model restarts logged for Thu 03/Nov/2016 - Wed 02/Nov/2016 No restarts reported
model restarts logged for Tue 01/Nov/2016
2016_11_01 11:14 h1ioppsl0
2016_11_01 11:14 h1psldbb
2016_11_01 11:14 h1pslfss
2016_11_01 11:14 h1psliss
2016_11_01 11:14 h1pslpmc
2016_11_01 11:23 h1calcs
2016_11_01 11:23 h1iopoaf0
2016_11_01 11:23 h1ioppsl0
2016_11_01 11:23 h1ngn
2016_11_01 11:23 h1oaf
2016_11_01 11:23 h1odcmaster
2016_11_01 11:23 h1pemcs
2016_11_01 11:23 h1psliss
2016_11_01 11:23 h1tcscs
2016_11_01 11:24 h1calcs
2016_11_01 11:24 h1iopasc0
2016_11_01 11:24 h1ioplsc0
2016_11_01 11:24 h1iopoaf0
2016_11_01 11:24 h1iopsusb123
2016_11_01 11:24 h1lscaux
2016_11_01 11:24 h1lsc
2016_11_01 11:24 h1ngn
2016_11_01 11:24 h1oaf
2016_11_01 11:24 h1odcmaster
2016_11_01 11:24 h1omc
2016_11_01 11:24 h1pemcs
2016_11_01 11:24 h1psldbb
2016_11_01 11:24 h1pslfss
2016_11_01 11:24 h1pslpmc
2016_11_01 11:24 h1susitmy
2016_11_01 11:24 h1susprocpi
2016_11_01 11:24 h1tcscs
2016_11_01 11:25 h1ascimc
2016_11_01 11:25 h1asc
2016_11_01 11:25 h1hpiham4
2016_11_01 11:25 h1hpiham5
2016_11_01 11:25 h1iopseih45
2016_11_01 11:25 h1iopsush2a
2016_11_01 11:25 h1iopsush2b
2016_11_01 11:25 h1omcpi
2016_11_01 11:25 h1susauxasc0
2016_11_01 11:25 h1susbs
2016_11_01 11:25 h1sushtts
2016_11_01 11:25 h1susim
2016_11_01 11:25 h1susitmpi
2016_11_01 11:25 h1susitmx
2016_11_01 11:25 h1susmc1
2016_11_01 11:25 h1susmc3
2016_11_01 11:25 h1susprm
2016_11_01 11:27 h1hpiham2
2016_11_01 11:27 h1hpiham3
2016_11_01 11:27 h1iopseih23
2016_11_01 11:27 h1iopsush34
2016_11_01 11:27 h1iopsush56
2016_11_01 11:27 h1isiham2
2016_11_01 11:27 h1isiham3
2016_11_01 11:27 h1isiham4
2016_11_01 11:27 h1isiham5
2016_11_01 11:27 h1susmc2
2016_11_01 11:27 h1suspr2
2016_11_01 11:27 h1suspr3
2016_11_01 11:27 h1sussrm
2016_11_01 11:29 h1hpibs
2016_11_01 11:29 h1hpiitmx
2016_11_01 11:29 h1iopseib1
2016_11_01 11:29 h1iopseib2
2016_11_01 11:29 h1iopseib3
2016_11_01 11:29 h1isibs
2016_11_01 11:29 h1isiitmx
2016_11_01 11:29 h1isiitmy
2016_11_01 11:29 h1susomc
2016_11_01 11:29 h1sussr2
2016_11_01 11:29 h1sussr3
2016_11_01 11:30 h1hpiham1
2016_11_01 11:30 h1hpiham6
2016_11_01 11:30 h1hpiitmy
2016_11_01 11:30 h1iopseih16
2016_11_01 11:30 h1isiham6
2016_11_01 12:05 h1alsex
2016_11_01 12:05 h1calex
2016_11_01 12:05 h1iopiscex
2016_11_01 12:05 h1iscex
2016_11_01 12:05 h1pemex
Tuesday maintenance. ADC addition to h1oaf0 caused dolphin crash in corner station. Rebooted h1iscex to check for ADC offset. No DAQ restarts required.
model restarts logged for Mon 31/Oct/2016 - Fri 28/Oct/2016 No restarts reported
SEI: No issues to report SUS: No issues to report PSL: Ultrasonic flow sensor installed, not reading back, in contact with vendor VAC: No issues to report FAC: Still searching for water leak, 1/2 gallon per minute CDS: Demod chassis swapped with spare, investigating in lab (alog 31181)
TITLE: 11/04 Owl Shift: 07:00-15:00 UTC (00:00-08:00 PST), all times posted in UTC
STATE of H1: Corrective Maintenance
INCOMING OPERATOR: Patrick
SHIFT SUMMARY: Sheila was working hard all night at 36W with a 6 hour lock. Broke lock about 45min ago and Richard is working on possibly broken POP90 demod input.
