YamaT-san reported the laser down again around 19:00.
I checked the chiller for the FB laser, and I confirmed that it was working. So, we suspected the same interlock trouble as the previous down. In addition, I suspected that,
According to Yuzu-san's information, the laser seemed to be healthy around 18:00 (JST).
Around 15:00??, YamaT-kun performed all DAQ restart.
Some electrical influence from the DGS system and the interlock system through the grounding might exist. However, in the previous down case, the laser down happened before the DGS maintenance activities.
Anyway, I asked Tanaka-kun, YamaT-san and Yuzu-san to enter the PSL room tomorrow, and to check the above 3 items, and to restart the laser again.
I measured noise spectra of the three error signals (REFL 45, 56, and 17) directly reflected from PRM to estimate the sensing noise limit of these channels, particularly that of CARM.
Ideally, the sensing noise is completely limited by the shot noise.
The attached figure shows the result with some light.
In addition, it is compared to that without light to measure the electrical dark noise.
At high frequencies, the dark noise remains a dominant factor, which should be the shot noise.
We need to increase the input power to the PDs.
There are large excesses at low frequencies compared to the dark noise.
It might be because the optics inside the cahmber around IFI are still in air, so I will perform the same measurement after vacuum pumping.
Another potential reason is the amplitude modulation caused by detuning of the RF sidebands.
I will check the spectra after the fine tuning again, as described in klog:29385.
Furthermore, even-number harmonics of 60 Hz are prominent in the spectra with light.
Since there are no harmonics in the dark noise measurement, it should be generated by the IMC control or unknown electrical coupling peculiar to the configuration with light.
After vacuum pumping, I will calculate the CARM sensing noise limit in the unit of Hz/Hz and the projection on the DARM sensitivity.
[Tanaka, Hirose, Komori]
Abstract:
We adjusted the common offset immediately after the input of the IMC LSC common mode servo (-5.0 ± 0.3 mV with 14 dB input gain) and the fundamental frequency to generate multiple RF sidebands (5.6243667(1) MHz) to keep the carrier and the RF sidebands just on resonance of IMC.
As the result, we achieved a precise estimation of the IMC length, accurate to 1 µm, L_IMC = 53.302438(1) m.
Details:
During the previous measurement in klog:29084, residual peaks at the modulation frequency of 1.023 kHz persisted in either I-phase or Q-phase demodulation signals even after tuning the RF sideband frequency.
We attribute this to an extra offset in the IMC length control, causing detuning of the carrier and either the upper or lower sideband.
To address this, we experimented with combinations of LSC offset tuning and sideband frequency adjustments.
The setup is the same as klog:29084.
Initially, we adjusted the sideband frequency to equalize the residual peak heights in both demodulation signals.
Subsequently, we fine-tuned the common offset of the IMC LSC common mode servo.
This method effectively reduced the height of both peaks simultaneously, although we have not understood yet an unexpected swap of the I-phase and Q-phase peaks with minor adjustments to the sideband frequency (approximately 10 Hz).
After several iterations of this procedure, the residual peaks nearly vanished (the red and blue lines), yielding the results described above.
However, one hour later, upon rechecking the peak height, we observed the reappearance of residual peaks (the magenta and cyan lines).
We were unable to eliminate these peaks by solely adjusting the sideband frequency and common offset, suggesting that both parameters had drifted during this hour.
The drift in IMC length may originate from the re-locking of the IMC, leading to differences in the locked point by a few um, and thermal expansion of the IMC mirrors and suspensions.
The offset drift may arise from electrical circuit and residual amplitude modulation due to slight mismatches in the input polarization to the EOM, caused by temperature drifts.
We must consider strategies to compensate for these drifts and assess their impact on interferometer sensitivity.
After the today's acceptance check for anticipated closing IFI-IMM-PRM next week, here uploaded some photos to show the ISS beam is passing through about the center of the relevant viewport window; the photos taken the last week.
[Komori, Tanaka, YokozaWashimi]
We performed the Hammering test for the IFI stack (+X, +Y side stack).
I just noticed that I made a mistake in the number of outputs of the Whitining Filter in the mini-rack. The number of Whitining Filter outputs on the mini-rack is 8, not 4.
kTanaka-san just checked the empty input ports of ADC in IOO0, IOO1 rack.
The following are the empty input ports.
For the mini-rack, I would like to use 4-11ch and 20-27ch in ADC2 and additionally 8-15ch in ADC0 and 24-31ch in ADC1.
I will check with others to confirm that we can use this port as an addition. Also, do additional cabling.
Komori, Tanaka
We confirmed that the beam positon of the reflection from PRM which is in the "MISALIGNED_BF" state seems to be almost the center of the HP beam dump. (see attached movie)
## what we did
[Ikeda, Takahashi]
We checked the OSEMs again. We took pictures of the OSEMs with a 360º camera (THETA). The flap for the OSEM#1, #4, and #5 were rotated by 40~50°.
[Hirata, Dan Chen-san]
We recovered PR3 suspension. Oplev position is around center, and IM V1 OSEM value (K1:VIS-PR3_IM_OSEMINF_V1_INMON) is about 6200.
posted by Miyoki instead of Kimura-san for the past activities on 24th April.
