TITLE: 08/12 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: CALM
Wind: 2mph Gusts, 0mph 3min avg
Primary useism: 0.02 μm/s
Secondary useism: 0.06 μm/s
QUICK SUMMARY:
Went to EQ Mode twice overnight. On the docket for today: HAM7 close-out begins, Input Alignment work will continue, CDS w/ DAQ restarts in afternoon, HAM8 Annulus Ion Pump activity, & DOE tour in the afternoon.
We have calibrated the two JAC steering actuators the PZT (IO_MB_M4) and the JM1, in μrad per drive count at DC. The scale comes from the second harmonic of the cavity transmission under a dithered drive, which is insensitive to DC misalignment and so needs no external angle reference.
By expanding the injected field in the cavity's own eigenmode basis, we can describe the misaligned as,
Ein(t) = E0 + δ(t) E1
with E0 the cavity's TEM00 mode and E1 the TEM10 (pitch) or TEM01 (yaw) mode, orthonormal. As long as the misalignment is small enough comparing to the beam size, the single complex coefficient δ carries the whole misalignment on that axis: its real part is a transverse displacement in units of the waist size, its imaginary part an angle in units of the divergence angle. Only the TEM00 is resonant, so the transmitted power follows the fraction of the input that sits in E0, i.e. 1 − |δ|2 for |δ|2 « 1.
Dithering a steering actuator makes δ oscillate about whatever value it already had:
δ(t) = δofs + δa cos(2πft)
where δofs is the static misalignment already present, and δa is the dither we deliberately applied, which is exactly the quantity we want in order to calibrate the actuator. TRANS signal (1 − |δ|2) can devided into three components with its frequecies:
frequency |
value | contains the unknown δofs? |
|---|---|---|
| DC | |δofs|2 + |δa|2/2 |
yes |
f |
2 Re(δofs*δa) |
yes — magnitude and relative phase |
2f |
|δa|2/2 |
no |
The static offset drops out of the second harmonic algebraically. 2f therefore delivers |δa| with no reference to the alignment state we happened to be sitting at, and with no external angle standard. The DC and f terms, the two one would reach for first, are both contaminated by it.
This is the whole point of the method, and it is directly visible in the plot. adding a static offset grows the 1f line by +528 % while the 2f line moves by +8 %, its own measurement noise.
I proceeded 4+1 measurement in total with the JAC locked. For each measurement, one actuator axis was dithered at 11 Hz, with the excitation injected on the channels below and the drive read back on the corresponding _OUT. I excited JM1/PZT PIT/YAW per one measurement, and the other one is the PZT_PIT excitation with static offset (30 cnts) to demonstrate that the 2f peak is not affected by the offset. Transmission was read on H1:JAC-TRANS_A_LF_OUT.
| record | excitation channel | drive read back on | amplitude at 11 Hz [cnt] | drive offset [cnt] | TRANS DC [cnt] |
|---|---|---|---|---|---|
PZT_PIT |
H1:JAC-PZT_PIT_EXC |
H1:JAC-PZT_PIT_OUT |
20.0 | 0 | 6451.2 |
PZT_PIT_ofs |
H1:JAC-PZT_PIT_EXC |
H1:JAC-PZT_PIT_OUT |
20.0 | 30 | 6442.5 |
PZT_YAW |
H1:JAC-PZT_YAW_EXC |
H1:JAC-PZT_YAW_OUT |
20.0 | 0 | 6442.6 |
JM1_PIT |
H1:SUS-JM1_M1_TEST_P_EXC |
H1:SUS-JM1_M1_TEST_P_OUT |
40.0 | 0 | 6445.5 |
JM1_YAW |
H1:SUS-JM1_M1_TEST_Y_EXC |
H1:SUS-JM1_M1_TEST_Y_OUT |
40.0 | 0 | 6440.2 |
|δa| is calculated from peak heights of the transmission at 22 Hz, converted to a mirror tilt using the local beam radius at each actuator from the current JAC reflected-path layout model (alog91472 comment), and calibrated into DC responce using each actuator's frequency response as measured (described below).
| actuator | axis | excitation channel | |δa|2 |
efficiency [μrad/cnt] | |
|---|---|---|---|---|---|
| at 11 Hz (as measured) | at DC | ||||
| PZT | PIT | JAC-PZT_PIT_EXC |
1.09e-5 | 0.0093 | 0.083 |
| PZT | YAW | JAC-PZT_YAW_EXC |
6.47e-6 | 0.0093 | 0.079 |
| JM1 | PIT | SUS-JM1_M1_TEST_P_EXC |
1.01e-5 | 0.0216 | 0.89 |
| JM1 | YAW | SUS-JM1_M1_TEST_Y_EXC |
1.67e-5 | 0.0254 | 0.92 |
The 11 Hz column is what the dither actually produced; the DC column is that value divided by the actuator's own response at 11 Hz, and is the number to use for a DC gain.
