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KAGRA MIR (Polarization)
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MarcEisenmann - 23:10, Tuesday 09 November 2021 (2731)Get code to link to this report
TAMA 1 (Shinkosha) birefringence measurement

This entry reports the birefringence measurement of TAMA #1 with 1.5cm radius, 0.25 mm step size, 0.5s wait time and 0.488mW input power.

Due to time constraints only 3 measurements were possible.

Note that the AC and DC was realigned before input polarization calibration and with sample and that here 0 deg polarization angle corresponds to s polarization.

The analysis code was checked using the Shinkosha7 data and produced identical results.

The main result is that polarization, theta and delta_n are quite uniform but the main variation corresponds also to the maximum absorption (see entries 2723 or 2672) while the triangular patterns does not seem to affect significantly these parameters.

Images attached to this report
2731_20211109150808_xsi0deg.png 2731_20211109150815_xsi30deg.png 2731_20211109150823_xsi60deg.png 2731_20211109150831_s0.png 2731_20211109150845_s1.png 2731_20211109150852_meandntheta.png 2731_20211109150858_deltan.png 2731_20211109150906_theta.png
Comments related to this report
SimonZeidler - 16:57, Wednesday 10 November 2021 (2733)

That looks very good, indeed!
What you can do in addition is to check for the second (negative) solution according to theory, as I reported last meeting.

An important point is also to be very precise with all input parameters. For example, it isn't enough to set the thickness to just 6cm or so but to take into account the refraction due to the inclination and the hence extended beam path.

R&D (FilterCavity)
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YuhangZhao - 21:19, Monday 08 November 2021 (2730)Get code to link to this report
BS mirror magnet replacement (2)

Matteo, Takahashi-san, Yuhang

Takahashi-san removed the jig and released BS earthquake stop this morning. Before closing vacuum chamber, we checked transfer function of BS and pitch/yaw coupling.

The transfer funtion shows in the first attached figure. We can see that the red line is close to reference below about 10 Hz. The deviation at low frequency is probably due to the air flow, while the deviation at high frequency is presumably due to acoustic coupling.

The pit/yaw coupling shows in the second attached figure. The green shows the coupling when we have magnet drop. The red curve is after we put new BS magnet, which got close to reference (blue curve). This figure shows that the BS mirror magnet replacement work is successful.

After confirming TF and coupling, we closed both PR and BS chamber and evacuated them. Now, we are using turbo pump to evacuate. Until the vacuum level reaches about 1e-8 mbar, we will open the gate valve between PR/BS and Input.

Images attached to this report
2730_20211108132052_20211108bsytfinair.png 2730_20211108132057_20211108bscouplinginair.png
R&D (FilterCavity)
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YuhangZhao - 20:55, Monday 08 November 2021 (2729)Get code to link to this report
In-vacuum Faraday measurement (2)

Matteo and Yuhang

To check what is the rotation angle of the Faraday rotator, we removed the HWP after it. We found the 2nd PBS reflected IR power decreased from 458uW to 192uW after removing HWP. This tells us that the rotation is arctan((458-192)/192) = 54 degree.

By adjusting the relative position between magnet and TGG crystal, we achieved reflection 213uW and transmission 226uW. In this case, the rotation is arctan(226/213) = 47 degree.

We put back HWP after optimizing HWP and found a transmission of 6uW from the 2nd PBS. After rotating HWP, we reduced it to 4uW.

In the end, we checked round trip loss of Faraday isolator using a IR HR mirror reflecting back the reflection from dichroic mirror. We found injection of 449uW, 2nd PBS reflection of 438uW, and total reflection of 390uW. The round trip losses from Faraday isolator is 11% now.

KAGRA MIR (Polarization)
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MarcEisenmann - 17:24, Monday 08 November 2021 (2728)Get code to link to this report
check of the setup

We found out that the TAMA 1 fast axis orientation was also quite uniform and similar to the aztec sample...

