TITLE: 10/26 Eve Shift: 23:00-07:00 UTC (16:00-00:00 PST), all times posted in UTC
STATE of H1: Aligning
INCOMING OPERATOR: Jeff
SHIFT SUMMARY: Slow recovery from a big maintenance day. There were ISS struggles in the beginning, then ALS was pointed to nowhere, followed by many hours trying to figure out why the IMC was not locking. While Sheila and I had seemed to have tried everything, the MC just suddenly locked by itself. The FSS PZT Mon may have been oscillating for a while which could have caused much of the issue, but we are not 100% sure that this was the only problem for that time. Initial alignment also had PRM and SRM waaaaaay off, which meant adjusting other optics after adjusting those as well. Just finished an initial alignment and starting up the chain before I hand it off to Jeff.
LOG:
DarkhanT, Yuki Inoue (KAGRA), RickS (SudarshanK assisting with image analysis over the phone - until the phone died).
Today, we went to Yend to investigate the apparent clipping that EvanG had discovered (see entry 30827).
We found that both beams were off centered on the aperture of the Rx module integrating sphere, with the Outer (lower) beam clipping on the aperture (see attached image). Blocking one beam and then the other revealed that the increased noise in the Rx power sensor spectrum was all due to the clipping of the Outer beam.
Camera images revealed that the beams had moved on the ETM as well (exonerating movement of the ETM as the cause of the movement on the Rx side).
Analyzing Pcal camera images we found the beam position offsets from the optimal locations were (x, y): Upper (-1.5, 1.8); Lower (-6.9, -2.5) (millimeters) Usual x,y convention: positive x, right; positive y, up.
Not knowing what had moved, we used the output steering mirrors in the Tx module to center the beams on the Rx intetrating sphere aperture (see attached photo).
After moving the beams, analysis of camera images (see attached) gave the following beam locations (x, y): Upper (-1.4, -0.9); Lower (-1.3, -1.4) (millimeters).
These are within our 2 mm tolerance.
We installed apertures at the output of the Tx module and at the input (just upstream of the steering mirrors) in the Rx module.
We will repeat the Yend calibration using the Working Standard as soon as possible.
Spectra look much better too! Attached are times from before Oct 11 maintenance work (blue), just after Oct 18 maintenance work (green), and this morning after the clipping had been fixed (red). Note that the amplitude of the 331.9 Hz has returned to the O1 amplitude. A trend of the mean power level over the last 10 days is also attached. The calibration discrepancy between TX and RX PD is likely now reduced. Previously, as identified by Shivaraj (LHO aLOG 30845), the discrepancy was ~4%. Now the discrepancy is less than ~1% as the end of the trend indicates.
Work Permit | Date | Description | alog/status |
6280.html | 2016-10-25 16:29 | DAQ NDS has bug which reports many errors to the log file when it encounters the new MD5 files. Fix is to remove this reporting from the nds process (note, not the daqd process). | 30875 |
6279.html | 2016-10-25 09:19 | Perform timing-related measurements at end stations. Output of the CW injection will be disabled for a short while. | 30854 |
6278.html | 2016-10-25 08:51 | Investigate apparent clipping of Pcal beam, first trying to determine which beam is clipping. Adjust alignment to relieve clipping. Re-calibrate if adjustment of alignment is required. | 30827 |
6277.html | 2016-10-25 08:31 | Perform scheduled maintenance to scroll compressor #3, #4, #5 @ X-End vent/purge-air supply skid. Maintenance activity will require for the compressors to run for brief periods of time. Lock-out/tag-out power to skid. | 30853 |
6276.html | 2016-10-25 08:07 | Increase the light on ISS PDA (first loop) [Change the neutral density filter to a less dense number?] | 30871 |
6275.html | 2016-10-25 07:31 | Update NDS2 client software to version 0.13.0 for Ubuntu 12 and Ubuntu 14 workstations. | 30843, 30859 |