LOG:
I looked over the mechanical drawings of the high power attenuator. The position of the mount holding the thin film polarisers is largely set by two dowel pins in the base and the machining tolerances. However the nominal angle of incidence of the design is 55.014 deg. The thin film polariser coating has a measured transmission of 99.552% and 0.036189% for p and s polarisations respectively, which is a ratio of ~2750:1. There is no information about the coating's sensitivity to incident angle but generally speaking these sort of coatings do tend to be a little sensitive to incident angle. That said, it might just be that the beam alignment into the high power polariser is off a little.
FAMIS#6495
No water was added to the crystal or diode chiller, both were at their nominal levels.
23:32 Adjusted fiber polarization for Y arm and tweaked X arm as well
23:35 /ligo computer crash, momentarily interrupted work stations and internet.
00:05 Robert out to EY. OpLev Damping L2 P gain ramped to 0 from -300.
00:39 a2l_min_LHO.py
00:42 script done
00:47 a2l_min_PR2.py
00:48 set observatory mode to 'commissioning' about 1 hour late.
00:50 script done
00:53 00:39 a2l_min_PR3.py
00:57 script done
01:28 damping violin modes: ETMY mode7 and ETMX mode4.Y- Mode 7; I changd gain from -20 to -60 significant damping occurred. X-Mode4 reversed phase from +60 to-60 and changed gain from -18.343 to -150. It seemed to be damping slightly but then returned.
02:37 after reverting ETMX Mode4 phase and changing gain to -120.343, the RMS value has come down to 4.42 from 4.59. I'm not sure if this is my doing or just a normal ringdown.
05:54 PI mode 27 ringing up. changed phase from 150˚ to 80˚.
05:08 Lockloss. Turning BRS back on at EY. Also, OpLev damping re-enabled back to -300 gain.
06:59 Turning over to TJ
I checked that the makeup air in the PSL enclosure was not limiting us at the 20% nominal setting. However, I found that at 100%, it would limit us. Figure 1 shows the difference in DARM between makeup air on/off at 100% fan speed. Red is makeup air on, Blue, off. I am particularly concerned with the regions such as between 15 and 22 Hz where the DARM noise increases but the microphone level does not increase. I don’t think we can make accurate estimates of air current noise using the microphones.
Another source of air currents that may produce jitter are the temperature variations along the beam path. Figure 2 shows a FLIR image of the beam path between the HPO and the DBB. I took this image on Monday. The table surface reading was 23 degrees C while the walls of the HPO were 26 degrees and the walls of the DBB were 26.5. I think that the temperature differences with respect to the table may generate an air current down onto the table, crossing the beam path, and up the sides of the boxes. The space between the Front end and the HPO is a similar channel. Downstream of the jitter-reducing PMC, near the main beam path under the periscope, lies the PI piezo controller (Figure 3). Because of its transformer, it is a warm 32 degrees C, nearly ten degrees hotter than the surrounding environment. The cool air coming in to replace the rising current above the controller may cross the main beam path. This would be very easy to move somewhat further away to test for any change in DARM.
for my own edification, I took a look at End X during a wind time on Oct 17. wind storm started at about 1 am Pacific time and went for about 8 hours. (note to self - repeat this for Oct 14 - see Jim Warner alog https://alog.ligo-wa.caltech.edu/aLOG/index.php?callRep=30547) I can see several things: 1) The wind direction indicator seems to work as long as the wind is blowing hard enough. This is great. Conversion is : add (180-37) = 143 degs. This makes 90 (towards -Y) into 233 (from the SW, up along the Y arm) see plots 1&2 for wind history during monitor period. 2) building tilt is still related to wind. From 1 mHz to 20-30mHz, the relation between floor tilt and wind-speed^2 is quite clear - good coherence, time series look similar. (plots 3&4) TF is odd though,(plot 5) it doesn't appear to follow Kramers-Kronig. 3) The wind speed indicator gives decent data at frequencies below 20-30 mHz. This limit is set by the discrete reporting levels in some ADC. (see plot 6) There may also be some low pass filters, but those are the biggest limit on data quality.
Here are some noise estimates for our current configuration (at 25W). The PMC PZT noise was measured before tuesdays fix, if I can get some time I will remeasure that tonight.
These curves are a combination of excess power measurements, gwinc curves for thermal and residual gas, and Evan Hall's noise budget code.
Obvious things that are still missing are frequency noise and ESD DAC noise.
Looking at the noise budget above, we should be limited by shot noise around 100Hz, so increasing the power should expose the noise more. I decided to try 35Watts to see what we can learn.
