 21:10:08 - 21:12:00 UTC
Screenshot of the scan data. Koji will post a more complete analysis (a la 13767)
I don't know if Lisa, Nic, and Jamie believe this or not, the mode matching was 0.82 for this scan, which was indeed worse than the result with ITMY.
Note that this mismatch still includes the effect of the misalignment. This scan involved more 1st order mode.
Should we just incorporate the 1st order into the 0th order, qualitatively to saying? In this assumption, both arms are not so different.
Carrier Mode | X arm (mA) | Yarm (mA) |
0th | 13.13 | 9.15 |
1st | 0.088 | 0.28 |
2nd | 1.65 | 1.25 |
|
|
|
1 - 2nd/(0th+1st) | 0.88 | 0.87 |
Here are the result of the mode decomposition for the Y arm
Carrier | |
Order | mA |
0 | 9.153 |
1 | 0.28 |
2 | 1.251 |
3 | 0.102 |
4 | 0.264 |
5 | 0.0192 |
6 | 0.04144 |
7 | 0.02544 |
8 | 0.0108 |
Upper sidebands (45MHz) | |
Order | mA |
0 | 0.319 |
1 | 0.005 |
2 | 0.0294 |
3 | 0.004 |
4 | 0.0065 |
Lower sidebands (45MHz) | |
Order | mA |
0 | 0.318 |
1 | 0.005 |
2 | 0.0297 |
3 | 0.004 |
4 | 0.0065 |
2nd order Upper sidebands (90MHz) | |
Order | mA |
0 | 0.0021 |
1 | 0.00002 |
2 | 0.00075 |
2nd order Lower sidebands (90MHz) | |
Order | mA |
0 | 0.0021 |
1 | 0.00002 |
2 | 0.00075 |
Upper sidebands (9MHz) | |
Order | mA |
0 | 0.13 |
1 | 0.0026 |
2 | 0.012 |
3 | 0.0012 |
4 | 0.0035 |
Lower sidebands (9MHz) | |
Order | mA |
0 | 0.13 |
1 | 0.0026 |
2 | 0.012 |
3 | 0.0012 |
4 | 0.0035 |
Sidebands of sidebands | |
(+/-9MHz+/-45MHz) | mA |
-54 | 0.002 |
-36 | 0.002 |
36 | 0.002 |
54 | 0.002 |
Carrier TEM00 | 9.15 | mA | |
Carrier TEMnm | 1.99 | mA | |
Sideband | 1.04 | mA | |
Mode matching | 0.821 |
Here "mode matching" is defined by 1-(CR_TEMnm / CR_TEM00)
Yes, that makes sense to me. Once the dither is working we can make more precise measurements. But I guess the point is that the mismatch is around 10%, and we don't see a significant asymmetry between X and Y as in L1.
no restarts reported
Alexa, Sheila, Kiwamu, Nic, Jamie, Lisa After some ITMX ISI work, PRY initial alignment work and more Guardian work, variable finesse technology has been used to bring the PRMI close to the dark fringe. This time the normalization of the error signals is done with POPAIR_A. The success is only in principle because once we arrived at the final step to transition to RF for MICH, an earthquake sadly hit us..the bad timing of this earthquake is unbelievable (#%$#&*&!). The positive news is that with this new alignment the recycling gain is somewhat higher than before. We don't have precise measurements because we haven't really locked stably on the dark fringe yet, but we think we had a recycling gain around 10 at some point during the MICH offset reduction sequence when the alignment was good. Jim's ITMX ISI measurements are about to start, and they will last until tomorrow around lunch time.
We've been having trouble isolating ITMX. The punchline is, I think I need to collect a new with the seismometers in low gain and redo the loops. The rest of this post is summary/posterity/flagellation. -Last week, Sheila complained about the performance of the ITMX ISI. -To fix this, I took a new transfer function, but in response to something somebody said somewhere, I used a different configuration than previous rounds. This time I left the T240 and L4C in high gain, where before I had usually run all the seismometers in low gain for the tf. -I ran through all the commissioning scripts, load new cart matrices, new blend filters, new damping loops, and new isolation loops. Loading everything went off with no problems. -Turning on the isolation loops was a different story. When I left on Tuesday, St1 was partially working, I never made it to St2. Kiwamu and Jaime were able to wrestle St1 into a semi functional state (alog 13746). -I've continued to wrestle with this. JeffK suggested less aggressive loops, which I have spent a lot of time making successively more and more conservative loops. The first two attached images show a representative old and new loop. The old loop (that Sheila complained about originally) is more aggressive: higher UGF, more gain peaking, more aggressive boost, less phase at UGF (14 degrees!). The newer loop seems pretty "easy" in comparison, but it took a lot to turn it on, and it still rings a little. -Another clue, suggested by BrianL, comes from looking at the damping filters. The third image shows one of the loops from ITMY and ITMX. The ITMX loop has 7X less gain, but otherwise looks the same; phase looks the same. The 7X is suspicious, because that is exactly the difference in the gain between the high and low gain of the L4C. I had noticed earlier that the DAC outputs when the ISI was only damping looked low (i.e. never higher than a count, when I thought a few tens of counts was more normal). -So, this afternoon, I tried turning up the gain on the St1 damping loops to 7x. The outputs of the DAC increased to what I thought were more normal numbers, and nothing went crazy. I tried turning loops on at this point, and it was still difficult, but eventually we got everything on for St1. Additionally, some of the ringing was alleviated by upping the gain on a few of the loops, so that is how I have left it. St2 is damping only still, but St1 has been running for the last 4-ish hours. -I looked at the St1 & St2 seismometers, as well as the op-levs to compare these not-so-great loops and the just damped state and it looks like the current arrangement is a little better than just damping. My last 3 images are the op-lev spectra, and the St2 seismometers. Pretty sure the big peak at 30hz is Kyle's pump cart, so a temporary issue. -I have scripts set to launch the tf at about 1 am. I may come in to work on this some more this weekend, I'll let the appropriate people know if I do.
