Reports of 34080
VIS (SRM)
ryutaro.takahashi - 13:40 Thursday 09 April 2026 (36728) Print this report
Comment to Adjustment of suspension (36711)

[Washimi, Takahashi]

We replaced the satellite box for the IM H OSEMs. The previous box is  S1604901 (Pic. 1 and 2). The new box is  S1807635 (Pic. 3 and 4). The OSEM outputs were changed as follows (Pic. 5). The transfer functions for H2 (Pic. 7), H3 (Pic. 8), and Y (Pic. 10) were the same as the previous measurements. The DC gain of the transfer functions for H1 (Pic. 6) and L (Pic. 9) was increased by 5dB. The H1 OFFSET in "K1 SRM IM OSEMINF FILTERS" was returned from -3700 to -6315.5.

  Previous New
H1 2790 3760
H2 5900 5940
H3 8380 8420

 

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VIS (SRM)
ryutaro.takahashi - 13:16 Thursday 09 April 2026 (36729) Print this report
Comment to Health check (36669)

I added the F0 transfer function measured with a modified template.

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VIS (SRM)
takaaki.yokozawa - 8:31 Thursday 09 April 2026 (36727) Print this report
Incident angle of the SRM oplev
According of the JGWDoc7268, the incident angle of SRM oplev is 37 deg.

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DGS (General)
takahiro.yamamoto - 3:11 Thursday 09 April 2026 (36726) Print this report
Comment to Migrating scripts from k1script1 to k1script0. (36519)
I started to migrate on-demand scripts.

Pico, Stepper, and temperature control scripts were migrated from k1script1 to k1script0.

Though traverser script was worked also on k1script0, it's launched from MEDM screen with hard-coded server name. So all MEDM screens must be also updated. Because it's so hard to do remotely, I'll do it next week.

Rebooter script doesn't work on k1script0 because it depends on the telnetlib package which was obsoleted from Python3.13 whic h is one of the system packge of Debian13. So I replaced a function defined in the telnetlib package as a function defined by the socket packages. I haven't tested this new code with connecting rebooter devices yet. It will also be done in next week. In addition, MEDM screens for rebooter on which the server information is hard-coded must be also updated.

HWP script also has a server connection settings with hard-coded manner. So it must be rewritten as the new script server information. Rewritten code was already prepared and will be tested next week.

Once these tests are complete, we plan to proceed with the actual deployment. These are remaining tasks of the migration work for k1script.
VIS (SRM)
ryutaro.takahashi - 0:33 Thursday 09 April 2026 (36725) Print this report
Comment to Health check (36669)

I checked the transfer functions of F1, BF, IM, and TM. The states during the measurement were READY for F1 and BF, TWR_FLOAT for IM and TM. The diaggui for F0 did not work. 

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MIF (General)
shun.saito - 23:44 Wednesday 08 April 2026 (36724) Print this report
Measurement of IR laser power and beam profile on the POS optical table

[Tanaka,Hirose,Saito]

In preparation for the measurements of PRCL and SRCL, we measured the IR laser power and beam profile on the POS optical table.
The laser power was approximately 15μW.

  • On the POS optical table, the IR laser passed through a periscope, a beam splitter that separates the green laser and IR laser, and a lens. It was then reflected by a mirror and finally directed toward PDs for S-polarization and P-polarization. We placed a power meter in front of the mirror to measure the laser power, which was approximately 15μW.
  • Next, we placed an additional mirror in front of the original mirror (at a position approximately 450 mm from the lens)(Photo 1) and measured the beam profile of the IR laser. In this measurement, the origin was defined as the center of the hole on the optical table where the additional mirror was placed. A beam waist was observed at approximately 263 mm, but the beam split into two at around 300 mm (Photo 2). Even at 575 mm, the beam remained distorted (Photo 3). The measurement was initially performed in the single bounce configuration. Considering the possibility of birefringence effects, the Y-arm was then locked. However, almost no change was observed (Photo 4).

The fitting results of the beam profile will be posted later.

