LOG-IN
Displaying reports 841-860 of 3273.Go to page Start 39 40 41 42 43 44 45 46 47 End
KAGRA MIR (General)
Print this report.
MarcEisenmann - 15:00, Friday 04 February 2022 (2829)Get code to link to this report
Check of power fluctuations

Katsuki, Marc

Recently we found out that there are large stripes visibles in the birefringence measurements.

Furthermore, if we check either the raw or normalized s and p polarizations power, their sum is not at all constant (see figure 1).

We installed a power meter at the beginning of the imaging unit and measured the pump power without sample (fig2) with sample (fig 3) and with sample moving as a birefringence measurement (fig 4).

The power is not stable at all...

While we could see something like +/- 1 % fluctuations during the polarization calibration, we can see that the long term peak to peak fluctuations seems to be around +/- 10 % during 30min and +/- 20 % during a birefringence measurement.

This explains why we see the stripes and why the sum of s and p polarizations power is not constant during a birefringence measurement.

Note that this large power fluctuations does not affect drastically the birefringence measurements as we don't see the stripes in them.

Furthermore, it seems that these power fluctuations are far more important at low power compared to high power (few watts for absorption measurements) because we can not see the stripes in these measurements.

Another by-product of this measurement is that we could estimate the background level of each PSD to be about 1uV.

Images attached to this report
2829_20220204042733_pol45signals.png 2829_20220204065727_nosample.png 2829_20220204065731_sample.png 2829_20220204065735_movingsample.png
R&D (FilterCavity)
Print this report.
NaokiAritomi - 17:34, Thursday 03 February 2022 (2828)Get code to link to this report
Input oplev spectra after evacuation

After the evacuation of input chamber, I aligned the input oplev by tweaking the steering mirror just after the oplev laser source.

Then I measured the input oplev spectra as shown in the attached figure. The input pitch and yaw oplev spectra look very similar now.

I checked the oplev beam height at the injection, readout viewports. The oplev beam height at the injection, readout viewports were 110mm, 106mm, respectively. I tweaked the injection steering mirror and made the both beam height 110mm, but the pitch and yaw oplev spectra still look very similar.

Images attached to this report
2828_20220203093412_20220203input.png
R&D (FilterCavity)
Print this report.
NaokiAritomi - 15:23, Thursday 03 February 2022 (2827)Get code to link to this report
Comment to A magnet of input mirror fell down (Click here to view original report: 2800)

Before I opened the gate valves between input/BS and input/arm, the pressures in input, BS, arm was 1.3e-6 mbar, 9.9e-10 mbar, 3.1e-8 mbar, respectively.

First I opened the gate valve between input/BS. After 1 hour, the pressures in input and BS chambers became 5.5e-7 mbar and 1.9e-8 mbar, respectively.

Then I opened the small/large gate valves between input/arm. The pressures in input, arm became 5.4e-7 mbar,4.5e-7 mbar, respectively.

R&D (FilterCavity)
Print this report.
YuhangZhao - 17:19, Wednesday 02 February 2022 (2825)Get code to link to this report
P-pol matching condition to old OPO

Michael and Yuhang

18.2% power is not coupled.

Images attached to this report
2825_20220202091859_wechatimg786.jpeg 2825_20220202091907_wechatimg785.jpeg 2825_20220202091916_wechatimg784.jpeg 2825_20220202091925_wechatimg783.jpeg 2825_20220202091932_wechatimg782.jpeg
R&D (FilterCavity)
Print this report.
YuhangZhao - 17:13, Wednesday 02 February 2022 (2823)Get code to link to this report
BAB matching condition to old OPO

Michael and Yuhang

We checked the mode matching condition between BAB and OPO. 13.2% power is not coupled.

Images attached to this report
2823_20220202091234_wechatimg787.jpeg 2823_20220202091241_wechatimg788.jpeg 2823_20220202091247_wechatimg789.jpeg 2823_20220202091253_wechatimg790.jpeg 2823_20220202091259_wechatimg791.jpeg
R&D (FilterCavity)
Print this report.
NaokiAritomi - 16:18, Wednesday 02 February 2022 (2822)Get code to link to this report
Comment to A magnet of input mirror fell down (Click here to view original report: 2800)

I started the evacuation of input chamber. First I used rotary pump until the pressure in the input chamber reaches below 0.1mbar. After I removed the rotary pump, I closed the small gate valve close to arm and opened the small gate valve close to the input chamber. I will wait until the pressure in the input chamber reaches the similar one in the BS chamber.

R&D (FilterCavity)
Print this report.
MichaelPage - 14:14, Wednesday 02 February 2022 (2821)Get code to link to this report
OPO replacement - Mokulab unit strange behaviour

Yuhang and Michael

We found an issue with the Mokulab unit used in the ATC cleanroom

We used 100 Hz 10 dBm 1Vpp signal from another function generator. Putting the signal into Mokulab IN2 and using the oscilloscope function shows no frequency signal and 4 mV offset. IN1 reads 9Vpp (+5.4, -3.6) at 118 MHz even with no connection.