S. Dwyer, G. Grabeel Completed the alignment of the HWS on the ISC table and end-Y for TCS. The green laser had some alignment issues after the power outage that a burt restore didn't fix. Sheila and I put the PZTs in the middle of their range of motion and realigned the beam onto the QPDs. After the green beam was aligned with the irises and centered on the QPDs I began aligning the TCS HWS side of the ISC table. The new layout worked really well and I was quickly able to get a good looking beam on the HWS. Unfortunately there is an issue with an incorrect pinout on the HWS cable so I will not be able to get the camera running just yet.
on OPSWS1. Please don't disturb the matlab session. The TFs should complete before noon.
Closed these loops with the controllers designed from the TFs taken yesterday. They turn on fine with Guardian and the ISI (w/ Lvl1 Controllers) only gets marginally excited during the process. The HEPI and ISI Guardians are not SEI Supervised and are each in EXEC control as there is no ROBUST_ISOLATED choice in the SEI Manager.
A safe.snap was taken. The only thing there is the open loop drive OFFSETs are still in place although the OFFSET is off.
I still want to study some performance but the positions are locking so good first step.
Jeff K, Betsy
While the SR2 M3 stage coil had previously been balanced using coil sensors, we tried to use the AS_C PD to repeat the measurement. AS_C is an in-vacuum PD on HAM6 behind SRM. Keita helped me center the beam on the PD with SR2 bias. We then used the SR2 LOCK-IN to drive the SR2 in the pringle mode at 5Hz, with 100k aplitude, at varying coil imbalance states. Unfortunately we could not see much change in the response when the M3 coils were balanced or unbalanced. Attached shows the unchanged peaks between the 2 states of coil unbalanace. SR2 pointing was restored to how we found it when we started.
Things to try next:
- Try on SR3
- Try using AS_B PD - a nearby WFS which does not have a lense in front of it - which maybe caused us a problem
For the record, the two states of balance in the plot are a "fresh" start, with the COILOUTF gains all set to unity, vs those "balanced" values found by Borja (see LHO aLOG 13229). Betsy had tried sweeping both the pitch and yaw imbalance by 20% in either direction and saw an inconsistent story at best -- however, she was sure to continually check for coherence between the drive and response channels and ensure that the IFO configuration was stable enough to provide light for the QPD. We also had WFS_AS_A_DC and WFS_AS_B_DC up with the plan to check if they were any more or less valid measures of the P and Y from SR2. Though there was signal, the assessment of their use for balancing was not as systematically studied as it was for AS_C. Very strange that this sensor didn't work out, which is why we'll try other QPDs/WFS and also look at driving other suspensions.
As reported before, ITMY OL is making a huge fake triangular wave motion of 10 minutes period mainly in YAW (CH1).
We know that the optic itself is not moving because we cannot see this anywhere else, e.g. look at CH7 (AS_C QPD) and CH8 (L2 stage OSEM of ITMY).
We know that this is not the intensity noise. The RIN of OL SUM (CH6) for this 10min thing is about 0.3% pk-pk while each quadrant (CH2-CH5) sees two orders of magnitude larger signal. In addition, the phase of SEG1 and SEG4 are the opposite of SEG2 and SEG3.
It appears that either the OL laser or the receiver or both are moving in YAW (unless the electronics of all four channels are conspiring together, which is very unlikely).
We could not find any apparent correlation between this fake OL motion and various FMCS and PEM channels. AOS people, please investigate.
The ITMX OL is also not functioning right now. The alignment should be checked.
The new H1 ITMs ROC (ITM03 and ITM11) are similar to the ones in L1, but they are swapped (the wavefront error is larger from X than from Y). Based on T1300954 (table 3) and Hiro's wisdom, the effective ROCs of the H1 optics, as measured in reflection, going through the bulk, are: R_ITMX (ITM03) = 1939.3 + (-10.92*2*1.457); R_ITMY (ITM11)= 1939.2 + (1.56*2*1.457); By looking at the L1 data in single bounce without TCS (below), one should expect something like ~20% mode mismatch for X and something somehow better for Y. L1 Mode mis-match: NO TCS: ITMX 14.5% ITMY 22% Even with an input beam perfectly matched to the PRM, I would expect something like: modematching asX with OMC = 0.8408 modematching asY with OMC = 0.91229
To improve the contrast while maximize the matching to the OMC, CO2 central heating should be applied to ITMX to match ITMY. Since we don't have central heating right now, one could use the ring heater to match ITMY to ITMX. This would make the matching to the OMC worse, but a better contrast.
See 13815 entry instead.