Adam Mullavey called and said he needed to run a measurement for today's maintenance. His measurement needed the PCAL X lines turned off, so he had me turn the amplitudes on those lines down to 0. Unfortunately, he ran into some permissions issues and couldn't do his measurement. LHO was out of OBSERVE from 14:21 to 14:34 for this, but as far as I know the only differences during that time were from turning off the pcal lines. Attached screen shot shows the settings we were running while observing. All the oscsin and osccos amplitudes were zero'd for the planned measurement. I've reverted them to the pictured settings now.
The end Y BRS is continuing it's slow drift and is getting close to going out of range, but should survive through the end of the run. It's possible, however, if it gets rung up by people working in the area, it could cause a problem for the damping loops and leave the BRS in an unusable state.
TITLE: 08/22 Eve Shift: 23:00-07:00 UTC (16:00-00:00 PST), all times posted in UTC
STATE of H1: Observing at 50Mpc
INCOMING OPERATOR: Jim
SHIFT SUMMARY: 39.5hr lock, many tours for the eclipse party. Quiet shift overall.
A. Urban, on behalf of the calibration group
The C00 vs. C01 comparison pages have been updated and include all C01 data from 2016-11-30 through 2017-08-01.
As part of this analysis, I've got updated PCAL-to-DARM ratio trends at 36.7, 331.9 and 1083.7 Hz (attached below).
Plots of both magntidue and phase residual timeseries trends are attached. These trends are computed by demodulating 300-second segments at each PCAL line frequency, then averaging to get a magnitude and phase out of each channel. In practice, I break up each 300-second segment into overlapping 100-second chunks, apply a Kaiser window, and then average over chunks to get a less noisy measurement. (It's basically Welch's method, except I'm demodulating rather than computing a PSD.) Finally, I remove most outliers that are due to locklosses and loud transient glitches. The same analysis was done on Livingston data; see L1 aLOG 35501.
In each plot below I show PCAL/strain trends for C00 (blue) and C01 (red) data. The trend shown in aquamarine applies a correction for f_cc to C01 data at the appropriate PCAL line frequency. Gray shaded regions correspond to times when we had a break in O2, once during the holiday season and once for commissioning work.
At mid and high frequencies, everything continues to be in order at the PCAL lines. You can see that in the bucket (331.9 Hz) all systematics are accounted for by f_cc and only very small (~1%) statistical fluctuations remain in C01. At high frequency (1083.7 Hz) there's a slight systematic offset at the level of 1% or so in magnitude and 1-2 degree in phase, which is consistent with Craig's error budget. However, in the C01 low frequency line there is a mounting phase offset prior to the May vent that becomes worse after the break: the offset is 2-3% in magnitude and about 2 degrees in phase from June all the way through August. I suspect this has to do with spring detuning in the signal recycling cavity, and will follow up on it soon.
J. Kissel I've processed the data from LHO aLOG 38232, in which I was looking to see if the complex, high frequency dynamics found in the UIM (L1) stage of H1 SUSETMY (see LHO aLOG 31603). Plots are attached; note that I've used the former 2016-11-17 data for ETMY. To guide the eye, I show the calibration group's dynamical model used during O2. Data shown with a coherence threshold of 0.75 or greater. I've not yet compared this against the unphysical, fitted update to the QUAD model that Brett developed for H1 SUS ETMY in CSWG aLOG 11197 It looks like - All suspensions see the "unknown" ~165 Hz resonance, though interestingly ITMY's mode appears to be split. ETMX and ITMY's are *strikingly* similar. - only ETMY and ITMX show what Norna suspects is the "UIM blade bending mode" at ~110 Hz. ETMY's is indeed the ugliest. - All but ETMX show evidence for resonances between 290 and 340 Hz, which are likely the (Suspension Point to Top Mass) wire violin mode fundamentals weakly excited by the UIM excitation. (see LHO aLOG 24917, T1300876) - All suspensions show their (UIM to PUM) wire violin mode fundamentals between 410 and 470 Hz (see LHO aLOG 24917, T1300876) - ETMY and ITMY's wire violin modes are *strikingly* similar; ITMX's modes are surprisingly low Q. - We don't see the TOP to UIM wire violin modes likely because I didn't excite up to high enough a frequency; they're between ~500-510 Hz for ETMY (modeled at 495 Hz). So now the question becomes -- what's the physical mechanism for this huge mystery resonance that's seen virtually identically in all QUADs? It seems quite a fundamental feature. Why is it split on ITMX? It would be nice to have similarly detailed measurement of L1's QUADs, but all evidence from calibration measurements on L1's ETMY UIM stage point to this same feature (see the discrepancy between model and measurement for the UIM stage, e.g. in 2016-11-25_L1_SUSETMY_L1_actuation_stages.pdf LHO aLOG 29899). Further, it's *still there* before and after their Bounce/Roll mode Dampers (BRDs) have been installed (i.e. the same feature is seen in O1 and O2 CAL measurements; the above linked measurement was after BRD install).
