Jenne D, Jennie W
Jenne noticed that our AS_A_YAW offset was on in the current state (PREP_FOR_LOCKING). We don't want this offset on currently as we are moving to a different spot on the OFI for which we need the picomotors, therefore we my need to rethink AS_A and B alignment offsets.
We turned this offset and the other AS_A and AS_B oiffsets off.
This is the only one I could find set in the ISC_LOCK guardian so I commented this line out.
elif self.counter==9 and self.timer['LoopShapeRamp']:
#ezca['ASC-AS_A_DC_YAW_OFFSET'] = -0.15 J Wright commented this out on 6th June 2024.
ezca.switch('ASC-AS_A_DC_YAW', 'OFFSET', 'ON')
I reloaded the ISC_LOCK guardian.
Thu Jun 06 10:09:03 2024 INFO: Fill completed in 9min 0secs
Gerardo confirmed a good fill curbside.
P. Baxi , J. Kissel
Finished characterizing (Channels 1 to 4) of the new 524KHz Analog OMC Anti-Alias Chassis - S2300162
BodePlot_Channel_1_4_freq_start_102.4KHz_Freq_stop_1KHz_Steps_100.pdf (raw data - available in DCC S2300162)
- We see the frequency response has minimal phase impact in the gravitational wave band, with deg of phase loss at 1000 Hz.
ASD_SR785_Channel_1_4_Freq_span_4to32K_32to256K_128to1024K.pdf (raw data - available in DCC S2300162)
- We see the noise of each of these 4 representative ADC channels is around ~20 nV/rtHz
Bode plot and ASD plots) Bode plot and ASD plots)
For the bode: We see the frequency response has minimal phase impact in the gravitational wave band, with 1.5 deg of phase loss at 1000 Hz.
TITLE: 06/06 Day Shift: 1430-2330 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Lock Acquisition
OUTGOING OPERATOR: TJ
CURRENT ENVIRONMENT:
SEI_ENV state: CALM
Wind: 5mph Gusts, 4mph 5min avg
Primary useism: 0.02 μm/s
Secondary useism: 0.26 μm/s
QUICK SUMMARY: H1 has been unlocked since 10:21 UTC this morning. It's been able to relock up to PREP_DC_READOUT_TRANSITION, but the OMC is not locked; OMC_LOCK is stuck in the SET_WHITENING state with a notification reading "DCPD gains not equal after whitening switch -- yikes!" (I've not seen this before; will start troubleshooting)
Looking into why the OMC couldn't lock this morning, it seems to me like the sequence of events went as follows (all times in UTC):
H1 sat in this position for several hours (owl operator wasn't notified, separate issue) until Sheila manually set the DCPD gains to what they should be (1), then the OMC was able to lock without issue and the IFO followed suit.
I believe this interaction happened because now that the DARM_OFFSET state has been moved to after all the ASC states, the OMC doesn't have as long to lock before we reach PREP_DC_READOUT_TRANSITION, and the OMC_LOCK DOWN state request happened in a bad spot. If we want to keep DARM_OFFSET where it is, we might want to change ISC_LOCK to give OMC_LOCK more time to lock the OMC before having it try again.
Ibrahim, Ryan S, Jenne, Sheila, TJ
TITLE: 06/06 Eve Shift: 2300-0800 UTC (1600-0100 PST), all times posted in UTC
STATE of H1: Observing at 146Mpc
INCOMING OPERATOR: TJ
SHIFT SUMMARY:
IFO is in NLN and OBSERVING (after a 24 hour outage) as of 07:59 UTC (cutting it real close H1...)
For the majority of the shift, I was unable to lock - here’s why:
On top of these, we have also had a few totally spontaneous lock losses which do not have tracks as egregious as the three above. Moreover, running INITIAL_ALIGNMENT seems to randomize what issue I face in that I either will be acquainted with a totally new problem or face no problems.
SDF Diffs Attached (All Seismic Related)
LOG:
None
IFO is still LOCKING (I know)
While violins were damping to turn on whitening (pretty steadily too), we lost lock unexpectedly. DRMI could not lock - PRMI could not lock and MICH Fringes could not lock PRMI. So now I'm doing an initial alignment.