We locked at 50Watts with similar settings 2 weeks ago without problems, but there were a few things to work out for locking at 35Watts:
There are now THREE a2l scripts that we will be running once during EACH lockstretch. Patrick mentioned them in his time log. I'm tagging Opsinfo with the information again.
cd /opt/rtcds/userapps/release/isc/common/scripts/decoup ./a2l_min_LHO.py ./a2l_min_PR2.py ./a2l_min_PR3.py
that is all :)
A note on the (3) A2L measurements.
As of this week, we want to run the ...LHO.py file at the beginning of locks (i.e. right after we reach NLN). It takes on the order of 10min.
Sometimes you might not want to run it. If the DARM specrtra looks good around 20Hz, then you are good. It's a judgement call, but in general, this helps with sensitivity. Will put this in the Ops Sticky Note wiki & should get in the Ops Checksheet soon.
(Thanks to Jenne & Ed for sharing the alogs about this!)
Over the last couple of days we noticed the POPAIR_B_90 was randonly jumping up and down.
Further investigating this, we found that just touching the SMA connector of the 90MHz LO of the POPAIR_B_90 demodulator box, the phase jumps by easily 90deg.
Smells like that LO input is broken - but we'd have to take the chassis out to fix it.
Found the SMA connectors to be over tight. I could not remove them with out pliers. The SMA insulating sleeves were in bad shape. The filter for 90MHz was not seated properly. Re-seated the filter, Change the rear panel with a new one. Made sure all of the connector inside the chassis were torqued properly. Re-installed chassis. Fault report 6599 https://services.ligo-la.caltech.edu/FRS/show_bug.cgi?id=6599 While in the LVE re-torqued all the SMA connections in the racks by the PSL. There were a number of loose ones. (AGAIN) We have a torque wrench lets use it.
In preparation for Robert's incursion into the VEA for testing.
J. Kissel, D. Tuyenbayev We're still not getting the IFO duty cycle to get the desired uncertainty on the single-frequency actuation strength scale factor measurement of the UIM and PUM stage and we're running out of time, so I've increased the SNR of these temporary lines by another factor of ~3 over yesterday's increase (see LHO aLOG 31108). Oscillator Freq (Hz) Old Amp (ct) New Amp (ct) ETMY UIM 33.7 180 500 ETMY PUM 34.7 81 300 Hopefully Robert's activities tonight won't impact the ~30 Hz region of the sensitivity, and we can turn things off soon.
Jeff K, Darkahn T,
We calculated actuation strengths of L1 (UIM), L2 (PUM) and L3 (TST) actuation stages using calibration lines from 6 lock stretches in the last two days.
Preliminary results are given in the attached plots. Standard deviation on estimations of AU and AP are ~1.2% and for AT is ~0.4%.
Data points were taken at GPS times with HOFT_OK_BIT = 1 (segments are listed below).
# seg start stop duration
0 1162123790.0 1162124750.0 960.000
1 1162124840.0 1162125190.0 350.000
2 1162125280.0 1162125480.0 200.000
3 1162127120.0 1162129210.0 2090.000
4 1162134280.0 1162137150.0 2870.000
5 1162162170.0 1162163370.0 1200.000
Increased line amplitudes will hopefully allow us to get AU and AP actuation strengths with subpercent 1-sigma error bounds.
Jeff K, Greg M, Darkhan T,
After the L1 and L2 line amplitude increase it seems that we got better uncertainties in the esitamtions of the sus. stage actuation strengths.
This time we filtered the data using the IFO range channel, we used 50 MPC as a threshold. And from the remaining data we made historams of three different time intervals. We did not yet investiage why the noise levels of the lines are different at each of these intervals. The uncertainties for A{U,P,T} are given for the least noisy interval (blue data points).
Jeff K, Greg M, Darkhan T,
We calculated [N/ct] actuation force factors calculated from the ~35 Hz independent L1, L2 and L3 lines:
KU = 8.012-8 +/- 3.873-10 N/ct ( std(KU) / |KU| = 0.0048 )
KP = 6.482-10 +/- 2.748-12 N/ct ( std(KP) / |KP| = 0.0042 )
KT = 4.253-12 +/- 1.679-14 N/ct ( std(KT) / |KT| = 0.0039 )
During a Nov. 4 lock stretch we got a factor of 3 improvement of the standard deviations compared to the previous day (blue data points vs. green).
In most recent 2 days we got more data with longer lock stretches, which can help us to better bound the uncertainties. Analysis of this data would require including an updated DARM digital filters, the IFO response changed on Nov. 5 (see LHO alog 31201) which can bias on our calculations if not taken into account.
