Ran a broad band and simulines meaurement starting at 1531UTC.
Simulines start:
PDT: 2024-05-30 08:37:11.822463 PDT
UTC: 2024-05-30 15:37:11.822463 UTC
GPS: 1401118649.822463
End:
2024-05-30 15:58:42,508 | INFO | File written out to: /ligo/groups/cal/H1/measurements/DARMOLG_
SS/DARMOLG_SS_20240530T153713Z.hdf5
2024-05-30 15:58:42,515 | INFO | File written out to: /ligo/groups/cal/H1/measurements/PCALY2DA
RM_SS/PCALY2DARM_SS_20240530T153713Z.hdf5
2024-05-30 15:58:42,520 | INFO | File written out to: /ligo/groups/cal/H1/measurements/SUSETMX_
L1_SS/SUSETMX_L1_SS_20240530T153713Z.hdf5
2024-05-30 15:58:42,524 | INFO | File written out to: /ligo/groups/cal/H1/measurements/SUSETMX_
L2_SS/SUSETMX_L2_SS_20240530T153713Z.hdf5
2024-05-30 15:58:42,529 | INFO | File written out to: /ligo/groups/cal/H1/measurements/SUSETMX_
L3_SS/SUSETMX_L3_SS_20240530T153713Z.hdf5
ICE default IO error handler doing an exit(), pid = 1172966, errno = 32
PDT: 2024-05-30 08:58:42.575781 PDT
UTC: 2024-05-30 15:58:42.575781 UTC
GPS: 1401119940.575781
TITLE: 05/30 Day Shift: 1430-2330 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Observing at 151Mpc
OUTGOING OPERATOR: Ryan S
CURRENT ENVIRONMENT:
SEI_ENV state: CALM
Wind: 4mph Gusts, 2mph 5min avg
Primary useism: 0.01 μm/s
Secondary useism: 0.07 μm/s
QUICK SUMMARY: Locked for 13 hours, range around 150+. Planned calibration and commissioning today from 830-1200PT.
As Ibrahim noted in his alog yesterday the LVEA and PSL dust monitors arent responding sicne Tuesday and need a power cycle at minimum.
I restarted the LVEA Dust server code, but still no communication with the LVEA MetOne monitors. The ethernet/serial converter h1seriall0 does respond, so it looks like an RS485 issue as TJ said. The dust monitors went offline 11:05 Tue Morning PDT.
TITLE: 05/29 Eve Shift: 2300-0800 UTC (1600-0100 PST), all times posted in UTC
STATE of H1: Observing at 148Mpc
INCOMING OPERATOR: Ryan S
SHIFT SUMMARY:
Decent shift with more Observing time compared to last night's shift. Notables for locking was the continue locklosses for FIND IR (even after an alignment). Pausing seemed to help. There was also a superevent as well (102nd of O4).
LOG:
Decent night even with winds and a lockloss. (H1 had issues getting past FIND IR.) Also managed a super event at the very beginning of this current 2+hr lock.
Jennie W, Sheila
Summary: We need to rerun this test with slightly different starting QPD offsets and a different amplitude to get a meaningful measurement of how the optical gain would be affected by changing the OMC alignment.
I started an injection into the OMC ASC loops (which feed back to the OMC and the OM3 pitch and yaw to keep the beams centred to specific offsets on OMC QPD A and B.
With this we can raster the OMC alignment and find which QPD offsets allow us to maximise optical gain.
The injection started at about 20:30 UTC while no squeezing was injected.
I used this template at /ligo/home/jennifer.wright/Documents/OMC_Alignment/20240419_OMC_Alignment_EXC.xml with amplitudes of 3 counts in all four degrees of freedom.
Within one cycle the OMC suspension saturated.
Why did we saturate with an injection amplitude of 3 as this ran the last time we did this test without any saturations?
Decreased amplitude to 1 to run it without saturating the OMC suspension.
Restarted at 20:39:07 UTC roughly.
Stopped injecting after 21:06:00 UTC.
Results inconclusive as changing the QPD in offset does not seem to change the noise injected around the calibration line between 410 to 411 Hz, so maybe we need to have higher injection amplitudes but start raster from different QPD offset set points so we don't staurate the suspension.
Looking at ndscope of the channels when they saturated.
OMC T2 and T3 saturated (this is an18 bit DAC). This is OMC pitch degree of freedom, which corresponds to Y direction in the OMC ASC loop basis.
Looking at the top left plot the POS Y DOF seems to correspond to the time of saturation and is the highest Y channel so we want to put in a +0.5 offset to this before the next time we run this raster to bring the input to the POS Y loop down in magnitude.