The frequency response itself comes from a separate set of four broadband actuator-to-wavefront-sensor records (300 s each, one actuator per record, see atatched plots), from which the JM1 suspension resonance and the PZT drive pole are fitted. Only the shape of those transfer functions is used; their absolute scale plays no role in the calibration.
The fitted frequency responses are:
f0 = 2.00 Hz, Q = 7.7 (PIT) and 1.80 Hz, Q = 5.4 (YAW)fp = 1.24 Hz (PIT) and 1.30 Hz (YAW)AOI compensation
Both actuators sit at a design AOI of 45°, and the rows above include the geometric correction that follows. A tilt whose rotation axis lies in the mirror surface and in the plane of incidence steers the beam by only 2θ cos(AOI), against the full 2θ for the axis perpendicular to that plane. At the PZT the suppressed axis is YAW in the cavity-referred channel naming (the HAM1 periscope exchanges the transverse planes downstream of it); JM1 sits after that periscope, so for it the suppressed axis is PIT. The assignments follow from each mirror's orientation, and the correction uses the design 45° rather than a value fitted to the measured ratio.
APZT = 500 μrad/V (T1500342) driven through an 18-bit DAC (±10 V differential, i.e. 20 V over 217 counts) and a differential-to-single-ended board (D1100457 v2, unity gain, read off its schematic), giving 0.076 μrad/cnt. No further driver gain applies on top, since the T1500342 figure is referenced at the controller's control input. Our result sits at 1.09× (PIT) and 1.04× (YAW) of this designed value.FAMIS 63911
PMC REFL has been rising very slightly, but otherwise, no major events of note.
(Travis S., Gerardo M.)
Around 11:00 am today we opened GV8 from soft close to allow for commissioners to peek down x-arm. The gate annulus for GV8 was burped into the annulus ion pump, almost no response. The 4 turbo pumps were isolated from the main vacuum envelope, the 4 large ion pumps are valved in, along with HAM6 ion pump (500 l/s), and we still have a filter cavity section valved into the main corner volume, the section from FCV-3 to FCV-4, and includes ion pump B-1 (150 l/s).
GV8 remained open for about 5 1/2 hours.
We closed GV8 around 16:30 local time.
Attached is a pressure response from gauges along the X-arm at the corner station.
TITLE: 08/11 Day Shift: 1430-2330 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Planned Engineering
INCOMING OPERATOR: Ryan S
SHIFT SUMMARY: GV8 was opened and closed today for Xarm alignment commissioning, ZM4 PSAMs adjustment was finished up. We had a small power glitch in the afternoon that tripped off the end station HEPIs.