Images attached to this report
VIS (SRM)
ryutaro.takahashi - 18:04 Wednesday 08 April 2026 (36723) Print this report
Comment to Adjustment of suspension (36711)

[Washimi, Takahashi]

  • We removed the 1kg ballast ring from the IP. The resonant frequencies for L and T were close to the reference (klog).
  • We investigated the IM H1 OSEM. Details are here.
  • We adjusted the H1 OSEM position to 2800 (near the middle of the dynamic range). The H1 OFFSET in "K1 SRM IM OSEMINF FILTERS" was changed from -6315.5 to -3700.
  • We checked the height of the TM/RM. One laser leveler (red) was set to the height reference on the chamber (Pic. 1). The other laser leveler (green) was set to the red line (Pic. 2). The red line consisted of the X+ side wire breaker on the RM (Pic. 3), and was 0.5mm higher than the marker on the front ring of the RM (Pic. 4). The green line also consisted of the X- side wire breaker on the RM (Pic. 5), and consisted of the marker on the front ring of the RM (Pic. 6).
  • We adjusted the gap of the EQ stops and took pictures of them.
Images attached to this comment
FCL (Electricity)
takashi.uchiyama - 15:58 Wednesday 08 April 2026 (36722) Print this report
Comment to Crackings of the utility pole for KAGRA power cable (27051)
2026/04/08

We started work for the cracked electric pole at the Mozumi mine entrance today. The work will continue by April 17.
In this work, we will build 1 electric pole to support power cables which give tension to the power pole.
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IOO (IMC)
kenta.tanaka - 15:46 Wednesday 08 April 2026 (36720) Print this report
Comment to IMC ASC unstable (36715)

This afternoon, I entered PSL and offloaded manually IP1 PZT PIT and YAW, which are used as DOF4 PIT and YAW controls. After that, IMC seems to be stable without any satuaration.

VIS (SRM)
ryutaro.takahashi - 11:51 Wednesday 08 April 2026 (36719) Print this report
Comment to Health check (36669)

We checked the IP transfer functions after removing the third 1kg ballast ring.  The resonant frequencies of the IP were changed from 59 to 66mHz for L and from 66 to 70mHz for T. They were close to the reference (63mHz for L, 70mHz for T).

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VIS (SRM)
ryutaro.takahashi - 11:48 Wednesday 08 April 2026 (36718) Print this report
Comment to Adjustment of suspension (36711)

[Washimi, Takahashi]

We investigated the IM H1 OSEM. The transfer function was recovered when the OSEM position was in the linear range, 5600 (Pic. 1). We swapped the stellite box channel for H1 and H2. The output was changed (Pic. 2) as shown in the table. Ch. 1 output was smaller than that of Ch. 2 in both cases. The satellite box has a problem. The transfer function of H1 using Ch. 2 showed a gain higher than the reference (Pic. 3).

  Before After
Ch. 1 5600 (H1) 4500 (H2)
Ch. 2 6000 (H2) 7500 (H1)

 

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IOO (IMC)
takaaki.yokozawa - 9:47 Wednesday 08 April 2026 (36717) Print this report
Comment to IMC ASC unstable (36715)
Before the -46 m, the IMC locked stably, and my work (initial alignment stared).
2nd locked failed (around -44.5 m), DOF5 P kicked and TEM10 IMC lock detected.
During the TEM10 IMC lock, IO guardian didn't go to the 1000(providing stable light) ASC didn't start in case of TEM10 IMC lock.
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IOO (IMC)
takaaki.yokozawa - 9:30 Wednesday 08 April 2026 (36716) Print this report
Comment to IMC ASC unstable (36715)
DOF4 P saturated two days before and DOF4 Y saturated 17 days before.
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IOO (IMC)
takaaki.yokozawa - 9:18 Wednesday 08 April 2026 (36715) Print this report
IMC ASC unstable
In this morning, I noticed that the IMC seemed unstable.

Fig.1. showed the time series of the ASC P DOFs.

DOF4 P saturated, that issue was already known.
Around the -23 m, IMC can be locked, but the TEM 10 mode in IMC trans(divided in pitch direction)
I touched the offset of the PZT1 and PZT2 in pitch, it recovered.