The gasket surface of the removed IFI flange was visually inspected. Based on the visual inspection results, the following three points are estimated to have caused this flange to leak.
1. scratches on the gasket surface of the flat flange with copper flange (thin vertical scratches can be observed when shining a light on it) One location
2. Scratches on the metal gasket surface (thin vertical scratches can be observed when illuminated by light) One scratch
Possibly traces of 1.
Uneven traces on the gasket seal surface If the gasket is tightened properly, the trace will be a circle of uniform width. Since the traces on the actual product are narrow and wide, there is a high possibility that the initial tightening of the claw clamps was not uniform.
Here are the countermeasures.
Since the instructions call for the flat flange with copper flange to be returned to the original mirror plate instead of using the copper flange, repair of the scratches on the flat flange gasket surface will not be performed. Instead, a visual inspection of the original mirror plate gasket surface is performed before installation. In addition, the gasket will be changed from a metal gasket to an elastomer gasket.
We connected the new cables to the photosensors and confirmed that the sensor is working.
Also, we checked the signals while touching the cables around BF but there seems no glitch.
So, new cables seems working well.
We will tie up the cables and fix them onto the payload.
[Hirata, Dan Chen-san]
We took photos for PRM payload earthquake stops. I uploaded today's photo to KAGRA dropbox.
During this work, we found two earthquake stops for test mass AR side were very close to the mirror surface(within 1mm?). We talked with Takahashi-san and Ushiba-san, and decided to withdraw them.
I checked the motion of the F0Y FR. I operated the stepper motor from -4563 step by 1000 steps. The BF Y signal didn't change until -16563 step. When I added one more -1000 step, the signal was changed from -770 to -850. Though the signal went back to -770 by 1000 steps, it didn't go in the plus direction anymore. The motor is working, but the motion of the wire receptacle on the bearing is not smooth due to the large friction.
[Ushiba, Tamaki, Komori, Takahashi]
We continued the photosensor recovery. The replaced cables were fixed onto the bottom of BF, the cable anchor (small hexagon), and the suspension rod with cable ties.
sorry, the legend was clipped.
It is same for all plots.
I plotted the high-resolution (3-hour data, 128s FFT) ASDs and Coherences for the geophones and ACCs on the OMC chamber, for the night time before vacuum breaking.
Miyakawa, Tanaka
### abstract
We found that the interlock that is sensing the temp on the beam dumper is activated. We reset the interlock according to the Uchiyama-san's info. Then the original fiber amp. started emitting laser. We don't know why the interlock was activated yesterday.
### What we did
[Hirata, Dan Chen-san]
We partially applied FC on PR3 HR side upper edge part. 15 min later, we pilled off FC. The target edge shape residues were successfully removed. We can see new two small dots, but they are far from the center.
I uploaded today's photo to KAGRA dropbox.
Tomorrow morning, we will recover suspension.
Yamamoto, Tanaka
After today's maintenance work we noticed that the laser output was at zero. We checked how long it had been zero and found that the laser output had dropped to zero all at once at around 10:50 today. According to Yamamoto-san, this was before the maintenance work had been carried out.
Later, when we looked at the laser controller screen via the webcam in the PSL, we saw the error message "temperature too High, Master Fault" (Fig, 1) The temperature displayed on the controller was 52°C, which was much higher than the nominal value of 23°C.
When we entered the mine, we first checked whether the chiller was working properly, and the chiller temperature display showed a nominal value of 19 degrees Celsius, which seemed to be working properly.
We then entered the PSL and touched the enclosure of the fibre amplifier and did not feel any heat in the enclosure. I also held up a sensor card around the laser's output port and found that a very weak light was emitted. The "seed" value on the controller was about 1.4. According to Nakano-san's manual, this "seed" value indicates the incident power to the fibre amplifier and should be between 1.0 and 2.5 as a nominal value. In other words, the incident power is considered to be normal. The current value of the NPRO controller was about 0.96 A, which is the nominal value, so the NPRO controller is probably normal.
According to Nakano-san's manual, in this case it was most likely a thermometer malfunction, which was fixed by switching off the laser, unplugging the connection cable from the amplifier to the PC and restarting the application, so we thought we would try this approach. However, at the beginning of the manual, there is a warning that if the amplifier is switched on while the seed laser is off, it may break down, while the operating procedure states that the power should be switched on from the amplifier. This contradicted the warning, and as we could not decide which was correct, we decided not to power down the whole laser today (although we are sure the warning is correct).
Instead, we first switched off the fibre amplifier only and restarted it. However, the situation remained the same. We then switched off the fibre amplifier, closed the app, and then restarted the amplifier and the app. However, the situation remained the same.
At this point, we noticed that before pressing the "ENABLE" button on the controller app, i.e. when the laser was not emitting, the thermometer on the controller was showing around 3.5°C, and when we pressed the "ENABLE " button was pressed, the value of the thermometer rose up to 52 degrees Celsius drastically. When the "STOP" button was pressed, the thermometer value suddenly dropped from 52°C to about 3.5°C. This seems to be an odd behaviour of the thermometer.
At any rate, as it was late, we finished today's investigation.
Tomorrow, we will try to restart the whole laser system including seed laser.