LOG:
| Start Time | System | Name | Location | Lazer_Haz | Task | Time End |
|---|---|---|---|---|---|---|
| 14:33 | FAC | Kim | LVEA | Y' | Tech clean | 15:11 |
| 14:59 | FAC | Chris | LVEA | Y | FAMIS checks | 15:26 |
| 15:26 | FAC | Chris | All Out BLDs | N | FAMIS checks around site | 17:44 |
| 16:09 | SEI | Carlos | LVEA | Y | Seismometer checks | 16:55 |
| 16:16 | SEI | Jim | LVEA | Y | SPI checks | 16:28 |
| 16:37 | OPS | RyanC | LVEA | Y -> N | LASER hazard transition, hazard to safe | 16:47 |
| 16:48 | EE | Fil | LVEA | N | Check JAC shutter connections | 16:52 |
| 16:48 | EPO | Jenne | LVEA | N | Tour | 17:30 |
| 16:52 | EPO | Camilla | LVEA | N | Tour | 17:25 |
| 16:54 | SQZ | Rahul, RyanS | LVEA | Y/N | HAM7 work, bifurcated laser hazard area | 18:15 |
| 17:21 | EPO | Corey | LVEA | N | Tour, in @ 12:00 | 17:34 |
| 17:46 | OPS | RyanC | LVEA | N -> Y | Laser hazard transition, safe bifurcated to hazard | 17:58 |
| 17:48 | VAC | Gerardo, Travis | LVEA | YES | Opening GV8 (XARM) | 18:13 |
| 18:07 | PEM | Michael, Shoshana, Huyen | LVEA | Y | NRS hardware under ITMY, Huyen out 18:21 | 19:45 |
| 18:22 | ALS | Jennie, Masayuki | LVEA | Y | ISCT1 table checks | 18:45 |
| 18:29 | SEI | Jim | CER | Y | Quick check SPI, CER maybe LVEA | 18:32 |
| 19:12 | ALS | Sheila, Masayuki | LVEA | Y | ISCT1 alignment checks | 19:26 |
| 19:15 | ISC | Betsy | LVEA | Y | Checks | 19:22 |
| 19:29 | CDS | Dave | CER | Y | Accelerometer checks | 00:28 |
| 19:43 | CDS/SAF | Patrick | MSR | N | Beckhoff safety computer investigation | 20:03 |
| 20:01 | FAC | Randy | LVEA | Y | Clean room checks | 20:58 |
| 20:02 | EE | Fil, Jackie | EndX | N | Reset VFD and remove analog cameras | 21:07 |
| 20:02 | SEI | Jim | EndX | N | Reset VFD recover HEPI | 20:33 |
| 20:03 | SQZ | RyanS | LVEA | Y | Beam profiles at HAM7 | 21:50 |
| 20:23 | SQZ | Rahul | LVEA | Y | HAM7 work, ZM4 | 21:23 |
| 20:59 | FAC | Randy | EndY then X | N | Clean room checks | 21:59 |
| 21:08 | EE | Fil, Jackie | EndY | N | Remove analog cameras | 21:39 |
| 21:25 | ALS | Sheila, Camilla | LVEA | Y | ISCT1 beatnote adjustment | 22:01 |
| 21:21 | SEI | Jim, Huyen | FCES | N | CPS checks/tests | 21:45 |
| 21:37 | SAF | Richard | Mechanical | N | HEPI pump checks | 21:50 |
| 21:39 | EE | Fil, Jackie | CER | Y | Remove analog camera electronics | 23:21 |
| 22:11 | PEM | Shoshana, Huyen | LVEA | Y | CRS laser | 22:24 |
| 22:19 | ISC | Sheila, Masayuki | LVEA | Y | ISCT1 alignment checks | 23:00 |
| 22:58 | SEI | Michael, Jim | LVEA | Y | Wiggle SPI cable, look at other cabling at TCS rack | 23:58 |
| 23:10 | VAC | Gerardo | LVEA | Y | Close GV8 | 00:28 |
| 23:22 | EE | Fil, Jackie | MSR | N | Remove analog camera electronics | 00:22 |
The gate phone microphone doesn't seem to be working well, one instance I heard nothing after answering, the next was garbled and full of static.
Camilla, Oli, Caroline, Masayuki, Sheila
R. Kumar, S. Dwyer, C. Compton, R. Short
Following the work done yesterday adjusting the preload on the ZM4 PSAMs (alog91471), Rahul and I set about adjusting it further today to get our calculated projected beam size on SRM close to where we want it. Using the same procedure as yesterday, I turned off the ZM4/5 PSAM drive chassis, Rahul went into HAM7, locked down ZM4, torqued the preload about 1/8" of a turn (it's hard to quantify a torque spec in this manner), then finally unlocked the suspension. I moved the ZM4 pitch alignment slider about -1400 counts to realign the beam on SQZT7 to our alignment irises as a result of this torque adjustment. I then proceeded to take a couple of beam profiles on the table with the M^2 device to see where we landed. This plot [initial] shows the difference between before and after this adjustment in terms of the projected beam at SRM with a few different PSAM settings on ZM4 and ZM5. The four points I took here informed us that we could stand to torque ZM4 a bit further to hopefully line up with the center of the plot.
Rahul went back into HAM7 and torqued another 1/8" and I took another couple of profiles after (I did not need to move ZM4's alignment sliders after this adjustment). I took a total of nine profile points here, all of which can be seen compared to other measurements today on this plot [full]. Since there are points in the bullseye, we decided to stop here and that this is where the ZM4 preloading will stay. This plot [final] shows just the beam profiles taken at our final preloading position.