2nd IMC locked loss happened a few seconds after the providing stable light, but this was the conflict with the XARM guardian.
After turned off the XARM guardian, IMC can be locked with long time.

Anyway, we need the offload of the DOF4 in some days.
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Comments to this report:
takaaki.yokozawa - 9:30 Wednesday 08 April 2026 (36716) Print this report
DOF4 P saturated two days before and DOF4 Y saturated 17 days before.
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takaaki.yokozawa - 9:47 Wednesday 08 April 2026 (36717) Print this report
Before the -46 m, the IMC locked stably, and my work (initial alignment stared).
2nd locked failed (around -44.5 m), DOF5 P kicked and TEM10 IMC lock detected.
During the TEM10 IMC lock, IO guardian didn't go to the 1000(providing stable light) ASC didn't start in case of TEM10 IMC lock.
Images attached to this comment
kenta.tanaka - 15:46 Wednesday 08 April 2026 (36720) Print this report

This afternoon, I entered PSL and offloaded manually IP1 PZT PIT and YAW, which are used as DOF4 PIT and YAW controls. After that, IMC seems to be stable without any satuaration.

VIS (IY)
ryutaro.takahashi - 8:44 Wednesday 08 April 2026 (36714) Print this report
Comment to Offload of GAS filters (36614)

I offloaded the BF GAS with the FR.

DGS (General)
takahiro.yamamoto - 2:28 Wednesday 08 April 2026 (36712) Print this report
Comment to Replacement of wrong combination of timing fiber for V2 IO chassis (36705)
[Ikeda, YamaT]

The timing fiber for EY0 was also replaced as OM3. But there was no improvement in the situation. Though we also tried to change an SFP module on the Timing Fanout and an LC-LC join connector, it's also no effect. This is a situation we are facing for the first time, and we do not have sufficient information yet. We are still doubting various possibility as a cause of this situation such as a version of Timing Slave, a part number of SFP module on the Timing Slave, a version of power distribution board, a dip switches on the power distribution board, etc.

It takes several tens of minutes to test whether this issue occurs, and verifying reproducibility and individual variations is expected to take several hours to half a day to validate a single hypothesis. Since conducting these tests at the end station is highly inefficient, we plan to perform reproducibility tests on the test bench.
VIS (SRM)
ryutaro.takahashi - 22:19 Tuesday 07 April 2026 (36711) Print this report
Adjustment of suspension

[Washimi, Takahashi]

We adjusted the suspension.

  • After offloading the BF and F1 GAS filters, we adjusted the V1/2/3 OSEM positions to the center of the range.
  • We removed the 1kg ballast ring from the IP. The resonant frequencies for L and T were changed (klog).
  • We investigated the small gain of the H1 OSEM in the IM transfer functions (Pic. 1). We checked the forward voltage of the diodes and resistance at the feedthrough flange (Table). They were normal. We calibrated the OSEM output by moving the IM body in the 1/4 pitch of the M4 screw for the EQ stop (Pic. 2). The maximum value was 7500 counts (Pic. 3). The calibrated coefficient was 0.136 um/count (Pic. 4). The original coefficient was 0.299 um/count.
Pin# H1 cf. H3
1-6 0.531V 0.531V
2-7 19.1Ω 19.0Ω
3-8 1.073V 1.072V

 

Images attached to this report
Comments to this report:
ryutaro.takahashi - 11:48 Wednesday 08 April 2026 (36718) Print this report

[Washimi, Takahashi]

We investigated the IM H1 OSEM. The transfer function was recovered when the OSEM position was in the linear range, 5600 (Pic. 1). We swapped the stellite box channel for H1 and H2. The output was changed (Pic. 2) as shown in the table. Ch. 1 output was smaller than that of Ch. 2 in both cases. The satellite box has a problem. The transfer function of H1 using Ch. 2 showed a gain higher than the reference (Pic. 3).