6274.html | 2016-10-24 15:05 | Remove view port covers in input optics area, output optics area and end stations. Plastic sheet will be available if not already present. LVEA/VEA will be laser hazard. | 30867 |
6273.html | 2016-10-24 14:36 | Add whitening filter to PMC HVMon channel. | 30846, 30859 |
6272.html | 2016-10-24 12:42 | Experiment with frame write priority/scheduling settings to help address re-transmit issues. We will reconfigure h1fw2 and if the changes do not cause regressions may move the configuration to h1fw0 & h1fw1. | 30859 |
6271.html | 2016-10-24 11:12 | E1600292 was approved and will be applied to the VCO in the corner station. This will remove 420kHz noise from the VCO +/- 24V rails. | 30869 |
6270.html | 2016-10-24 10:55 | Remove and replace UPS batteries for Y-END, X-END, Y-MID, X-MID, and Corner Station vacuum racks. | 30823 |
6269.html | 2016-10-24 10:22 | Start and run QDP80 pumps (minimum of 30 minutes as routine PM) * Energize Main Turbo Pump controllers and note indicated pressures on either side of fore line isolation valve (aka "Safety Vale") * with header side of Safety Valve at minimum pressure, dump accumulated gas withing turbo pump into fore line via briefly opening Safety Valve * Record pressures in turbos afterwards as "t0" for long term rate-of-rise measurement | 30873 |
6268.html | 2016-10-24 10:12 | Install picomotors into the mounts for mirrors M06 and M07. This will allow remote tweaking of the beam alignment into the PSL PMC. The PSL will remain up, although we will close the external shutter when actually installing the motors. The beam alignment into the PMC will need to be re-done after the installation. | 30798, 30801 |
6267.html | 2016-10-24 10:04 | Check/recharge AR HEPI Fluid Accumulators: All SEI platforms down, Fluid Pump Stations Off, check pressure in Accumulators, recharge as needed. Return system to operation. 2ish hours. | 30850 |
6266.html | 2016-10-24 09:50 | Install gutter on the north side of the OSB Building. | |
6265.html | 2016-10-24 06:41 | Perform quarterly lubrication of all Axivane Supply Fans on site. | |
6264.html | 2016-10-21 15:16 | Expand H1EDCU_DAQ.ini to include the new DAQ diagnostics EPICS channels. DAQ restart required. | 30859 |
6263.html | 2016-10-21 13:52 | Removal of ISI-WIT projections of GS13s into supension point, as is now covered by SEI models (E1600028). Also revamp of SUS channel storage in the frames (E1600316). | 30728, 30821, 30844, 30859 |
6262.html | 2016-10-21 13:34 | Pull/Extend picomotor controller cable (DB25) cable from ISCT1 into PSL. Cable will then be connected to picomotor breakout box D1101738 inside PSL. | 30726 |
6261.html | 2016-10-21 09:24 | Do a noise measurement on the PSL HV power supply in the CER mezzanine. | 30781, 30725 |
6260.html | 2016-10-19 14:07 | Turn off Proxmox server to install more memory (Proxmox is a virtual host that holds: Matlab license server, autoburt and H0epics) those server will shutdown as well during the installation time. | 30859 |
6259.html | 2016-10-19 13:41 | Improve diagnostics: better error check for ALS end stations when locked with red; enable device info. | 30842 |
Previous Work Permits | |||
6247.html | 2016-10-17 08:57 | Pull power and network cable for RGA in corner station. Work will consist of climbing over HAM4 and pulling around BSC2 and BSC3. | 30635, 30799 |
Keith found the source of our full disk. When md5 checksums where added to the frame directory the NDS server began logging error messages for each non .gwf file that was found. This ended up contributing to huge log files +90GB.
We have updated the nds process to quiet these messages as this is no longer an error condition.
See work permit 6280 and bug 1054.
Cyropump #4 was generating alarms today, both before and after Dewar fill. After trending signals, it appears the LLCV and exhaust noise has been growing over time. Pump fill level and LLCV setting stabilized after I opened the bypass exhaust valve. Wondering if the check valve is faulty. Will test tomorrow. I have removed and reinstalled it a couple times in the last month with TC testing.