The outliers were removed in a following way:
- Took >= 50 MPC data and removed data points that fall outside of 2-sigma std. deviation (some large outliers were not filtered by this step);
- one more time calculated std. and mean in the remaining data points and removed 2-sigma outliers (this step helped to remove large outliers).
- The mean and 2std. of these data points were shown with black solid line and dashed lines.
The final reported mean values and standard deviations were taken from the blue data points ( GPS [1162252470, 1162271230] ), L1 and L2 data was least noisy during this period. This mean value and its std. were shown with blue solid and dashed lines.
Attached is a 60 day trend of PT140 which is a one of the new Inficon BPG402s? IP7 and IP8 have been a steady 5000 volts for this time period. Is this a gauge thing? I haven't been intimate with what Gerardo, John and Chandra have learned regarding the behavior of these new wide-range Bayard-Alpert/Pirani hybrids but this slope looks "not insignificant"
That slope looks really fishy. Are both IPs fully pumping? What does HAM6 pressure look like (also hot cathode ion gauge)? Did PT 170 and 180 flatten out after degassing?
We think that the pressure increase is due to temperature, see attached. aLOG noting temperature change.
Since we are talking temperature change in the LVEA, note the vertical change on some of the optics (BS and ITMs), other are affected as well.
J. Kissel, M. Evans, D. Barker, H. Radkins A confusing bit of settings wrangling* after the unplanned corner station computer restarts on Tuesday (LHO aLOG 31075) in the SUSITMPI model meant that a large fraction of the EPICs records in the ITM PI system were wrong. As such, we believe this was the cause of battles with Mode 27's PI a few nights ago (LHO aLOG 31111). In order to fix the problem, we used the hourly burt backups in /ligo/cds/lho/h1/burt/yyyy/mm/dd/hh:mm/ to restore settings all settings to Monday (2016/10/31), before the computer restarts. Further, Matt performed a few spot checks on the system, and suspected it good. *Settings wrangling: There were several compounding problems with the SDF system which meant that (1) The front-end did not use the safe.snap file upon reboot, and restored bogus values (2) The safe.snap file, which we'd thought had been kept up to date, had not been so since May. Why? (2) The safe.snap file for SUSITMPI used upon restart, /opt/rtcds/lho/h1/target/h1susitmpi/h1susitmpiepics/burt/safe.snap, is a softlink to /opt/rtcds/userapps/release/sus/h1/burtfiles/h1susitmpi_safe.snap. Unfortunately, *only* that model's safe.snap that had its permissions mistakenly set to a single user (coincidentally me, because I was the one who'd created the softlink from the target directory to the userapps repo.), and *not* the controls working group. That means Terra Hardwick, who had been custodian of the settings for this system, was not able to write to this file, and the settings to be restored upon computer reboot had not been updated since May 2016. Unfortunately, the only way to find out that this didn't work is to look in the log file, which lives in /opt/rtcds/lho/h1/log/${modelname}/ioc.log and none of us (save Dave) remember this file existed, let along looked at it before yesterday **. There are other files made (as described in Hugh's LHO aLOG 31163), but those files are not used by the front-end upon reboot. I've since fixed the permissions on this file, and we can now confirm that anyone can write to this file (i.e. accept & confirm DIFFs). We've also confirmed that there are no other safe.snap files that have their write permissions incorrectly restricted to a single user. ** Even worse, it looks like there's a bug in the log system -- even when we confirm that we have written to the file, the log reports a failure, e.g. *************************************************** Wed Nov 2 16:39:10 2016 Save TABLE as SDF: /opt/rtcds/lho/h1/target/h1susitmpi/h1susitmpiepics/burt/safe_161102_163910.snap *************************************************** Wed Nov 2 16:39:10 2016 ERROR Unable to set group-write on /opt/rtcds/lho/h1/target/h1susitmpi/h1susitmpiepics/burt/safe.snap - Operation not permitted *************************************************** Wed Nov 2 16:39:10 2016 FAILED FILE SAVE /opt/rtcds/lho/h1/target/h1susitmpi/h1susitmpiepics/burt/safe.snap *************************************************** (1) This is quite alarming. Dave has raised an FRS ticket (see LHO aLOG 6588) and fears it may be an RCG bug. I wish I could give you mode information on this, but I just don't know it. In summary, we believe the issues with SUSITMPI have been resolved, but there's a good bit of scary stuff left in the SDF system. We'll be working with the CDS team to find a path forward.
The LLO CDS system has scripts running that do regular checks on file permissions on the /opt/rtcds file system to try to catch these. Please contact Michael Thomas for details. We'll check that we are looking for this issue as well (and are acting when problems are found)
I've opened FRS6596 to do the same snap file permissions checking as LLO.