J. Kissel Figured I'd make the same in-air vs. in-vac comparison of the whole 6 x 6 transfer function matrix for H1 SUS PR3 like I did for SR3 in LHO:83831. D R I V E D O F L T V R P Y L -- meh meh meh eand YI R T meh -- nd eand meh meh E S V YI YI -- nd meh nd P R meh eand YI -- YI meh D O P eand YI YI YI -- nd F Y YI nd nd nd nd -- Recall the legend is YI = Yes, Interesting. DC response magnitude is a bit different between vac and air, but not by much and all the resonances show up at roughly the same magnitude. meh = The resonant structure is different in magnitude, but probably just a difference in measurement coherence eand = The cross coupling is expected, and not different between air and vac. nd = Not Different (and unmodeled). The cross-coupling is there, but it doesn't change from air to vac. (1) For some reason, the data quality on the upper diagonal is worse for the PR3 in-air TFs vs. SR3's but better on the lower diagonal. The "mehs" in PR3's cases are more "man, I wish the coherence was better so we could make a better statement." (2) For the most part, the same DOFs that are "Yes, Interesting" for PR3 are "Yes, Interesting" for SR3. Needs a more careful study, but we're only looking at crappy in-air vs. good in-vac data because we're vented right now, and we want to see if it's sensible to measure these things in air, fit the data, and trust that that fit will work in vacuum. Given that we're seeing *any* of these elements as "Yes, Interesting -- there's a difference between in-air and in-vac" means that we're getting scared away from do that -- the problem is hard enough! We'll probably just end up waiting for the SUS to be back at vacuum in a few weeks.
I am adding a comparison between SR3 and PR3 in the attached pdf.
These are the in vacuum measurments for SR3 from 2024-08-08 (in solid red) vs. the in-vacuum ones for PR3 from LHO aLog 80683 (in dashed blue).
At a glance, the M1 Transverse and Vertical couplings to M1 Yaw are at the level we considered *bad* for PR3, so I think we might have to consider these couplings into account when we implement the estimator. We will have to see how the ISI interacts with these couplings before deciding that it is a problem.
Laser Status:
NPRO output power is 1.839W
AMP1 output power is 69.11W
AMP2 output power is 139.0W
NPRO watchdog is GREEN
AMP1 watchdog is GREEN
AMP2 watchdog is GREEN
PDWD watchdog is GREEN
PMC:
It has been locked 1 days, 3 hr 1 minutes
Reflected power = 22.81W
Transmitted power = 104.6W
PowerSum = 127.4W
FSS:
It has been locked for 2 days 23 hr and 35 min
TPD[V] = 0.8157V
ISS:
The diffracted power is around 4.2%
Last saturation event was 4 days 5 hours and 23 minutes ago
Possible Issues: None reported
Corey, Mitch, Randy, Jim
This morning we finished the gross cleaning of the outside of the storage container for the HAM1 ISI. This sat outside for many years so we started with pressure washing a week or two ago. Today, we wiped the outside of the can as best we could and shifted it into the staging building. We did another cleaning inside, getting what we could out of the latches vacuuming as we went. We then opened the can and cleaned both sealing surfaces of the can, the oring seal and scrubbed the ISI platform multiple times with alcohol wipes. After lunch we wiped it down a final time, used a bit of steel wool to remove some stubborn stains on the bottom of the platform then moved the ISI onto the suspended platform. The ISI is held in place with 4 3/8-16 screws through the top of stage 0 and around 10 all thread studs threaded into the support platform. Lid flew back on and we are ready for the trip to the OSB. Randy moved the install fixture into the LVEA yesterday, so we just have to move the ISI, install cart and lifting bridle to the LVEA. Looking pretty good for ISI install Monday or Tuesday.
Visually the ETMY HWWD looks nominal, all power LEDs are green. To test I unplugged the top monitor connector and after a few seconds the LED-FAULT red led lit up. After 8 seconds I plugged the monitor connector back in which cleared the LED-FAULT light.
Attached trend shows the HWWD STAT go to 8 (led current fault) and the countdown timer started counting down from 20 minutes (seconds channel shown).
It appears there is no problem with the HWWD unit itself, and the change in behavior since the power outage must be related to something upstream (satellite amps). I'll pass this onto Fil for further testing.
At this point I'm not sure if the ETMY hardware watchdog system is fully functional, but bear in mind this is a secondary watchdog to the IOP SWWD.
