19:26UTC - 12:26PT, truck at receiving
19:37:35UTC - Commissioning , Praxair on site
Praxair takes about 2.5 hours, so expect to be in Commissioning until about 22:15UTC.
There is a second Praxair truck expected today as well.
19:44UTC - Richard, Filiberto, Mid-Y
19:45:55UTC - engaged FM2 on DHARD_Y, Sheila's filter
- heard the rumbling of the truck in the CR, and saw the range drop to 55Mpc just before engaging the filter
- apparently the truck had to turn around and go to the Y arm, which is the rumbling I heard
TITLE: IFO returns to Observe after multiple large earthquakes over the last 4 hours.
ASSISTANCE: Hugh (HAM5 SEI clearing all Guardian issues), Sheila (bounce-roll mode damping)
TIMELINE:
15:00UTC - start of shift, high ground motion
- SYS_DIAG telling me ISS defracted power is too high - I reduce the slider. Defracted power was 12 and went to 9.
15:47:12UTC - ground motion just coming down enough to relock, first DRMI lock since the earthquake in Canada
16:09:36UTC - IFO made it to Bounce Violin Mode Damping
16:19:37UTC - IFO unlocked
- A couple more DRIM locks that didn't survive.
- Four more 5-6 magnitude earthquakes come in and prevent locking.
18:04:31UTC - IFO ready to lock, and this starts the locking sequence that resulted in the IFO going to Low Noise
- Longer than usual time from ready to Low Noise, and one reason was that the roll mode on ITMY was about 4, so with Sheila's help I started the damping of the roll mode manually, and waiting for it to improved = 20 minutes
18:55:04UTC - IFO in Low Noise
18:58:57UTC - IFO in Observe
All buildings are beginning to respond to the lower outdoor temperatures so Bubba and I have turned on heaters in both end stations and the LVEA.
One stage of HC5 is now on in the LVEA. This will impact the input chambers the most. The response appears to be ~0.5 F.
The End stations have variac control so these have been incremented from 4ma(off) up 8.5ma
TIME: 16:39UTC, 9:39PT
STATE OF THE IFO: Unlocked
EXPLANATION: The IFO did lock and made it past ENGAGE_ASC_PART3, but then another earthquake arrived, and broke the lock, and ground motion is high.
Video0's striptools have been modified, and now they have a red background, due to the channels DHARD_Y and DHARD_P.
When making a change to a screen, it's important to test it in all situations. Maybe this addition worked quite well during our long lock, but right now with earthquakes and relocking, the change to the striptools have rendered them unusable.
FOM image attached.
This is a symptom of a rung up roll mode. Cheryl spent the last few minutes damping it (ITMY) and now these displays are back to looking normal.
Following Sheila's entry (alog 21708), I've tried to figure out which locklosses where due to Earthquakes during the week of Sep 10th (ER8).
Out of the 22 locklosses seen this week, I've counted 6 locklosses due to EQs. Sheila counted 9, I'll double check my conclusions with her.
| EQ | Location | Ground Velocity at LHO | Status | Lock Loss time |
| 5.9 | Alaska | 5.99 microns/s | Lockloss | 1125916264.5625 |
| 5.2 | Mexico | 1.08 microns/s | Lockloss | 1126042739.0625 |
| 5.7 | New Zealand | 1.16 microns/s | Lockloss | 1126127070.8125 |
| 6.3 | Indonesia | 3.20 microns/s | Lockloss | 1126427496.4375 |
| 6.1 | Papua New Guinea | 2.90 microns/s | Lockloss | 1126448905.3125 |
| 8.3 | Chile | 170 microns/s | Lockloss + SEI trip | 1126480080.5625 |
The ground velocities represent the maximum amplitude predicted by the Seismon software. These predictions could be inaccurate by a few percents.
Six examples is not enough to do some accurate statistics, but the behavior observed during ER8 doesn't contradict the conclusions drawn from ER7 (see DCC T1500230). My conclusions were:
Note: among the 16 remaining locklosses, some of them are due to a high ground motion, but EQ is not the cause (wind? human activity?).
TITLE: 9/24 OWL Shift: 7:00-15:00UTC (00:00-8:00PDT), all times posted in UTC
STATE OF H1: Unlocked. Waiting out Earthquake.
SUPPORT: None (& not needed)
SHIFT SUMMARY:
More action during this shift with the end of the long lock stretch (no obvious reason for lockloss by Jim, although he said he mentioned 45MHz issues for end of that lock). Went through an alignment & then had a 4hr lock, and then had another Unknown lockloss. Then while trying to bring back H1 had some issues (noted earlier). And now handing off unlocked H1 with seismic ringing down from Vancouver EQ.
