No restarts reported.
the alingment offsets are off on both TMSs, and Arnaud's measurement is started.
Sheila, Kiwamu,
The goal tonight was to add TOP and UIM of ETMY to the DARM actuator in order to increase the control bandwidth. This worked fine and the UGF was pushed a bit higher and it is now 4 Hz.
As Sheila reported on alog 11787, we prepared ETMY. So we started using ETMY in addition to ETMX. Since ETMY's ESD is not ready yet, we used only TOP and UIM of ETMY. This helped the DAC range of the UIM stage and therefore we could push the UGF a bit higher. At the end, we ended up a UGF of about 4 Hz. The infrared RMS is now about 90 Hz. We didn't redesign the low-frequency boost this time as our target was to have a higher UGF. The attached is the ALS diff spectrum (shown in red), with the spectra from yesterday for comparison. You can see that the noise is suppressed below 4 Hz. Currently the UGF is limited by UIM and TST which saturate at high frequencies.
Arnaud, Sheila, Kiwamu,
We copied the plant inversion filters from ETMX UIM to ETMY, and ran a transfer function to test it. The results are saved in /ligo/home/sheila.dwyer/ALS/HIFOXY/Y_UIM.xml
I imported the measurement into foton, and compared it to the low pass blend (which was on when I took the measurement) and a pedulum at 1 Hz with a Q of 1, which is what our plant is supposed to be with the inversion. They match pretty well, screenshot attached. Since our inversion of the ETMX top mass and the UIm match for the resonances that are common, we just copied the ETMX top mass plant inversion to ETMY and decided to try this out.
Also, we tried using an offset for the ESD drives, which should give us a bit more range. With the bias at 125000cnts, I added an offset of -51777 counts to each of the quadrants, following the math in T1400321. At 4 Hz, we measured a factor of 1.77 more gain , at 6 Hz 1.6 more gain.
This time it was probably our fault, kicking the suspension
also ETMY ISI tripped, also our fault
We don't know why this tripped, there is a spike in the PEM 1-3Hz FOM.
Yesterday night, I tried to run SR2 M2-M2 and M3-M3 (lower stages) in chamber transfer functions after the osems were centered on wednesday. Although both M2 and M3 watchdogs tripped during the measurement, so I am running it again tonight. (This time, I decreased the drive and increased the watchdog threshold).
Decreasing the drive didn't help either since I ended up with measurements without coherence. This morning I tried to drive M2 stage with high amplitude sinewaves at the resonant frequencies of the suspension for each DOF (L P and Y) to see if the osems would saturate. They don't. So a drive of 500 000 (cts) for L and 20 000 (cts) for P and Y (which is the limit before saturating the DAC) should be optimum at all frequencies. Started a new measurement which will run today.
This time, phase 3a M2-M2 and M3-M3 measurements of SR2, in air, with the HAM-ISI locked were succesful. The actuation is functioning, and the transfer functions for the three degrees of freedom are similar to the model.
There is one interesting feature to note for M2 stage. From 10Hz, the measured tf rolls up, as if some extra zeros were added to the tf. I checked the osem output filters, and they seem to compensate correctly for the coil driver (looking at the state diagram in state 1).
Attached are some SR2 phase 3a spectra for future reference
(David H, Thomas V, Greg G, Alasitair H, Matt H)
Well if yesterday was "The Empire strikes back", today was "Return of the Jedi" and the good guys had a win.
You may remember from this mornings alog that we had been having a few troubles with the alignment of TCSx.
After a brainstorming meeting with Aidan the decision was made to ignore the path defined by the flipper mirrors having problems with (what is supposed to be the central heating path) and align what is the annular heating path (which only uses mirrors) to the output beam splitter and through the irises defining the beam path up the periscope, into the chamber and onto the CP. We will then use the central heating mask instead of the annular heating mask (in the location the annular heating mask would be ), and thus temporarily turn the annular heating beam path into the central heating beam path.
The first step we did was to use a HeNe beam to adjust the output beam splitter and the beamsplitter just before the on table power meter so that the front and back reflections were in the same plane (they werent installed that way). We then went all the way back to the first large gold mirror after the polarisers (which are after the beckhoff controlled HWP) and mirror by mirror in the annular (now temporary central heating) beam path made sure that they were set so that the beam was in a plane with the table at a height of 4 inches.