Attaching a set of slides summarizing the on-going efforts to reproduce the beam path from SR3 through the OFI. Two sets of the beam spot position measurement on SR2 and SR3 were used to "calibrate" the slider moves and to simulate the beam position for other alignment configurations using Zemax. The slides are posted to the dcc https://dcc.ligo.org/E2400189-x0 The aLogs with the beam spot position measurements: beam spot 1 measurement aLog77443 beam spot 2 measurement aLog78119
[Jenne, Sheila, Jennie, RyanS, Ibrahim]
The interferometer has remained fussy all day. I suspect we may have some alignment issue somewhere, since the AS_AIR camera looks a little bit lobe-y and wrong in yaw. Twice now, if we've gotten past the DARM_OFFSET state and convinced the OMC to lock (which it will do with the autolocker once the darm offset is at the full value of 9e-5), we're able to at least start powering up.
My hypothesis of why we might be needing this alignment offset, is that increasing the DARM offset is letting more carrier light go to the AS port, and the the AS WFS loops are seeing that and responding poorly. So, this alignment offset helps kepe them in the right spot. That's not a very satisfying story though.
Earlier, I had tried moving SR3 by +/- 1urad on the slider in yaw (reverting afterward to the previous slider val), but that didn't really help. I also tried offsets in AS_C and AS_A pointing, but neither of those had the same improvement in the AS camera or POP90. They would improve momentarily, but after the rest of the ASC caught up, we still had the lobe-y look on the AS camera.
Jennie also noted earlier (and it happened at least both of these last two power ups) that we're saturating the OMC suspension when we power up (before moving spots). But, after all the ASCs catch up, it's no longer saturated. So, we're close to the edge of what the OMC suspension can do, but it seems surviveable.
Attached are screenshots at CHECK_DRMI_ASC of the AS air camera, without and then with my hokey offset of 0.6 in SRC1 yaw. You can see that with the offset in place, the camera image is much more centered and nice looking.
For posterity, here are the mattermost versions of the notes, starting with this message:
There may be some additional low frequency noise, which could be due to whatever is causing our alignment woes. At this point, I'm going to let Ibrahim bring down the violin modes and put us in Observing, and hopefully we'll be able to address this tomorrow during commissioning.
TITLE: 06/05 Day Shift: 1430-2330 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Lock Acquisition
INCOMING OPERATOR: Ibrahim
SHIFT SUMMARY: It's been a busy shift of troubleshooting. See alogs 78251, 78258, and 78259 for summaries of the first half of the day's events. Since then, we had trouble locking DRMI where buildups looked very unstable and there were several locklosses at different places in the DRMI acquisition steps. Eventually DRMI was able to lock (Jim reverted some sensor correction-like changes he put in Monday, but unsure if this had any effect) and we made it up to engaging ASC. Sheila had moved the DARM_OFFSET state to between the ENGAGE_ASC and SOFT_LOOPS states, but we found that increasing the DARM offset again caused the PRG to drop as we had been seeing in the morning. I wasn't fast enough to lower the DARM offset, so we lost lock. On the next attempt, we ran through both ENGAGE_ASC and SOFT_LOOPS before running DARM_OFFSET, but we still saw the drop in PRG as before. I was able to turn off the DARM offset in time, then Jenne started to step it up slowly to see where things became unstable. When she reaced the nominal value of 9e-5, things still looked okay and the OMC was able to lock, so we proceeded to DC readout and powered up to 25W. At this point, Robert went into the LVEA to take pictures through a HAM2 viewport, and sometime around then, we lost lock (unsure exactly if he was the cause). We've since relocked and continue to troubleshoot why we canot turn on the DARM offset reliably.
Handing off to Ibrahim as troubleshooting is ongoing.
LOG:
| Start Time | System | Name | Location | Lazer_Haz | Task | Time End |
|---|---|---|---|---|---|---|
| 21:03 | SAF | HAZARD | LVEA | YES | LVEA is Laser HAZARD | Ongoing |
| 15:31 | FAC | Karen | Opt Lab | N | Technical cleaning | 15:56 |
| 16:24 | SQZ | Terry | Opt Lab | Local | SHG work | 18:55 |
| 19:48 | SQZ | Terry | Opt Lab | Local | SHG work | 23:47 |
| 20:09 | FAC | Mitchell | EY | N | Checking wind fence | 20:41 |
| 20:44 | VAC | Gerardo, Jordan | LVEA | - | Checking ion pump | 20:52 |
| 21:59 | CAL | Francisco | PCal Lab | N | Measurements | 23:59 |
Andrei, Sheila, Naoki
We've observed that the reduction of the observable range is accompanied by the presence of "whistles", high-magnitude frequency-modulated signals in the spectrum in SQZ FC WFC.
