I keep forgetting to reset the dust monitor alarm levels after IOC restarts so I wrote a little script to check all of the dust monitor alarms levels and reset them if needed based on E1600132. It does not reset the LVEA ones, it just notifies, as these ones alarm levels are sometimes modified.
The scripts is called check_dm_alarms_lvls.py and lives at /ligo/cds/userscripts/. I've also updated the wiki with this info.
Oli, Daniel, Fil, Betsy, Rahul
We have re-installed SUS RM1 and RM2 Tip Tilt suspensions into HAM1 chamber with the new ISI table - see several pictures attached below. RM1 is on the left (towards PSL side) hand side of this picture and RM2 is on the right (zoomed in). Both the suspensions are positioned roughly as per D1000313_V19, and will be fine tuned (pitch and yaw of the mirror as well) during beam alignment work. The blade springs of both the suspensions have been un-muted - see LHO alog 83984 for details.
Both RM1 and RM2 have been plugged-in to their electronics chain. We had to perform some troubleshooting with RM1 after observing grounding issues. At first Fil and Daniel ruled out any issues with the satellite box and in-air cables. After some investigation, the grounding issue was suspected to be coming from the in-vacuum quadrupus cable (connecting to the Bosem), which is an old cable and looks worn out too.
This morning I replaced the old Bosem cable (D1000228_v3 s/n S1105240) with a 55in long (D2100049 S/N 2200358) cable. Before connecting it to the Bosem, Daniel and I verified that the cable is fine (i.e not grounding) and later on we connected each pin (Bosem) one by one. We had to re-adjust the Kapton tape (installed for additional shielding) since the cable bosem connector was grounding to the chamber. After all these modifications, we can confirm that RM1 and RM2 are free from any grounding issues for now. We will check again before closing the chamber.
Next, I will start taking measurements on these suspensions and will post their health report soon.
We have been running the dust monitor vacuum pumps with the assumption that they had to be set to 19 inHg according to T2100415, I went out to ENDY to test this out. When I first checked out the vacuum pump, it was at 20.5 inHg, the flow meter on the dust monitor was reading at 2.8 L/min which is what we want, I then lowered the pumps pressure down to 13 and rechecked the dust monitor and its flow was now at ~2.7. I then adjust the pump down to 10 which brought the dust monitors flow to 2.65. These 1/10s of a L flow are correctable by adjusting the internal flow rate on the dust monitor. Before I left I reset the pumps pressure to 19 inHg.
It seems like we do not need to have the vacuum dust monitor pumps set to 19 inHG, the dust monitors flow rate isn't as strongly dependent on it as we thought?
Closes FAMIS 26397, last checked in alog 84018
Laser Status:
NPRO output power is 1.841W
AMP1 output power is 70.43W
AMP2 output power is 140.4W
NPRO watchdog is GREEN
AMP1 watchdog is GREEN
AMP2 watchdog is GREEN
PDWD watchdog is GREEN
PMC:
It has been locked 2 days, 23 hr 11 minutes
Reflected power = 23.28W
Transmitted power = 105.5W
PowerSum = 128.8W
FSS:
It has been locked for 1 days 20 hr and 35 min
TPD[V] = 0.8003V
ISS:
The diffracted power is around 3.7%
Last saturation event was 1 days 20 hours and 35 minutes ago
Possible Issues:
PMC reflected power is high
Closes FAMIS 26040. Last checked in alog 83968.
HAM4, HAM7, HAM8, EX ST1 all have elevated peaks, mostly around 1Hz line. This is expected due to high maintenance and vent activity.
Closes FAMIS 26375. Last checked in alog 84000,
Everything is under threshold. There are different fans on than last week so difficult to compare. MR FAN3 in CS has a slightly higher noise character in last 3 days
While prepping the HAM1 ISI for testing last night, I noticed that one of the HAM2 HEPI L4Cs seemed non-responsive. It seems this has been the case for quite some time, 206 days according to the attached ndscope. Something happened on Oct 1st last year that cause this L4C to suddenly have only ~1/50th the signal the H2 L4C on the HEPI to sees. I have poked at it a bit, checked cabling on the pier and gently hit the foot to see if I could revive the sensor. I have a couple other tests I want to do before deciding to remove the actuator to replace the sensor, not exactly eager to have to do that.
Dry air skid checks, water pump, kobelco, drying towers all nominal. Dew point measured at HAM1, reading -43.8°C
. Main turbo pumps, XBM, YBM and OMT, all nominal, and temperature is good and stable. HAM6 turbo pump and cart are nominal.
WP12488 HAM8 ISI binary readback broken following site outage FRS33798
Fil, Erik, Jim, Dave:
Yesterday we power cycled the binary input/output and interface chassis, which did not fix the issue. Today we stopped all the models on h1cdsh8, powered down the computer, then power cycled the IO Chassis.