Shift Activities:
12:35 H1 Lockloss (nothing obvious: seismic quiet, and all the H1 strip tools showed nothing obvious before lockloss)
During Lock Acquisition, during 2nd locking attempt, had issues with ALS XARM:
1) You can either misalign SRM using the SUS_SRM guardian, or use a new state in ALIGN_IFO called SET_SUS_FOR_PRMI_W_ALS.
2) Request OFFLOAD_PRMI from the DRMI guardian.
3) Once PRMI locks adjust PRM and BS alignment until you get about 80 counts on POP90 and 50 counts on POP18.
4)Realign SRM by undoing whatever change you made in step 1.
5) Request DRMI_1F_OFFFLOADED from the ISC_DRMI guardian.
Waited for DRMI to lock again. Several times I had a Verbal Alarm which sounded like "Slip Mode"? What do we do about this? It looked ugly on AS-AIR video. Had "Slip Mode" alarms a few times while waiting for DRMI, and then the Vancouver earthquake arrived!
After recovering ISIs and ETMy, took ISC_LOCK to LOCKING_ALS, but haven't made it there yet (the guardian log keeps saying "Waiting for arms to settle"). The 0.03-0.1Hz seismic band was ramping down, but flattened out at 0.3um/s (which is over an order of magnitude from normal quiet levels). Perhaps we should wait for this to come down to normal levels.
At 13:54 Verbal Alarm posted Earthquake.
Looks like Magnitude 5.5 from Vancouver Island at 13:49. (Terramon did not alert us to this one.) 0.03-0.1hz seismic has increased 3 orders of magnitude (!) and 0.1-0.3Hz seismic has increased 2 orders of magnitude.
ETMy & all BSC ISIs have Watchdogs have tripped.
H1 had a ~46Hr lock that ended toward the end of Jim's shift. He noted DRMI was looking pretty ugly. I waited DRMI a little, but eventually gave Sheila's new PRMI procedure a try, but POP18 & POP90 remained at a flat zero and PRMI never locked. So went through the Initial Alignment procedure (I went slow & took notes since this is something we do rarely.). Alignment was and getting to NOMINAL_LOW_NOISE were straightforward.
Reason for Lockloss?
I saw nothing obvious from seismic signals when I walked in, everything quiet! Jim mentioned ASAir/OMC video spots took an odd move prior to lockloss. H1 was trending down over 6hrs before the lockloss, and Jim mentioned this could be the RF45 issue which has been coming up.
Initial Alignment Notes:
Accidental Slip Out Of Observation Mode: 9:04:15 - 9:04:33
While making the entry above and updating the Initial Alignment wiki, I wanted to look at a pull-down of an ISC Guardian node. Clicking on the ALS_YARM node pull-down dropped H1 out of Observation & into Commissioning. (after cursing, I quickly checked things and took H1 back to Observation)
(I didn't bother touching the Observatory Mode button during this short slip.)
TITLE: 9/24 OWL Shift: 7:00-15:00UTC (00:00-8:00PDT), all times posted in UTC
STATE OF H1: H1 in lock acquisition after ~45hr lock.
OUTGOING OPERATOR: Jim W.
SUPPORT: None
QUICK SUMMARY: DRMI looked ugly. Tried Sheila's new procedure for PRMI, but POP90 & POP18 were flat at zero. Proceeding with an Intial Alignment.
Title: 9/23 Eve Shift: 23:00-7:00UTC
State of H1: Re-locking after loss of 46 hr lock
Support: Most of the commissioning crew was here when I arrived, Jenne held out till 6 UTC
Shift Summary: Mostly quiet untill lockloss at 6:30
Activity Log:
23:00 ish JeffK doing PCAL measurements
1:00 ish I load new code for event triggers
5:00 ish RFAM starts acting up, range starts trending down more
6:30 Lock loss, no obvious cause, I start trying to recover
Durring yesterday's maintence window I made some excitations on both transmons to investigate the noise peaks around 75-85 Hz. The main conculsions are that the coupling from TMS X L drive to DARM is bilinear while the coupling from TMSY is linear, and it seems likely that TMSX motion accounts for some significant part of the unexplained noise in the H1 noise budget (21162) even at frequencies where there is no coherence between DARM and the X QPDs.
