TITLE: 04/13 Eve Shift: 23:00-07:00 UTC (16:00-00:00 PST), all times posted in UTC
STATE of H1: Commissioning
OUTGOING OPERATOR: Jeff
CURRENT ENVIRONMENT:
Wind: 26mph Gusts, 21mph 5min avg
Primary useism: 0.07 μm/s
Secondary useism: 0.14 μm/s
QUICK SUMMARY: Robert, Jenne, et al. doing some commissioning work in LVEA HAM 1 enclosure. LLO is finally back up and commissioners have been notified to wrap up their work. No issues regarding the IFO were handed off.
At the request of Rick and Sudarshan, the HIGH_FREQ_LINES Guardian node will start at 5751.3Hz and then decrease by 500hz every 24 hours after a lock loss. Currently the end is set to be at 1000hz, but it sounds like it will most likely be stopped manually before then.
Lower limit is now set to 2000Hz instead of 1000hz.
Committed the following files to the SVN repository /opt/rtcds/userapps/trunk/sus/h1/burtfiles/h1susprocpi_safe.snap /opt/rtcds/userapps/trunk/psl/h1/burtfiles/fss/h1pslfss_safe.snap /opt/rtcds/userapps/trunk/sus/h1/burtfiles/h1susitmy_observe.snap /opt/rtcds/userapps/trunk/sus/h1/burtfiles/h1susitmx_observe.snap /opt/rtcds/userapps/trunk/sus/h1/burtfiles/h1susprocpi_safe.snap /opt/rtcds/userapps/trunk/psl/h1/burtfiles/fss/h1pslfss_safe.snap /opt/rtcds/userapps/trunk/cal/h1/burtfiles/h1calcs_OBSERVE.snap
The attached image shows the condensate that has accumulated in our VBOD Main Turbo's exhaust after several years and many bake loads. This is a maglev turbo that has only been backed by scroll pumps and that has only pumped Class-A prepped parts.
Dropping the intent bit to commissioning so Robert can work on the list below. I just spoke with LLO and they are still working their issues. Will keep in contact with LLO Ops on status. Commissioning Activities: 1). Shake input arm below 8 Hz 2). Bang on HAM6 to make sure dust doesn’t produce blip glitches 3). Look into mitigating scattering on ISCT1 so we can use POP AIR
Optical lever trends: ITMY SUM has dropped from around 40K to less than 20K.
Commissioning and relocking this morning, while LLO is down. Environmental has been troubling, with high and gusty winds and a couple of small earthquakes. The primary microseism is elevated with the wind. Ran A2L repair script due to YAW coherence up to 0.9. After clearing SDF Diffs for PSL-FSS_COMMON_GAIN and IMC-REFL_SERVO_IN1GAIN went back to Observing while commissioners are resetting for the afternoon.
Everything looks fine here.
If you happen to be on one of the Debian machines, I've been working on the Python scripts for this task. They can be launched from the bottom two buttons (BSC CPS Python & HAM CPS Python) on the OPS>>WEEKLIES screen. They now plot properly calibrated spectra for the CPS with sensor noise specs and save images of the spectra directly to your Desktop folder. The script also looks at the high frequency ASD average (over 80-120 hz) and will say on the xterm window which sensors (if any) are "out of spec". Sadly, these scripts won't work on the Ubuntu machines, because their scipy.signal libraries are too old and don't include welch. Maybe if operators find this workflow easier (push 2 buttons, look at plots, check xterm, and attach images to alog, done) we can convince Hugh to change the FAMIS task.
Per Keita: Spoke with Brian O’Rielly. LLO will be down for an unknown period. LLO ops will contact LHO ops when they are about an hour from relocking. Robert will be doing commissioning work until 13:00. The intent bit has been changed to Commissioning.
These are the commissioning tasks Robert will be working on: 1) Look into mitigating scattering on ISCT1 so we can use POP AIR 2) Bang on HAM6 to make sure dust doesn’t produce blip glitches 3) Put heat source under beam path on PSL to test jitter from air path 4) Shake input arm below 8 Hz 5) Probably for a later date: laser vibrometer on swiss cheese baffle
Hard to tell glitches from optical manipulation to lockloss spikes with these plots. HAM2 (not used) plots are the only ones that seem off spec. Currently OpLev damping is turned off IFO wide except for BS damping only during acquisition.
All looks well. Powers tracking humidity. Odd, little (very marginal)bump in chiller plots. I don't think this is any cause for concern.
Over the past few days and for the foreseeable future I'm running a python script which looks for ADC,TIM,IPC glitches on the end station computers. It scans roughly once a second (not synced to GPS but rather runs a loop and then waits one second). For all models running on the machines h1suse[x,y], h1seie[x,y] and h1isce[x,y] it reports any STATE_WORD which have non-zero values after the upper bits have been masked. For any model with an IPC error, it scans each IPC receiver channel and reports any non-zero error counts (plus IPC type and name of sender). Any latched errors are subsequently cleared by the once-a-minute issuing of a DIAG_RESET by a cronjob (actually happens at about 3 seconds in the minute).
Once I've accumulated some statistics, I'll post a report.