Betsy, Camilla, Sheila, Tony, Robert
After Wednesday’s discovery that the PUM-level inter-chain stops would prevent us from overlaping the ITMY AR optical lever beam and the arm-cavity side CPY beam (overlapping these beams gives the correct orientation of CPY), we decided to back off the adjustment just a little to reduce the chance of touching and leave the beams closer than prior to the vent, though not overlapping. At the end of Wednesday, the beams that were supposed to be overlapped were about 0.18 of the ITMY HR - ITMY AR spot distance. They were still at 0.18 Thursday morning and, after backing off a little, were at 0.22 of the HR-AR distance (with the same 0,0 slider settings they started out at 0.32).
These measurements were made with the R0 sliders at 0 pitch and 0 yaw. We also found the slider settings for the closest approach (see figure). At this closest approach the spots only differ by 0.085 of the HR-AR distance (3.4e-4 radians).
I calibrated the CPY sliders assuming the ITMY HR - ITMY AR spots were 4e-3 radians apart, due to the 0.08 degree wedge with assumed 1.45 index of refraction (coatings not considered). I get 0.63 microradians per slider unit in pitch and 0.69 in yaw. The calculated separation of the HR-AR spots, 4e-3 radians, was approximately equal to the measured separation, 3.8 e-3 radians, assuming we were 32 meters from the test mass.
I took transfer functions for ITMY's M0 and R0 to check for any rubbing that might have been caused by the negative pitch adjustment made to R0 (83865). Most importantly, we wanted to make sure that a negative pitch offset in the R0 OPTICALIGN OFFSET sliders wouldn't cause R0 to hit anything when driven. The negative pitch means that R0 is tilted away from M0, so the bottom of R0 juts towards the bottom of M0.
First I took a set of regular R0 transfer function measurements with the R0 offset sliders at 0. These look good.
I then set the R0 Pitch offset slider to -250, which we are unlikely to go past (typically that slider is set to mid +200s). We called this the 'closest approach'. I wasn't able to set the slider to its full offset of -440, because then the DAC range is so limited that we aren't able to drive it to take any measurements. These transfer functions also all look good. We especially made sure that Pitch was looking good and not rubbing anywhere.
To be even more certain that we weren't going to end up with anything touching, we ran a few transfer functions on M0 with a 'double closest approach' setup. With the R0 Pitch slider still set to -250, I changed the M0 Pitch slider to +250, tilting the bottom of M0 towards the bottom of R0, putting them even closer. I then checked Pitch, Vertical, and Yaw, with Pitch being the most important in telling us whether we were anywhere near close to having them hit anything. Those also all came back clean (Yaw looks weird but Jeff assured me that that's due to cross-coupling movement that went away when we reran it with damping loops on*).
We are confident that the adjustments made in the chamber didn't put us at risk of rubbing, and so doors are clear to go on. Once doors are back on we will check again.
These measurements have been committed to svn and can be found at:
.../QUAD/H1/ITMY/SAGR0/Data/2025-04-10_1800_H1SUSITMY_R0_WhiteNoise_{L,T,V,R,P,Y}_0p01to50Hz.xml r12208
.../QUAD/H1/ITMY/SAGR0/Data/2025-04-10_2200_H1SUSITMY_R0_WhiteNoise_{L,T,V,R,P,Y}_0p01to50Hz.xml r12208
.../QUAD/H1/ITMY/SAGM0/Data/2025-04-11_1600_H1SUSITMY_R0_WhiteNoise_{V,P,Y}_0p02to50Hz.xml r12212
Results have been committed to svn and can be found in:
.../QUAD/H1/ITMY/SAGR0/Results/2025-04-10_1800_H1SUSITMY_R0_ALL_TFs.pdf r12210
.../QUAD/H1/ITMY/SAGR0/Results/2025-04-10_2200_H1SUSITMY_R0_ALL_TFs.pdf r12210
* Full explanation from Jeff: "the 'weirdness' in yaw is the several frequency points where the reference looks smooth as a function of frequency between resonances, and the new data has 'lots' of single-data-point excursions from that smoothness. I attribute this to lack of coherence, and lots of motion on the QUAD. Yaw is a differential measurement of F2 and F3. We’re already having to drive less than normal because we have large offsets on. But also, we typically see that since there’s lots of motion, the imperfect calibration of the F2 and F3 sensors shows up, and lots of other DOF’s resonances show up at a low level where they shouldn’t. Turning on the damping loops and measuring again with them on is the confirming evidence that this is what’s going on. We took the same TF with the R0 and M0 chains damped and they look good."
Measurement | Mass? | R0 OPTICALIGN OFFSET Pitch value | M0 OPTICALIGN OFFSET Pitch value | Description |
2025-04-10_1800 | R0 | 0 | -108 (nominal) | nominal |
2025-04-10_2200 | R0 | -250 | -108 | R0 closest approach; R0 bottom tilted towards M0 |
2025-04-11_1600 | M0 | -250 | +250 | R0, M0 both closest approach; bottoms tilted towards each other |
Adding a PDF of the M0 measurements taken earlier, along with L, T, and R for M0 taken in that same configuration. These cannot be analyzed because they were taken with a different bin width, but more official measurements will be taken next week.