If anyone needs to fit this data to try out their FDIDENT skills, the data from the above concatenated transfer UIM to TST functions is attached, in the same format as before for ETMY. Analysis script lives here: /ligo/svncommon/CalSVN/aligocalibration/trunk/Runs/O2/H1/Scripts/FullIFOActuatorTFs/ process_H1SUSQUAD_L1_HFDynamicsTest_20170814.m
I'm attaching the l2l st2 gs13 measurements for ITMX that we used for closeout after install. The 160 hz feature doesn't seem to show up on the ISI. The 300 hz feature maybe does? I don't think it's very conclusive.
TITLE: 08/21 Eve Shift: 23:00-07:00 UTC (16:00-00:00 PST), all times posted in UTC
STATE of H1: Observing at 52Mpc
OUTGOING OPERATOR: Jeff
CURRENT ENVIRONMENT:
Wind: 7mph Gusts, 3mph 5min avg
Primary useism: 0.01 μm/s
Secondary useism: 0.10 μm/s
QUICK SUMMARY: 31.5hr lock, rode thorugh a few earthquakes, eclipse event tonight.
Committed the following modified files to SVN repository.
The minutes from the 12:00 weekly pre-maintenance meeting, usually held at 09:30. Planned Tuesday Maintenance items: (1). The window may extend past 12:00 due to TMDS Testing at End-X (2). Jeff K. needs IFO up for 15 to 20 minutes after 08:00 to run BSC ISI coupling measurements (3). Jeff K. Running charge measurements (4). Jason will be making the weekly PSL Diode current adjustment (5). Possible cleanroom moves (WP #7116) (6). Filiberto will hold off in dressing new cables into HAM6 rack until next week.
Nothing unusual to report.
Quiet first half of shift. Back to triple coincident observing after LLO recovered from this mornings earthquake. No problems or issues to report at this time.
TITLE: 08/21 Owl Shift: 07:00-15:00 UTC (00:00-08:00 PST), all times posted in UTC
STATE of H1: Observing at 53Mpc
INCOMING OPERATOR: Jeff
SHIFT SUMMARY: Quiet Shift
LOG:
Not much happened. Just rode out a good eq from Mexico, max ground blrms got to 1 micron, seismon predicted .6 microns. I didn't see if seismon actually gave advance notice or not.
FAMIS4535
All looks good.
TITLE: 08/20 Eve Shift: 23:00-07:00 UTC (16:00-00:00 PST), all times posted in UTC
STATE of H1: Observing at 52Mpc
OUTGOING OPERATOR: Corey
CURRENT ENVIRONMENT:
Wind: 1mph Gusts, 0mph 5min avg
Primary useism: 0.01 μm/s
Secondary useism: 0.08 μm/s
QUICK SUMMARY: 7.5hr lock, all is calm.
TITLE: 08/20 Day Shift: 15:00-23:00 UTC (08:00-16:00 PST), all times posted in UTC
STATE of H1: Observing at 53Mpc
INCOMING OPERATOR: TJ
SHIFT SUMMARY:
Kenai & Stefan Balmer were my helpers earlier in the shift.
Virgo has a segment which is running over 60hrs long!
LOG:
Notables: ISS saturation about 6hrs ago & PMC Refl is high.
Laser Status:
SysStat is good
Front End Power is 33.89W (should be around 30 W)
HPO Output Power is 154.7W
Front End Watch is GREEN
HPO Watch is GREEN
PMC:
It has been locked 5 days, 4 hr 12 minutes (should be days/weeks)
Reflected power = 17.05Watts
Transmitted power = 56.95Watts
PowerSum = 74.0Watts.
FSS:
It has been locked for 0 days 5 hr and 56 min (should be days/weeks)
TPD[V] = 1.43V (min 0.9V)
ISS:
The diffracted power is around 3.3% (should be 3-5%)
Last saturation event was 0 days 5 hours and 54 minutes ago (should be days/weeks)
Possible Issues:
PMC reflected power is high
All is quiet here other than the lockloss this morning. I had Kenai & Stefan here to fill in as operators when I made breakfast. Currently in 3.5+hr Triple-C segment.
TITLE: 08/20 Day Shift: 15:00-23:00 UTC (08:00-16:00 PST), all times posted in UTC
STATE of H1: Lock Acquisition
OUTGOING OPERATOR: Jim
CURRENT ENVIRONMENT:
Wind: 7mph Gusts, 4mph 5min avg
Primary useism: 0.01 μm/s
Secondary useism: 0.09 μm/s
QUICK SUMMARY:
As Jim and I were chatting before he left, H1 broke lock! (No obvious seismic reasons or anything else seen for a cause). Currently taking back up.
Notes On Relocking So Far:
It's been a couple of weeks since I've locked.
The PRMI cavity looked dead at first, so I went to CHECK MICH FRINGES, & it still looked like it was in the doldrums, but managed to see that it needed some BS YAW---miraculously PRMI then locked on the quick.
As TJ noted, AS90 is different (for the PRMI locking steps, it is up around 2000 counts [just barely visible on StripTool], so I ignored that channel). The PRMI/DRMI transition looked odd/slow motion during the transition, but made the switch without breaking lock.
Other than that, had no issue with getting back to OBSERVING.