This also did not fix the problem. Investigation continues.
Some changes to the RM1/RM2/PM1:
All other things equal the local damping loops should have the correct sign now. Thic change will also require a sign change in the ASC centering servos.
FAMIS27814
Our cadence is a bit off from biweekly, but no matter since no water was added and the chillers look good (updated the T2200289 sheet). There is a small amount of blueish gunk starting to form in the wire mesh diffuser in the TCSX chiller. I didn't see any of these in our parts bin so I'll put a few on order.
Fri Apr 25 10:08:57 2025 INFO: Fill completed in 8min 53secs
Gerardo confirmed a good fill curbside.
FranciscoL, SheilaD, JoeB
In summary:
I regenerated the mcmc fit on report 20250327T160138Z at 5, 10 and 20 Hz, to compare how the mcmc model would change given different frequency ranges for the fit. We see that the residual of the measurement to the model is better as we increase the minimum frequency threshold. We think this is due to external effects, aside SRC, confusing the model.
We want to give more validity to our observations on alog 83592 -- that the sensing model at low frequencies is a good descriptor of the sensing function. On 83592, I claimed that the observed changes in the sensing function come from changes in SRCL detuning. This is backed up by a low residual on the measured/modeled sensing function. In today's alog, we evaluate how well the model describes the sensing function by (1) having a *low* residual and (2) decreasing the optical spring frequency.
The first three figures attached ('sensing_mcmc_compare_*Hz.png') are the sensing function plots generated by pydarm for measurement 20250327T160138Z. This measurement is not a representation of a calibrated interferometer, since we tuned the SRCL detuning (83585).
From the transfer function on the left, the green dots represent the measurement, the orange trace is the mcmc model from the measurement, and the blue trace is the mcmc model from the last validated calibration measurement (20250222T193656Z). The residual from the measurement to both models are plotted on the right, matching the colors of the respective models. We are interested in the change of the orange trace when we modify the frequency range of the fit.
Each figure has a pair of vertical lines denoting the limits on the frequency range used for the fit. I regenerated the measurement report for 05, 10, and 20 Hz for the minimum frequency. The maximum frequency at 1200 Hz was not changed.
For the residual plots, we see that the magnitude is largest when fitting to 5 Hz, and that the change between the 10 and the 20 Hz fits is negligible. For illustration purposes, I plotted the different sensing models, along with the measurement, together in the last figure (20250327T160205Z_compare_models). The phase plot is not the same as the plots given by pydarm due to missing factors. We see that the three models match above 30 Hz in magnitude.
For the optical spring frequency, we see a decrease from 2.19 Hz to 0.43 Hz when fitting to 10 Hz, and 20 Hz, respectively. This decrease on the SRC spring suggests that the model does not fit the sensing function well, below 20 Hz.
So, regenerating the sensing model shows that the model is good when we see anything above 20 Hz. But we see from the measurement that the SRCL detuning does change the sensing function at low frequencies. The model, however, cannot fit the data from the measurements at these frequencies. We have seen before (80267) that angle to length cross coupling influences the sensing function in the low frequencies. A scenario of cross coupling affecting the sensing function could explain why the model cannot fit the measurement.
Repeating the analysis on cross-coupling, as done in 80267, could improve the sensing function.
TIL; pydarm edition:
The approach that enabled me to regenerate pydarm reports, albeit messy, was to
Modify the pydarm_cmd_H1.yaml
that is in the report to be regenerated, in this case 20250327T160138Z. In particular, the mcmc_fmin
value.
Once the YAML file is configured, run
This command will re-run the calibration report, and, by using the configuration that lives in that directory, make a new model to the sensing function measurement.
TITLE: 04/25 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: 1mph Gusts, 0mph 3min avg
Primary useism: 0.06 μm/s
Secondary useism: 0.09 μm/s
QUICK SUMMARY:
IFO is in PLANNED ENGINEERING for VENT
Some planned tasks for today:
Work safe!
Jordan, Janos, 04-24-2025, ~15:00 The wire gaskets for VBO-C and VBO-D have been leaking continuously for a very long time. Lots of vendors have been contacted, and after a lot of unsuccessful tests, it seems that we finally found the good one manufactured by Torr Scientific (UK). This gasket is extremely annealed, butter-soft, needs super careful handling, but even after some suboptimal installation steps (mea culpa), it finally sealed a new chamber successfully. We tested it right after receiving (had a thriller with customs) with a new C+B chamber, pumped it down and tested on the same day. After the test, we let the pump running during the weekend just to see the ultimate pressure it can reach. They are still very pricey though, 193 GBP (= 257 USD)/pc., even in the case of purchasing 100 pcs., it's 147 GBP (= 196 USD)/pc. So, certainly not an optimal, long-term solution, but a good bridge between having nothing and manufacturing our own.
