Shoshana, Michael, Jeff, Tony
We spun the NCal as a life check while we were on site. At first the NCal wouldn't turn on and threw a 'NCal power' error. Power-cycling the motor power by replugging the AC cable running to the Beckhoff motor controller (black cable coming from the left in attached picture) fixed the error. We spun the rotor up to 10 Hz for a few minutes before spinning it down.
NCal Settings:
Motor Frequency Request: 1040 ct
Motor Ramp Gain: 0.01
Motor Low Pass Time Constant: 5
TITLE: 05/15 Day Shift: 1430-2330 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Planned Engineering
INCOMING OPERATOR: None
SHIFT SUMMARY:
Vac Folks are still in the LVEA working on the Top VAC Flange Guage.
The Ground checks were done on HAM1
The Ring Heater for SR3 is being left on all night.
BRS team has been pumping down the BRS, seems like perhaps they are mostly done and may go back to EY clean up some wiring.
HAM1 Suspentions seem to be saturating a lot today , but there was a lot of activities on ther ISI and ontop of the HAM1 chamber.
There was some Wind fence work done today at EX, where another Bee hive was spotted on a tumble weed. So please Bee aware, of the TumbleBees.
LOG:
| Start Time | System | Name | Location | Lazer_Haz | Task | Time End |
|---|---|---|---|---|---|---|
| 14:57 | Sys | Corey | LVEA HAM1 | N | Taking Pictures of inside HAM1 | 16:44 |
| 15:05 | FAC | Chris | EX | N | Getting parts | 15:05 |
| 15:34 | VAC | Jordan | LVEA | N | Purge Air checks. | 15:48 |
| 16:17 | FAC | Kim & Nellie | LVEA | N | Technical cleaning | 16:17 |
| 16:31 | EE | Fil | LVEA HAM1 | N | Ground loop checks | 19:03 |
| 16:35 | PEM | Carlos, Keit, Robert | X-arm Vault | N | Magnatometer calibration | 19:18 |
| 16:36 | SEI | Micheal R. & Shoshana | EY | N | Closing up BRS | 18:41 |
| 16:51 | FAC | Kim & Nellie | EX | N | Technical cleaning. | 17:45 |
| 17:10 | SUS | Rahul | LVEA | N | Ground loop checks with Fil | 19:03 |
| 17:31 | VAC | Jordan & Gerardo | LVEA | N | Vacuum system tests | 18:15 |
| 17:31 | EE | Daniel | LVEA | N | Helping Fil do ground loop checks. | 19:03 |
| 17:58 | VAC | Janos | LVEA | n | Vacuum Test | 18:14 |
| 17:59 | TCS | TJ & Camilla | LVEA HAM4 | N | Replacing Hartman SLED | 18:53 |
| 18:16 | VAC | Jordan & Gerardo | MY & EY | n | Vacuum tests. | 19:53 |
| 19:32 | SEI | Jim | LVEA HAM1 | N | Setting up measurements. | 21:32 |
| 19:36 | NCAL | Micheal R & Shoshana | EX | N | Pluging in NCAL to spin off the cobb webs | 20:34 |
| 19:45 | SEI | Randy, Corey, Mitchel | EX | N | Wind fence work | 22:34 |
| 19:54 | VAC | Travis & Gerardo | MX & EX | N | vacuum tests | 20:34 |
| 20:35 | VAC | Jordan, Travis, Gerardo | LVEA HAM1 | N | Testing Vac equipment & helping Jim | 23:40 |
Camilla C, TJ S
The two corner station HWS SLEDs were last swapped back in October 2023 (alog73371), going a bit long than our usual ~1 year before swapping. Today we swapped them with fresh SLEDs following the T1500193 procedure, calibrated their power channels, and started the code back up with fresh references.
HWS starting values
Power as measured from fiber launcher: IX 480uW IY 180uW
Power reported into epics: IX: 1.88 IY: 0.36
SLEDs removed:
X - https://ics.ligo-la.caltech.edu/JIRA/browse/QSDM-790-5--00-11.21.380
Y - https://ics.ligo-la.caltech.edu/JIRA/browse/QSDM-840-5--00-03.20.479
HWS ending values
SLEDs installed:
X - https://ics.ligo-la.caltech.edu/JIRA/browse/QSDM-790-5--00-11.21.382 2.5mW = 165mA = 660mV (on TP with 250mA/V) Max current set to 155mA
Y - https://ics.ligo-la.caltech.edu/JIRA/browse/QSDM-840-5-0-00-06.18.005 2.5mV = 100mA = 400mV (on TP with 250mA/V) Max current set to 95mA
Power measured at fiber launcher: 2.2mW for both
To calibrate the H1:TCS-ITM{X,Y}_HWS_SLEDPOWERMON channel, we turned off the SLEDs, found the dark offset, turned the SLED back on, and then changed the gain. These values are in the SDF screenshots attached.
