With Yokozawa-san
We performed the initial alignment for Xarm, Yarm, OMC and PRMI.
With Yokozawa-san
We performed the initial alignment for Xarm, Yarm, OMC and PRMI.
[Smith, Hirose, Saito]
The optic that was identified as a BS in the previous experiment (klog:37052) was replaced with a mirror. In addition, while attempting to correct beam clipping on the edge of a mirror, it was found that the beam was not passing through the center of the 150 mm focal-length lens. Since the beam was laterally displaced, an attempt was made to move the lens sideways. However, due to the mounting configuration, the lens could not be translated laterally. Modifying the mount to allow lateral adjustment would likely cause interference with a nearby mirror and shift the lens from its original position. Therefore, it will be necessary to move the mirror instead. Furthermore, because two lenses were removed during the alignment procedure, mode matching must be redone. In addition, the short distance between the 150 mm focal-length lens and the nearby mirror, as well as the difficulty of adjusting the mirror near the lens, have led us to consider redesigning the optical layout.
To align the Aux. beam axis with SRC axis more precisely, we would like to use the flash transmitted from SRC. We estimated the flash power on AS PD when 1W Aux. input power was injected from the SR2 AR side. The power just after trasmitting SRM seems to be ~65 uW and this beam is transmitted to AS port via OSTM (T = 3%). Then, the estimated power on AS DC PD is ~2 uW. Therefore, it maybe too low to obtain the flash with AS PD.
So we put new DC PD (Thorlabs, PDA100A2) in OMC REFL path for monitoring the flash instead of AS PD. The channel for OMC REFL DC is already existed (maybe it was used previously but now it is not used.). So I connected the new DC PD to the channel (K1:OMC-REFL_DC). I confirmed the PD response with DGS.
However, the alignment work on POS table seems not to be completed (Maybe Saito-kun reported detail later). So I put the beam dumper in front of the PD and blocked the beam by the dumper for now.
1. For the single-bounce configuration, the following suspension states were requested:
PRM: MISALIGNED_BF
ITMX: MISALIGNED_BF
ETMY: MISALIGNED
SRM: MISALIGNED
All others: LOCK_ACQUISITION
2. In the case of locking with 7.8 mW and 16.2 mW on DC PD B, OMMT2 and OSTM were actively controlled to optimize their alignment using the in-vacuum OMC QPDs, whereas no alignment control was applied during locking with 1.6 mW.
This is because the alignment control using the in-vacuum OMC QPDs did not work well due to the very low power on the OMC QPDs; however, this is expected to have little impact on the results.
1. For the single-bounce configuration, the following suspension states were requested:
PRM: MISALIGNED_BF
ITMX: MISALIGNED_BF
ETMY: MISALIGNED
SRM: MISALIGNED
All others: LOCK_ACQUISITION
2. In the case of locking with 7.8 mW and 16.2 mW on DC PD B, OMMT2 and OSTM were actively controlled to optimize their alignment using the in-vacuum OMC QPDs, whereas no alignment control was applied during locking with 1.6 mW.
This is because the alignment control using the in-vacuum OMC QPDs did not work well due to the very low power on the OMC QPDs; however, this is expected to have little impact on the results.
After the calibration work, we moved the RxPD back to its nominal position and found that its output had changed from the pre-work value. We investigated the cause and found that the alignment between the integrating sphere and the plate underneath it had slightly shifted. We realigned the integrating sphere with the plate, and the RxPD output returned almost to its original value.
[Tanaka, Hirose, Saito]
A 10 dB attenuator was added, reducing the beat signal level from 23 dBm to 10 dBm. The open-loop transfer function of the PLL was then measured. The results suggest that the sub-laser PZT responds with a frequency change to the frequency-difference signal from the PFD, rather than responding with a frequency change to a phase-difference signal. In addition, the alignment of the sub-laser beam incident on SRY was performed using two irises. The sub-laser PZT was then driven, but no flashes were observed at the AS port. This is likely because one of the optics expected to be a mirror was actually a BS, the beam was clipping on the edge of a mirror, and the observation was being made at the AS port. In the next experiment, the BS will be replaced with a mirror, the alignment will be redone, and a PD will be installed at the OMC reflection port to observe the flashes.
