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KAGRA MIR (General)
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MarcEisenmann - 10:56, Friday 15 October 2021 (2711)Get code to link to this report
realignment

Katsuki-san, Marc

In order to mitigate the misalignment induced by the sample, we decided to move the 2 PDs closer to the waist.

For that, we also needed to change the ODs mounts for a smaller one.

We confirmed that with the realignment the maximal power of s or p polarizations with sample is smaller than the maxima without sample.

We started measurement with s polarization at input and the AZTEC sample rotated by 180 deg

KAGRA MIR (Polarization)
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MarcEisenmann - 13:16, Thursday 14 October 2021 (2710)Get code to link to this report
Comment to Polarization angle as a function of input polarization (Click here to view original report: 2704)

Just to clarify :

There is some input polarization angle for which the the s polarization power is higher with sample than the maximum without sample.

This hints for either scattered light but more probably some misalignment (maybe the beam hits the side of the PDs that fakes strong power?)

KAGRA MIR (General)
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MarcEisenmann - 13:13, Thursday 14 October 2021 (2709)Get code to link to this report
shinkosha evaluation plate #10

Shinkosha evaluation plate # 10 is available inside PCI clean room.

Documentation is below the PC.

KAGRA MIR (General)
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MarcEisenmann - 13:12, Thursday 14 October 2021 (2708)Get code to link to this report
HWP problem solved

After spending time trying to use another PC, another usb hub, another usb cable and others Kinesis version that all failed I installed a spare motorized HWP and confirmed that it worked perfectly fine.

It is now possible to control perfectly fine the 2 motorized HWPs at the same time.

R&D (FilterCavity)
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YuhangZhao - 13:44, Tuesday 12 October 2021 (2707)Get code to link to this report
Check of filter cavity mirror suspension on 2021/10/12

Michael and Yuhang

We checked filter cavity alignment yesterday. The pico-motor of PR/BS and END mirrors are moved. The movement of PR is to recover its reference on BS chamber. The movement of BS is to recover its reference in filter cavity transmission camera. The movement of END mirror is to recover the flash.

After these movement, we checked the oplev spectrum as attached in this elog. They look fine. So this time, no touching issue of mirror was found.

Images attached to this report
2707_20211012064423_vis202110122.png 2707_20211012064428_vis202110123.png
KAGRA MIR (Polarization)
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MarcEisenmann - 12:22, Monday 11 October 2021 (2706)Get code to link to this report
check of aztec sample after earthquake and HWP controller investigation

Katsuki-san, Marc

This morning we went to PCI to check the ATEC sample.

We found out that the peak visible in the polarization angle measurement is likely due to a dust so we removed it. Except that the sample seems perfectly fine.

We brought a laptop with Kinesis installed and connected it to the motorized HWP.

We got the same issue as with the PC (only jog by 1 deg).

We tried to home it and will check after lunch.

If problems persist we will contact Thorlabs and switch the 2 motorized HWP as the other is working fine.

KAGRA MIR (Polarization)
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MarcEisenmann - 11:06, Monday 11 October 2021 (2705)Get code to link to this report
bifringence measurement of AZTEC sample with no rotation

This entry reports the birefringence measurement of the AZTEC sample with no rotation,

Note that a quite strong earthquake happend right after the measurement with input polarization = 0 deg...

Note that in that case the input polarization angle of 0 deg is made with hwp angle = 346 deg..

While the mean value of the polarization angle measurement seems reasonable, there is now a strange 'peak' on the top right of the sample...

We'll go to PCI to check if the sample is fine.

Images attached to this report
2705_20211011040553_pol0deg.png 2705_20211011040556_pola27deg.png 2705_20211011040601_pola45deg.png 2705_20211011040604_pola79deg.png 2705_20211011040608_s0.png 2705_20211011040612_s1deg.png 2705_20211011040620_deltantheta.png 2705_20211011040624_deltan.png 2705_20211011040627_theta.png 2705_20211011040632_polarelat.png
KAGRA MIR (Polarization)
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MarcEisenmann - 11:03, Monday 11 October 2021 (2704)Get code to link to this report
Polarization angle as a function of input polarization

In order to further investigate the effects of the input beam incident angle we mesured the polarization angle as a function of the input beam polarization angle.

Data are attached to this entry.

Note that :

There are input polarization angle for which the s polarization power transmitted with sample is higher than transmitted s polarization power without sample..

The minimum s polarization seems to be reached for hwp  angle = 71 deg (ie 26 +45 deg) and using this polarization to normalize our signals means that the hwp angle = 341 deg that was assumed to be fully s polarization is in fact 10 deg polarization angle...

Images attached to this report
2704_20211011040330_polacheck.png
Non-image files attached to this report
Comments related to this report
MarcEisenmann - 13:16, Thursday 14 October 2021 (2710)

Just to clarify :

There is some input polarization angle for which the the s polarization power is higher with sample than the maximum without sample.