These extra measurements have been committed ot the svn and can be found at:
.../QUAD/H1/ITMY/SAGM0/Data/2025-04-11_1600_H1SUSITMY_R0_WhiteNoise_{L,T,R}_0p02to50Hz.xml r12215
Fri Apr 11 10:10:04 2025 INFO: Fill completed in 10min 1secs
Morning dry air skid checks, water pump, kobelco, drying towers all nominal.
Dew point measurement at YBM , approx. -42C
Attached is the Trello showing what has been achieved this week and what is on the books for today. Many things started yesterday were (expectedly) not finished in 1 day so will roll to today, namely finishing feedthru (and some cable) population in the empty HAM1 chamber, and evaluating ITMY and it's reaction chain for closeout given the new CPY slight pitch change. The ISI is ~en route from the staging building to the LVEA ~today in prep for install early next week. Things seem to be on schedule with how I had them laid out in the plan, even after the Monday schedule loss due to the gnarly power outage and EE component failures which took the vent staff all day to recover from.
TITLE: 04/11 Day Shift: 1430-2330 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Planned Engineering
OUTGOING OPERATOR: None
CURRENT ENVIRONMENT:
SEI_ENV state: MAINTENANCE
Wind: 5mph Gusts, 3mph 3min avg
Primary useism: 0.02 μm/s
Secondary useism: 0.22 μm/s
QUICK SUMMARY:
Left over tasks from yesterday:
On the docket for today is:
BSC8 - Prep for Closeout
BSC8 - DOOR ON
HAM1 - Prep for ISI install
VAC Start Feedthru Swap
The IAS support tube survey will likely not happen as the recent power outage has seemingly damaged the FARO (specifically its external temperature sensor) and it needs to be seen by their service team. We are waiting to hear about a rental unit in the meanwhile.
Today's activities:
The new RF 5-way coax cable in the feedthrus are a little tight in the 5-way cross, but seemed to work ok. Also, the connections on the 4.5" feedthru port are a deep pocket connection so I was not convinced that the new connector was fully seated since you could not visually see it. Marc came out and checked continuity to settle my fears given the newness of this joint and the fact that we have many more to do. All good so far.
Picture of the completed D6 port on HAM 1, with new feedthrus and assembled five way cross extension.
Because of the tightness of the connectors when pushing the 4.5" feedthru into the D6b cross (namely the D6-5wx2 port), Fil and I checked for grounding on all of the ports/connections on this cross. All passed. Travis noted some tightness on the 5-way cross port 5wx4 on D1 opposite the chamber as well. So, Fil and I started checking these and indeed found a ground loop "fail" on both 25pins of the D1-5wx4 cross. We will try to swap in new style 25pin cables D2000456 which have entirely PEEK connector to see if that mitigates this. More to come in separate log.
WP 12451
The air RFPD cables were disconnected from the HAM1 feedthroughs (D6 and D5) and pulled back to ISC-R2. Cables were disconnected from the patch panels and removed from the rack. The air REFL WFS cables going to ISCT1 were removed, this included POPAIR_X. Daniel started installation of the new/modified patch panels in ISC-R2. The long RF cables will be re-terminated/labeled next week in the EE lab with female SMA connectors.
F. Clara, R. McCarthy, M. Pirello, D. Sigg
TITLE: 04/10 Day Shift: 1430-2330 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Planned Engineering
INCOMING OPERATOR: None
SHIFT SUMMARY:
Most things from today are either done or partially done.
