Kyle, Chandra
We tested the leaks in GV12's gate o-rings by flooding the gate annulus with dry N2 (with active turbo connected and ready to be valved in to evacuate) and discovered the adjacent volumes' pressures rise too high too quickly. The Y2 beam tube rose to 7e-8 Torr and CP4 side rose to 1.4e-6 Torr in less than one minute. We may try to jog the gate on Monday to see if we can get a better seal, at least on inner o-ring. Will also re-evaluate the bake enclosure dimensions so see if gate annulus tubing can stay (GV11's definitely gets in the way and had to go).
We realized that we did not get any email or text alarms when we should have - pressure was well past the 5 minute and 15 minute set point thresholds on PT-245B and PT-256B. Will contact Dave B. about this.
TITLE: 01/27 Day Shift: 16:00-00:00 UTC (08:00-16:00 PST), all times posted in UTC
STATE of H1: Planned Engineering
INCOMING OPERATOR: None
SHIFT SUMMARY:
LOG:
14:13 Terry out to Squeezer bay
16:00 Karen ad Vanessa out to EY
17:00 Karen and Vanessa back
17:04 Karen ad Vanessa back to EY - with stock
17:05 Marc out to LVEA-returning chassis to SUS rack near HAM
17:12 Dust Monitor at EY not responding
17:21 Betsy out to EY
17:32 Betsy power cycled dust monitor 2 at EY
17:40 Patrick reset the HV at EX
17:43 Travis, Danny, and Angus to EY
17:47 Patrick back
17:57 Richard out to LVEA - camera check PSL
18:01 Richard back
18:06 Terry back
18:20 Betsy back
18:23 Greg out to LVEA - resetting TCSY LASER
18:28 N out to optics lab
18:30 Greg back
18:37 Kyle and Chandra moving new ION pump from large high bay to S side floor near HAM4
18:40 Betsy out to EY
19:19 Terry and N back
19:19 Greg out to LVEA - movin curtains from TCSY to TCSX
19:20 Angus, Travis and Danny back
19:40 Dany out to LVEA - pics
20:00 Danny back
20:00 Betsy back
20:05 Jeff back
21:14 Tvo and Sheila out for lunch
21:45 Kyle out to MY
22:02 Peter and Jeff B out to LVEA- ITMX camera
22:10 N, Sheila and Terry into optics lab
22:16 Kyle back
22:30 N back
22:54 Kyle and Chandra to MY
00:10 Jeff and Peter finished with the ITMX and ITMY cameras.
J. Kissel, for A. Bell, T. Sadecki, and D. Sellers While on my way to and from B&K hammering the EY PCAL periscope, I snapped a few publicity photos of Angus, Travis, and Danny who were fine-tuning the alignment and measuring violin modes of the brand new fibers of newly suspended H1 SUS ETMY. Thanks and keep up the good work, gents!
The violin modes were remeasured (with 0.25 Hz accuracy) position (Hz) fibre S/N +X/+Y 504.5 S1400157 -X/+Y 503.0 S1400159 +X/-Y 513.25 S1800486 -X/-Y 510.5 S1800491 as these will shift after in-chamber alignment, we didn't go for higher accuracy. The laser we used was quite noisy and should be replaced before using the kit again.
In order to compensate for the missing mass of the new holey AERM optic being installed in the ETMY suspension, I had to rework the PenRe mass to be heavier. SYS had designed a heavier new set of parts to swap, and I'll report that the rebuild went smoothly - the weigh compensation was pretty spot on and the install of the parts which we have had fit troubles with in the past, went in easy (thanks to Eddie's tweak on the design based on my feedback).
For the record, the weights of these masses are as follows. Note, the idea is to make the old PenRe mass plus the old ERM mass weight equal the total of the new sets, such that the suspension hangs in the same vertical position as before.
| OLD ETM01 mass | 25,993g | NEW AERM07 | 14,873g |
| OLD PenRe mass | 53,236g | NEW PenRe mass | 64,356g |
| Total | 79,229g | 79,229g |
Assembly weighs of the new PenRe:
| OLD PenRe | New PenRe | |
| Keeping Same Main Body | 29,857g | 29,857g |
| Keeping Same batch of small parts | 3,002g | 3,002g |
| Keeping Same wire clamp assys | 168g | 168g |
| Cans and Plates (new and old species) | 19,087g | 30,284g |
| Addable mass assys, to make total weight | 1,122g | 1,045g |
| Total from above | 53,236g | 64,356g |
Doh - Typo, the ETMY AERM is AERM06, not 07.
The difference in weight between these 2 is a negligable 8g however.
I created a medm screen to control all of the illuminators and added it to the sitemap under SYS. The controls for the illuminators in the corner station are not connected to the hardware yet. I also removed the link to the older analog video camera medm screen.