This hints for either scattered light but more probably some misalignment (maybe the beam hits the side of the PDs that fakes strong power?)

KAGRA MIR (Polarization)
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MarcEisenmann - 10:58, Monday 11 October 2021 (2703)Get code to link to this report
Comment to birefringence measurement of rotated AZTEC sample (Click here to view original report: 2698)

We also measured extra polarizations and results are attached to this entry.

Furthermore, I also computed the relationship between the input polarization angle and the polarization angle of the sample (see last figure).

Images attached to this comment
2703_20211011035721_pola99deg.png 2703_20211011035725_pola133deg.png 2703_20211011035758_thetav2.png 2703_20211011035816_0.png 2703_20211011041227_polarelat.png
R&D (FilterCavity)
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MichaelPage - 15:12, Friday 08 October 2021 (2702)Get code to link to this report
OPO replacement - alignment

Yuhang and Michael

After discussion in the TAMA filter cavity meeting on the 29th of September, we realigned the OPO, noting the following points:

  • The OPO assembly position with respect to the rotation stage has been set up so that rotating one of the upper screws results in OPO yaw rotation, and rotating both upper screws results in X translation (horizontal direction perpendicular to propagation axis). Likewise, rotating one of the lower screws results in OPO pitch rotation, and rotating both lower screws results in Y translation. See figure 1.
  • We confirm that the first stage of the OPO alignment starts with the beam entering the curved HR side (figure 2). This was noted with the black dot in figure 4 of 2682, which is closer to the flat faced side of the plastic holder (i.e. the incoupling mirror is mounted on the opposite side of the assembly from the periscope). The rationale is described in Matteo's thesis with respect to the SHG. We do it this way to ensure that the optical axis and OPO central axis are coincident before placement of the incoupling mirror. After placing the incoupling mirror, the cavity can be scanned for removal of higher order modes. Then, when the alignment of OPO/incoupler is confirmed, the assembly can be turned around for the finesse measurement.
  • The beam size of the CC/p-pol beam entering from the HR surface of the OPO in the TAMA experiment is nominally 36 um (Marc 936)
  • The distance of the beam from the f = 75 mm lens to the beam waist is measured to be 125 mm (2515). It is estimated that the OPO should be about 57 mm from the top of the periscope (figure 3). Note that there is a mistake in the figures of that elog entry - the predicted waist size of 20 um is with the lensing action of the meniscus (incoupler). Without the incoupler, the beam waist should be 25 um, as measured. However, as noted above, this beam size is setup for the OPO cavity finesse measurement, which is performed after the alignment of the incoupler.

 

The OPO has been aligned by using the camera to make a reference point (figure 4), placing the OPO, then ensuring that the incident and reflected beams overlap. We confirmed reflection/incidence overlap at the AOM exit port and Faraday Isolator. The beam is also centered on the target as indicated by the camera. In the future, we should take note to have the modulators and FI be further away from the OPO cavity for easier alignment of the reflected beam.

One of the wires detached from the DSub unit (figure 5). It appears to be the positive end coming from the OPO thermistor.

Images attached to this report
2702_20211008080757_rotationstage.jpg 2702_20211008081226_setup3.png 2702_20211008081233_beamdistance.jpg 2702_20211008081237_tvdot.jpg 2702_20211008081244_detachedwire.jpg
KAGRA MIR (Polarization)
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MarcEisenmann - 21:05, Tuesday 05 October 2021 (2699)Get code to link to this report
Resetup of the imaging unit

Katsuki-san, Marc

After investigating the effect of the AZTEC sample rotation, we decided to try to act on the imaging unit part.

We removed the OD (2 and 3) in front of the PBS in the imaging unit and added similar OD in front of each PD.

We tried to tweak the alignment as best as we could but because we installed the OD with a quite large angle to try to mitigate effects of scattering we don't have a balance powers on the 2 PD.

In order to have a beam small enough on the PDs we had to replace the lens before the PBS by one from the FC Newport lens box (f = 125 mm)

Anyway we started measurement in this new configuration.

KAGRA MIR (Polarization)
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MarcEisenmann - 21:03, Tuesday 05 October 2021 (2698)Get code to link to this report
birefringence measurement of rotated AZTEC sample

In order to investigate the reason of the seemingly uniform theta distribution, we decided to start new measurements with the AZTEC sample rotated.

I marked the position of the holder, rotated the sample and measured an arc length of 3 cm that corresponds to a rotation of the sample by 34.4 deg (radius is 5 cm).

I took several measurements that are reported in the attached figures.

An important thing to notice is that I found I made mistakes in the use of the code.