Once the beam got to the output beamsplittler, the beamsplitter and the last gold mirror before the periscope was used to align the beam to the irises that we had defined to put the beam correctly into the chamber. I roughly made sure that the beam transmitted through the output beam splitter was going to the on table power meter, and the beam path that would go to the FLIR camera was beam blocked as I no longer no that the beam path is correct (I removed the lens there so that needs to be reinstalled).
A HeNe beam was setup to trace through the irises (heading in direction of going towards the periscope). Once the optic beam path had been re-established I swapped out the 1" irises we had (which had clipping on the beam occuring) for 2" irises. We then inserted a 2 inch gold mirror into the path between the 2 irises and sent the HeNe beam down towards HAM5 and the target that we had set up at a distance that mimicks where the CP would be. An "X" was marked on the card and the HeNe aligned to this "X' and the FLIR camera setup so that this spot was centered on the camera.
HeNe beam removed and the CO2 beam projected onto the target. Good to see that the CO2 beam appears to hit exaclty where the HeNe indicated it should (lets out sigh of relief)....so this should mean that the CO2 beam should go into the chamber and onto the CP correctly. Whilst doing the projection we also placed in the central heating mask (it has been rotated 90 degrees so that the rejected beam is directed towards the edge of the table not the center of the table as indicated in the drawing because the beam dump would not fit) and used the projection to help center the mask. Worked well...and success was declared. I dont have the pics of the projection, but pics were taken.
All beams have beam blocked so that if wanted to run the laser around the clock we can (we wont be until given the go ahead by the local LSO). A bugzilla list (Bug 868...https://services.ligo-wa.caltech.edu/integrationissues/show_bug.cgi?id=868) has been made of the tasks that can think of that are still outstanding/need to be done for this table.
One concern: A couple times today we had further issues with the HWP. We would dial up an angle for it to go to, the MEDM screens would indicae that the HWP was at the angle we had requested yet it physically was at a different angle. I have asked Thomas to look into tomorrow as this is a concern.
Pic:
TCScurrentalignmentstanding shows a quick summary of whats aligned and what still needs to be done
Awesome work. Great job doing a difficult operation in a safe manner--thanks. I think we can start running TCSx unattended starting Monday.
Some pictures from the FLIR of the projection in action. These pictures show the projection and the projection through the heating mask onto our paper target. The heating seen was about 2° C above ambient and the ruler in the picture is 12"
Pics of projection setup and also the table as it stood when I left thursday night
J. Kissel, for K. Izumi, and S. Ballmer Now that Stefan and Kiwamu have the first reasonably successful evening with ALS DIFF (see LHO aLOG 11759), I wanted to make an assessment of how their filter design ended up compared to my original design (see LHO aLOG 11676). I attach the frequency dependence of each stage, divided into the distribution filters, plant inversion filters. Then I attach total path (with gain filters included). There's still a little bit of confusion about the distribution of over-all gain of the system i.e - the ALS DIFF PLL's error signal, which serves as the DIFF sensor, had a some calibration filters turned OFF for some reason, leaving the output in [V] instead of the planned [um] - converting the overall SUS actuator gain to be [ct_{TST DAC} / um_{ISC IN}] has not yet been installed, leaving the actuator gain still in [ct_{TST DAC} / ct_{ISC IN}] so it would take some work to understand the over gain of the loop and/or with which UGF Stefan and Kiwamu ended up. Contrasting the creation of the super actuator between SB + KI vs. mine: - They've used the blend filters I've installed identically, so no mystery there. - For the plant inversion, they've diverted from my design in two ways: - A much more accurate inversion of the resonant forest for each stage, resulting in high Q filters with long impulse responses -- the price paid for phase accuracy - They've inverted the resonant forest for the TST stage, creating a resultant very high-Q resonant feature in