Next, the mirrors were adjusted so that the main laser beam followed the optical path intended for the sub-laser beam entering the interferometer. Two irises were then installed along this path and aligned to the main laser beam. The sub-laser alignment was subsequently adjusted so that it also passed through the two irises. The main laser was then blocked, leaving only the sub-laser beam incident on SRY. The sub-laser PZT was driven with a triangular waveform generated by the Moku:Lab function generator, and the AS port was monitored for flashes. However, no flashes were observed. This is likely because the optical power incident on SRY was too low. The laser powers measured at Spots 1~5 in Photo 2 were as follows:
Spot 1: approximately 130 mW
Spot 2: approximately 390 mW
Spot 3: approximately 780 mW
Spot 4: approximately 1.0 W
Spot 5: approximately 1.1 W
From these measurements, the laser power incident on SRY is estimated to be approximately 130 mW, which corresponds to only about 0.25 μW at the AS port. Such a small signal is likely buried in noise. The reduction in laser power between Spot 2 and Spot 1 occurred because the optic between them was a BS rather than a mirror. In addition, the reduction in power between Spot 4 and Spot 3 may be due to the beam clipping on the edge of the mirror.
Therefore, in the next experiment, the BS between Spot 2 and Spot 1 will be replaced with a mirror, and the alignment will be adjusted so that the beam does not clip on the edge of the mirror between Spot 4 and Spot 3. However, even after these modifications, the power at the AS port is expected to increase only to approximately 0.97 μW. Therefore, a PD will be installed at the OMC reflection port, and flashes will be monitored there instead.
Workers: Dan Chen, Jiahui Xiong, Misato Onishi
We performed monthly Pcal-X calibration on 2026/06/09.
After the calibration, we updated EPICS parameters related to the Pcal-X system. No issues were found.
| EPICS Key | Before | After | Δ (After − Before) |
|---|---|---|---|
| K1:CAL-PCAL_EX_1_OE_R_SET | 0.98353 | 0.98379 | 0.00027 |
| K1:CAL-PCAL_EX_1_OE_T_SET | 0.98353 | 0.98379 | 0.00027 |
| K1:CAL-PCAL_EX_1_PD_BG_RX_V_SET | -0.00390 | -0.00384 | 0.00006 |
| K1:CAL-PCAL_EX_1_PD_BG_TX_V_SET | 0.00483 | 0.00477 | -0.00006 |
| K1:CAL-PCAL_EX_1_RX_V_R_SET | 0.50217 | 0.50205 | -0.00012 |
| K1:CAL-PCAL_EX_2_INJ_V_GAIN | 0.95152 | 0.95265 | 0.00113 |
| K1:CAL-PCAL_EX_2_OE_R_SET | 0.97404 | 0.97473 | 0.00069 |
| K1:CAL-PCAL_EX_2_OE_T_SET | 0.97404 | 0.97473 | 0.00069 |
| K1:CAL-PCAL_EX_2_PD_BG_TX_V_SET | 0.00389 | 0.00389 | 0.00000 |
| K1:CAL-PCAL_EX_2_RX_V_R_SET | 0.49783 | 0.49795 | 0.00012 |
| K1:CAL-PCAL_EX_WSK_PER_RX_SET | 1.49025 | 1.49085 | 0.00060 |
| K1:CAL-PCAL_EX_WSK_PER_TX1_SET | 0.52750 | 0.52749 | -0.00001 |
| K1:CAL-PCAL_EX_WSK_PER_TX2_SET | 0.38816 | 0.38837 | 0.00021 |
After the calibration work, we moved the RxPD back to its nominal position and found that its output had changed from the pre-work value. We investigated the cause and found that the alignment between the integrating sphere and the plate underneath it had slightly shifted. We realigned the integrating sphere with the plate, and the RxPD output returned almost to its original value.
A CAL Tcam session was performed to obtain beam position information necessary for Pcal. The parameters have already been updated, and SDF has been accepted.
Operator: Dan Chen
Update Time: 2026/06/09 05:54:18
| EPICS Key | Before [mm] | After [mm] | Δ (After - Before) [mm] |
|---|---|---|---|
| K1:CAL-PCAL_EX_TCAM_PATH1_X | -0.87474 mm | -2.41683 mm | -1.54209 mm |
| K1:CAL-PCAL_EX_TCAM_PATH1_Y | 66.37439 mm | 65.57365 mm | -0.80074 mm |
| K1:CAL-PCAL_EX_TCAM_PATH2_X | -0.37755 mm | 1.41852 mm | +1.79607 mm |
| K1:CAL-PCAL_EX_TCAM_PATH2_Y | -67.02710 mm | -66.64088 mm | +0.38622 mm |
Update Time: 2026/06/09 05:54:58
| EPICS Key | Before [mm] | After [mm] | Δ (After - Before) [mm] |
|---|---|---|---|
| K1:CAL-PCAL_EY_TCAM_PATH1_X | 0.76950 mm | -0.69068 mm | -1.46018 mm |
| K1:CAL-PCAL_EY_TCAM_PATH1_Y | 65.80570 mm | 62.58426 mm | -3.22144 mm |
| K1:CAL-PCAL_EY_TCAM_PATH2_X | 1.39102 mm | 0.14883 mm | -1.24219 mm |
| K1:CAL-PCAL_EY_TCAM_PATH2_Y | -69.21742 mm | -69.03655 mm | +0.18087 mm |
[Tanaka, Hirose, Saito]
Using the 20 dB RF amplifier and the 40 dB RF amplifier, the beat signal amplitude was increased to 23 dBm. After replacing the phase detector with a Phase Frequency Discriminator (PFD), it was confirmed that the beat signal frequency followed changes in the LO frequency. However, the error signal appeared to oscillate at approximately 260 kHz. This oscillation may be caused by a resonance of the sub-laser PZT.