LOG:
Start Time |
System |
Name |
Location |
Lazer_Haz |
Task |
Time End |
---|---|---|---|---|---|---|
14:00 |
FAC |
Kim, Nellie |
LVEA |
n |
Tech clean |
17:37 |
14:57 |
FAC |
Randy |
LVEA |
n |
Prepping for craning |
15:26 |
15:28 |
SEI |
Jim, Mitchell, TJ, Jennie |
LVEA |
n |
HAM1 Stack removal cont (TJ out 18:02, Mitchell,Jennie out 18:10) |
18:14 |
15:29 |
VAC |
Jordan |
LVEA |
n |
Purge air checks |
15:39 |
15:56 |
SEI |
Corey |
LVEA |
n |
Joining HAM1 SEI crew |
18:13 |
15:57 |
EE |
Fil |
OpticsLab |
n |
Making cables |
18:33 |
15:58 |
ISC |
Camilla |
LVEA |
n |
HAM1 optics checks |
18:00 |
16:00 |
Betsy, Robert, Tony, Sheila |
LVEA |
n |
CPY work |
18:16 |
|
16:14 |
EE |
Marc |
OpticsLab |
n |
Helping Fil with cables |
18:33 |
16:28 |
ISC |
Elenna |
LVEA |
n |
Joining Camilla |
18:00 |
16:55 |
Richard |
LVEA |
n |
Checking that everyone is working safely |
17:30 |
|
17:03 |
VAC |
Travis |
LVEA |
n |
Grapping parts |
18:25 |
17:09 |
VAC |
Jordan, Melina |
LVEA |
n |
Grabbing parts |
19:07 |
17:29 |
FAC |
Tyler, Erik |
Roof |
n |
Inspecting skylights |
17:34 |
18:34 |
EE |
Fil, Marc |
LVEA |
n |
Removing HAM1 cables |
19:48 |
18:52 |
HAM1 |
Camilla, Elenna |
LVEA & Optics Lab |
N |
Cleaning optics & getting parts |
19:24 |
19:08 |
FAC |
Nellie |
HAM Shack |
n |
Tech clean |
21:03 |
19:35 |
Jennie |
LVEA |
N |
Take care of used wipes |
19:54 |
|
19:35 |
Jennie |
OpticsLab |
n |
Putting wipes away |
19:45 |
|
19:35 |
VAC |
Travis |
LVEA |
n |
HAM1 cable work |
23:28 |
19:39 |
VAC |
Jordan, Melina |
LVEA |
n |
HAM1 cable work |
23:28 |
19:42 |
Tony, RyanC |
LVEA |
n |
BSC8 inventory |
20:51 |
|
19:47 |
FAC |
Randy |
LVEA |
n |
Craning |
21:44 |
19:54 |
EE |
Fil, Marc |
LVEA |
n |
Pulling more cables (Marc out 20:45) |
22:26 |
19:57 |
TJ |
LVEA |
n |
Dropping off stuff |
20:05 |
|
20:01 |
Betsy |
LVEA |
n |
HAM1 cable help |
20:44 |
|
20:05 |
ISC |
Josh, Keita, Jeff |
OpticsLab |
y(local) |
Testing SPI (Jeff out 22:04)(Keita out 23:43) |
23:51 |
20:14 |
ISC |
Camilla, Elenna |
LVEA |
n |
Continuing optics check |
22:17 |
20:27 |
Richard |
LVEA |
n |
Seeing Marc and Fil |
21:54 |
|
20:28 |
CDS |
Dave |
EY |
n |
Labeling a bad port |
21:28 |
21:08 |
Tony |
CER-ish, pcal lab |
n |
Putting box back |
21:13 |
|
22:26 |
Marc, Fil |
LVEA |
n |
Helping Betsy |
23:10 |
|
22:26 |
Betsy |
LVEA |
n |
Pulling cable help |
23:26 |
|
22:27 |
Richard |
LVEA |
n |
Checking in on everyone |
23:27 |
|
23:07 |
HAM1 |
Camilla & Elenna |
HAM1 |
N |
First contacting & optics cleaning |
23:42 |
Elenna, Camilla
We started to inspect the optics and beam dumps removed from HAM1 in 83836. They look dustier than expected, but after first contacting the optics are looking good, more to do...
The In-Vacuum RFPD cables needed for HAM1 were re-terminated. Connectors that mate to the feedthrough are the new 5-way coaxial connectors. The connector that connects to the PD was not modified. Total of 11 cables were re-terminated. Cables were tested for continuity and a TDR test was performed using the Keysight FieldFox Analyzer.
D1300278 Qty 7 length 156”
D1300278 Qty 4 length 106”
F. Clara, C. Gray, M. Pirello
The following cable serial numbers were modified, 4 short, 7 long:
S1301446 short
S1301447 short
S1301450 short
S1301458 short
S1301467 long
S1301468 long
S1301469 long
S1301470 long
S1301472 long
S1301473 long
S1301476 long
Images of cable modifications attached below:
This morning I ran a full IPMI sensor scan on all the realtime front ends and h1susauxex could only see one of its two redundant power supplies. I drove out to EX to inspect and found that both PS look fine with green LEDs. One at a time, I disconnected the power cord and pulled the PS out of the chassis, waited until the LED extinguished and then reinserted. This has made no change to the IPMI Sensor reporting. I'll flag this unit as an exception when reporting failed power supplies.
IPMI Sensor h1susauxex:
h1susauxex: OK | (2215) Chassis Intru | OK |
h1susauxex: OK | (2818) PS2 Status | Presence detected |
IPMI Sensor h1susauxey for comparison:
h1susauxey: OK | (2215) Chassis Intru | OK |
h1susauxey: OK | (2751) PS1 Status | Presence detected |
h1susauxey: OK | (2818) PS2 Status | Presence detected |