TJ, Camilla, Sheila
TJ and Camilla got the HWSs working, and now we turned on the SR3 heater at 15:54 UTC, 2W requested power. This is to do a check of the SR3 heater calibration and range similar to 27262
SR3 heating up can be seen on the HWS signals but is not particulatly clear, see attached.
Looking at when this test was done at LLO, the lens changing happened over a period of three hours and the lens power increased in the same direction on both HWS, so its possible our HWS are not a good witness for the SR3 curvature change.
Aidan calculated 2.45 uD/W at LLO, and we get 9.44 uD/W (from the H1:TCS-ITM{Y,X}_HWS_PROBE_SPHERICAL_POWER trends with an estimated noise of 4.48e-12uD/W.
Looked closer at these HWS signals during SR3 heater heat up and cool down. In all these plots, the two t-cursors are used as the reference and shown HWS live image.
Some strange things:
With the numbers from ITMY HWS only, and looking at the 3hr 11 m cooldown in Camilla's photo, the lens change is 6.68e-6 Dioptres/W taking into account that the HWS beam passes twice through SR3.
After talking with Camilla, she reminded me the change in RoC (delta R) =/= 2/(delta D),
where D is defocus (1/focal length).
but instead delta R = 2/(2/R + delta D) - R
Where R=36.013m is given in https://git.ligo.org/IFOsim/ligo-commissioning-modeling/-/blob/main/LHO/yaml/lho_O4.yaml?ref_type=heads
delta R comes out as 4.3mm +/- 0.18 mm (which is the same order of magnitude as the change Aidan measured in alog #27262 at LLO).
The error was estimated from looking at the noise on the spherical power and propagating through the calculation of delta R.
(CoreyG, MitchR, RandyT)
This morning, Randy watered down the sand roads. Later, Mitch & Randy swapped in the new (& better) rigging hardware for the Wind Fence on all the big poles.
This afternoon, 2 (of5) horizontal cables were installed at Location #4 (of 6).
And of course a new bee hive was observed. This one is up in the Wind Fence vicinity, and is forming on....a tumbleweed! Tyler was notified and he checked it out.
Next up is continuing to install horizontal cables at location #4, 5, & 6. Then panel install and securing panels.
Closes FAMIS26511, last checked in alog82660
The lack of switching recently is due to the vent, but they all show switches during the last quarter.
[Sheila, Elenna]
Alog 84230 contains an extensive report of the beam profile measurements in HAM1 along the REFL path. Keita did a fit of the measurements along the WFS sled to determine that the gouy phase separation of the REFL WFS is good. I have now taken all the data, starting just before RM1 through the WFS sled measurements and run a fit.
Looking back at T1300960, which does a similar fit model from the measurements in the REFL path, there is some confusion about what the input q to HAM1 is, and this resulted in some doubt about the radius of curvature of both RM1 and M5, whose design specs are 1.7 m. That code uses RoCs that are 1.75 m for each mirror, which Sheila and I think is a bit far out of the range of the specification (see E1100056).
There is a total of 8 measurements, four taken around the WFS sled and four taken around the RM1-RM2-M5 area (a ninth measurement of the beam size at the LSC REFL diodes is not included). I added these measurements to the model, as well as RM1, RM2, M5, L101 and L102. I ran a fit based on these components and the beam profile measurements.
The beam path results are shown in this first plot, where RM1 and M5 RoC are set to 1.7 m (as in spec). The astigmatism shows waists upstream of RM1 are separated by over 1 m. I color coded traces for horizontal and vertical, and o's and x's mark the measurement locations that were fit. However, I didn't include any angle of incidence in this calculation, which would probably adjust this result slightly (it appears the AOIs are probably 10 degrees or less). For completeness, I also included the results if we assume the RM1 and M5 RoC are 1.75 m, in this plot. In this result, the upstream waists are 2 m apart.