  Before After
Ch. 1 5600 (H1) 4500 (H2)
Ch. 2 6000 (H2) 7500 (H1)

 

Images attached to this comment
ryutaro.takahashi - 18:04 Wednesday 08 April 2026 (36723) Print this report

[Washimi, Takahashi]

  • We removed the 1kg ballast ring from the IP. The resonant frequencies for L and T were close to the reference (klog).
  • We investigated the IM H1 OSEM. Details are here.
  • We adjusted the H1 OSEM position to 2800 (near the middle of the dynamic range). The H1 OFFSET in "K1 SRM IM OSEMINF FILTERS" was changed from -6315.5 to -3700.
  • We checked the height of the TM/RM. One laser leveler (red) was set to the height reference on the chamber (Pic. 1). The other laser leveler (green) was set to the red line (Pic. 2). The red line consisted of the X+ side wire breaker on the RM (Pic. 3), and was 0.5mm higher than the marker on the front ring of the RM (Pic. 4). The green line also consisted of the X- side wire breaker on the RM (Pic. 5), and consisted of the marker on the front ring of the RM (Pic. 6).
  • We adjusted the gap of the EQ stops and took pictures of them.
Images attached to this comment
ryutaro.takahashi - 13:40 Thursday 09 April 2026 (36728) Print this report

[Washimi, Takahashi]

We replaced the satellite box for the IM H OSEMs. The previous box is  S1604901 (Pic. 1 and 2). The new box is  S1807635 (Pic. 3 and 4). The OSEM outputs were changed as follows (Pic. 5). The transfer functions for H2 (Pic. 7), H3 (Pic. 8), and Y (Pic. 10) were the same as the previous measurements. The DC gain of the transfer functions for H1 (Pic. 6) and L (Pic. 9) was increased by 5dB. The H1 OFFSET in "K1 SRM IM OSEMINF FILTERS" was returned from -3700 to -6315.5.

  Previous New
H1 2790 3760
H2 5900 5940
H3 8380 8420

 

Images attached to this comment
MIF (General)
hirose.chiaki - 19:22 Tuesday 07 April 2026 (36709) Print this report
Replaced the PDH LO for GRX with the measurement LO and checked the number of optical components

[Tanaka, Ushiba, Hirose]

In preparation for the PRCL and SRCL measurements, we replaced the PDH Local Oscillator(LO) for the GRX with the measurement LO and checked the number of optical components.

  • We prepared an LO to do phase-locked loop (PLL) using the sub-laser and main-laser beams by combining them in the POS table. A phase-locked loop (PLL) cannot operate properly unless the LO has a lower noise level than the phase noise. The LO for the GRX’s PDH is a High-spec LO (photo1 below) that can also be used for the PLL, so we will use this one. We replaced the LO for the PDH with a new one(photo1 above, photo2, photo3) that satisfied for PDH.
  • For this experiment, we plan to use the mirrors, HWP, PBS, and lenses stored in the front room of the PSL. Mirror mounts, lens mounts, HWP mounts, IRIS, and other items will be taken from the areas around the POP and IMCREFL.
  • We confirmed the number of optical components(excluding the 2-inch mirror) in the current PSL front room, so I posted the details(JGW-T2415582-v6) on JGWdoc.
Images attached to this report
VIS (SRM)
ryutaro.takahashi - 16:11 Tuesday 07 April 2026 (36710) Print this report
Comment to Health check (36669)

I checked the IP transfer functions after removing the second 1kg ballast ring.  The resonant frequencies of the IP were changed from 55 to 59mHz for L and from 63 to 66mHz for T. They are still lower than the reference (63mHz for L, 70mHz for T).

Images attached to this comment
MIF (General)
takaaki.yokozawa - 10:29 Tuesday 07 April 2026 (36708) Print this report
Initial alignment and TCam photo session
I performed the initial alignment (Xarm and Yarm) and TCam photo session.
The analysis of the TCam image would be performed later
VIS (EX)
ryutaro.takahashi - 10:02 Tuesday 07 April 2026 (36707) Print this report
Offload of GAS filters

I offloaded the F0 GAS with the FR.

DGS (General)
takahiro.yamamoto - 2:42 Tuesday 07 April 2026 (36706) Print this report
Comment to Migrating scripts from k1script1 to k1script0. (36519)
All EPICS IOCs were also moved to k1script0.
Now all resident scripts and services were migrated.
I will start to migrate on-demand scripts tomorrow.

