Unfortunately after swapping out the 16bit-DAC card in h1oaf0 almost two weeks ago, yesterday we got another zeroed-dac event. At 11:53 PDT, Sunday 25th September, the h1iopoaf0 model recorded an ADC, DAC and DK error in its STATE_WORD and from then onwards was correctly outputting zeros to all DAC channels. As usual, this was instructing the TCS chillers to drive to a low water temperature, and 52 minutes later the chiller tripped the TCS lasers (12:45 PDT).
Because we received both an ADC and DAC error, we could try swapping the first and second ADC cards.
T.J. has made his EPICS alarm announcement for this event more insistent, repeating every 2 minutes. If the control room can restart the models on h1oaf0 in time, we think the laser trips could be averted.
It's been a suspicion that, lately, switching DBB shutters has been causing IMC to lose lock. Perhaps this action is causing just enough noise to perturb the injection locking? Until further investigation is done, scans will be taken at times when the mode cleaner can be down for a period of time such as maintenance days.
Weekly Xtal - No changes from last week
Weekly LASER - No changes from last week
Weekly Env - RH for ANTERM, LASERRM and DIODERM are higher than last week. All temps seem to show no change.
Weekly Chiller - nothing unusual except for the change made to the flow rate on 2/19
Given the number of trips over the last week (which are easily seen on the above attached trends), everything looks normal.
Summary of H1's nice night. (Almost 9hr lock with range going from 60 to 70Mpc).
Discussion about running over before/after holiday break, O2 Break, operator 24/7 coverage.
Open Work Permit review.
Maintenance:
Trouble with MODE17 (ITMX 15542 Hz) could be due to instability from large phase changes with slight frequency drift in our damping loop. Mechanical mode frequency at beginning of a cold lock sits around 15541.875 Hz and has drifted to 15541.95 Hz after about three hours. The previous bandpass filter carried ~40 deg phase change over that time. In an effort to fix this, I've made two BP filters that are shifted versions of one another to be turned on as the frequency migrates. The guardian uses the PLL frequency monitor to track the average frequency change of the mode peak and make the filter change switch at the appropriate time. Fall offs and notches in the filters are such that center of BP --> switching point ~10 deg. I've watched the guardian successfuly make this change.
Proof of concept appears to have worked; Mode17 was kept stable throughout frequency drift well beyond the previous 3 hourish mark. Lockloss occured after ~6 hours from the partner Mode25 who saw a phase change of ~140 deg over this time, eventually probably driving up this usually easily dampable mode. Attachment shows freq drift over last night's lock. I've added stepping bandpasses to both modes (controlled with the guardian) now to accomodate frequency drift over much longer locks.
I have moved IM2 and IM3 closer to their O1 alignment values, as indicated by Cheryl's alog 29948. At the same time, I was walking the POP_A offsets to keep the jitter coupling low. I had an excitation from 310-350Hz on IM3 yaw, but the effect it had on DARM didn't really change during this series of moves. But, the other jitter/intensity peaks seem to have perhaps gotten a teeny bit better. More significantly, this set of moves improved the carrier recycling gain as well as the 45 MHz sideband buildup in the SRC.
IM2 and IM3 I only moved in yaw, however this made their pitch values also line up more closely with their O1 values. IM2's witness sensors read (P: 608, Y: -209) while IM3's witness sensors read (P: 1954, Y: -32). The POP_A offsets are currently (P: 0.39, Y: 0.47). This gives a carrier recycling gain of 30.5.
If the IFO is a struggle to lock tomorrow, trend the IM2 and IM3 witness sensors and put them back. I'm leaving them in their new spots for tonight.
I also ran a2l.
We should check in the morning if these IM2 and IM3 positions help get us away from the REFL PD clipping that Sheila has been looking into.
IFO left undisturbed starting 08:20:00 utc.
This lock lasted for 8+hrs. PI modes 17 and 25 rang up and kept increasing in their amplitudes until the lockloss.
Going to stay with changes to the IMs Jenne made (from Cheryl's suggestion) for getting back to an O1 alignment.
Operator NOTE: This will give us a list of a few WARNINGs on the Guardian DIAG_MAIN (if we are happy with where the IMs are, we'll want to update Guardian to ACCEPT this IM alignment).
Especially with the DRMI needing alignment help during most re-locks, I have created a new state to help check BS-only alignment.
Recall that if the DRMI flashes don't look so good, you can select the PRMI_Locked state that Sheila created some time ago. This state will misalign the SRM and attempt to lock the power recycling cavity with the arms held off resonance.
Sometimes though even these flashes aren't very good, and the PRMI isn't catching lock. Now you can select the new state Check_MICH_Fringes in the ISC_LOCK guardian, and it will misalign the PRM. This state is currently not set to try to lock MICH, so it'll never look quite like MICH_dark_locked from initial alignment. But, you can watch the flashes on the AS air camera, and move the BS until they are as circularly symmetric as possible. Note that sometimes you'll only see a few flashes per minute, so this requires a bit of patience, but it's often still faster than giving up and doing a full initial alignment. Once the flashes on the AS air camera are circularly symmetric, re-select PRMI_locked. This will realign the PRM, and go back to the usual locking sequence.