I forgot to post the the results from yesterday.
As can be seen from the spectrogram while we were doing the OMC alignment scan, there were a lot of glitches during this period which may limit us in using the BLRMS as a measurement of optical gain as some of these glitches were at both BLRMS frequencies we look at - ie. 410 - 411, 800 - 900 Hz.
Looking at zoomed in time series of GDS calib strain and OMC DCPD these glitches can also be seen.
The plot of OMC DCPD BLRMS at the calibration line frequency against QPD offsets seems to show they are quite flat in frequency and so we can't get any gain from adjusting the QPD offsets at this alignment into the OFI.
TITLE: 05/29 Day Shift: 1430-2330 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Observing at 145Mpc
INCOMING OPERATOR: Corey
SHIFT SUMMARY:
IFO is in NLN since 17:45 UTC
IFO States for the day has been:
14:25 UTC: OBSERVING
14:45 UTC: Lockloss - after initial alignment, we went into planned comissioning from 16:00 UTC to 19:00 UTC. IFO stayed in down during this time for comissioning tasks. After these, we began to lock again.
17:45 UTC: Reached NLN and went into COMISSIONING
19:11 UTC: OBSERVING after comissioning tasks wrapped up
20:30 UTC: COMMISSIONING impromptu comissioning time coinciding with LLO since neither site had a fully locked IFO during the original alotted time. An hour of comissioning time was agreed upon.
21:34 UTC: OBSERVING
23:30 UTC: Shift End - OBSERVING
LOG:
Start Time | System | Name | Location | Lazer_Haz | Task | Time End |
---|---|---|---|---|---|---|
15:53 | SYS | Jeff | LVEA | N | Grabbing 786 by HAM6 | 16:02 |
16:02 | FAC | Karen | MY | N | Technical Cleaning | 16:02 |
16:03 | FAC | Kim | MX | N | Technical Cleaning | 16:51 |
18:22 | SAF | Ryan | LVEA | Y | Transition to laser hazard | 18:38 |
18:23 | PEM | Robert | LVEA | Y | Stray beam force measurements | 19:11 |
19:13 | SAF | LVEA | IS | LASER | HAZARD | 05:53 |
20:41 | PEM | Robert | LVEA | Y | Stray beam force measurements | 21:28 |
21:04 | TCS | Camilla | Opt Lab | Local | CO2 laser testing | 23:04 |
21:04 | SEI | Mitchell, Jim | MX | N | Looking at in-air cables | 21:40 |
23:09 | TCS | Camilla, Terry | Opt Lab | Local | CO2 Laser Testing | 02:10 |
TITLE: 05/29 Eve Shift: 2300-0800 UTC (1600-0100 PST), all times posted in UTC
STATE of H1: Observing at 148Mpc
OUTGOING OPERATOR: Ibrahim
CURRENT ENVIRONMENT:
SEI_ENV state: CALM
Wind: 18mph Gusts, 12mph 5min avg
Primary useism: 0.06 μm/s
Secondary useism: 0.09 μm/s
QUICK SUMMARY:
H1's been locked almost 5.5hrs and seem a little calmer than yesterday at this time, althought we've had some gusts approaching 30mph. No items to hand over from Ibrahim for locking tonight (other than possibly proactively run an Initial Alignment if there are ALS or DRMI/PRMI issues
FAMIS 26304, last checked in alog77997
Only notable change was yesterday, where the new fan bearing on CS fan 6 looks to have lowered the noise picked up by the vibrometer.
Sheila, Camilla
Checking SQZ:
Checking IFO:
Naoki, Sheila, Camilla
We tried this alignment and the middle, mainly changing pitch alignment. Both of these were considerable worse. We went back to yesterdays alignment, hand adjusted ZM4/6 in ASQZ then ran SCAN_SQZALIGN. Sdf's attached accepted.
Back to 4.5dB of SQZ above 1kHz and our reference 100-100Hz. SQZ seems to still be injecting low frequency noise.
Kappa_C is 0.5% better in this new SRC spot, plot attached.
Last night and today we are in a different spot through the OFI. See Sheila's alog 78096 for the move that was made.
Overall, SR2 and SRM yaw are much closer to center in this position, however SRM pitch is farther from center. I did a quick double check of the SRM pit, and indeed this is where it wants to be.