Starting from the code available in the PC the modifications for our current setup are :

DC gain = 10

AC gain = 1000

DC is s - pol

AC is p pol

While the gain were correct, the previous figures were made with inverted AC and DC !

Also, the incident polarization angle was wrongly estimated (ie no normalization).

Note that to estimate the delta_n distribution it has to be multiplied by 1e6 to properly compute variance and mean.

Now all these modifications have been implemented for these figures.

Furthermore, the HWP working condition could be recovered a bit and all the reported measurements are made with the HWP between 341 deg ( s-pol) and 26 deg (p pol).

As a brief summary of the results :

- s0 and s1 absolute values are now similar

- delta n and theta increase with the incident polarization angle

Images attached to this report
2698_20211005140044_90deg.png 2698_20211005140049_10deg.png 2698_20211005140053_12deg.png 2698_20211005140058_18deg.png 2698_20211005140102_30deg.png 2698_20211005140106_46deg.png 2698_20211005140110_60deg.png 2698_20211005140118_76deg.png 2698_20211005140122_s0.png 2698_20211005140126_s1.png 2698_20211005140131_meandeltan.png 2698_20211005140136_theta.png 2698_20211005140140_deltan.png
Comments related to this report
MarcEisenmann - 10:58, Monday 11 October 2021 (2703)

We also measured extra polarizations and results are attached to this entry.

Furthermore, I also computed the relationship between the input polarization angle and the polarization angle of the sample (see last figure).

R&D (FilterCavity)
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YuhangZhao - 22:14, Monday 04 October 2021 (2697)Get code to link to this report
Measurement of time series for BAB PDH signal (hitting on different position of end mirror)

Raffaele suggested to put time series together with spectrum of BAB PDH signal. The spectrum was measured in elog2573.

The last time of FC aligned was about one month ago. However, the alignment work took less than 20min today. In addition, the BAB alignment to FC didn't drift away too much. Although I didn't check higher order modes, the BAB transmission was about 430 counts.

After optimizing BAB transmission to about 460 counts, I took time series and put together with spectrum as attached figure.

Images attached to this report
2697_20211004152527_compare5.png
KAGRA MIR (General)
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MarcEisenmann - 14:25, Thursday 30 September 2021 (2696)Get code to link to this report
SHINKOSHA evaluation plates

There are now 4 SHINKOSHA evaluation plates inside the PCI clean room.

I marked the 7,11 and 14 on the side close to the ingot position marking.

KAGRA MIR (Polarization)
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MarcEisenmann - 13:36, Thursday 30 September 2021 (2695)Get code to link to this report
Comment to AZTEC birefringence measurements (Click here to view original report: 2694)

new measurement with 30 deg polarization finished.

The results (especially of the theta distribution) seems to agree with our hypothesis that the previous measurement with input polarization 30 deg was something like 30+90 deg.

Images attached to this comment
2695_20210930063645_polaangle30degv2.png 2695_20210930063649_thetav2.png
KAGRA MIR (Polarization)
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MarcEisenmann - 18:48, Wednesday 29 September 2021 (2694)Get code to link to this report
AZTEC birefringence measurements

I attached to this entry several results extracted from measurements with incident polarizations 90 deg (ie s-pol), 60 deg, 45 deg and 30 deg. They are made based on a python code kindly shared by Simon.

It seems this sample is more uniform than the SHINKOSHA #7.

The s0 component is far smaller while the s1 component is larger. A possible explanation could be (from MIR meeting discussion) that the birefringence appearing here is not due to stress but to the crystal axis orientation with respect to the pump beam optical axis.

The delta n distribution seems to be quite identical for all incident polarizations and the offset might be due to the cutting angle of this sample.

A possible explanation for the offset on the theta distribution for incident polarization of 30 deg could be explain by having rotating the incident polarization by more than 90 deg.

Indeed, the HWP software now is stuck at 15 deg whatever the polarization...

I started again this 30 deg incident polarization while only decreasing the value of the HWP angle.

Images attached to this report
2694_20210929114535_polaangle90deg.png 2694_20210929114540_polaangle30deg.png 2694_20210929114543_polaangle45deg.png 2694_20210929114547_polaangle60deg.png 2694_20210929114556_s0.png 2694_20210929114600_s1.png 2694_20210929114604_birefringence.png 2694_20210929114607_deltan.png 2694_20210929114612_theta.png
Comments related to this report
MarcEisenmann - 13:36, Thursday 30 September 2021 (2695)

new measurement with 30 deg polarization finished.

The results (especially of the theta distribution) seems to agree with our hypothesis that the previous measurement with input polarization 30 deg was something like 30+90 deg.