For both fits, I used the qs that Paul and Lisa calculated as the seed qs in T1300960. Sheila and I are in the process of confirming these qs by doing the beam propagation of the IMC waist to the HAM1 table. To clarify, a la mode forces you to supply some input seed beam for propagation and fitting, so I supplied this seed, since you want to use something you think is pretty close to the true value. However, it only uses that seed as a starting point and then fits the data points supplied. The resulting incoming beam to RM1 is fit as:
horizontal = waist 1.60 mm, 6.4 m upstream of RM1 (RM1 RoC 1.7 m)
vertical = waist 1.52 mm, 7.5 m upstream of RM1 (RM1 RoC 1.7 m)
or
horizontal = waist 1.99 mm, 2.07 m upstream of RM1 (RM1 RoC 1.75 m)
vertical = waist 2.06 mm, 4.2 m upstream of RM1 (RM1 RoC 1.75 m)
The code I wrote is attached to this alog. Below are tables of the beam profile measurements (copied from 84230), and the specs of the mirrors and lenses I used.
| Measurement location | Distance (relative to RM1), mm | wx [um] | wy [um] |
| before RM1 | -1162 | 4038.9/2 | 4206.2/2 |
| before RM1 | -314 | 3950.6/2 | 4315.0/2 |
| between RM1 and RM2 | 511 | 1650.9/2 | 1805.1/2 |
| after RM2 | 1377 | 2304.8/2 | 2335.9/2 |
| WFS A | 3460 + 94 | 670.26/2 | 778.95/2 |
| WFS B | 3460 + 466.5 | 793.73/2 | 711.29/2 |
| downstream of sled 1 | 3460 + 788.5 | 1484.15/2 | 1387.24/2 |
| downstream of sled 2 | 3460 + 1092.5 | 2253.78/2 | 2119.24/2 |
| Component | Location (relative to RM1), mm | Specification |
| RM1 | 0 | Rc= 1.7 m (1.75 m) |
| RM2 | 856 | Rc= -0.6 m |
| M5 | 1751 | Rc= 1.7 m (1.75 m) |
| L101 | 2977 | f = 333.6 mm |
| L102 | 3180 | f = -166.8 mm |
| Horizontal seed for starting point only | -1e-3 | q=2.8071 + 13.3724i |
| Vertical seed for starting point only | -1e-3 | q=2.5071 + 13.0988i |
FAMIS 26408 - PSL Weekly Check
Laser Status:
NPRO output power is 1.849W
AMP1 output power is 70.39W
AMP2 output power is 140.6W
NPRO watchdog is GREEN
AMP1 watchdog is GREEN
AMP2 watchdog is GREEN
PDWD watchdog is GREEN
PMC:
It has been locked 0 days, 2 hr 14 minutes
Reflected power = 23.66W
Transmitted power = 105.4W
PowerSum = 129.0W
FSS:
It has been locked for 0 days 0 hr and 3 min
TPD[V] = 0.7928V
ISS:
The diffracted power is around 3.4%
Last saturation event was 0 days 2 hours and 13 minutes ago
Possible Issues:
PMC reflected power is high
Fil, Rahul
This morning we finished ground loop checks on HAM1 chamber, since Jim was done with final cabling work. The only grounding issues we found were in RM1 and PM1, hence we removed pin1 from the in-air cable (connecting Satamps).
D0902810 aLIGO SUS HAM 1-2 System Wiring
T1200131 Grounding and Shielding at LIGO
D1900511 ISC/SQZ Wiring Diagram
The following were checked for ground loops:
To get a good chamber ground connection, testing was done at the feedthroughs. Normally done at the ISC racks. Shorts found on RM1, PM1, and both beam diverters.
With suspensions in safe mode, the termination shielding was repaired on the following PM1 cables:
F. Clara, R. Kumar
Thu May 15 10:11:20 2025 INFO: Fill completed in 11min 16secs
Dry air skid checks, water pump, kobelco, drying towers all nominal.
Dew point measurement at HAM1 -43.9 °C.
FAMIS - 26378 Checking HVAC Fans Vibrometers.
Fans dont look too bad aside from H0:VAC-MY_FAN_270_1_ACC_INCHSEC which seems to be a Noisier fan.
TITLE: 05/15 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: 12mph Gusts, 8mph 3min avg
Primary useism: 0.02 μm/s
Secondary useism: 0.08 μm/s
QUICK SUMMARY:
LVEA is LASER Safe. Hartman Lasers are on but are Eye safe and are ~780nm green/blue in color.
HAM1 ISI is currently unlocked.
Today's Agenda:
CS:
HAM1 optical Alignment checks
HAM1's Glamour shots.
HAM1 Ground Checks.
Cable Tray work.
GOUI phase measurements in the output arm
TCS work?
EX
More wind fence work.
EY
SEI BRS work.