First, the alignment was adjusted to maximize the beat signal. The signal level under various RF amplifier configurations was as follows:
No RF amplifier: -51 dBm
40 dB RF amplifier only: -5 dBm
20 dB RF amplifier only: -20 dBm
40 dB RF amplifier followed by the 20 dB RF amplifier: 8 dBm
20 dB RF amplifier followed by the 40 dB RF amplifier: 23 dBm
Therefore, lock acquisition was attempted using the phase detector with the 20 dB RF amplifier followed by the 40 dB RF amplifier. A 1 MHz low-pass filter was applied in the SR560 used for feedback to the sub-laser PZT, while a flat filter was implemented in Moku:Lab. Various gains and integrator settings were tested. However, no behavior indicating that the beat frequency was being pulled toward the LO frequency was observed.
Next, the phase detector was replaced with a PFD. With a filter consisting of an overall gain of -6 dB and an integrator providing 6 dB of gain at 1 Hz (Photo 1), it was observed that the beat signal frequency followed changes in the LO frequency. In the lower plot of Photo 1, the red trace represents the error signal and the blue trace represents the feedback signal. Since the feedback signal changed when the LO frequency was varied, the LO frequency and beat signal frequency were measured for feedback signal levels of approximately 0 V and ±1 V. The beat signal spectrum exhibited a shape with a dip at the center and peaks on both sides (Photo 2). Therefore, the frequencies of the two peaks were measured, and their average was taken as the beat signal frequency. In Photo 2, the light red trace corresponds to a feedback signal of approximately +1 V, while the red trace corresponds to a feedback signal of approximately -1 V.
The results are summarized below:
Feedback Signal LO Frequency Beat Signal Frequency
Approximately -1 V 85.066 MHz 85.16 MHz
Approximately 0 V 88.066 MHz 87.99 MHz
Approximately +1 V 89.666 MHz 89.74 MHz
In addition, when using a flat filter and gradually increasing the gain, the error signal began oscillating at approximately 260 kHz, and the width of the beat signal increased. This oscillation may have been caused by a resonance of the sub-laser PZT. The corresponding error signals and beat signals are shown below:
Flat filter with a gain of -6 dB (Photo 3), corresponding beat signal (Photo 4)
Flat filter with a gain of 0 dB (Photo 5), corresponding beat signal (Photo 6)
Flat filter with a gain of +6 dB (Photo 7), corresponding beat signal (Photo 8)
Date: 2026/06/08
Member: Dan Chen, Misato Onishi, Seiya Matsuo
We performed our usual WSK calibration at UToyama.
The results look no problem.
| Case | Alpha (Main Value) | Alpha (Uncertainty) |
| Front WSK, Back GSK | -0.911724 | 0.000357 |
| Front GSK, Back WSK | -0.909858 | 0.000275 |
Comparing with previous results, no significant issues were found.
Attached graph is the result summary including the latest measured data.
I offloaded the BF GAS with the FR.
[Tanaka, Fujimoto, Saito]
The alignment was adjusted to maximize the beat signal, resulting in a beat signal level of approximately -55 dBm, which was the same as in the previous measurement (klog:37031). It was also confirmed that the sub-laser PZT was operating properly. The mixer currently in use (ZX05-1-S+) was then replaced with a phase detector (ZRPD-1+) purchased by Dan-san, and lock acquisition was attempted. However, no lock was achieved. Furthermore, when an RF amplifier was inserted after the high-pass filter while using the phase detector, the signal was amplified without waveform distortion, unlike the behavior observed in the previous experiment (klog:37031).