Following entries will report all measurements that were taken but here we report the various checked performed :

 

- with 14.7 mW input power and OD 2 the maximal power reaching the QPD was below 0.6 mW (maximum recommended by Thorlabs)

- the output voltage of the QPD with this optical power is about 1.4 V (consistent with the responisitivty of the QPD at 1064 nm)

- to avoid saturation of the lockin amplifier (at 1V) we placed 6dB attenuator and the lockin voltage was indeed divided by 2

- the spectrum of the signal show clearly the peak at the chopper frequency and harmonics (note that 3rd harmonic is stronger than 2nd)

- the beams alignment before the QPDs were tuned to always be inside the sensor with and without sample

- the 2 QPDs signals have the expected behavior when changing the input beam polarization angle

- the maximum of the QPDs with sample correspond to about 0.9 of the maximum without sample (consistent with sample reflectivity checked with power meter)

 

- for the last measurement (will be precised in the entry) we reduced the incident power to 0.588 mW, removed the OD and the laser linewidth to avoid as much as possible possible back-scattering and recentered the beam with and without sample before every measurement

R&D (FilterCavity)
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MichaelPage - 14:14, Monday 08 November 2021 (2727)Get code to link to this report
In-vacuum Faraday measurement

Yuhang, Michael

We took the opportunity to measure the vacuum FI loss when the vacuum tanks were opened, using BAB. The vacuum Faraday isolator assembly can be seen in the photo (figure 1). The polarizers are two mirrors tilted at 55 degrees (Brewster polarizers). The black tube is the Faraday rotator. Attached to the end of the rotator is the half wave plate. From the reflection of the second polarizer, the IR beam hits the dichroic mirror, where it is recombined with green. Instead of propagating to the filter cavity, we used a mirror (furthest left in the photo) to reflect the beam back through the Faraday. Then, we measured the power in the following locations:

P1 in: Incident power at the first polarizer, coming from the squeezer table
P1 ref: Reflected power after P1 in
P1 tra: Power transmitted through the first polarizer, with respect to P1 in
FR/HW tra: Power after one pass through the Faraday Rotator and Half Wave plate
P2 ref: Power reflected from the second polarizer after coming from the Faraday
P2 tra: Power transmitted through the second polarizer, with respect to FR/HW tr
Di in: Incident power on the dichroic mirror
Di ref: Reflected power from the dichroic mirror
RT P1 tra: Power transmitted through the first polarizer after two trips through the Faraday.

There is some weirdness with the power meter measuring more power after reflection from certain components, but it consistently happens in certain positions (P1 ref, P2 ref, Di ref), which makes us think it's more to do with the power meter geometry. It makes precise measurement of losses to be difficult. Still, we can draw two conclusions: 1) the polarizers have low transmission of the order of 1%, and 2) the round trip loss through the FI assembly is about 14%. We took several measurements at the positions that were causing problems. Also, the p-pol PLL unlocked at a couple of points (between columns 4/5, 10/11 on the table below)

 

Power measurement (units of uW)

  1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16
P1 in 446 461   400 424 439 422 412         429 425 417 415
P1 ref 448 434 437                   427 427 428 426
P1 tra 4 4                            
FR/HW tra 447 443 430                   407 407 395 415
P2 ref 432 440   330 413               416 404 415 412
P2 tra 3 2                            
Di in                 415 395 419 422        
Di ref                 392 400 422 419 412 412 407 413
RT P1 tra           377 371 353         355 352 357 372

 

Avg. RT P1 tra/P1 in = 0.857
RT P2 transmission = 2 uW

Images attached to this report
2727_20211108053432_399a3366.jpg
Comments related to this report
MichaelPage - 14:15, Monday 15 November 2021 (2736)

I only just remembered this but we also measured the beam height (70mm) before and after the Faraday assembly, as shown in the photos.

R&D (FilterCavity)
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MichaelPage - 13:22, Monday 08 November 2021 (2726)Get code to link to this report
BS mirror magnet replacement

Takahashi R., Matteo, Marc, Yuhang, Michael

The BS chamber was opened and the magnet was glued.

Photos of the process are attached.

The BS vacuum tank was closed on Friday, and then the PR chamber was opened and the portable cover moved over PR.

