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KAGRA MIR (Scattering)
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DanChen - 09:11, Friday 17 June 2022 (2981)Get code to link to this report
Some report links to klog about mirror scattering measurement
Let me put some klog links related to mirror scattering measurement.
  • 16 May 2022: "Laser scattering measurement (test samples and ITMY)" link
  • 07 June 2022: "Camera calibration for scatter light measurement of mirror" link
  • 16 June 2022: "Mirror scattering estimation" link
  • 17 June 2022: "Clean up of the mirror scattering measurement set up": link
KAGRA MIR (Absorption)
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MarcEisenmann - 23:21, Wednesday 15 June 2022 (2979)Get code to link to this report
start of AZTEC #4 absorption

With help of Yuhang we removed #3 from the translation stage.

Then, I measured the bulk reference sample at the usual position and got R = 0.611 cm/W.

I installed the 1.5 inch sample and measured its absorption at the longitudinal center.

I measured about 35 ppm/cm which is compatible with old measurements.

Finally, again with Yuhang help, we installed the #4 and started absorption measurement.

KAGRA MIR (General)
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MarcEisenmann - 23:19, Wednesday 15 June 2022 (2978)Get code to link to this report
Soleil-Babinet compensator actuator replacement

Marc, Yuhang

Yesterday I tried to remove the 4 screws  holding one of the 2 crystal.

Once they are removed, it is possible to access 2 set screws that fix the linear translation stage.

The 4 screws were really tight and I only manage to remove 3.

With Yuhang help, we tried to remove the fourth one without success.

In the end, we broke a screwdriver head inside the screw..

Fukushima-san from ATC helped us to remove it today.

After that the linear translation stage was replaced with a motorized one and the Soleil-Babinet is now closed with 3 out of 4 screws (need to purchase the broken one).

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MichaelPage - 01:32, Wednesday 15 June 2022 (2977)Get code to link to this report
Mirror mount replacement along SHG path

Yuhang and Michael

We replaced the mirror mount for the beam splitter that goes into the SHG. The new mirror mount is much smaller, allowing us to more easily remove ghost beams and scattered light from the squeezer bench.

The beam splitter was replaced by roughly using an iris, SHG opening and GRMC EOM as beam position references. First, the beam splitter was moved by hand to align to the references. Fine tuning allowed us to recover the SHG mode matching to slightly better than the previous alignment condition.

Reference SHG alignment is shown in figure 1 and 2. BS model number is in figure 3. The mirror mount type is shown in figure 4.
 

Images attached to this report
2977_20220614183040_20220614172255.jpg 2977_20220614183044_20220614172246.jpg 2977_20220614183048_20220614191246.jpg 2977_20220614183155_20220614172204.jpg
Comments related to this report
YuhangZhao - 16:47, Monday 20 June 2022 (2984)

A proper beam dump thorlabs LB2 (1um - 12um) is installed for the newly replaced BS mount (as shown in Fig.1).

Although we can see some green light, let's remind that it is because the camera sensor is more sensitive to green as our eye. There are proper Dichroic mirrors to remove them.

KAGRA MIR (General)
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MarcEisenmann - 20:36, Monday 13 June 2022 (2976)Get code to link to this report
AZTEC #4 delivered

Marc, Yuhang

Today the AZTEC #4 was delivered.

We brought it to the PCI cleanroom and applied first contact on one surface.

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NaokiAritomi - 16:11, Monday 13 June 2022 (2975)Get code to link to this report
BS picomotor was recovered

[Takahashi, Aritomi, Marc, Yuhang, Michael]

Since the BS picomotors didn't work, we opened BS chamber and checked the picomotor. We found that BS was stuck at the stopper because we moved BS picomotor too much. After Takahashi-san adjusted suspension, BS picomotors worked well. Before we close the chamber, we aligned green. We moved PR to make the green beam at the center of BS and moved BS to make the green beam at the center of first target. 