The previous spots (with the previous SR3 alignment) are recorded in alog 77443.
ampl [cts] of line at 31.0 Hz | A2L gain step size when minimizing | CAL-DELTAL line reduction factor | Final A2L gain | Inferred new spot position [mm] | Change from alog 77443 position | |
SR2 P2L | 1.0 | 0.1 | 100x | -1.0 | -2.0 | 13.1 mm other side of center |
SR2 Y2L | 1.0 | 0.1 | 100x | +0.3 | 0.6 | 9.7 mm other side of center |
SRM P2L | 2.0 | 0.1 | 50x | -5.5 | -11.1 | 4.3 mm farther from center |
SRM Y2L | 2.0 | 0.1 | 30x | +1.85 | 3.7 | 3.5 mm closer to center |
Attached are the saved SDF diffs for both Observe and Safe snap files.
Sheila and Keita have recently found and fixed sign convention errors. Please see alog 78393 for the corrected interpretation of A2L gains.
Sheila, Camilla. During this May 28th/29th SRC alignment, the OFI sees larger than usual temperature swings on locklosses and powerups. See plot attached. We saw similar larger OFI temperature swings on the re-locking attempts after our April 22nd optical gain drop before we changes alignments, shown in 78399 and second attached plot. Is the beam in this alignment hitting something in the OFI? Could be more likely the yaw alignment as that is common in both alignments with larger temperature swings.
FAMIS 25993, last checked in alog77948
No appreciable difference that I can see compared to last check.
Sheila added a new boost in DHARD to the guardian, and we relocked with it successfully, so I have accepted the SDF diff in Observe.
TITLE: 05/29 Day Shift: 1430-2330 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Observing at 142Mpc
OUTGOING OPERATOR: Ryan S
CURRENT ENVIRONMENT:
SEI_ENV state: CALM
Wind: 5mph Gusts, 4mph 5min avg
Primary useism: 0.01 μm/s
Secondary useism: 0.08 μm/s
QUICK SUMMARY:
IFO just lost lock 14:47 UTC and now relocking
Dust monitors also have a few warnings:
*H1:PEM-CS_DUST_LVEA6 WARNING: dust counts did not change, please investigate
*H1:PEM-CS_DUST_LVEA10 WARNING: dust counts did not change, please investigate
*H1:PEM-CS_DUST_PSL101 WARNING: dust counts did not change, please investigate
*H1:PEM-CS_DUST_PSL102 WARNING: dust counts did not change, please investigate
BLRMs through our locks last night attached. Low frequency noise changes, this doesn't seem related to the wind.
TITLE: 05/29 Eve Shift: 2300-0800 UTC (1600-0100 PST), all times posted in UTC
STATE of H1: Wind
INCOMING OPERATOR: Ryan S
SHIFT SUMMARY:
A bit of a wind storm at the beginning of the shift but luckily strongest winds only lasted about an hour and allowed for locking shortly thereafter. Had about 4-5hrs of observing during this shift (with another lockloss minutes before the end of the shift).
LOG:
LATE Squeezer Entry For Yesterday!
Yesterday for the lock at the beginning of the shift (NLN around 100utc after the winds), the Squeezer did not lock on its own and also needed to run the scan_alignment_fds + sqz_angle states; also Naoki tweaked ZM4 a little before H1 eventually went to Observing. Below are the SDF diffs screenshots which were accepted:
Andrei, Sheila
We've analyzed the time-traces of the effective range (H1:CDS-SENSMON_CAL_SNSW_EFFECTIVE_RANGE_MPC
) along with the alignment channels FC_WFC_A(B)
and AS_A(B)_RF42
(see attached figures). We found no observable dependance between those.
During the time period being investigated in this alog on May 27, LASSO flags H1:TCS-ITMX_CO2_ISS_CTRL2_OUT_DQ as strongly correlated with the range. This channel and other related channels have been flagged as highly correlated to the range in recent days, but this time period shows the strongest correlation.
Jumps in this TCS channel correlate with range jumps, as shown in the attached comparison of the TCS and range trends on May 27.
Tagging TCS
This TCSX ISS correlation is a bit odd since we aren't using the ISS and the AOM, I believe, is completely unplugged. That said, I looked at some of the channels in that system and there is some extra noise seen around the times Derek posted (see May 16th example). I wonder if this points to a larger grounding issue or some other electrical problem that is seen more broadly.
These range fluctuations that we think are related to the squeezer started (I think) on May 16th: 77869
The first time cursor in the attached screeshot shows that range drip which I thought was traffic related at the time. Looking at the long term trend of this CO2 ISS control signal, there is a chance in charachter at this time, with more drifts in the signal level since. The second screenshot shows that this channel had a large jump on May 17th around 20:04-22:33 UTC.
There is a DARM BLRMS that may be more useful for tracking this noise than just looking at range, H1:OAF-RANGE_RLP_3_OUTPUT. (third screenshot shows this also had a change point and drifts more since May 16th.)