Images attached to this report
2726_20211108051809_dsc00542copy.jpg 2726_20211108051827_dsc00570copy.jpg 2726_20211108052002_dsc00571copy.jpg 2726_20211108052018_dsc00572copy.jpg 2726_20211108052032_dsc00573copy.jpg 2726_20211108052047_dsc00574copy.jpg 2726_20211108052103_dsc00579copy.jpg 2726_20211108052117_dsc00580copy.jpg 2726_20211108052125_dsc00581copy.jpg 2726_20211108052141_dsc00587copy.jpg
KAGRA MIR (General)
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MarcEisenmann - 17:37, Tuesday 26 October 2021 (2725)Get code to link to this report
Modifications and realignment of birefringence readout

Katsuki-san, Marc

We removed all the readout of the birefringence. The reason being that the photodetectors size was quite small wrt to the beam size. This means that performing the alignment without sample might not be so accurate for the case with sample.

First we replaced the optical breadboard from imperial holes size to metric ones.

Then we reinstalled the PBS, the ODs and tried to installed the new PSD (PDQ80A) that have quite larger sensor size but are also sensitive to visible light.

In order to have a larger beam on the PSD, we replaced the lens in front of the PBS by a 100 mm focal one.

Sadly, because the PSD sensor is 4 cm above the screwing hole, it was quite tricky to find proper post.

Therefore, we also installed 2 steering mirrors just after the ODs.

Finally, we installed laserline filters right in front of the PSDs.

We took time to put label on various cables.

The alignment was checked (ie we confirmed that the maximal power of both ac and dc is reached without sample).

I just started birefringence measurement of the TAMA T1 sample with s polarization at the input.

The 'bad news' is that the gain of the PSD requires to change the gain of both lockin amplifiers depending on the input polarizations.

R&D (FilterCavity)
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MichaelPage - 16:36, Monday 25 October 2021 (2724)Get code to link to this report
OPO replacement - incoupling mirror

Yuhang and Michael

 

When we went to place the incoupling mirror, we found that the screw threads for adjusting the incoupling mirror position were mismatched - the screw threads on components 1 and 28 (assiemepdopov3asm.pdf) have 1mm pitch while the micro adjuster screw has much smaller thread pitch. It will take some time to have the proper components ready.

Images attached to this report
2724_20211025093019_inputcouplerthreads.jpg 2724_20211025093023_microadjusterthreads.jpg
Non-image files attached to this report
KAGRA MIR (Absorption)
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MarcEisenmann - 21:17, Friday 22 October 2021 (2723)Get code to link to this report
TAMA T1 absorption measurement

This sample absorption has been remeasured as there was some discrepancy with measurement few years old.

This one agrees with the one I did few months ago : absorption is around 18 ppm

(Pin = 7.316W, Pt = 6.29W, R = 0.8342 ppm/cm)

There are however strange patterns on the XZ YZ measurements that were not present before.

Images attached to this report
2723_20211022141708_xy.png 2723_20211022141711_xz.png 2723_20211022141714_yz.png
R&D (FilterCavity)
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RyutaroTakahashi - 17:06, Thursday 21 October 2021 (2722)Get code to link to this report
Comment to Filter cavity BS mirror is found to have some problems (Click here to view original report: 2712)

We started evacuation of the BS chamber yesterday. I opened the gate valve between BS and NM2 today.

KAGRA MIR (General)
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MarcEisenmann - 18:49, Wednesday 20 October 2021 (2721)Get code to link to this report
Comment to aztec polarization angle as a function of input polarization angle (Click here to view original report: 2716)

Fitting this data with a cosine gives input polarization equal to output sample polarization for angle about 41.34 deg and the phase about -6.5 deg

R&D (FilterCavity)
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YuhangZhao - 16:29, Wednesday 20 October 2021 (2720)Get code to link to this report
Comment to Filter cavity BS mirror is found to have some problems (Click here to view original report: 2712)

Marc, Matteo, Takahashi-san, Yuhang

We opened BS chamber today to check if there is any issue for the magnet.

We found one magnet falls down as shows in the attached figure.

Takahashi-san will help us prepare a replacement magnet. The replacement work will be done in the next next week.

Images attached to this comment
2720_20211020092948_wechatimg148.jpeg
R&D (FilterCavity)
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YuhangZhao - 11:54, Wednesday 20 October 2021 (2719)Get code to link to this report
Comment to Filter cavity BS mirror is found to have some problems (Click here to view original report: 2712)

We have done some more check before opening the BS vacuum chamber.

