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.
Optical table keeps the temperature around 297K even when HPBD temperature reaches around 365K.
[Tanaka, Fujimoto, Saito]
Following klog:36995, a high-pass filter with a cutoff frequency of approximately 12 MHz was added to suppress the 900 kHz noise originating from the sub-laser. In addition, the beat signal was found to be approximately 10 dB lower than in the previous measurement (klog:37020), although the cause remains unclear. Lock acquisition was then attempted, but no lock was achieved. An RF amplifier was also inserted after the high-pass filter; however, although the beat signal amplitude increased, the signal waveform became distorted.
The beat signal was then re-examined and found to be smaller than in the previous measurement (klog:37020). To investigate this, the alignment was readjusted, the RFPD was reinstalled, and the polarization was varied. After reinstalling the RFPD, the DC output became saturated, so the sub-laser power was reduced to 0.825 mW. Ultimately, the beat signal level reached approximately -55 dBm (Photo 5). This is about 10 dB lower than in the previous measurement (klog:37020). The reduction cannot be explained solely by the decrease in sub-laser power, and the cause remains unclear. However, very little fluctuation in the beat signal amplitude was observed.
Next, lock acquisition was 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 using the low-pass filter of an SR560 instead of Moku:Lab while varying the gain, but no lock was achieved. In addition, when the sub-laser temperature was lowered from 31.51 ℃, a beat signal was still observed at 29.74 ℃. Based on the absolute frequency measurement reported in klog:36760, this is believed to be due to a mode hop. PLL operation was also tested at this temperature, but lock acquisition was again unsuccessful.
Finally, an RF amplifier was inserted after the high-pass filter in an attempt to increase the beat signal amplitude. Although the beat signal became larger, its waveform became significantly distorted (Photo 6). When the mixer was removed, the waveform returned to a clean shape, indicating that the mixer was responsible for the distortion. Therefore, this RF amplifier is not suitable for the present application.
One of possibilties why SRCL build up is lower than our expected is detuned from the resonance point. Actually, When DRMI was locked, RF51 I was not zero even though SRCL error signal by 1f was zero (fig.1). This offset is often caused by RFAM. So I checked current RFAM status of each demodulated signal from each REFL RFPD when the single bounced beam from PRM is on each PD.
Fig.2 shows that REFL demodulated signals and DC powers on REFL PDs. As you can see, RF56, RF45 seems to have some RFAMs. On the other hands, 3f PDs seems to be zero. Therefore, The offset on SRCL error signal cannot be explained by RFAM.
[Ushiba, Hirose]
We checked their Open-loop Transfer Function. We adjusted their gain and confirmed the phase margin.
And the adjusted filter is replaced. We also confirmed that the control stabilizes when switching to AC in the “ALIGNED state”.
We confirmed that switching to DC in the lock acquisition state stabilizes the control.
If the TM doesn't seem to stabilize in Lock acquisition state, it's better to set it to ALIGNED state and apply IM control.
By the way, there are several thermometers attached around the high power beam dump. One of them would be on the top surface of the optical table in the IFI chamber, probably. How about their values?
[Ushiba, Hirose]
Because the SRM was highly unstable in the 0.1–1 Hz band, we switched off the integrator in the OLDAMP of the IM stage and switched on a “DC” filter acting as an integrator into the TM stage.
After that, the integrator was further adjusted to include a gain of 10 dB or more in the 0.1–1 Hz range.
Furthermore, regarding the Damp filter, since the phase does not rotate in the high-frequency band, the high-frequency section of the current filter was replaced with a Chebyshev filter.
We also adjusted the gain to ensure phase margin stability in the UGF.
(FIG1, FIG2: PIT and YAW filter with sus model. Blue shows before adjustment, and red shows after adjustment.)
Currently, I have added modified filters to FM3 and FM5 of the PITYAW control filters for the SRM and TM OLDAMPs. After PLL work is completed, I will run tests, and if stability appears to be sufficient, I will replace the current filters in FM1 and FM9 with these modified ones.
Note:
・The suspension model was already included in OLDAMP's FM10. We have confirmed that this is a filter, just like the following files that will be updated in the latest health check.
/users/VISsvn/HealthCheck/PLANT_SRM_PAY_FLOAT_TM_TEST_{P,Y}.xml
・The Chebyshev filter is normalized such that the peak gain in the passband is 0 dB. In the 1 dB ripple Chebyshev filter used here, the DC gain is −1 dB. Therefore, a gain of +1 dB was applied to the entire filter to set the DC gain to 0 dB.
[Ushiba, Hirose]
We checked their Open-loop Transfer Function. We adjusted their gain and confirmed the phase margin.
And the adjusted filter is replaced. We also confirmed that the control stabilizes when switching to AC in the “ALIGNED state”.
We confirmed that switching to DC in the lock acquisition state stabilizes the control.
If the TM doesn't seem to stabilize in Lock acquisition state, it's better to set it to ALIGNED state and apply IM control.
Recently, high power IMC output with misaligning PRM is often used and sometimes IMC is kept locking with high power over night, which results in making HPBD hot,
So, I discussed with uchiyama-san and decided to add the safety function in the IMC guardian.
If hitting 10W beam for 8 and 24 hours, HPBD temperature becomes 350K and 370K, respectively.
So, I set the threshold at 365K as shown in fig1.
From now, if the HPBD temperature exceeds 365K, IMC lock will be lost once to make IMC output smaller.
During the work, I noticed we have two ZERO_SERVOOFFSET state with the same index.
Since this state is not used, I didn't change them but it would be better to renew the IMC guardian.
By the way, there are several thermometers attached around the high power beam dump. One of them would be on the top surface of the optical table in the IFI chamber, probably. How about their values?
Optical table keeps the temperature around 297K even when HPBD temperature reaches around 365K.
Since the satellite box was replaced, we haven't observed any glitches. Very good. We'll keep our eyes on it until the next maintanance day.