Tomorrow we will move on to final closeout checks in HAM7.
I ran a health check TF on ZM4 and it looks good.
2026-08-11_2200_H1SUSZM4_M1_WhiteNoise_L_0p02to50Hz.xml
2026-08-11_2200_H1SUSZM4_M1_WhiteNoise_P_0p02to50Hz.xml
2026-08-11_2200_H1SUSZM4_M1_WhiteNoise_Y_0p02to50Hz.xml
Jennie W, Sina K, Jim W,
Summary: Yesterday we had a check through the SPI model just to make sure we have turned on everything and that all is working well, we got as far as ascertaining that no light was making it to the PDs on the ISIJ and K benches and also did some other checks on the LO aand longitudinal IFO paths.
Couple of things we discovered/checked:
NB: We found out today that the shutter controller for our laser pick-off was not connected - Jim and Fil have now solved this (alog #91467).
TITLE: 08/11 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: CALM
Wind: 9mph Gusts, 4mph 3min avg
Primary useism: 0.01 μm/s
Secondary useism: 0.06 μm/s
QUICK SUMMARY:
The M2 stage of the BS has been moving a lot since yesterday afternoon ~21:17 UTC, the oplev damping has grown with it.
The BS oplev damping was turned back on by me inadvertently yesterday. The OLDAMP Gain increases happened right as I requested DOWN from the ISC_DRMI guardian. Masayuki and I did notice additional motion on the BS yesterday but we didn't know at the time whether it was due something we did or from something someone else was doing. Now, looking at the timing of the grd state request and confirming by looking at ISC_DRMI.py, I can say that the BS oplev damping was 1.) turned on by accident and 2.) can be / should be turned back off.
I tried to SDF the oplev damping off, see 91267, but I never checked what the guardians do. I recommend we change the guardian code to not engage oplev damping until we can diagnose why it isn't working, specifically, saturating the suspension.
Workstations were updated and rebooted. This was an OS packages update. Conda packages were not updated.
Rahul, Ryan, Sheila
Today we think that we found a rapid way to iterate the psams preloading, and we made a couple of changes for ZM4.
Frst Ryan and I measured the beam profile with ZM5 psams servo set to -8V, and ZM4 psams PZT votlage at 0V,
Rahul can add the details of how he did this, but he added about 1/8 turn of torque to the ZM4 psams. We then turned the laser back on, and took a beam profile measurement. Unfortunately the profiler software got into a strange state where the beam waist seemed to be at a very different position and it would not calculate the original beam parameters. We thought this was because the beam profile had changed dramatically, and Rahul backed off the preload by 1/8 of a turn. As we were remeasuring the profile Ryan S noticed that the range of the translation stage displayed on the screen went only from 0-100mm, while it normally goes from 0-200mm. The software would not allow Ryan to reset the measurement range parameter, until we powered the profiler off, exited the software, and started both up again.
After this, we saw that indeed we had a reasonable q measurement, although not really an improved mode matching. It does seem promising to adjust ZM4 this way, as each iteration took about 30 minutes including our confusion about the beam profiler.
S. Dwyer, J. Oberling, L. Dartez This afternoon we went to ISCT1 to align the green beam from the PSL Green PD, and ALS COMM PD. This is pre-peek prep so that by the time the peek takes place we don't need to worry about the beam alignment from the PSL. We struggled a little bit to find an alignment that agreed with the crystal and the downstream PDs. We were able to get a beam onto the COMM PD. Sheila thinks that what we set up so far is more than enough to get a beatnote during the arm peek. We aligned the green beam onto the green PD but for some reason couldn't get see a readout signal that corroborated that the beam had made it onto the diode. We tried doing some troubleshooting, which included a local cable swap and adjusting the PD placement on the table. Neither were successful and, given the time of day, we opted to revisit at a later time. The important part thing is that the COMM PD _was_ seeing the beam.
Jennie and I were looking at the SPI with Sina during a call today and Sina pointed out there was no power on the first PDs on the SPI breadboard. She said there was a witness pd in there SPI laser chassis that could be checked with a multimeter next to the chamber, so I went and checked that this afternoon. I'm not totally sure what all of the labels meant, but I think there is no laser light on the pd in the interface chassis. The SPI_LP_M1_PD was at 0v, the other two, SPI_LPMON_M2_RFMEAS and SPI_LPMON_M3_RFREF were at ~.8v regardless of the state of the CDS control of the SPI pick off shutter, which I had Ryan toggling remotely. We've talked to Ryan and Jason about going into the PSL tomorrow to check the function of the SPI pick off shutter, I think we will also try to check the output of the fiber at the chassis with a laser card at least. Not sure how hard it would be to look with a power meter.