1. Check BS P and Y transfer functions. They are similar with reference as shows in the fig1 and fig2.

2. Check coupling between P and Y. A substantial coupling increase is found as shows in the fig3.

3. We tried to close BS local control loop. But failed.

The results of test 2 and 3 make us really need to open BS chamber to check. The opening work is scheduled to be in this afternoon.

Images attached to this comment
2719_20211020045400_bsptf20211020.png 2719_20211020045405_bstf20211020.png 2719_20211020045411_bscoupling20211020.png
KAGRA MIR (Absorption)
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MarcEisenmann - 20:57, Tuesday 19 October 2021 (2718)Get code to link to this report
TAMA T1 absorption measurement started

Today I tried to tweak the input pump power and did several long Z scan to find the 2 surfaces of the sample.

Because it did not succeed at first, I reinstalled the bulk reference sample and got R_bulk = 0.8342 cm/W

Finally, by taking 10 averages and mean I could see the surfaces and started the measurement at Z_center = 62.75 mm

Using the value of this long Z scan the absorption is consistent with the previous measurement :

AC ~ 1.5e-4V

DC~4V

Ptrans = 6.290W

Pinc = 7.315W

gives absorption ~ 22 ppm/cm

Measurement is on-going with 0.5mm step size and 30 mm radius.

Do not touch the sample this week !

KAGRA MIR (General)
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MarcEisenmann - 20:22, Monday 18 October 2021 (2717)Get code to link to this report
Preparation of TAMA T1 measurement

Katsuki-san, Marc

Today we removed the AZTEC sample in order to prepare the absorption and birefringence measurement of the TAMA T1 sample.

We reinstalled the steering mirror in the injection part to dump the sample reflection (see fig1)

We installed a flipping mirror before the birefringence readout to redirect the pump beam to the high power power meter (see fig2).

We reconnected the absorption photodiode to the lockin amplifier.

We installed the surface reference sample and with z = 42.3mm and zIU = 66 mm we got R_surf = 18.72 /W

We installed the bulk reference sample with z = 40.95 mm  and zIU = 65.7 mm and got R_bulk = 0.6679 cm/W.

We installed the TAMA T1 and using DC values could find Y_center = 121.92 mm and X_center = 326.74 mm.

We increased the pump laser current to 6A (beforehand we changed the HWP angle that control the power to 9 deg that corresponds to the min pump power) which gave Pt ~6.1W.

We realigned the DC at the previous z_center (62.4mm) and did long z scan but could not find clear surfaces absorption neither on the AC nor the phase.

This seems to confirm that this sample absorption is quite low ( previously measured at 18 ppm).

Because it is the first time using such high power with all the birefringence optical component we turned off the laser today and will start the absorption measurement tomorrow morning.

Images attached to this report
2717_20211018131636_img20211018173101.jpg 2717_20211018131641_img20211018173109.jpg
KAGRA MIR (General)
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MarcEisenmann - 20:12, Monday 18 October 2021 (2716)Get code to link to this report
aztec polarization angle as a function of input polarization angle

Katsuki-san, Marc

Today we checked the relationship between the input polarization angle and the AZTEC sample polarization angle.

We confirmed that thanks to the realignment the maximal power of both photodiode is reached without sample.

Further analysis to follow.

Images attached to this report
2716_20211018131224_aztecpolaangle.png
Comments related to this report
MarcEisenmann - 18:49, Wednesday 20 October 2021 (2721)

Fitting this data with a cosine gives input polarization equal to output sample polarization for angle about 41.34 deg and the phase about -6.5 deg

KAGRA MIR (Polarization)
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MarcEisenmann - 20:09, Monday 18 October 2021 (2715)Get code to link to this report
birefringence measurement of AZTEC in same orientation as absorption measurement

Here are the figures.