the inversion filter to balance the zero in the TST to TST plant at 0.87 [Hz]. I did not invert the TST stage, and managed to scrounge up enough phase for the *model* to be stable (but this means little compared with reality.) - Instead, they've turned the TST (and each subsequent stage above) into a 1 [Hz], Q = 1, single pendulum. Unfortunately, since the ALS DIFF lock isn't too terribly stable, we can't get more than a few frequency data points to confirm stability, but we'll try again tonight. I think the reasons why they were saturating with the overall unity gain frequency only at ~1.2 [Hz] (as opposed to my model of 15 [Hz]) is because of the mystery factor of 4 missing from the TST mass drive (see LHO aLOG 11676), and because we still don't have ETMY up and running because of ESD woes (yet to be aLOGged) -- i.e. a factor of 8 in drive strength that's missing. According to all the modeling done thus far and now a measurement, we really need it! Next up -- find the factor of four in the ESD and fix it! ------------------- Relevant Configuration Record (gain = 1.0 if not mentioned): H1:ALS-C_DIFF_PLL_CTRL FM3 "antiVCO" FM4 "cnts2V" G = 10.0 (LSC Input Matrix element = 1.0) H1:LSC-DARM_IN FM1 "ALSDIFF" FM2 "invPlant" FM3 "Boost" G = 10.0 (LSC Output Matrix element = 1.0) H1:SUS-ETMX_L3_ISCINF_L (these were the extra last minute filters added to try and manipulate the overall super-actuator from saturating) FM6 "p5z50" FM7 "p5z50" H1:SUS-ETMX_M0_LOCK_L FM1 "invL2L1" (part one of plant inversion filter) FM2 "invL2L2" (part two of plant inversion filter) FM3 "top/tst" (gain only filter to compensate for the gain ratio) FM5 "blend LP" H1:SUS-ETMX_L1_LOCK_L FM6 "invL2LNEW" (part one of plant inversion filter) FM7 "patch" (part two of plant inversion filter) FM8 "LISOfit" (part three of plant inversion filter) FM9 "uim/tst" (gain only filter to compensate for the gain ratio) FM3 "blendHP" (UIM-TOP HP complement) FM4 "blendLP" (UIM-TST LP complement) H1:SUS-ETMX_L3_LOCK_L FM6 "MatchedinvL2L" (part one of plant inversion filter) FM7 "patch" (part two of plant inversion filter) FM4 "blendHP-M0" (TST-TOP HP complement) FM5 "blendHP-L1" (TST-UIM HP complement) H1:SUS-ETMX_L3_LOCK_BIAS_INMON = 125000 [cts] No linearization algorithm installed.
Stefan, Kiwamu,
We spent this afternoon to continue working on the PRMI lock. After an adjustment of the MICH gain, it became able to reliably lock.
Even though it stays locked for typically 2 minutes or so, it looses the lock for unknown reason.
(The gain adjustment)
To get the PRMI stably locked, the MICH gain had to be significantly reduced. The original gain setting by guardian was 16, but this was too big to have a UGF at around 10 Hz. At the end of the exercise, the gain ended up to be 2. I don't understand why it needs to be such low. Anyway, once the gain was adjusted, it locked repeatedly and no gain peaking or saturation were found. Good. I didn't change the PRCL gain at all -- it was fine with the original gain of 1.4. The attached is a screen shot of the PRMI buildup in striptool. The power build up observed by POP18 was 70 at highest and typically between 40 and 60. This is almost the same as before (see alog 10472). This corresponds to a power recycling gain of approximately 6.
(Lock losses)
For some reason, it typically unlocks after a couple of minutes. According to the feedback as well as error signals, it is not due to servo instability. Also I didn't see a sign of saturation in PRM, PR2 or BS. A funny thing is that the MICH loop acts odd before it looses lock. The attached below is time series of various feedback signals when the PRMI lost lock. It unlocked at t=29 sec. As clearly seen in the plot, the MICH feedback suddenly became quiet at t=28sec -- it seems as if a low-pass filter was enabled. I looked into two lock loss events and both events exhibited the same behavior. I believe that this is the last obstacle which prevents us from robust lock. This needs to be fixed.
There are currently 364 unmonitored conlog channels after I updated the list this afternoon. These are all ASC channels and appear to be due to the fact that a make install has been done without a restart. Since we expect a restart soon, I will leave the conlog channel list as is.
With much help from Apollo Mark we positioned and torqued down 170kg (10)xD0901075-03 Bulk Trim Mass per the layout on D1001139-v2. I did NOT viton damp any of these--SEI will take care of that after things settle.