We also found that the BS oplev beam is hitting off center of BS. We tried to make it at the center of BS, but the reflection was hitting the pillar of BS suspension so we left it as it is.

Finally, we closed the chamber and started the evacuation.

Some notes for future alignment:

  • We should not move picomotor ramdomly. We should move the picomotor little by little by looking at some references. We should not lose the green beam at the first target as much as possible.
  • When we have the suspension or picomotor issue and open the chamber, we should make sure the green alignment at GV between BS/input and first target before closing the chamber.  
  • We should measure the oplev spectra/transfer function and each coil response before closing the chamber
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NaokiAritomi - 15:16, Wednesday 08 June 2022 (2974)Get code to link to this report
BS picomotor does not work again

[Aritomi, Marc]

At the beginning of today, the BS picomotor was working well. However, after some BS alignment, BS picomotor does not work again... We don't know the reason but maybe because we moved the BS picomotor too much. We need to open BS chamber again.

KAGRA MIR (Polarization)
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MarcEisenmann - 14:03, Tuesday 07 June 2022 (2973)Get code to link to this report
Comment to Birefringence measurement of AZTEC #3 (Click here to view original report: 2971)

There were some mistakes in the analysis so these results are not correct.

I'm also starting to doubt the way we analyze our measurements so I'm thinking to speed up the installation of the Soleil-Babinet compensator for this characterization.

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NaokiAritomi - 15:04, Monday 06 June 2022 (2972)Get code to link to this report
BS picomotor replacement

[Takahashi, Aritomi, Marc]

We replaced the two broken BS picomotors. After the replacement, we confirmed that the picomotors are working well. We started the evacuation of BS chamber. We will open GV between input/BS tomorrow.

KAGRA MIR (Polarization)
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MarcEisenmann - 13:02, Friday 03 June 2022 (2971)Get code to link to this report
Birefringence measurement of AZTEC #3

This is a report of AZTEC #3 birefringence measurements where each map had for parameters : X_center = 400.735 mm, Y_center = 122.105 mm, Z_center = 70.275 mm, with 70 mm radius.

Birefringence characterization :

Figures 1 to 6 are the usual polarization measurements, 7 to 9 summarize informations about the stress tensors and delta n and theta distributions.

The sample seems quite uniform and is now a good candidate for KAGRA (it also had quite low absorption).

 

c axis orientation estimation :

In figure 10, I tried to compute from the mean output polarization the orientation of the sample c axis.

The mean output polarization is fitted by a sine square as a function of the input polarization where errorbars represent 1 sigma uncertainty.

From this fit, it seems that if we inject 50.23 deg input polarization we should have the same at the ouput.

In order to constrain a bit more the fit I am now doing a measurement with p polarization at the input and then will start the measurement at the polarization angle that should be conserved throughout the sample.

Images attached to this report
2971_20220603055858_pol0.png 2971_20220603055902_pol15.png 2971_20220603055907_pol30.png 2971_20220603055912_pol45.png 2971_20220603055916_pol60.png 2971_20220603055921_pol75.png 2971_20220603055925_s0.png 2971_20220603055928_s1.png 2971_20220603073339_deltantheta.png 2971_20220606042202_caxis.png
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MarcEisenmann - 14:03, Tuesday 07 June 2022 (2973)

There were some mistakes in the analysis so these results are not correct.

I'm also starting to doubt the way we analyze our measurements so I'm thinking to speed up the installation of the Soleil-Babinet compensator for this characterization.

KAGRA MIR (Polarization)
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MarcEisenmann - 18:17, Tuesday 31 May 2022 (2970)Get code to link to this report
start of AZTEC #3 birefringence measurement

Marc, Matteo

We installed the AZTEC #3 on the translation stage.

We tuned the input laser power to have better SNR on the PSDs.

With about 2 mW power and 3 dB attenuator before the lockin amplifier we are roughly at half the PSDs saturation and about 0.6 V in the lockin-amplifier (saturation at 1 V).