Kyle, Chandra We ran all QDP80 roughing pumps on site today for maintenance and for refresher (WP 6269); checked for gross leaks in foreline/turbo volumes. Found one at MX. EY as found pressure foreline = 14 Torr turbo = 0.58 Torr after rough pump down and following valve isolation foreline = 0.040 Torr turbo = 0.036 Torr MY as found pressure foreline = 2.3 Torr turbo = 0.60 Torr after rough pump down and following valve isolation foreline = 0.013 Torr turbo = 0.022 Torr LVEA - vertex as found pressure foreline = 2.2 Torr turbo = 0.67 Torr after rough pump down and following valve isolation foreline = 0.017 Torr turbo = 0.022 Torr LVEA - Xbeam manifold as found pressure foreline = 12 Torr turbo = 0.63 Torr after rough pump down and following valve isolation foreline = 0.021 Torr turbo = 0.039 Torr LVEA - diagonal as found pressure foreline = 5.4 Torr turbo = 0.54 Torr after rough pump down and following valve isolation foreline = 0.026 Torr turbo = 0.039 Torr LVEA - Ybeam manifold as found pressure foreline = 5.4 Torr turbo = 0.48 Torr after rough pump down and following valve isolation foreline = 0.025 Torr turbo = 0.034 Torr MX as found pressure foreline = 780 Torr turbo = 1.0 Torr after rough pump down and following valve isolation foreline = leaking turbo = 0.084 Torr EX as found pressure foreline = 6.6 Torr turbo = 0.43 Torr after rough pump down and following valve isolation foreline = 0.017 Torr turbo = 0.026 Torr The leak in the X-mid fore line is between the Turbo Header isolation valve and the Turbo fore line Safety Valve. Removed and examined the NW seals but nothing obvious. We verified each QDP80 shuts down with the absence of N2 purge seal gas supply except the Y-end QDP80 which did not shut down. Y-mid pump turned off due to overheating because cooling water was not valved in initially. It leaked a small puddle of coolant and ran OK upon cooling. We pumped down the purge air line in LVEA unintentionally.
FRS 4559
WP 6247
EX:
1. Placed HWS camera on seperate power supply. The power supply is underneath the ISCTEX table.
2. Finished cabling for RGA at EX.
LVEA:
1. Placed HWS cameras (X & Y) on seperate power supplies.
2. Terminated network cable for RGA in LVEA. Network cable is pulled to SUS-R3. Connection to switch needs to be made in CER.
2. Placed power distribution boxes (24V regulated down to 12V) for the ITM spool cameras, for both X and Y arms.
2. Placed junction box and landed power cables on top of H1:SUS-R5. This is part of the ongoing work for the 24V digital power distribution.
3. Started work on junction box on top of H1:SUS-R6.
The software for the HWS cameras needs to be restarted.
F. Clara, E. Merilh
[Changed the power level on PDA]
I went into the PSL today and changed the ND filter that was screwed on the PDA photodetector module (30415) in order to change the power level of the photo diode. Before the change the PDA DC singal read a relatively small value of 2.2 V. After the change, the DC signal became 3.8 V which is close to what PDB says 3.9 V. Indeed, the voltage readouts for the two diodes shown in the medm became close to each other (~ 4.5V). The new ND filter is actually a stuck of 0.2 and 0.5 abrorptice ND filters. It was an ND1 before.
[New setting for ISS inner loop]
The gain slider now should be 18 dB (which used to be 30 dB, 30415). This gain gives us a UGF of 54 kHz. This means that the open loop transfer function is almost identical to the one with PDB used as the in-loop sensor (29942) as expected. In fact, we can now switch the sensor between PDA and PDB without changing the reference offset or gain while keeping the loop closed. Though this typically changes the diffraction power by a few %. The new gain is now accepted in SDF.
The attached is a plot of the measured open loop transfer function with PDA. Also the raw data is attached. Also, I attach a noise spectrum seen at one of the analog output for measuring the transfer function.
M. Pirello, A. Ramiez, E Castrellon
Work Permit 6271
Per ECR E1600292 we applied the VCO capacitor mod to all 5 VCO's in the corner station and one at each end station. This process includes replacing the 10nF capacitors on C79 and C80 with 2uF capacitors, and checking the voltage rails to verify elimination of the 420kHz oscillations.