WP 7312 I updated and restarted the h0vacex and h0vacey PLCs to create separate sync units for each Inficon gauge. The X2-8 and Y2-8 Inficon gauges are still powered off, but no longer disabled in TwinCAT. With the addition of the separate sync units this no longer prevents the remainder of the system from running. I burtrestored both h0vacex and h0vacey to 6am local time this morning. The high voltage at each end station has likely tripped off and will need to be reset.
I reset the high voltage at end X.
TITLE: 01/26 Day Shift: 16:00-00:00 UTC (08:00-16:00 PST), all times posted in UTC
STATE of H1: Planned Engineering
OUTGOING OPERATOR: None
CURRENT ENVIRONMENT:
Wind: 24mph Gusts, 20mph 5min avg
Primary useism: 0.04 μm/s
Secondary useism: 0.45 μm/s
QUICK SUMMARY:
Terry, Sheila
We seem to have a mix up with our fiber collimators. We measured the beam profile out of our 532 nm collimator this afternoon, because our mode matching into the OPO is very poor, and found it to be 52 um. This afternoon Terry and I measured the waist out of both of our collimators for both wavelengths.
| 532 nm horizontal waist | 532 nm vertical waist | 1064 nm horizontal waist | 1064 vertical waist | |
| collimator supposedly for 532 (SN4) | 52um @ 0.11m | 53 um @ 0.10m | 256um @ 0.27m | 253um @ 0.27m |
| collimator supposeldy for 1064 | 209um @0.22m | 255um @ 0.33m | 155um @ -0.22m | 156um @ -0.23m |
The 532 collimator that we have is SN4. Maggie sent a link to a git where she has measured data from SN4 for 532nm, this data shows that the waist is 264 um 0.6 meters from the collimator. I am not sure right now what the serial number of our 1064 collimator is, but the data on the git says SN01 has a waist of around 280um @0.3 meters while SN17 and 18 have waists around 315/320um.
It seems like the most plausible explanation is that we have the collimators swapped somehow even though we have been careful not to do that since taking them out of the bag. If the one that we think is the 532nm SN4 is really 1064nm SN01, these measurements aren't as crazy, although there is still a discrepancy between the waist position of the 1064 beam coming out of our SN4 collimator and what Maggie measured for SN01.
The data for all four of the measurements that Terry and I took this afternoon are in the comments in the attached script.
The collimators can be (quite easily, I would say) distinguished by looking at them, if you know the "color code". The 1064nm ones have a milky looking color, while the 532nm ones have a pink-ish color. Hope this helps to confirm your theory..
Jenne, Keita, TVo
Successful locking of the OMC on the 00-mode!
First, the OM1-OM2-OM3 path into the OMC using QPD_A and QPD_B as a reference and closing the loops. This left OM1 pretty close to railing in yaw and so there were some attempts to offload OM1 onto the other two but it would rail the OMC actuators when the loops were engaged. We remedied this by zeroing the OMC alignment sliders while the OMC_ASC loops were on (this worked pretty smoothly). So Jenne offloaded again so that we do the least amount of optics sliding/rotating on the HAM6 optics table.
Fil turned the high voltage on for the PZT so that we could try to lock. There was some confusion when the OMC_DC_IN1 was railing when sweeping the PZT_OFFSET, this is still not clear why so we turned off all stages of whitening to avoid saturating. Then we were able to achieve lock after Keita turned off the purge air, we've left the purge turned on but lower than the previous setting.
Jenne pointed out that having about 1mW of input power from HAM5 should register about 1mA on the OMC_DC_SUM_OUTPUT when on the right mode and we're getting about that with PZT_OFFSET = 1.8.
Nutsinee, Marc, Terry, Daniel
We finally wrestled the new TTFSS to the ground. Ugf is around 500kHz with good phase margin and somewhat less good gain margin. The crossover is around 10kHz. It cannot be raised by much due to two smaller peaks in the 70-95kHz range. A couple of electronics modifications were needed.
For the frequency counter of the beat note to work we need >-12dBm pf RF power in the cable going towards the CER. Ideally we have at least 0dBm. The beat note strength from the photodiode was only around 30mV and we had to change the directional coupler in the TTFSS preamplifier to a splitter to give us more umpf.
Kyle, Gerardo We vented GV12's annulus volume (minus the gate volume) with bottled UHP N2 and observed no leaks into the CP4 volume. Next, we pumped out the vented volume, combined the gate annulus volume and then administered UHP N2 into the entirety of the annulus volumes. We observed pressure rises on both the Y2 module side of the closed gate valve as well as the CP4 side - thus indicating that both the inner and outer gate O-rings leak. We evacuated the system, isolated the gate annulus volume, restarted the AIP (pumps all but gate volume in this configuration) then isolated and shut down the connected turbo+cart. Another useful test would be to fully vent the annulus volumes adjacent to the leaking gate annulus volume and then "dump" this gas all at once as a step change into the gate annulus volume and then observe how much time we would have to decouple plumbing and install a blank on one of the two gate annulus pump ports and a pump port valve on the other gate annlulus pump port as was done to GV11 yesterday.