Measurements on-going (one map is 5h40 and we need at least 6)

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MarcEisenmann - 17:56, Tuesday 31 May 2022 (2969)Get code to link to this report
Trial to decouple input oplev

Following work in 2958, I had to tune the position of the input oplev tilt PSD to have enough space to move the shift PSD on its rail.

To perform decoupling between shift and tilt, I injected a line at 0.94 Hz (length mechanical resonance frequency) with 200 counts amplitude on input mirror length.

I moved the lens on the rail, for each position recenter the beam on the tilt PSD and measured the peak amplitude at 0.94 Hz.

Result is reported in fig 1.

It seems that for pitch, the ideal lens position should be about 12.2 cm while it should be about 11 cm for yaw.

For yaw, the peak was always present and as suggested by Matteo could be caused by the easy excitation of yaw when exciting length.

EDIT : corrected z units from mm to cm.

Images attached to this report
2969_20220601065810_20220531oplevinput.png
KAGRA MIR (General)
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HomareAbe - 09:23, Tuesday 31 May 2022 (2968)Get code to link to this report
calibration of Soleil-Babinet compensator
Abe, Marc

We put HWP with rotation mount before compensator and try to measure retardation of HWP as entry 2965.

We maximize p-pol power to rotate the HWP:
s = 19.9 mV
p = 648 mV

We rotate HWP and compensator to 45deg.(same direction)
we maximize p-pol power again and record value of the Vernier screw.

d = 6.84 mm

s = 766 mV
p = 16.8 mV

P-pol power was too low. It should be pure p-pol but p-pol power did not change even though we rotate the Vernier screw.
I think polarization direction was parallel to fast(slow) axis of compensator.

Retardation of HWP N_hwp is given by
N_hwp = 1-6.84/13.365
= 0.488

13.365 is calibration parameters measured in entry 2965.
KAGRA MIR (General)
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MarcEisenmann - 21:57, Monday 30 May 2022 (2967)Get code to link to this report
Switch to birefringence measurement

Today with Matteo we removed AZTEC #1 and repeated bulk calibration (R = 0.5769 cm/W) which is compatible with before.

Then, I installed a steering mirror to make the pump beam goes to the birefringence imaging unit.

Using the 2 razors blades I measured the beam position on the last steering mirror of the injection unit.

Then I move the razor blade as far as possible in z and place it in either horizontal or vertical where the beam is located on the last steering mirror.

Note that during the horizontal position tuning it is important to make sure that the beam is still aligned into the power-meter.

I then tuned both horizontal (fig 1) and vertical (fig 2) to reach angles of incidence of 0.014 and 0.006 deg respectively.

This is more than a factor 30 below the KAGRA precision requirement on the c-axis orientation so it is fine.

I connected s polarization to AC and p polarization to DC. (ie old lockin amplifier).

I reduced the laser power to about 359 uW so that we have at maximum about 1V on the lockin amplifier.

I tuned QWP and HWP (0.1 deg precision) to inject linear polarization :

hwp = 336.2 deg (s pol)
AC_min = 355/1e6
DC_max = 9.86*1/10

hwp = 21.2 deg (p pol)
AC_max = 746000/1e6
DC_min = 2.98*0.1/10

The PSD is far from saturating so maybe we could increase a bit the pump laser power and add attenuators before the lockin amplifier.

Images attached to this report
2967_20220530145216_20220530horizafter.png 2967_20220530145229_20220530vertafter.png
KAGRA MIR (Absorption)
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MarcEisenmann - 14:43, Monday 30 May 2022 (2966)Get code to link to this report
AZTEC #1 new measurement

We had some concerns with previous calibration of AZTEC #1 absorption measurements so we repeated the measurements.

With R = 0.5648 cm/W we have about 60 ppm/cm absorption which is compatible with previous estimation.