Cable at shutter controller on IOT1L was not connected. DB9 was connected to ouput CH2.
Jennie Wright, Masayuki Nakano, Khanh Vu This morning we worked on several tasks on the IOT1 table, including installing the camera and shutter, profiling the beam, and calibrating the DC power. We identified a new location for the camera using the beam transmitted through JACR_M5. During this process, Masayuki noticed that the beam was being clipped by the shutter. We suspect that the beam may have been clipped for some time. We then installed the camera in its new location, and Masayuki aligned the shutter on the table. Next, we profiled the beam for the wavefront sensors. We found that the Gouy phase separation between the two WFSs is approximately 70 degrees. We decided to leave the current configuration as it is since the separation is good enough. Masayuki will make a plot and perform a more detailed calculation later. We also maximized the laser power in the REFL path by optimizing the waveplate angle. When JAC is unlocked, the measured power on the RFPD is 5.1 mW, and the trigger PD voltage is 0.28 V. When JAC is locked, the measured power decreases to 0.4 mW, and the trigger PD voltage is 0.02 V. Since the beam is split evenly, each WFS receives approximately 2.55 mW of optical power. Finally, we calibrated the DC readout of RFPD by converting counts to mW. Before performing the calibration, Masayuki checked the alignment and recentered the RFPD. He then recorded two sets of measurements, each averaged over 10 seconds: Measurement #1 * JAC_REFL_A_LF_INMON: 1072.3966186523437 counts * DC power: 4.4 mW Measurement #2 * JAC_REFL_A_LF_INMON: 1073.5228637 counts * DC power: 4.5 mW After the calibration, we updated filter number 10 with the new coefficients.
The beam profile between the beamsplitter and the JAC WFS was measured. Here I fit a Gaussian beam to those measured beam sizes and convert the WFS locations into Gouy phase.
The measured beam diameters were fit independently in x and y with the standard Gaussian beam model, w(z) = w0 * sqrt(1 + ((z - z0)/zR)^2) with zR = pi * w0^2 / lambda and lambda = 1064 nm:
| w0 [um] | z0 [m from JACR_BS4] | zR [cm] | |
|---|---|---|---|
| x | 141.2 | 0.377 | 5.89 |
| y | 151.9 | 0.370 | 6.81 |
The beam is slightly astigmatic, so x and y are treated separately throughout.
The positions of WFS A and WFS B were measured with a ruler from the same reference as the profile scan: WFS A at z = 0.325 m, WFS B at z = 0.410 m. The corresponding Gouy phases, psi(z) = arctan((z - z0)/zR), are:
| WFS A [deg] | WFS B [deg] | Separation [deg] | |
|---|---|---|---|
| x | -41.3 | +29.5 | 70.8 |
| y | -33.5 | +30.4 | 63.9 |
The separation is 71 deg in x and 64 deg in y, not the optimal 90 deg. This is not optimal, but it is not terrible either: the two WFS remain well separated in Gouy phase and the sensing matrix would not be close to degenerate. Given the time available we did not optimize the layout.
If we want to optimize it later, the fix is straightforward: moving WFS A upstream (toward the BS) by about 5 cm in x / 7 cm in y, i.e. from z = 0.325 m to roughly z = 0.27 m, brings the separation to 90 deg. WFS B does not need to move.
Additional context for the work described above: The motivation for the table work came from the difficulties we had with the sensing and input matrices of the JAC ASC loops. In pitch, the PZT and JM1 signals are well separated, but their responses in yaw are too similar. This is problematic because we need the two wavefront sensors to distinguish between the motions of the two actuators. While identifying a new location for the camera, Masayuki noticed that the shutter was clipping approximately half of the beam on the left side. We suspect that the beam may have been clipped for some time and that this may be related to the yaw issue, since the clipping affects yaw more strongly than pitch.
Today we installed the iris to block the ghost beam on the JAC REFL path with an iris, and to re-measure the beam profile with it in place. The ghost beam was produced by the laser window which picks off the partial power of the JAC reflection beam (~0.4%). Since this laser window doesn't have the wedge on it, the AR reflection is not well separated. We observed this interference during the original beam profile measurement in this thread.