The PSL tripped around 21:37 UTC, it took us about an hour to recover from this . We called Jason and Peter, Jason called back and walked me through restarting it remotely. I added about 200mL of water to the chiller, there was water on the floor in front of the chiller. Jason confirmed that this is normal, and that the turbulence and bubbles in the chiller tube are from a known slow leak.
PSL tripped due to the power meter flow. The 1st attachment shows the power meter flow dropping just before the crystal chiller interlock trips. The 2nd attachment shows the power meter flow dropping ~1 second before the FE flow drops. Interestingly, it takes ~6 seconds after the power meter flow drops and the crystal chiller interlock trips for the crystal chiller flow to drop (3rd attachment). Not sure if this is due to the rate that the Beckhoff PC polls the crystal chiller, or if it really takes 6 seconds from interlock trip to chiller shutdown (I suspect the former). The full timeline of the trip, assuming t0 = 21:37:51 UTC (time of trip):
Filed FRS #6319.
Before restarting all the models on OAF, I accepted diffs on CAL CS, OAF, and SUS proc PI. a screenshot is attached for PI.
There were two periods of unexplained motion of ITMY during undisturbed overnight lock on Sep 23. Both ISIs, plus all levels of the suspension (including oplevs) saw it, but there's nothing evident in the HEPI sensors or the ground. These events made two periods of large noise in DARM (first plot), a few minutes apart, and a few minutes before lockloss due to PI. At that point, the PI didn't seem to be having any effect. The full Omega scan shows that ITMY has lots of anomalous motion. The second-stage ISI GS13s see a quick transient with rich structure (plots 2 and 3). The ST1 sensors see something similar but much less distinctly. The L1 OSEM clearly sees a line below 1 Hz rung up for more than a minute afterward (plot 4). I was not able to find anything on the ground sensors or HEPI that could have rung this up. I haven't looked as closely at the second event. I think this warrants more followup by someone familiar with the seismic isolation.
Kiwamu, Terra, Lisa 3 earthquakes, 2 user errors and 1 PI gave us the opportunity to extensively test our lock acquisition sequence today. (It works pretty well actually. The weakest part is the DRMI lock: the interferometer ends up always misaligned right after an unlock, and it requires manual adjustments all the times to get DRMI to lock. Once the DRMI locks, than the locking sequence rarely fails.) Today we explored the (allegedly) jitter/intensity noise as function of interferometer alignment (SRM alignment, CSOFT/DSOFT and PRC1 offsets). More details will follow, but the bottom line is that we have been able to increase the recycling gain (max 31, typically 28-29, with PRC1_Y offset= -0.06, CSOFT_P = +0.120), the cavity pole (360, typically 340), and minimize "jitter", but we have not been able to do everything at the same time. All the noise tuning steps (including the now standard CO2X 240 mW power) are in the guardian, except the IMC WFS offsets. We also run A2L. We leave the interferometer locked with the SRM aligned by hand to minimizes jitter noise (ASC still open), with recycling gain 29 and cavity pole ~340 (as measured by CAL_CS_TDEP_F_C channel). The range is approaching 70 Mpc. Observe intent bit set at 9:17 UTC, Sep 25.
P.S.: The summary pages are not working for H1 (they do for L1): https://ldas-jobs.ligo-wa.caltech.edu/~detchar/summary/day/20160925
Modes 17 (15542 ETMX) and 25 (15541 ETMY) continue to give us trouble; about three hours into the lock Mode 17 will get high enough that Mode 25's PLL will jump to it, after which Mode 17 rings up quickly. Matt had set up a lower bandwidth loop in the PLL of these to help prevent this and yesterday I tightened it up even more. We've still lost lock the past two nights from these modes. To this end, I'm leaving Mode 25 in BYPASS with a 1Hz BP (still wider than I've seen it shift in frequency over many locks).
Peter (on phone), Kiwamu
We restarted the PSL at around 3:20 local with no problem. Later, I added 130 ml to the crystal chiller which was found to be beeping for a low water level. This cleared an error message on the display and the beep sound.
Kiwamu, Nutsinee
We did a quick test with the HWS yesterday hoping it might fix the issue of HWSY sled reflected off the CP (alog29905). We first moved the ITMX and ITMY CP by a few hundred counts to confirm that only HWSY has sled reflection from CP. Then we swapped the X(790nm) sled and Y(840nm) sled then repeat the process. HWSY still had most of its reflection from the CP. The conclusion is, using different wavelength didn't matter.
We removed the HWS plates and stopped the code. This configuration still remained.
During this test we noticed that HWSX looks clipped. Not sure when did this started happening but Kiwamu said the data from HWSX he's been using make sense. No major misalignment to the SR3, ITMX, and BS in the past few days. A small touch to the top and bottom periscope fixed this clipping.
The sled has been swapped back. This happened on Sunday. HWS plates are still off.