Good news! Let's take some detailed measurements (as possible), also how close they fit over the flange lip, etc. Will help us when we start fabrication in house.
Oli, Matt, Camilla
Late entry, Jim and I worked the last few half days to lace up all of the cabling for SUS, SEI, and IO/ISC in prep for the main reinstall of table components. Fil, some Richard, and I did preliminary ground loop checks on all SUS and IO/ISC cables so we have a handle on the situation before complicating with components. I routed cables on the table top in an attempt to be near where things plug in but also not in the way of landing objects. Further dressing and coiling will be needed after troubleshooting plugins with components as we go. Pics of the pre round of cabling.
TITLE: 04/24 Day Shift: 1430-2330 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Planned Engineering
INCOMING OPERATOR: None
SHIFT SUMMARY:
IFO is in PLANNED ENGINEERING for VENT
Productive day where most of the work was spent on HAM1 cabling, followed by RM1 install.
Of note:
LOG:
Start Time | System | Name | Location | Lazer_Haz | Task | Time End |
---|---|---|---|---|---|---|
14:39 | FAC | Kim | LVEA | N | Tech clean | 15:52 |
14:39 | FAC | Nellie | LVEA | N | Tech clean | 15:52 |
15:45 | VAC | Jordan | LVEA | N | Purge air checks | 16:03 |
15:45 | SUS | Betsy | LVEA | N | Cabling HAM1 | 18:59 |
15:52 | FAC | Nellie | H2 | N | Tech clean | 16:07 |
16:07 | SUS | Randy | YARM | N | QUAD Moving | 23:24 |
16:33 | SUS | Richard | LVEA | N | Cabling/H.O.R.S.E. | 17:03 |
16:50 | SUS | Mitchell | EX, EY | n | FAMIS tasks | 22:50 |
16:56 | SUS | Travis | LVEA | N | Cabling | 17:06 |
17:07 | FAC | Kim, Nellie | MY, MX | N | Tech clean | 18:51 |
17:53 | VAC | Jordan | MX, MY | N | Emergency Pump Survey | 18:38 |
17:53 | VAC | JaNos | MX,MY | N | Emergency Pump Survey | 18:37 |
18:23 | ISC | Camilla, Matt | LVEA | N | Measuring viewport heights | 18:54 |
18:39 | PCAL | Tony | PCAL Lab | N | TSA to France + stickers | 20:07 |
19:01 | SUS | Jim | LVEA | N | Cabling | 23:00 |
19:31 | FIT | Ryan C | LVEA | N | Respiratory and Perspiratory Regulation Test (Walk) | 20:04 |
19:56 | ISC | Matt, Rahul, Camilla, Oli | LVEA | n | HAM1 ISC installation | 23:23 |
19:59 | VAC | Jordan | MY, MX | N | Turbo Pump Checks | 22:50 |
20:00 | SUS | Betsy | LVEA, Opt Lab | N | Walkabout + Feed Through Cable Work | 21:56 |
20:03 | VAC | Travis | Opt Lab | N | Feedthru Cable Work after turning compressor off | 22:48 |
20:19 | VAC | Janos | LVEA | N | VAC checks | 20:28 |
20:41 | CDS | Fil, Dave | FCES | N | HAM8 Post Outage Glitch | 22:59 |
21:07 | VAC | Vacuum Convoy | YARM | N | Beam Tube Experiment Walkabout | 21:56 |
21:49 | PCAL | Tony | PCAL | N | Measurements and general lab affairs | 22:22 |
22:59 | EE | Fil | HAM1 | N | helping Rahul | 23:24 |
23:24 | SUS | Betsy. Fil, Rahul, Daniel | LVEA | N | RM1 Things | 23:40 |
S. Koehlenbeck, J. Freed, J. Kissel, J. Oberling, R. Short
The SPI pick-off path installation on the H1 PSL table is now complete. The beam in the new SPI path has been reduced to 20mW and is currently being dumped with a razor dump between SPI-L1 and SPI-L2. Pictures attached reflect the final installation and layout, which will be be reflected in the updated as-built layout at a later date.
Associated entries: 83925, 83933, 83956, 83961, 83978, 83983 (and more to come)
ECR E2400083 IIET 30642 WP 12453 Here's Ryan's birdseye view labeled with all the components. For details of the components, see the SPI BOM, T2300363, exported from its google sheets to -v4 as of this entry.
Tagging EPO for photos.
83996 Power In ALS / SQZ / SPI Paths Post SPI Pick-off Install