And now, the iris dumps the ghost beam, and we made a new the beam profile measurement. I made a good JAC REFL optical model which obtained by the fitting the beam profile measurement. We will use this model for the WFS signal calibration.
An iris was placed on the REFL path, between the first pick-off mirror and the first lens. To position it, the beam profiler was set just after the beam shutter, and the iris was closed while watching the profile, until the ghost was blocked and the main beam was left untouched. Actually, Since the ghost beam is very close, the main beam is partially blocked as shown in the attached pics. We will see if it would have any effect on our WFS signals.
1/e2 diameters along the REFL path, with JACR_MB4 as the origin:
| z [inch from JACR_MB4] | -21 | 3.5 | 5.5 | 7.5 | 9.5 | 11.5 |
|---|---|---|---|---|---|---|
| horizontal [μm] | 4440 | 1360 | 1140 | 895 | 696 | 500 |
| vertical [μm] | 4540 | 1360 | 1111 | 873 | 661 | 461 |
On-table distances were also measured: JACR_L1 to JACR_MB4 = 24", JACR_MB4 to WFS A = 12.5", JACR_MB4 to WFS B = 15.5".
I made a model of the beam propagation of the JAC REFL path from PSL to JAC and IOT1. This model was fitted to the new profile, with the PMC waist as origin.
Taken as known. The positions of lenses in PSL (IO_MB_L1/L2/L3) and of the JAC waist are the design values, i.e. the PSL bench to HAM1 relative distance is trusted.
Taken as unknown. The design placed the IOT1 table only loosely, and the periscope that matches the HAM1 beam height to the table height was estimated roughly. The distance from the JAC input to the IOT1 table is therefore the principal free parameter, allowed ±30 cm; it enters the calculation as the position of JACR_L1 measured from the PMC waist. The profile measurement was referenced to JACR_MB4, which carries its own error, so the JACR_MB4-JACR_L1 distance is a second free parameter.
The profile carries astigmatism, so a yaw tilt was allowed on each of the four lenses (three on the PSL bench, one on IOT1). This is deliberately over-parameterised: the individual tilts should not be read as physical alignment errors. However, the aim of this analysis is not to measure how each lens sits but a model accurate enough for the following calculation. So as long as the aquired prameters are physically reasonable, we can use these numbers as the following calculations.
One note:
The HAM1 periscope (JAC_M1/JAC_M2) rotates the beam 90 degrees about its axis, so the transverse planes swap on the way to JAC: bench x (YAW) descends from the upstream sagittal channel and bench y (PIT) from the tangential one. A tilt therefore gives astigmatism of opposite sign depending on which side of the periscope the lens sits. This is the reason why the x/y beam size flipped at periscope in the attached plot.
| parameter | fitted | vs design |
|---|---|---|
| JACR_L1 position from PMC waist | 11.4768 m | -21.5 cm |
| JACR_MB4 to JACR_L1 | 0.6004 m | -0.36" |
| yaw tilt, IO_MB_L1 / L2 / L3 | -16.9° / -7.1° / -1.8° | - |
| yaw tilt, JACR_L1 | -3.2° | - |
The fitted path from the JAC input to the IOT1 table comes out about 21.5 cm shorter than design, which is the scale of looseness that was expected there.
Astigmatism at the WFS planes
Expressed as the difference in accumulated Gouy phase between the two transverse axes:
| model | from the measured profile alone | |
|---|---|---|
| WFS A | -4.10° | -4.96° |
| WFS B | -10.61° | -10.32° |
Taking the cavity eigenmode as the reference, the fitted injection-lens tilts imply a mismatch of 0.48 % (tangential) and 0.43 % (sagittal), 0.91 % combined. Small enough not to conflict with the measured mode matching (~1%).