Now that ISC is done with their alignment, I have been working on testing the ISI. Last night TJ and I unlocked and balanced the ISI, I did some quick tests to make sure the actuators were pushing where I expected them and found the horizontal and vertical actuator for each corner was swapped, so I switched the cables at the chamber. This morning I did some tests like range of motion and CPS linearity and some quick spectra to check that all of the sensors looked more or less the same and a quick set of tfs to look for rubbing. Now starting my long overnight tfs, so hopefully there are no big eqs overnight. If those go well, I hope to have everything for the testing report by the afternoon tomorrow.
Attached images are some of the tests I did today. First image is CPS linearity, which looks kind of ratty because I think the purge was too high, but otherwise looks okay. Second image shows unlocked asds for the CPS, GS13s and L4Cs. No glaring issues, but the kind of noisy V2 GS13 and CPS made me think some rubbing or high purge was happening. Last image is a set of tfs I used for chamber closeout comparing the measurements on HAM8 from last year to HAM1 today. Looks okay for a quick measurement.
L2L tfs look good. Still have some other information to collect.
My testing is done. Testing report is uploaded to E2500128. Payload was light by a lot during testing, it did not get better in chamber and there were a lot of beam dumps that got added that I don't have weights for, so the payload section of the report should be taken with a grain of salt.
Fil, TJ, Camilla. WP 12533
We turned back on the RH and SR3 heater chassis which were turned off for venting. After these were turned on, ITMX came back to it's nominal value of 0.44W/segment.
TJ and I played with the inverse RH filters for a while on ITMX (instructions 50777), turning ITMX up to 0.5W for a couple of hours, it doesn't really make sense to us what it was doing as it drops the power lower than the requested power which seems un-intuitive 68549. Now back at nominal 0.44W/segment with the RH inverse filter guardian back to NOMINAL (off).
ETMY had come back to the incorrect value after the April power outage (last saved Beckhoff value maybe), so TJ turned that back to the nominal 1.3W/segment on ETMY too.
TITLE: 05/14 Day Shift: 1430-2330 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Planned Engineering
INCOMING OPERATOR: None
SHIFT SUMMARY:
HAM1 Purge air has been turned Down.
HAM1 ISI is Currently Unlocked.
It got too windy to work on the Wind Fence while elevated at EX, so wind fence work was postponed.
SEI BRS team found a broken cable on the BRS System.
TCS team Turned on the Hartman Wave front lasers. These are Eye safe lasers that have a power output of less than a mW. So if you see a blue-green ~780nm beam it MAY be from that.
Bees are still at EX.
LOG:
| Start Time | System | Name | Location | Lazer_Haz | Task | Time End |
|---|---|---|---|---|---|---|
| 14:33 | FAC | Randy | EX | N | Wind fence work | 17:46 |
| 14:45 | FAC | Kim & Nellie | LVEA | N | Technical cleaning | 15:31 |
| 15:18 | SEI | Corey | EX | N | Wind fence work | 17:46 |
| 15:52 | EE | MARC | EE LAB | N | Control Room Quiet Time for TEST N EE Lab | 16:52 |
| 16:02 | Bees | Mitchel | EX | N | Moving a box of Bees | 17:47 |
| 16:09 | VAC | Jordan | LVEA | N | Purge Air checks. | 16:29 |
| 16:18 | sei | Jim | Remote | N | HAM1 SEI health checks STAY AWAY | 18:18 |
| 16:31 | PEM | Robert , Carlos, Keit | EX | N | Getting parts | 16:51 |
| 16:52 | FAC | Nellie | EY | N | Technical cleaning | 18:12 |
| 17:53 | SEI | Randy | EX | N | Getting Equipment. | 18:33 |
| 18:12 | FAC | Nellie | LVEA | N | Technical Cleaning | 19:10 |
| 19:11 | FAC | Nellie | EY | N | Dropping off supplies | 19:41 |
| 19:23 | TCS | Camilla | LVEA | No | Turning on an Eyesafe Hartman laser | 19:26 |
| 19:38 | SEI | Michael R & Shoshana | EY | N | Pumping Down BRS | 20:33 |
| 19:43 | TCS | Camilla | LVEA | N | Power cycling the Hartman cameras | 19:47 |
| 19:55 | SEI | Jim | LVEA Ham1 | N | Locking ISI & Adjust CPS | 21:14 |
| 20:09 | VAC | Jordan | LVEA | N | Looking for parts | 20:18 |
| 21:08 | VAC | Travis | MidY | N | Looking for Eye bolts | 21:20 |
| 21:13 | FCA | Mitchell & Randy | LVEA | n | Liberating totes from their resting place | 23:13 |
| 21:14 | SEI | Jim | LVEA | N | Turned down Purge air | 21:14 |
| 21:21 | VAC | Travis & Jordan | LVEA | N | Craning over the X arm | 21:49 |
| 21:42 | TSC | Camilla & TJ | CER | N | Turning on HighVoltage for the Ring Heaters. | 21:46 |
| 21:50 | Guard | TJ & Olli | Control rm | N | Testing new guardian code | 23:12 |
| 22:05 | SEI | Michael R & Shoshanna | EY | N | BRS Wiring | 22:40 |
| 23:18 | VAC | Janos | Mid X&Y | N | Cryo pump survey | 01:18 |
[Shoshana, Michael] We've started preparing to install the BRS mass adjuster to the End-Y BRS. The plan is to follow the same procedure/same parts as the End-X install outlined in LIGO-T2400043 and SEI log 1886 (https://alog.ligo-la.caltech.edu/SEI/index.php?callRep=1886). We've taken apart the BRS and discovered that doesn't match the designs on the DCC. How the parts are arranged blocks access to where the pico-motor mount should attach, but we think we have a work around that should work. The electronics/wiring of the BRS is as expected and we've finished all the wiring for the pico-motor so that it should attach to the feed through. Assuming all goes well we plan on installing the mass adjuster parts and begin testin.