Images attached to this report
2966_20220530074322_yz.png 2966_20220530074327_xz.png 2966_20220530074331_xy1.png 2966_20220530074336_xy2.png 2966_20220530144825_xy3.png
KAGRA MIR (General)
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MarcEisenmann - 11:49, Monday 30 May 2022 (2965)Get code to link to this report
Soleil-Babinet compensator calibration

Abe, Marc

First we realigned the setup and tuned both HWP and QWP to inject s polarization.

With ceiling lights off we got :

hwp = 5.5 deg seems pure s
s = 915mV
p = 9.98 mV
hwp = 320.5 deg
s = 22.2 mV 
p = 805 mV

We installed the Soleil-Babinet compensator and tried to align it with auto-collimation.

However, while acting on the yaw steering screw, the retaining spring jumped outside the mount (even if we didn't felt any resistance or didn't reach the end of the screw range...)

Matteo helped us to reinstall it using the ones of an old mirror mount.

Once it was fixed, we could align the SBC without issue.

Tuning the SBC to reach maximal s polarization at the readout we measured :

s = 20.4 mV
p = 652 mV

We can not reach as pure s polarization as before ...

Next step is to use the detent stop by 45 deg and use the Vernier screw to reach again pure s polarization, press the zero of this Vernier, move it again so to reach the next s polarization.

We measured d  = 13.365 mm and got :

s = 21 mV
p = 673 mV

d is our calibration parameters and we can now use it to start measurements.
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NaokiAritomi - 16:06, Friday 27 May 2022 (2963)Get code to link to this report
Comment to Squeezer p-pol (Click here to view original report: 2961)

The beatnote can be seen with lower reference level (10dBm) as shown in the attached picture.

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2963_20220527090614_img9200.jpg
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NaokiAritomi - 15:33, Friday 27 May 2022 (2962)Get code to link to this report
BS pitch/yaw picomotors seem to be broken

[Takahashi, Aritomi, Marc]

Since the BS pitch/yaw picomotors didn't move, we opened the BS chamber and checked BS suspension. All magnets are fine, but BS was touching the earthquake stopper so Takahashi-san adjusted the BS suspension. 

However, BS pitch/yaw picomotors still don't move. We can hear the sound of picomotor, but the sound is smaller than usual. We also checked BS X/Y/Z picomotors. BS X/Z picomotors moved with usual large sound, but BS Y picomotor did not move without any sound.

To check if the problem is due to the picomotor itself or not, we disconnected the wire for BS yaw picomotor and connected it with a spare in-vac picomotor. The spare in-vac picomotor can be moved so the problem should be the picomotor itself. We have not checked the BS pitch picomotor, but we guess the problem would be the same. Since we have only one spare in-vac picomotor in TAMA, Takahashi-san will bring some spare in-vac picomotors from KAGRA and replace them next next Monday. 

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NaokiAritomi - 23:24, Monday 27 June 2022 (3002)

I found an old elog420 which also says that BS Y picomotor doesn't work.

R&D (FilterCavity)
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MichaelPage - 02:54, Friday 27 May 2022 (2961)Get code to link to this report
Squeezer p-pol

I couldn't find the p-pol laser and sidebands on the spectrum analyser (figure 1). I made sure the DDS board was reset properly, the lasers had proper current and temperature, and the beam was going into the fiber. I also tried disconnecting and reconnecting p-pol cables that I could see. Maybe something is disconnected elsewhere?

CC seems ok (figure 2)

Images attached to this report
2961_20220526195241_20220526233155.jpg 2961_20220526195246_20220526233159.jpg
Comments related to this report
NaokiAritomi - 16:06, Friday 27 May 2022 (2963)

The beatnote can be seen with lower reference level (10dBm) as shown in the attached picture.

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MichaelPage - 02:51, Friday 27 May 2022 (2960)Get code to link to this report
Comment to TAMA DGS upgrade (Click here to view original report: 2951)

I changed the root password back to normal. For me it was just Linux paranoia to make the root password different but I guess it doesn't matter here.