Today, we measured the violin modes of the new monolithic ETMy with the goal to determine what contributed to the large-ish pitch offset we were seeing. Nothing egregious was found from violin modes themselves, so we decided to attempt to fix the pitch by re-stress-relieving the stock welded to the horns. This technique has been done before, once here at LHO and once at LLO with success. This time around, we went from ~5mRad differential pitch to ~500 uRad differential pitch. Now, if only we could get a factor of 10 improvement in other aspects of LIGO in the course of a day. . .
See final alignment numbers at this alog.
Jim and I went in today and tried our hand at some of the bolts on the periscope. We had high hopes since the 3IFO periscope looked good and the bolts freed easily. Unfortunately, these bolts had their hexes almost stripped on many, if not most, of the bolts (see attachments). With some breaker bars we managed to get out all of the ones we need for the vibration absorbers, and then we started on some for the baffle panel brackets with Betsy guiding us to the correct ones. Overall it was a good success with more work tomorrow. And we only bent 3 wrenches in the process!
Also, I didn't get any pictures of where we left off, check back tomorrow.
TITLE: 01/25 Day Shift: 16:00-00:00 UTC (08:00-16:00 PST), all times posted in UTC
STATE of H1: Planned Engineering
INCOMING OPERATOR: None
SHIFT SUMMARY:
LOG:
16:03 Christina out to LVEA
16:45 Hugh out to LVEA - working atop HAM6
16:50 Set Very Large EQ button because of 5.8mag of the coast of N Cali
16:53 reset ACT SEI trip at ETMX
16:57 reset MC1 wd, HAM2 ISI CPS trip, and ITMY ACT trip. The latter has been problematic this morning.
18:03 Jeff K out to LVEA - talk to Hugh on top of HAM6
18:04 N out to squeezer bay
18:13 Marc out to LVEA - check on ZM1; pull TTFS unit from squeezer bay.
18:22 Betsy Tj Jeff K and Jim out to EY - B&K Hammer and Reaction chain
18:27 Sheila ou to optics lab
18:29 Travis called from EY - the welding team is out there (Danny, Angus and him)
19:43 Noticed Fil out on LVEA floor at output.
21:32 Richard into CER - HV supplies
21:36 Marc out to LVEA - SUS rack by HAM5
21:50 Sheila out to optics lab
21:54 Betsy out to EY
22:04 Jim and TJ out to EY
22:45 Kissel back
22:53 Marc back
23:13 Kyle out to MY and EY
23:38 Jeff B out
23:59 Greg out to TCSY table to reset the LASER
24:00 EOS
A. Bell, J. Oberling, D. Sellers, T. Sadecki, K. Toland
The final 2 fibers were welded to the new ETMy. The monolithic was successfully suspended and IAS measurements were taken. I'll let Jason fill in the numbers, but the differential pitch is a bit larger than we generally hope for but not grossly so. Good work team!
Violin mode measurements to commence tomorrow.
Final alignment numbers for the new ETMy monolithic. All measurements were done with the ETMy suspended; the PUM and UIM were both locked. All numbers assume the reader is looking in the -Y direction (i.e. at the AR surface of the ETMy); this is opposite the notation used in the alignment notebook, which is done from the perspective of the aligment equipment (i.e. looking at the HR surface of the ETMy). The pitch measurement was done after this afternoon's correction of the differential pitch; before the correction the differential pitch was 5.53 mrad down.
The serial numbers of the fibers used and their locations in the monolithic are as follows:
J. Kissel, R. McCarthy, M. Pirello FRS Ticket 9771 After solving all of ZM2's signal chain problems (all of which were mis-jumpered boards inside its new HAM-A coil driver and US Sat Amp, see LHO aLOG series starting with 40237), I'd accidentally told Marc to jumper the SatAmp to the AOSEM setting (ZM2, an HTTS, uses BOSEMs). He's jumpered it to the BOSEM setting this morning, so I've taken another diagnostic suite. Turns out, though the OSEM sensor response dropped by an inconsequential ~13%, ZM2's BOSEMs don't care whether they're read out with a Sat Amp jumpered in the AOSEM or BOSEM configuration. Richard and I recall that perhaps all US sat-amps are jumpered to the same configuration, because (as Richard specifies) one species of OSEM doesn't use the feature implied in that configuration, it just needs to be jumpered to either/or. So we recall having set all US sat-amps one way (or the other). We'll figure out which (by checking the OMs and RMs), and set all the new US Sat Amps (for OFI, ZMs, and VOPO) the same way. For all intents and purposes, ZM2 is now fully functional.
J. Kissel, M. Pirello, R. McCarthy Marc has verified that all US Sat Amps are jumpered to the BOSEM position. As such, we need not make any change to the current configuration of the Sat Amp, and we should consider the electronics and suspension in its final functional state. Thanks for all your help Marc!
Dave Barker rebooted alarm system this morning after a crash yesterday morning.