Next, the 1.9 MHz low-pass filter located between the mixer and the SR560 was moved from immediately before the SR560 to immediately after the mixer. PLL lock acquisition was then attempted using Moku:Lab with a 10 kHz low-pass filter while varying the gain and adding an integrator. However, no behavior indicating that the beat frequency was being pulled toward the LO frequency was observed. Lock acquisition was also attempted without using Moku:Lab by varying the gain of the SR560 low-pass filter, but no lock was achieved. In addition, a 10 kHz low-pass filter was applied to the SR560 used in the feedback path to the sub-laser PZT, while a flat filter was implemented in Moku:Lab. However, lock acquisition was still unsuccessful. The mixer currently in use (ZX05-1-S+) was then replaced with the phase detector (ZRPD-1+) purchased by Dan-san. Various Moku:Lab filter configurations were tested in the same manner as before, but lock acquisition was again unsuccessful.
Next, while continuing to use the phase detector, an RF amplifier was inserted after the high-pass filter. Unlike the result obtained in the previous experiment (klog:37031), the signal amplitude increased while maintaining a clean waveform (Photo 1). The error signal also increased in amplitude and became saturated. Therefore, the gain of the SR560 was reduced from 200 to 5. Under these conditions, the error signal amplitude was approximately 384 mVpp (Photo 2).
[Fujimoto, Tanaka, Takano]
We diagonalised the SRM oplev. Now, the coupling from other DoFs is below 1% at the resonance frequencies.
We noticed that when we shake SRM TM in Pitch we observed motion in Yaw as well. At first, we suspected the actuator couplings, but the health check results obviously told us the coupling of the sensor (the tilt oplev), see Fig. 1 (Pitch) and Fig. 2 (Yaw) (blue: measurement in 2022, green: before the diagonalisation, red: after the diagonalisation). The 2x2 matrix about the coupling between pitch and yaw is as follows:
| OUT \ IN | Pitch | Yaw |
| Pitch | 1 | 0.19 |
| Yaw | -0.32 | 1 |
After normalisation:
| OUT \ IN | Pitch | Yaw |
| Pitch | 0.952 | 0.187 |
| Yaw | -0.305 | 0.982 |
Using this matrix, we calculated its inverse and multiplied it by the current SENSALIGN matrix from the left. The health check results using the new SENSALIGN matrix are shown in the figure: in both Pitch and Yaw, the coupling is below 1% at the resonance peak frequencies.
[Fujimoto, Tanaka, Takano]
We continued the DRMI optimisation. We could stably lock DRMI with POP17Q for MICH, instead of REFL51Q. REFL51 signals looked strange, probably due to a bad demodulation phase. ADS implementation was tried, but not succeeded yet.
We continued the DRMI locking trial. This time, we investigated the REFL51 signals and discussed whether they could be used for locking. As reported here, there is an offset on both REFL51I and REFL51Q, but we don't understand its mechanism. In addition, the locking with REFL51Q for MICH looked unstable, so we decided to change the MICH control signal from REFL51Q to POP17Q for better stability. With POP17Q, stability seemed to be improved so much. The lock can now be kept for more than 10 minutes.
The measured open loop transfer function for each loop are shown in Fig. 1 - 3. They looked stable enough, but sometimes we observed that MICH control got unstable and started oscillation at apparently a random frequency in 20 - 40 Hz. It may be that because of the alignment, MICH sensing gain increased, and the phase margin got smaller, or another control loop sucked the phase margin in the MICH loop via unknown couplings. Anyway, MICH control seems the key to better stability of DRMI control.
Once DRMI got stable, we injected the dithering signal in SRM and tried the phasing of SRM ADS with AS34I signal. The phase of the transfer function from the dithering LO to the signal (AS34I) is shown in Fig. 4. The measured phase was put in ADS, and tried to engage the control for SRM. It was not obvious how it worked, because the buidup level of AS34I looked almost the same due to its large fluctuation. Then, ADS of other mirrors, PRM, BS and IMMT2 were engaged using POP90I signal, but it seemed that the feedback signal made the alignment worse. We should tune the phases of the other mirrors as well for full ADS in DRMI.
With DRMI locked with POP17I&Q and REFL135I, the REFL51 signals were quickly examined. Obviously, both REFL51I and REFL51Q had a large offset. When the demodulation phase was rotated, the offset value also changed in sine curve for I phase and in cosine curve for Q phase (Fig.5). We don't know the source of these offsets, probably either MICH or SRCL has this offset.
Now that we can lock DRMI without REFL51 signals, the investigation is easier than before. I hope these issues will be solved soon and DRMI will be locked using fully 3f signals.