Sheila created several plot overlays to demonstrate this dependence. Specifically, we selected the Lock : Range : DMT-SNSL_EFFECTIVE_RANGE_MPC and SQZ : Subsystems : SQZ FC WFC plots and overlaid them to highlight the relation between them.
DARM_comparison.png plot contains the 18th of May 2024 DARM during the “whistle” and during its absence. ≈0.5 dB difference is observed.
TITLE: 06/05 Eve Shift: 2300-0800 UTC (1600-0100 PST), all times posted in UTC
STATE of H1: Lock Acquisition
OUTGOING OPERATOR: Ryan S
CURRENT ENVIRONMENT:
SEI_ENV state: CALM
Wind: 13mph Gusts, 11mph 5min avg
Primary useism: 0.04 μm/s
Secondary useism: 0.38 μm/s
QUICK SUMMARY:
IFO is LOCKING at DARM_OFFSET
We're experiencing issues with the Power Recycling Gain. Jenne, Sheila and Ryan S are troubleshooting it currently. This is preventing us from locking.
Naoki, Sheila
To estimate the FC backscatter noise, we excited the FC IR error signal. The attached figure shows the FC IR error signal and DARM with (red)/without (blue) exciation. Although the FC IR error signal is excited by a factor of more than 30 between 10-100 Hz, the excess noise in DARM is small so the FC backscatter noise should be much smaller than DARM.
Jennie W, Jenne D, Sheila
The other day I designed a new notch to get rid of a bump we had been seeing at 17.75Hz. We think this is the bounce mode of the BS coupling into the MICH loop. The notch for this in LSC-MICH has not been updated since the BRDs were installed I think, and there is no notch for this mode in the ASC-MICH_P and ASC_MICH_Y loops.
Changes made to ISC_DRMI.py
Added Bounce-roll notch (FM8) to MICH2 (line 457) in DRMI_LOCKED state and took out line turning on notch at 15Hz (line 456).
#ezca.get_LIGOFilter('LSC-MICH2').switch_on('FM10') # Turn on the BounceRoll FM10 in LSC FM
ezca.get_LIGOFilter('LSC-MICH2').switch_on('FM8') # Turn on the BounceRoll FM8 in LSC FM 05/06/2024 J Wright
Added bounce-roll notch to PREP_PRMI_ASC in FM MICH_P and MICH_Y in FM9. These were added to lines 690 and 692.
zca.get_LIGOFilter('ASC-MICH_P').only_on('INPUT','FM3','FM9','FM10','OUTPUT', 'DECIMATION') #SED increased gain by 20db (removing FM1) Oct 28 2019. added in BR for damped mode at 17Hz 05/06/2024 J Wrightezca.get_LIGOFilter('ASC-MICH_Y').only_on('INPUT','FM3','FM4','FM7','FM9','FM10','OUTPUT', 'DECIMATION')#change LP from LP6 to ELP15 SED DDB March 17 2019, added in BR for damped mode at 17Hz 05/06/2024 J WrightAdded these same filters in PREP_DRMI_ASC state in FM MICH_P and MICH_Y in FM9 in lines 920 and 922.
ezca.get_LIGOFilter('ASC-MICH_P').only_on('INPUT', 'FM1','FM3','FM9','FM10','OUTPUT', 'DECIMATION')# added in tuned BR for 17Hz mode J Wright 05/06/2024.ezca.get_LIGOFilter('ASC-MICH_Y').only_on('INPUT', 'FM1','FM3','FM4','FM7','FM9','FM10','OUTPUT', 'DECIMATION')#change LP from LP6 to ELP15 SED DDB March 17 2019, added in tuned BR for 17Hz mode J Wright 05/06/2024.Just undid these changes in case they prevent us locking DRMI as we keep falling put from ENGAGE DRMI ASC in ISC_LOCK guardian.
I turned these filters on when we got to NLN at the start of today's commissioning period. Since they didn't unlock us and seem to possibly make the noise at 17.7Hz better in DARM I have put them back in ISC_DRMI as detailed above and reloaded it. I will post a high resolution spectra next time we get a good lock stetch.