In the first attached screen shot you can see the DARM spectra durring some of my excitations in the upper panel and TMS QPD spectra in the lower panel. In the QPD spectra, you can see that the X end QPDs have some excess noise compared to Y. These spectra were from a time when I had a TMSX longitudnal injection at 75 Hz (this is the same time as the yellow DARM trace). There is a narrow line in the X QPD spectra, but in the DARM spectrum the line that appears is about 1 Hz wide, indicating there is some bilinear coupling. The excitation either did not show up or was very small in the QPD sums.
I also made a few injections into TMSY longitudnal which produced only narrow lines in DARM, both X and Y injections are shown at 100 Hz for comparison.
We can attempt to make projections of this noise into DARM using the ratio or the injection line peaks or the rms of the injection peaks to estimte the coupling. I drove longitudnally and the only good witness sensor we have is an angular sensor. If the coupling mechanism is something like scatter off the QPDs that goes directly back into the arm, DARM would be mostly sensitive to the longitudnal TMS motion and if the QPDs are only seeing the unintentional length to angle coupling the projection from the normal level of the QPD spectra to the normal level of DARM could be an overestimate. This projection does show that this would be within a factor of 10 of DARM from about 100 Hz down to at least 75 Hz.
Perhaps when we get a chance we can try misaligning TMSX to see if we can reduce the noise in DARM this way.
AS Keita suggested, I checked if some of this noise (or at least the linear coupling seen for TMSY) could be simply that my drive on TMS moves the ISI and that motion propagates down the quad to the test mass. This seems to be much too small to explain the observed coupling.
Using the GS13s, and the calibration for them that Jim told me, the table motion caused by my 75 Hz drive to TMSX was 4.9 nm/rt Hz, while my 90 Hz drive to TMS Y caused the table to move 3.4 nm/rt Hz. Using the quad model, The table motion is attenuated by 281 dB at 75 Hz and 294 dB at 90 Hz. The test mass motion induced due to my TMSX drive would be 4e-23 m/rt Hz at 75 Hz, and 6.724e-24 m/rt Hz for TMS Y. (too small to explain the lines in DARM).
Of course it is possible that the coupling mechanism is through the motion of the ISI, not TMS.
L1 went out of lock. At H1 we turned off the intent bit and injected some hardware injections. The hardware injections were the same waveform that was injected on September 21. For more information about those injections see aLog entry 21759 For information about the waveform see aLog entry 21774. tinj was not used to do the injections.The commands to do the injections were: awgstream H1:CAL-INJ_TRANSIENT_EXC 16384 H1-HWINJ_CBC-1126257410-12.txt 0.5 -d -d >> log2.txt awgstream H1:CAL-INJ_TRANSIENT_EXC 16384 H1-HWINJ_CBC-1126257410-12.txt 1.0 -d -d >> log2.txt ezcawrite H1:CAL-INJ_TINJ_TYPE 1 awgstream H1:CAL-INJ_TRANSIENT_EXC 16384 H1-HWINJ_CBC-1126257410-12.txt 1.0 -d -d >> log2.txt awgstream H1:CAL-INJ_TRANSIENT_EXC 16384 H1-HWINJ_CBC-1126257410-12.txt 1.0 -d -d >> log2.txt To my chagrin the first two injections were labeled as burst injections. Taken from the awgstream log the corresponding times are approximates of the injection time: 1127074640.002463000 1127074773.002417000 1127075235.002141000 1127075742.002100000 The expected SNR of the injection is ~18 without any scaling factor. I've attached omegascans of the injections. There is no sign of the "pre-glitch" that was seen on September 21.
Attached stdout of command line.
Neat! looks good.
Hi Chris, It looks like there is a 1s offset between the times you report and the rough coalescence time of the signal. Do you know if it is exactly 1s difference?
Yes, as John said, all of the end times of the waveforms are just about 1 second later that what's in the original post. I ran a version my simple bandpass-filtered overlay script for these waveforms. Filtering both the model (strain waveform injected into the system) and the data from 70-260 Hz, it overlays them, and also does a crude (non-optimal) matched filter to estimate the relative amplitude and time offset. The four plots attached are for the four injected signals; note that the first one was injected with a scale factor of 0.5 and is not "reconstructed" by my code very accurately. The others actually look rather good, with reasonably consistent amplitudes and time delays. Note that the sign of the signal came out correctly!