R&D (FilterCavity)
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MichaelPage - 16:33, Wednesday 29 September 2021 (2691)Get code to link to this report
OPO replacement - alignment of OPO assembly

Yuhang and Michael

We had some trouble aligning the OPO inside the holder (initially without the input coupler). A photo is shown in figure 1. The OPO assembly is contained on the white plastic mount and has a small ~ 5mm hole at both the entrance and exit. The mount past the OPO assembly is a beam splitter that goes to a camera and photodetector. The two mirrors on the bottoms left and right are the steering mirrors. However, these are used to control the horizontal and vertical alignment of the beam before placing the OPO. Our approach was to constrain the cavity axis prior to placing the OPO - we make sure the beam stays at constant height, send it to a camera and then mark the position of the beam on the TV (fig 2). The OPO cavity is placed so that the entry hole has the input beam centered and the exit hole aligns with the previous mark on the TV screen. Then, in theory, we only need one degree each of pitch and yaw (i.e. a rotation stage) to align the OPO to the cavity axis and match the incident and reflected beams. An illustration is shown in figure 3. As seen with the arrangement of the periscope, a yaw misalignment of the reflected beam when inspected at the prompt reflection translated to a pitch misalignment of the reflected beam when inspected past the periscope (fig 4).

Using the alignment setup described, we couldn't meet the alignment conditions. We tried again by moving the OPO assembly (and the OPO  curved HR surface) closer to the centre of rotation of the rotation stage. Actually, after all of this we found that the camera wasn't very stable on the mount as well, so we fixed it properly.

Initially we put the modulators on the edge of the table so that their connecting cables wouldn't get in the way during the experiment. However, in retrospect, it would have been better to put the OPO assembly on the edge of the table since the alignment of the OPO is the most delicate task.

Images attached to this report
2691_20210929092332_periscope20210927180455.jpg 2691_20210929092340_tvdot.jpg 2691_20210929093459_opoalignmentdrawing.png 2691_20210929093503_periscopedrawing.png
KAGRA MIR (Polarization)
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MarcEisenmann - 09:23, Wednesday 29 September 2021 (2693)Get code to link to this report
Comment to AZTEC sample measurement started (Click here to view original report: 2688)

This morning I put back the correct lockin parameters.

 

I started a measurement so that the polarization angle is close to 45 degrees.

This time, a new trouble with the HWP appeared : I can change the polarization angle (quite visible from the relative change of the p pol and s pol photodiodes) but the value on the angle value on the Kinesis software does not change.

I'll investigate this issue after all required measurements for this sample are finished.

KAGRA MIR (Polarization)
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MarcEisenmann - 00:31, Wednesday 29 September 2021 (2692)Get code to link to this report
Comment to AZTEC sample measurement started (Click here to view original report: 2688)

I did a series of measurements while changing the polarization angle by 90 degrees.

I did not recorded the required max/min of s and p polarizations to have accurate calibrations of the measurements.

So today I restarted measurements with incident p pol, s pol and started a 30 degrees polarization angle measurement.

However, there was another WIndows update... As it is not possible (yet?) to fully control the 2 lockin amplifiers from remote, I can not restart the measurement for today.

Furthermore, the HWP2 controller is not recognized by the software after acting strangely in the past days (only jog by 1 degree otherwise it resets the current angle to 0 and still move by 1 degree...)

 

For the new measurement a possibility could be to start by an absorption measurement before switching to birefringences ones.

This would assure 100 % that the orientation of the sample during all measurements is the same.

R&D (FilterCavity)
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MichaelPage - 21:41, Monday 27 September 2021 (2690)Get code to link to this report
OPO replacement - input coupler, OPO electronics assembly

Yuhang and Michael

We assembled the input mirror assembly for the OPO cavity as per 812. The only thing to mention here is the orientation of the input coupler convex surface (fig 4 and 5).

We then connected the interface electronics for controlling the Peltier, thermistor and piezo. The Peltier, thermistor and piezo each have two connecting wires that must be soldered onto whatever means we are using to connect them to their controllers. We soldered these onto a PCB connector. The Peltier and thermistor are connected to a DSub-9 cable going to the Thorlabs temperature controller (Peltier +ve pin4, -ve pin 5, thermistor +ve pin 2, -ve pin 3). The piezo wires were soldered to a LEMO F port.The connecting wires had to be soldered outside the cleanroom - the OPO cavity and input coupler assembly were placed in plastic zip lock bags and sealed so that only the wires were coming out (fig 6). This way they could be protected from fumes and dust.

The Peltier and thermistor were tested using the temperature controller. We saw that we could stabilise the resistance to ~10 kOhm. The piezo also made the expected high-pitched noise when it was actuated (~ 2 kHz test signal).

Images attached to this report
2690_20210927142943_20210916162240.jpg 2690_20210927142951_20210916163449.jpg 2690_20210927142958_20210916164003.jpg 2690_20210927143005_20210916172220.jpg 2690_20210927143012_20210916172335.jpg 2690_20210927143046_20210924184302.jpg