Corner Station Units:
S1200563, S1200559, S1200560, S1200564, S1200558
End X:
S1200561
End Y:
S1200566
Notes:
End X, there was a very inconvient clean room pole directly in the path of extraction for the VCO from the rack. We had to relocate 2 chassis to angle the VCO enough for removal. All chassis were put back in their original positions before leaving.
End Y, this VCO required more capacitance to remove all of the 420kHz noise on the -24V Rail, with the addition of a 2nd 2uF capacitor, the noise was eliminated.
After going through my notes, the following should also be logged.
VCO S1200563 is outfitted with a PLL board. This board is attached to the existing board via an SMA-T connector on the Low Noise VCO Board. This connector was very loose when we opened up the chassis, and the end that is supposed to connect to the PLL board was disconnected and wedged between two VCO modules. The SMA was very loose here. We showed Richard this and he advised us to remove the SMA-T and the SMA jumper cable which was disconnected, we then used an SMA cable torque wrench to ensure proper torque on the connectors.
When we worked on the 2nd PLL VCO chassis (S1200564), we noticed that the SMA-T was torqued, and the SMA jumper was attached to the PLL board.
We checked the cleanliness of the double paned port between the PSL and HAM1. The photo shows a smudge on the outside surface that extends into the center of the port. We think that a cleaning would help. There is dust on the inner pane, but I think the smudge on the outside is the most dangerous.
Robert, Cheryl, Gerardo
TITLE: 10/25 Day Shift: 15:00-23:00 UTC (08:00-16:00 PST), all times posted in UTC
STATE of H1: Planned Engineering
INCOMING OPERATOR: TJ
SHIFT SUMMARY: Entire shift was dedicated to maintenance activities.
LOG:
15:17 Kissel taking SUSes down for model work
15:25 Joe D to mids and ends for first aid kit maintenance
15:26 Fil, Ed to EX HWS camera work
15:30 Marc, Richard to LVEA
15:33 Cristina and Karen to ends
15:40 Gerardo to EY
15:52 Fan lubing complete
15:54 Kyle to EX
15:55 Cintas on site
15:56 Chandra to LVEA
15:59 Marc and Alfredo VCO work
16:04 Hugh to LVEA
16:07 Gerardo to EX
16:08 Pcal team to EY
16:13 Bubba and Richard to LVEA
16:20 Keita, Evan to EX then EY for timing measurements
16:26 Richard out
16:30 Betsy to LVEA
16:32 Robert to LVEA
16:42 Jason resetting Purple People Noise Eater
16:45 Joe D done
17:00 Cristina back, going to LVEA
17:01 Ed, Fil to back, going to LVEA
17:05 Hugh done
17:12 Corey to LVEA 3IFO inventory
17:17 Karen to LVEA
17:20 DAQ restart
17:46 Corey out
17:49 Betsy out
17:58 Chandra working on vacuum roughing pumps
18:11 Norco on site
18:17 Robert to EY
18:30 Kiwamu to PSL
18:41 Richard to EY for RGA work
18:46 Evan G and Keita to EX, Marc done
18:56 Hugh done
19:06 Jason and Peter to PSL picomotor work
19:26 Evan G and Keita done
19:36 Fil to beer garden for RGA work
19:57 Marc, Liz to EX, then EY VCO work
20:18 Peter, Jason out
20:28 Dave to both ends
20:49 Kyle to EX
20:51 Corey to both mids
20:54 Hugh to LVEA
21:02 Chandra to MY
21:04 Dave out, Kiwamu out, Hugh out
21:17 KIwamu to LVEA OLTF of ISS
21:25 Jason, Peter to PSL, Sheila to PSL racks
22:07 Kiwamu, Kyle done
22:29 Fil, Ed done
22:40 Sheila, Ed to look at TCSX laser
22:48 Marc, Liz done
I added 500ml of water to TCSY chiller.