08:33 Jeff and Andres heading out to work on SR3 08:58 Apollo done craning box for Joe D. at mid Y 09:19 Betsy going into HAM4, baffle and payload work 09:32 Let car from fire department in through gate 09:45 Praxair driver called to report that he was 10 - 15 minutes away 09:47 Travis and Margot heading out to work on the ACB in the LVEA test stand Rick investigating PSL ISS locking problems. He adjusted the ISS reference signal (H1:PSL-ISS_REFSIGNAL) from -1.79 to -1.69 and the ISS locked with ~ 8% diffracted power. David H. going to get parts from the LVEA X slab, then Hartman sensor work for ~30 minutes. 10:27 David H. done, out of LVEA 10:56 Jeff and Andres done at HAM5 11:03 Sheila working on the end Y ISC table 12:24 Justin transitioning the LVEA to laser hazard for TCS work 12:35 School tour in control room 13:03 Thomas V. restarted the H1ECATC1 system manager to add links for the TCS Y rotation stage. He then went to connect the stage to the H1 PSL ENV Beckhoff chassis (requiring a power cycle of this chassis). 13:10 John W. to end Y chiller yard to look at water system 14:24 Hugh heading out to add dummy mass payload to ISI table in HAM5 15:45 I updated the conlog channel list using the file that Dave generated yesterday. The number of unmonitored channels is taking a long time to come down.
We have notice a steady patter of IPC receive error on the LSC model for the H1:LSC-[X,Y]_TR_A_RFM signals coming from ISC EX and EY for many week. Lately with an increase in the number of ISC IPC channels this error rate has been increasing (it used to be one an hour or so).
It should be noted that these are almost always single errors, i.e. one data error in 16384 in a one second period. Very occasionally the error rate is 2.
I have just measured the number of errors over a 10 minute period for the IPC channels. The Y arm signal gave 30 errors (average of one every 20 seconds), the X arm gave 5 errors (average one every two minutes).
I have also noted that:
there are other RFM IPC channels coming from ISC end stations to LSC which don't show any errors (H1:ALS-[X,Y]_ARM_RFM).
there are the same number of IPC channels from X and Y arm, so why is the Y error rate 6 times higher?
Even at 30 errors in 10 minutes this is an error rate of 0.0003%
Robert had tried to operate the YEND chiller 1 on its variable speed drive but had difficulties with it.
I spent some time out in the chiller yard today and the chiller now appears to be working at 35 hz (rather than the line frequency) I am not sure why it is working now but it may have just been a startup issue after having sat for a long time with no water flow through the heat exchanger. I did have trouble starting the unit but ran the frequency up to 50hz where the chiller started and continued to run. After several hours I have dialed the frequency down to 35 hz. Temperatures in the heat exchanger(evaporator) appear to be normal. The error message when tripped was " Chilled Water Flow(Ent Wtr Temp)"
If there are problems with cooling in YEND please switch to the other chiller. (Or call me)
john
Plot attached.
(Alexa, Daniel)
Continuing yesterdays work we locked on PRX and installed the beampspitter in the POP path in front of POPAIR_A. The beam was very weak and we had some fun aligning it. We needed an additional lens (ROC 500mm) to keep the beam small. After the beam combiner we measured 170nW of power. Another short focal length lens was installed after the combiner to focus the beam down. We are still missing a photodetector.
We have set up the ISCT1 ALS-Y-GREEN digital video camera (number 05 on the camera overview screen). We have left the CCD on the table in case we need it for any reason. We are still using the CCD camera for the x-arm, but the digital video camera is ready and in place when we want to swap that out.
I also brought BBPD (S1200247) from MY to ISCT1. The PD is mounted. Power and cables are still needed, but Kiwamu indicated we can borrow the 3f PD power from the legacy PD interface.
I have removed the CCD camera used for the y-arm beam and returned it to the shelves by the field racks.
I placed an ND06A (25±4% transmission for 1064nm) before the 50/50BS to reduce the power coming in from the PSL reference path. We also have a ND10A (10±4% transmission for 1064nm) readily avaliable (and it's an easy swap) if need be. The BBPD max incident power is 50mW for 1064nm. I have not measured the incident power yet.
Thanks to Stefan and Kiwamu, we got PRMI locked. This is much easier to work with :). I was able to do a rough aligmnet of the two beams by adjusting the BS. It remains to install the BBPD, but we have everything ready, so this should not take long and we should be able to finally do our measurement tomorrow.