PMC eigen mode
| axis | w0 [μm] | zR [mm] |
|---|---|---|
| tangential (u) | 546.312 | 881.232 |
| sagittal (v) | 549.028 | 890.016 |
The waist sits at z = 0 in both axes. Downstream of the periscope the tangential channel becomes bench y (PIT) and the sagittal channel bench x (YAW).
z is given from the PMC waist (the model's own origin) and from JACR_MB4 (the origin the bench profile was measured against).
| element | z from PMC waist [m] | yaw tilt [deg] | source |
|---|---|---|---|
| PMC waist | 0.000000 | - | origin |
| IO_MB_L1 | 0.900000 | -16.86 | design / tilt fitted |
| IO_MB_L2 | 0.960000 | -7.12 | design / tilt fitted |
| IO_MB_M4 (PZT) | 2.812000 | - | design |
| IO_MB_L3 | 2.900000 | -1.75 | design / tilt fitted |
| HAM1 periscope (JAC_M2) | 7.040000 | - | design; x/y swap |
| JM1 | 7.268000 | - | design |
| JAC input mirror | 7.576000 | - | design |
| JAC waist | 7.826000 | - | design |
| JACR_L1 | 11.476799 | -3.15 | fitted |
| JACR_MB4 | 12.077174 | - | fitted (via JACR_L1 distance) |
| WFS A | 12.394674 | - | measured from JACR_MB4 |
| WFS B | 12.470874 | - | measured from JACR_MB4 |
| parameter | fitted value | design | allowed range |
|---|---|---|---|
| JACR_L1 from PMC waist | 11.476799 m | 11.691967 m | ±30 cm |
| JACR_L1 to JACR_MB4 | 0.600375 m | 0.609600 m | ±1" |
| yaw tilt, IO_MB_L1 | -16.8588° | 0 | ±20° |
| yaw tilt, IO_MB_L2 | -7.1210° | 0 | ±20° |
| yaw tilt, IO_MB_L3 | -1.7534° | 0 | ±20° |
| yaw tilt, JACR_L1 | -3.1527° | 0 | ±20° |
Keita, Sheila, Tony, Jennie W
Before the JAC PZT problem, I did get an hour or so of alignment time in. Summary: we now have light on LSC POP and POP X for the same PM1 alignment, and ITMX is back to the alignment that should point down the arm. We have the expected power in LSC POP path, but a factor of 20 too small in both DC and RF signals in the popair path.
These screenshots show MICH fringes with 10W input power, where I started and where I ended. The idea was to move to the ITMX alignment that Jenne Driggers found using the arm beam here: 89738. I watched the mich fringes and AS camera while moving the ITM, moved the beam splitter to keep the michelson fringes, and as Keita suggested moved PR3 to keep the beams on the ISCT1 refl camera. This did cause the michelson fringes on the LSC pop diode to get smaller, when that happened I paused, went to the PR2 spot move guardian state, and adjusted PR3 to bring the fringes back on LSC POP. After bringing the ITMX yaw alignment back I could see that there is now light on POPX and LSC POP A for the same PM1 alignment.
When I walked ITMX pitch, I had to also adjust yaw several times as I went along to keep the mich fringes. I also adjusted PRM to keep PRX alignment good as I moved along. Looking at this screenshot of the brief time when PRMI was flashing, the POP A LF flash was about the O4 power level (91211), as was reflair A, but popair has too little power. The result of this was that PR3 started the day 56urad away from the O4 slider, but is not -15urad. PR3 yaw started the day close to the O4 slider but is now -47urad.
I also adjusted the POP X dark offsets so that this QPD will be less confusing to read, SDF screenshot attached.
We tried walking PR3 in PR2 spot move to allow us to centering POP X without saturating PM1, this alignment is shown in this screenshot, but when we then aligned PM1 to put the beam on LSC POP, we were missing power there.
| POP A LF | POPAIR B LF | REFLAIR A LF | MICH IN1 (REFLAIR A 45 Q) | PRCL IN1 (REFLAIR A 9I) | POPAIR B RF18 | POP X NSUM | |
| PRMI O4 | 200-400 | 200 | 2-10 | +/-6000 | +/-600 | 80-100 | |
| PRMI yesterday | 100 | 6 (10 today) | 2.5-4 | +/-20 | +/-100 | 5 | |
| PRX O4 | 0.5 | ||||||
| PRX now | 0.5 | ||||||
|
MICH dark O4 1468885440 |
7 | 1 | 0.01 | -0.5 (dark level -0.6) | |||
| MICH dark PM1 -265 P -2364 Y) | 0 | 1 | 0.01 | 3.1 (centered) | |||
| MICH dark PM1 0,0 | 4 | 1 | 0.01 | 0.2 (P and Y both close to -1) |
The MICH dark time that I labeled as O4 above was actually from July, a better time to use for O4 (chosen from a list that Tony generated of MICH dark times) would be 1457969940 which is May 28 2025 00:15:42 UTC.