[Shoshana, Michael] We've managed to get all of the hardware/parts installed in and we've closed up the BRS chamber. We had to add an inch of shims beneath to motor mount in order to get it to fit/align properly, but otherwise there were only minor complications during installation. We've tested the pico-motor and the mass adjuster using the pico-motor driver that we brought from UW and both seem to work fine. For in air balancing, we left the new mass adjuster centered to increase range for future adjustments for when the BRS is pumped down and running, and tried to just stick to moving masses that are inaccessible when the BRS chamber is pumped down. We unfortunately reached the maximum range with the internal masses and had to slightly move the manual mass adjustment system (what is currently used to adjust the center of mass) from center, but that might be returned to center after we re-balance it when it's pumped down. Right now the resonance frequency looks to be around ~7mHz (around 130 second period) which is about the same as it was before Mass Adjuster installation, but we'll check again after the chamber has been pumped down. Tomorrow we'll finish all of the wiring and electronics to hook up the pico-motor to the LIGO system. The plan is to pump down the BRS chamber tomorrow and re-balance and test the pico-motor some more. The reference pattern has a higher intensity than expected and we aren't sure why. Right now our best guess is that the light source drifted slightly, and we'll look into it more tomorrow.
EPO tag for BRS pics
[Shoshana, Michael] Pumped down the BRS chamber overnight and started the ion pump this morning and got it down to 1.9e-6 Torr before we left end End-X. We also wired up the picomotor to the LIGO picomotor controller system. It is hooked up to the 7th channel X-direction and we tested it out and were able to hear it spinning for both directions. The BRS's thermal insulation was reapplied the box closed and the temperature sensors and heating plate were all re-attached and plugged back in. The reference beam's intensity has gone down to be closer to normal somehow, so it doesn't seem to be anything to worry about We might go back to End-Y one more time tomorrow to clean up the wiring and do a final check of the vacuum pressure. We waited for the temperature to equilibrate a bit before balancing because we were hoping that as the temperature rises it would drift back to center, but we ended up using the mass adjuster to try and balance it. It looks like the + - wires for the damping were switched, meaning when the damping was on it would ring up the BRS. Fixed by changing a line in the BRS code[IF H1_ISI_GND_BRS_ETMY_CAPDRIVE>=0] by switching the [>=0] to [<=0] and switching [H1_ISI_GND_BRS_ETMY_CAPOUTL] and [H1_ISI_GND_BRS_ETMY_CAPOUTR], and [H1_ISI_GND_BRS_ETMY_RELAYL] and [H1_ISI_GND_BRS_ETMY_RELAYR] FROM THE END-X INSTALL: Coupling/decoupling move: 1.25k steps Maximum: +-140k steps Be careful: +-100k steps NOTE: MOVING PICOMOTOR +(POSITIVE) DIRECTION TRANSLATES TO MOVING THE BRS UP TOTAL MOVEMENT TODAY:+21k steps
Centered both ETMY and ETMX BRSs. For ETMX net movement was +2200 steps, for ETMY net movement was -3200 steps. For ETMX we saw that the DRIFTMON was moved by about ~3.27 counts per step, and ~2.3 counts per step for ETMY
Cleaned everything up for the ETMY BRS and relabeled all the wires. The final reading that we saw for the ion pump was 9.9e-7 Torr (186uA, 6950V) which seems about right. We left some extra mass adjuster parts with Jim just in case.
Shoshana, Michael
We took tilt subtraction spectra as a final life check of the BRSs. Both BRSs appear to be in good working order and doing their jobs well.