Images attached to this report
2715_20211018130857_0deg.png 2715_20211018130902_15deg.png 2715_20211018130906_30deg.png 2715_20211018130909_45deg.png 2715_20211018130912_60deg.png 2715_20211018130916_s0.png 2715_20211018130919_s1.png 2715_20211018130923_theta.png 2715_20211018130927_deltan.png 2715_20211018130931_meandeltantheta.png 2715_20211018130934_polarela.png
KAGRA MIR (Polarization)
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MarcEisenmann - 20:06, Monday 18 October 2021 (2714)Get code to link to this report
birefringence measurement of AZTEC sample rotated by 180 deg

During the week-end we took birefringence measurements of the AZTEC sample rotated by 180 deg and back to same orientation as the absorption measurement (ie 0 deg).

Due to some mistakes it was not possible to perform too many measurements (once labview is exited it reset the lockin amplfiier to absorption measurement)..

To avoid confusion I report here the measurement with 180 deg rotation.

Images attached to this report
2714_20211018130535_0deg.png 2714_20211018130539_45deg.png 2714_20211018130543_64deg.png 2714_20211018130547_70deg.png 2714_20211018130554_polarela.png 2714_20211018130559_s0.png 2714_20211018130603_s1.png 2714_20211018130607_theta.png 2714_20211018130610_deltan.png 2714_20211018130613_meandeltantheta.png
R&D (FilterCavity)
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YuhangZhao - 17:03, Monday 18 October 2021 (2713)Get code to link to this report
Comment to Modification of the GRMC Servo-filter (Click here to view original report: 1271)

Recently, it is found that GRMC loop cannot be closed. To check what is the problem, I disconnected the slow scan of MZ and put MZ PZT offset to a value that GRMC transmission is the highest. After that, according to the original setting, I have done following checks

0. GRMC has a good alignment.

1. PDH signal has 316mV pk-pk checked from EPS1.

2. GRMC has loop sign of INV, which is as design.

3. The RF source phase is reloaded. The phase of RF source is 125deg. When it is changed to 35deg, the signal around resonance becomes flat. This indicates the RF signal phase is still a good one.

4. There is a switch which has +/- sign. This doesn't decide the sign of control loop. But when we use this type of servo for CC1/2 controls, we need to flip this switch. I tried to flip this switch, but it doesn't help to close loop.

5. GRMC transmission is checked to have 1.13V peak. This is two times smaller than the value written by Pierre.

6. Loop gain is 3 as usually used.

7. Threshold for peak identification is -0.55V. This is as required.

8. The GR power reaching AOM is measured to be 44mW, whose nominal value is 50mW.

These checks show little issues but they should not prevent the GRMC locking. More investigation is required.

R&D (FilterCavity)
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YuhangZhao - 15:57, Monday 18 October 2021 (2712)Get code to link to this report
Filter cavity BS mirror is found to have some problems

After the earthquake on 7th this month, we confirmed the normal operation of vacuum system, mirror suspension system. Especially, the filter cavity alignment was recovered and mirror's oplev shows usual spectra.

However, we found already that the driving of BS has problem. The problem is when we try to move yaw or pitch, the beam reflected by BS moves diagonally.

To confirm if there is any issue for magnets, I took a photo of BS magnets. Attached photo shows this check. Two red boxes indicate the location of four coil-magnet actuators. An arrow points to the magnet which seems to be broken. This magnet may be knocked during earthquake and get tilted. So the coil cannot drive it properly.

Images attached to this report
2712_20211018085711_57.png
Comments related to this report
YuhangZhao - 11:54, Wednesday 20 October 2021 (2719)

We have done some more check before opening the BS vacuum chamber.

1. Check BS P and Y transfer functions. They are similar with reference as shows in the fig1 and fig2.

2. Check coupling between P and Y. A substantial coupling increase is found as shows in the fig3.

3. We tried to close BS local control loop. But failed.

The results of test 2 and 3 make us really need to open BS chamber to check. The opening work is scheduled to be in this afternoon.

YuhangZhao - 16:29, Wednesday 20 October 2021 (2720)

Marc, Matteo, Takahashi-san, Yuhang

We opened BS chamber today to check if there is any issue for the magnet.

We found one magnet falls down as shows in the attached figure.

Takahashi-san will help us prepare a replacement magnet. The replacement work will be done in the next next week.

RyutaroTakahashi - 17:06, Thursday 21 October 2021 (2722)

We started evacuation of the BS chamber yesterday. I opened the gate valve between BS and NM2 today.