I ran the daily BBH search with the injected template on the last two injections (1127075235 and 1127075742). For 1127075235; the recovered end time was 1127075235.986, the SNR was 20.42, the chi-squared was 29.17, and the newSNR was 19.19. For 1127075242; the recovered end time was 1127075242.986, the SNR was 20.04, the chi-squared was 35.07, and the newSNR was 19.19.
KW sees all the injections with the +1 sec delay, some of them in multiple frequency bands.
From
/gds-h1/dmt/triggers/H-KW_RHOFT/H-KW_RHOFT-11270/H-KW_RHOFT-1127074624-64.trg
/gds-h1/dmt/triggers/H-KW_RHOFT/H-KW_RHOFT-11270/H-KW_RHOFT-1127074752-64.trg
/gds-h1/dmt/triggers/H-KW_RHOFT/H-KW_RHOFT-11270/H-KW_RHOFT-1127075200-64.trg
/gds-h1/dmt/triggers/H-KW_RHOFT/H-KW_RHOFT-11270/H-KW_RHOFT-1127075712-64.trg
tcent fcent significance channel
1127074640.979948 146 26.34 H1_GDS-CALIB_STRAIN_32_2048
1127074774.015977 119 41.17 H1_GDS-CALIB_STRAIN_8_128
1127074773.978134 165 104.42 H1_GDS-CALIB_STRAIN_32_2048
1127075235.980545 199 136.82 H1_GDS-CALIB_STRAIN_32_2048
1127075743.018279 102 74.87 H1_GDS-CALIB_STRAIN_8_128
1127075742.982020 162 113.65 H1_GDS-CALIB_STRAIN_32_2048
Omicron also sees them with the same delay
From :
/home/reed.essick/Omicron/test/triggers/H-11270/H1:GDS-CALIB_STRAIN/H1-GDS_CALIB_STRAIN_Omicron-1127074621-30.xml
/home/reed.essick/Omicron/test/triggers/H-11270/H1:GDS-CALIB_STRAIN/H1-GDS_CALIB_STRAIN_Omicron-1127074771-30.xml
/home/reed.essick/Omicron/test/triggers/H-11270/H1:GDS-CALIB_STRAIN/H1-GDS_CALIB_STRAIN_Omicron-1127075221-30.xml
/home/reed.essick/Omicron/test/triggers/H-11270/H1:GDS-CALIB_STRAIN/H1-GDS_CALIB_STRAIN_Omicron-1127075731-30.xml
peak time fcent snr
1127074640.977539062 88.77163 6.3716
1127074773.983397960 648.78342 11.41002 <- surprisingly high fcent, could be due to clustering
1127075235.981445074 181.39816 13.09279
1127075742.983397960 181.39816 12.39437
LIB single-IFO jobs also found all the events. Post-proc pages can be found here:
https://ldas-jobs.ligo.caltech.edu/~reed.essick/O1/2015_09_23-HWINJ/1127074640.98-0/H1L1/H1/posplots.html
https://ldas-jobs.ligo.caltech.edu/~reed.essick/O1/2015_09_23-HWINJ/1127074773.98-1/H1L1/H1/posplots.html
https://ldas-jobs.ligo.caltech.edu/~reed.essick/O1/2015_09_23-HWINJ/1127075235.98-2/H1L1/H1/posplots.html
https://ldas-jobs.ligo.caltech.edu/~reed.essick/O1/2015_09_23-HWINJ/1127075742.98-3/H1L1/H1/posplots.html
all runs appear to have reasonable posteriors.
Here is how Omicron detects these injections: https://ldas-jobs.ligo-wa.caltech.edu/~frobinet/scans/hd/1127074641/ https://ldas-jobs.ligo-wa.caltech.edu/~frobinet/scans/hd/1127074774/ https://ldas-jobs.ligo-wa.caltech.edu/~frobinet/scans/hd/1127075236/ https://ldas-jobs.ligo-wa.caltech.edu/~frobinet/scans/hd/1127075743/ Here are the parameters measured by Omicron (loudest tile): 1127074640: t=1127074640.981, f=119.9 Hz, SNR=6.7 1127074773: t=1127074773.981, f=135.3 Hz, SNR=11.8 1127075235: t=1127075235.981, f=114.9 Hz, SNR=12.8 1127075742: t=1127075742.981, f=135.3 Hz, SNR=12.4
The BayesWave single IFO (glitch only) analysis recovers these injections with the following SNRs: 4640: 8.65535 4773: 19.2185 5253: 20.5258 5742: 20.1666 The results are posted here: https://ldas-jobs.ligo.caltech.edu/~meg.millhouse/O1/CBC_hwinj/