Work Permit | Date | Description | alog/status |
6573.html | 04/11/17 01:37 PM | Move the high frequency lines to 5501.3 Hz and 6001.3 Hz | 35479 |
6572.html | 04/11/17 12:41 PM | Install SRC detuning time dependent tracking. Includes update to CAL-CS front-end model, GDS gst-lal calibration pipeline code, updates to the science frame channel list which need to be included in all down stream channel lists so that the GDS pipeline can use those channels. Requires DAQ restart, and modification to separate DMT Frame Broadcaster channel list. Corresponds to gstlal release 1.1.5. | 35462, 35474, 35478 |
6571.html | 04/11/17 10:16 AM | Duplicate of WP 6570 | |
6570.html | 04/11/17 10:16 AM | Add back in two PEM general ADC channels to the DAQ frame. Both will be 4kHz. DAQ restart required. | |
6569.html | 04/10/17 04:44 PM | Unlock MC to reduce ifo. light at End Stations, block OptLev beam, switch off ALS beam, energize illuminator, capture ETM photos for Pcal beam localization investigations. | |
6568.html | 04/10/17 02:35 PM | Reduce the cell phone texter alarm level for all LN2 Dewars from 20% to 15%. FRS7835 | |
6567.html | 04/10/17 01:39 PM | 1. Update DMT calibration code to gstlal-calibration-1.1.5-v1: i. Bug fix for time immediately before and after data dropouts. CALIB_STATE_VECTOR now marks this time as bad. For a description of the problem, see https://alog.ligo-la.caltech.edu/aLOG/index.php?callRep=32486 ii. New algorithm to compute SRC detuning parameters. These are written to the channels GDS-CALIB_F_S and GDS-CALIB_SRC_Q_INVERSE, but no corrections to them are applied to h(t). The calibration group wishes to further develop this so that corrections are applied to h(t), perhaps for O3. (Will turn this on only when new filters are ready.) iii. Addition of option --cancel-callines to remove calibration lines. This is a command line option, meaning we may choose not to use it yet. If used, GDS-CALIB_STRAIN is unaffected. Rather, an additional channel, GDS-CALIB_STRAIN_CLEAN, is written out, which has the calibration lines removed. 2. Run "yum update" to install all patches and updates on all 3 DMT boxes, h1dmt0, 1, and reboot. This is to install updated ROOT library packages and get latest OS patches to bring DMT boxes up-to-date. | 35471, 35472, 35478 |
6566.html | 04/10/17 10:31 AM | Spin up turbo pump attached to OMC vacuum tube in LVEA; run Kobelco dry purge air compressor system and QDP80 rouging pumps in mech. room. The purpose of this task it to test equipment needed for vertex vent. | 35465 |
6565.html | 04/10/17 09:57 AM | Swap the ITMy oplev laser for a new one. K. Venkateswara noted in LHO alog 35341 that the ITMy oplev had a feature at ~0.44Hz that appeared immediately after the March 7th laser swap and seemed to be causing range drop issues with H1. It is hoped a new laser will remove this feature. No viewports will be exposed during this work. | 35470 |
6564.html | 04/07/17 10:09 AM | Return ETMX PCIe card to ETMX HWS computer. | 35469 |
6563.html | 04/06/17 09:42 AM | Measure L2A TFs for MC2, Install L2A filters. | 35464 |
6562.html | 04/06/17 09:07 AM | Determine the left-right relation in the Hartman wave front sensor (HWS) image by intentionally tilting the ITMX mirror by several micro radians. This measurement will not let the interferometer stay locked. | 35364 |
6561.html | 04/06/17 08:23 AM | Regular bi-weekly calibration sweeps. Will be done during commissioning period between 9a - 1p. | 35361 |
Previous W.P. | |||
6541.html | 03/27/17 08:40 AM | Perform scheduled maintenance to scroll compressors at Y-MID vent/purge-air supply skid. Maintenance activity will require for the compressors to run for brief periods of time to check compression. Lock-out/tag-out power to skid as required. | 35149, 35480 |
TITLE: 04/13 Owl Shift: 07:00-15:00 UTC (00:00-08:00 PST), all times posted in UTC
STATE of H1: Observing at 59Mpc
INCOMING OPERATOR: Jeff
SHIFT SUMMARY: Been locked for 17 hours. Wind seems to be picking up.
LOG:
Beam position based on exciting the pitch(yaw) DOF and then changing P2L(Y2L) gain to minimize the peak. Both measurements use a sign convention that is consistent with UR coil values. The Dec 2013 alpha numbers are as posted, however the beam distance numbers have been recalculated. In Dec 2013 the conversion from alpha to mm was 37.5mm/alpha, and the current conversion is 42.2mm/alpha.
13 Dec 2013 | 21 Mar 2017 | change | |||
alpha | beam distance from center, mm | alpha | beam distance from center, mm | mm | |
MC1 pitch | -0.043 | +1.81 | -0.057 | +2.42 | +0.6 |
MC1 yaw | +0.029 | +1.22 | +0.089 | +3.76 | +2.5 |
MC2 pitch | -0.062 | +2.62 | -0.183 | +7.72 | +5.1 |
MC2 yaw | -0.048 | -2.03 | -0.020 | -0.084 | +1.2 |
MC3 pitch | +0.041 | -1.73 | -0.051 | +2.15 | +3.9 |
MC3 yaw | -0.052 | -2.19 | -0.135 | -5.70 | -3.5 |
The animation that's attached shows the ideal IMC alignment in a dashed magenta line, the Dec 2013 alignment in red, and the Mar 2017 alignment in blue. Green markers show the optics, squares are MC1, triangles are MC2, and circles are MC3.
The lines and markers accurately represent the optics and the beam changes, but are not to scale. I altered some numbers to make the changes visible in this animation.
13 Dec 2013 | 21 Mar 2017 | change | |||
alpha | beam distance from center, mm | alpha | beam distance from center, mm | mm | |
MC2 yaw | -0.048 | -2.03 | -0.020 |
-0.84 |
+1.2 |
23:18 Jenne, Heather, Robert, and Vaishali out of the LVEA
23:19 Back to Observing