[Stuart A, Jeff K] While debugging and commissioning the LLO ITM LV ESD monitoring I noticed that there is an ADC channel discrepancy in the h1susauxb123 model (see below, just ITMX shown). It is noted that there is an unorthodox convention for the order of the LV ESD monitor channels (as given in D1500464), which is already taken account of in the library LVESD_STAGE_MONITOR_MASTER part (see below). However, in h1susauxb123, the ordering for the ESD quadrants assigned to ADC_7 mistakenly switch the order n.b. this occurs for both ITMX and ITMY LV ESD monitoring. Therefore, I've made the correction to the l1susauxb123 model (see below, just ITMX shown), and LLO shall rebuild, reinstall and restart the model at the next opportunity.
Ticket open in FRS: #6511.
The power supplies for the h1isce[x,y] timing slave cards were inadvertently glitched this morning during maintence when diagnostics equipement was being plugged in. We have labeled these power outlets to prevent future occurance. Models were restarted with no problems.
as part of the cleanup following the filling of /opt/rtcds on Sunday, this afternoon at 12:50 PDT I started a 'zpool scrub rtopt' file system cleanup on h1fs0. At the time of this alog the system is predicting the will complete in 8 hours (11pm PDT).
If anyone notices any slow down of EPICS data from front ends, please contact me.
Pumps will continue to run at X-end RGA for a few more days. Closed cal-gas isolation valves. Manually reducing variac's by ~10% every 2 hrs. today. Bake Summary: Approximately 90% of surface area soaked between 180C < temperature < 210C for 96 hrs.. Additional 72 hrs. manual incremental ramp up. ~10% surface area tapered down to ~90C at turbo inlet line-of-site during soak period. .
We recorded AI output of PCAL injection as well as PCAL_DAC_FILT thing together with witness GPS 1pps using Tektronics MSO4043 (1 sec with 1Msample per channel, and 2 sec with 1Msample per channel).
We also recorded the digital output of the PCAL injection as well as digital input of the PCAL_DAC_FILT thing.
Evan will look at the timing comparator data.
These will be analyzed in the near future for further timing sanity check.
Data is stored at /ligo/svncommon/CalSVN/aligocalibration/trunk/Runs/PreER10/H1/Measurements/timing. Analysis forthcoming...
Analysis complete. See LHO aLOG 30965.
TITLE: 10/25 Eve Shift: 23:00-07:00 UTC (16:00-00:00 PST), all times posted in UTC
STATE of H1: Lock Aquisition
INCOMING OPERATOR: Jeff
SHIFT SUMMARY: Locking DRMI/PRMI was not easy, it required large adjustments and waiting a good amount of time. useism is also getting pretty high so I tried the WINDY_USEISM state, brought it back to WINDY because I couldnt tell which was better. Aside form that the commissioners are working.
I should probably just remove or rename the WINDY_USEISM state. It may have a use, but I think people are taking the configuration guide on the SEI_CONF screen too literally. I'm reluctant to try to make the guide more accurate because I'm not a cubist. The WINDY_USEISM state should be thought of as a more wind resistant state than the high microseism configuration we used during O1 (USEISM in SEI_CONF). Anyone remember how hard locking was with 15mph winds and high microseism during our first observing run?
We are getting into new territory with the current configuration (implemented during the windy, low microseism summer), but looking at the locks last night, it looks like the WINDY configuration is still what we want to use. The five attached plots are the ISC_LOCK state, SEI_CONF state (40 is WINDY, 35 is WINDY_USEISM), the ETMX Z 30-100mhz STS BLRMS (in nm, so 1000=1 micron) and the corner station windspeed. The last plot shows all four channels together, red is the ISC state, blue the SEI_CONF state, green is the STS BLRMS, black is the wind. It's kind of a mess, but it gives a better feel for the time line.
Microseism was high over this entire period (around 1micron RMS), wind was variable, so this was a good time to test. I think the take away is that the WINDY state was sufficient to handle the high microseism for the 2 NLN locks over this stretch, and is very probably more robust against the wind than the WINDY_USEISM state.
This is great to know. I was pretty sure that you said WINDY is good for almost every situation, but I thought it worth a try.
Tagging OpsInfo so we can get the lastest