IOCs built as standard ones
cam_ioc, das0_ioc, and weather_ioc running on k1script1 as Debian10 system had been built as a standard IOC under the EPICS-3.14.5 environment without any special configuration. Linked shared objects by these applications didn't depends on detailed library versions and they was able to be launched on k1script0 as Debian13 only with LD_LIBRARY_PATH for EPICS-3.14.5. It's a troublesome to be required LD_LIBRARY_PATH to launch them every time. So I rewrote RUNPATH injected in the ELF binary files by
> patchelf --set-rpath /kagra/apps/epics-3.14.12.3_long-deb13/base-3.14.12.3/lib/linux-x86_64 /path/to/AppName
They can be now launched without LD_LIBRARY_PATH and ELF binaries for Debian10 is archived as target/AppDir/bin/linux-x86_64/AppName-deb10.

IOCs built including special dbd definition with support module
cryocon_ioc, sys_ioc, and vac_ioc had been built with a special dbd definition with support module under the EPICS-3.14.5 environment. Because support module depends on shared object that version is not available on Debina13 system. So rewriting RUNPATH doesn't work well for this case. But these IOC didn't use a function of special dbd at all. So I rebuilt them as a starndar IOC under the EPICS-3.14.5 environment. An old build for Debian10 is archived as target/archive/IOC/AppDir-deb10

IOCs built under different EPICS version environment
cryhx_ioc had been built as a standard IOC under the environment of different EPICS version from /kagra/apps/epics-***. It seemed to be built with EPICS installed in the system region from Debian10 basic repository because of (probably) forgetting to load /kagra/apps/etc/epics-user-env***.sh before executing a build command. Anyway, it doesn't have a compatibility with an environment of Debian13 at all. So I started over from the configure step, not just the build. An old configured application for Debian10 is archived as target/archive/IOC/k1cryhx.
DGS (General)
takahiro.yamamoto - 0:58 Tuesday 07 April 2026 (36705) Print this report
Replacement of wrong combination of timing fiber for V2 IO chassis

[Ikeda, YamaT]
 

Abstract

In recent these days, we replaced IO chassis from V1 to V2.
(K1TEST0 in klog#33560, K1IX1 in klog#36572, K1IY1 in klog#36625, K1EX0 in klog#36654, and K1EY0 in klog#36692).
Real-time models on these front-ends seemed to work well.
But they had a problem that a IRIG-B timing took so long time to be stable when the cold boot of the front-end computer was performed.

Last weekend, we realized that this might be caused by a mix-up of different fiber-optic cables.
So we replaced fiber-optic cables of K1TEST0, K1IX1, K1IY1, and K1EX0 to the correct combination.
After then, the issue of the timing synchronization taking too long no longer occurred.

We had no enough time to go to Y-end today, so we will do same thing for K1EY0 tomorrow.
 

Details

The V2 IO chassis uses a new cable connection standard, and some of its specifications are different from those of the V1 IO chassis. The most significant difference is that the data transfer cable between the front-end computers and the IO chassis has been changed from custom-made HIB optical fiber to standard MTP fiber (OM3). Thanks to this change, we are no longer constrained by the limited availability of HIB cables and we can provide additional IO chassis as spare ones and/or for new instruments in future e.g. filter cavity.

In addition to this change, timing fiber cable in the IO chassis was also changed to the OM3 cable. Strictly speaking, the SFP port of the timing slave was directly accessible from the front panel on V1 IO chassis and any SFP module could be attached, so there were no internal cables. In other words, it is more accurate to say that the interface was changed rather than the cable standard.

Until now, OM1 cables have been installed for multimode optical fiber, not just for timing signals. (Since single-mode fiber, OS1, is used for long-distance connections, this is slightly off-topic.) So the most of timing slaves in the V1 IO chassis were connected to the timing fanout with OM1 cable and we had reused them for V2 IO chassis when we had replaced IO chassis from V1 to V2.