After much time diagnosing locking issues this morning (see alogs 78251 and 78258 for the main events), we eventually reached NLN after damping violin modes in OMC_WHITENING for 40 minutes. Almost two minutes after reaching NLN, Robert attempted to ramp the bias on ITMY, but accidentally changed it immediately, which unlocked the IFO at 19:38 UTC.
H1 is currently relocking. We're scheduled for commissioning time until 22:00 UTC, so if we can get back to low noise, we'll spend time commissioning until then.
Wind was brutal today, so I was messing with the controls on the BSCs to try to help. Mostly just running RX/RY sensor correction from St1 to St2 on the BSCs. Sensor correction is focused on improving the ~.4hz motion and doesn't really affect the motion outside that. I don't think this really helped, winds calmed down after I left at 5:30 and Ryan is almost all the way NLN now, so I will leave the extra sensor correction running for tonight. I'll accept SDFs for tonight, then turn it back of during maintenance tomorrow.
Wind and lock losses make a comparison challenging, but the blrms trends show the (log scale) improvement ETMY sees when it's turned on over .3-1hz. Top trace is the St2 RX GS13 blrms, middle trace is the gain for the sensor correction, sc is on when it's 1, off at 0. Bottom trace are the .3-1hz ground blrms. For the las 3-ish hours the St2 RX motion is lower with the sensor correction on even when the ground is moving more in this frequency band.
These changes were reverted today, in case they were causing issues with locking. ASC was engaged at the time, I didn't see any effect turning this stuff off, so I think they were probably benign.
With the difficulties locking, I tried changing some of the CPS diff filters to get the end station ISI to follow the corner ISI. The CPS diff uses a band pass filter to reduce the differential motion between the ISI, but this filter can inject motion at the microseism. Microseism is low, I'm guessing the arms are struggling more with the below .1hz motion. In the attached image the filters we had been using, are the red trace, blue is what I switched to. It kind of seemed to help, but I think we lost lock after I left the room. I'll leave this running for now, going to try a couple other things.
These changes were reverted today, in case they were causing issues with locking. ASC was engaged at the time, I didn't see any effect reverting to the old configuration, so I think they were probably benign.
LLO noted a 10 Hz comb that was attributed to the IRIG B monitor channel at the end station connected to the PEM chassis. (https://alog.ligo-la.caltech.edu/aLOG/index.php?callRep=71217)
LHO has agreed to remove this signal for a week to see how it impacts our DARM signal.
EX and EY cables have been disconnected.
Disconnection times
| EX | GPS 1400946722 | 15:51:44 Tue 28 May 2024 UTC |
| EY | GPS 1400947702 | 16:08:04 Tue 28 May 2024 UTC |
I checked H1:CAL-PCALX_IRIGB_DQ at gps=1400946722 and H1:CAL-PCALY_IRIGB_DQ at gps=1400947702. From 10 seconds prior to the cable disconnection to 1 sec before the cable disconnection, IRIG-B code in these channels agreed with the time stamp after taking into account the leap second offset (18 sec currently).
Note that the offset is there because the IRIG-B output from the CNS-II witness GPS clock ignores leap seconds.
I fixed things in https://svn.ligo.caltech.edu/svn/aligocalibration/trunk/Common/Scripts/Timing/ so that they run in the control room with modern gpstime package and also the offset is not hard coded. I committed the changes.
Please reconnect the cable soon so we have independent witness signals of the time stamp. There could be a better implementation but we need the current ones until a proper fix is proposed, approved and implemented.
I have checked the weekly Fscans to look for similar 1 Hz and 10 Hz combs in the H1 data (which we haven't see in the H1 O4 data thus far), or any obvious changes in the H1 spectral artifacts occurring due to the configuration change May 28. I do not see any changes due to this configuration change. This may be because the coupling from the timing IRIG-B signal may be lower at LHO than it is at LLO. I do notice that there is some change around the beginning of May 2024 that the number of line artifacts seems to increase; this should be investigated further. Attached are two figures showing the trend of 1 Hz and 10 Hz comb, where the black points are the average comb power and colored points are the individual comb frequency power values; color of the individual points indicates the frequency. Note that there is no change in the last black data point (the only full-1-week Fscan so far).
The IRIGB cables at EX and EY have been reconnected (PEM AA Chassis CH31).