Although the real-time models themselves were running well also in this configuration, there remained a mystery as to why it took several hours for the IRIG-B timing to stabilize after a cold boot of the front-end computer. Figures 1 and 2 show the fluctuations in the IRIG-B value following a cold boot on EY0 and IX1, respectively. Both of them shows that it takes o(hours) time to stabilize the IRIG-B value within normal range (5-20us). And also, for EY0 (Fig.1), it's reproduced in 3 times trial.

The IRIG-B value is not the primary source of timing synchronization but merely serve as a cross-check. However, if they fall outside the normal range, RFM and Dolphin communication will fail. As a result, a global control cannot be done. Even if it took so long time to stabilize IRIB-B value, it finally went to normal range. So we was able to resume global control by waiting this fantastic time. But waiting time as o(hours) was serious from the view point of effective downtime of the digital system for keeping commissioning time and also observing time.

At first, we didn’t realize the relation between the IRIG-B issue and fiber cables standard, but we finally noticed that OM1 and OM3 cables have different core diameters (62.5 μm and 50 μm, respectively) and that mixing them can cause speed reductions and instability especially for the long distance connection in Ethernet case. To be honest, I wasn’t sure if the same discussion applied to Timing synchronization, but We decided to try unifying the fiber cable as OM3.

After replacing the fiber cable, we didn't need to wait that IRIG-B timing was stabilized. And it's not reproduced in a few times power-cycle. After replacing the fiber cable, we didn't need to wait that IRIG-B timing was stabilized. And it didn't appear also in a few times power-cycle. So we concluded that the IRIG-B issue was induced by the mismatch of the optical fiber standard. Today, we was able to complete a replacement work for K1TEST0, K1IX1, K1IY1, and K1EX0. Reaming K1EY0 will be processed tomorrow.

Images attached to this report
Comments to this report:
takahiro.yamamoto - 2:28 Wednesday 08 April 2026 (36712) Print this report
[Ikeda, YamaT]

The timing fiber for EY0 was also replaced as OM3. But there was no improvement in the situation. Though we also tried to change an SFP module on the Timing Fanout and an LC-LC join connector, it's also no effect. This is a situation we are facing for the first time, and we do not have sufficient information yet. We are still doubting various possibility as a cause of this situation such as a version of Timing Slave, a part number of SFP module on the Timing Slave, a version of power distribution board, a dip switches on the power distribution board, etc.

It takes several tens of minutes to test whether this issue occurs, and verifying reproducibility and individual variations is expected to take several hours to half a day to validate a single hypothesis. Since conducting these tests at the end station is highly inefficient, we plan to perform reproducibility tests on the test bench.
VIS (SRM)
ryutaro.takahashi - 22:00 Monday 06 April 2026 (36704) Print this report
Comment to Investigation of BF GAS (36675)

[Washimi, Takahashi]

We recovered the flags touching the OSEM bodies in the IM. We rotated the IM with the yaw picomotor, aligning the TM with the F0 yaw FR. The H3 flag was released easily (Pic. 1 and 2), then the H1 (Pic. 3) and V2 (Pic. 4) flags touched the OSEM bobies. Though we tried to find good relative geometry between the IM and the IRM, we could not find it. The strategy was changed; we adjusted the positions of the OSEM bodies, moving the base panel of the OSEMs. The axial positions of the H1, H3, and V1 OSEMs were also adjusted. We rotated the H2, H3, and V3 flags to be perpendicular to the LED-PD line in the OSEM.

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DGS (General)
satoru.ikeda - 18:01 Monday 06 April 2026 (36703) Print this report
Updated k1vissrmt model file; removed unnecessary DAQ channels

We have updated the k1vissrmt model file and removed unnecessary DAQ channels.

Requests from Ushiba-san and R.Takahashi-san
Related to K-Log#36664
[K1SRM]
 model: k1vissrmt
 detail: Change the input ADC channels for ACC_H1, 2, and 3 from 20, 21, and 22 to 21, 22, and 23

Request from YamaT-san
 We have commented out K1EDCU_TESTIOC.ini from the DAQ master file.
 

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Non-image files attached to this report
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