Using 1 MHz signal into the spectrum analyzer function likewise shows no signal, just -131 dBm floor. Using a T connector from the function generator to oscilloscope and Mokulab, we see that the signal on the oscilloscope is reduced when switching from Moku IN2 to IN1, but no change when switching IN1 input impedance between 50 Ohm and 1 MOhm.

Mokulab function generator output works fine though, we have been using it to scan the cavity.

KAGRA MIR (Polarization)
Print this report.
MarcEisenmann - 09:53, Wednesday 02 February 2022 (2820)Get code to link to this report
Comment to stripes in polarization measurement (Click here to view original report: 2809)

I have now taken 3 measurements with s polarization at the input that saturated the lockin amplifier..

It seems that we can really easily saturates the p polarization.

Indeed, it is connected to the old lockin amplifier where the range (0 to 1 V) is changed depending on the sensitivity setting we are using.

Now I'm injecting about 160 uW of power but when doing the measurement with s polarization it seems that the p polarization power changes by more than a factor 14...

I'm starting hopefully the last measurement with s polarization at the input where the sensitivity of the old lockin is set to 100 mV despite the value at the center being 0.2 mV.

It would be convenient to have a new lockin amplifier to avoid this issue...

KAGRA MIR (General)
Print this report.
MarcEisenmann - 09:45, Wednesday 02 February 2022 (2819)Get code to link to this report
Comment to from TWE to birefringence (Click here to view original report: 2816)

For easier comparison with direct measurement with PCI (see elog 2755), I show here the absolute value of delta n flipped both horizontally and vertically .

It seems that the larger delta n area have somehow a close triangular shape.

Images attached to this comment
2819_20220202014603_dnunwrapflip.jpg
KAGRA MIR (Polarization)
Print this report.
MarcEisenmann - 14:03, Tuesday 01 February 2022 (2817)Get code to link to this report
Comment to stripes in polarization measurement (Click here to view original report: 2809)

I had a look at the normalized Is and Ip data.

As seen in figures 1 and 2 which show respectively the s and p polarizations normalized intensities the stripes are mainly present in s polarization.

This was not the case for the previous measurements (see figures 3 and 4) were stripes were actually visibles in both s and p polarizations...

Also it seems that p polarization is saturating..

Images attached to this comment
2817_20220201060331_pol0isstripes.png 2817_20220201060335_pol0ipstripes.png 2817_20220201060343_pol0isstripes.png 2817_20220201060347_pol0ipstripes.png
KAGRA MIR (Polarization)
Print this report.
MarcEisenmann - 13:52, Tuesday 01 February 2022 (2816)Get code to link to this report
from TWE to birefringence

Recently I've been trying to compute birefringence from TWE measurements of spare ETMY based on Aso-san's computation.

I'm using the S1thruS2 measurements with roll angle of the mirror of 45, 90, 135, 225, 270 and 315 deg with 20 measurements averaged.

The code I wrote does the following :

1) Find the real center and roll angle of each TWE maps

Hirose-san who did the TWE measurements at Caltech placed 3 markers on the mirrors.

First I overlapped 3 circles on the markers of the map with roll angle of 90 deg as it is the same orientation as the PCI measurement.

Then, I changed the centering of all other maps + rotated them to match the circles positions of the 90 deg one.

See figures 1 to 6 for the TWE maps (piston, tilt and curvature removed) without rotation and 7 to 11 for the rotated maps.

2) Sanity check of the RoC

OSCAR is used to removed the piston, tilt and focus of the TWE measurements but states that the removed RoC is about -716 m..

This is actually due to the Fizeau interferometer setup. Computing the RoC taking into account the clear aperature and position of the reference sphere gives a mean RoC = 1.9 km (as expected).

Especially, we recovered the same RoC as measured by Hirose-san with 270 deg roll angle.

3) Combining TWE maps into birefringence

Using 4 rotated maps, it is then possible to compute the spare ETMY birefringence (delta n and theta the fast axis orientation) as in figure 12.

Actually, because there is an arctan(2*theta) used, theta is only defined between -pi/4 and pi/4 that causes some wrapping of theta (and therefore delta n as well).

So in figure 13 I used an unwrapping algorithm to try to remove this wrapping. Results are reported in figure 13.

We can recognize so similar patterns to the measurements with the PCI setup. Final conclusion should be done after a new direct measurement with the beam at normal incidence).

4) Next steps

- Tune the unwrapping algorithm -> still some issue at the bottom of the map

- Check the orientation of the mirror during PCI and TWE measurements to understand why there seems to be both a vertical and horizontal flip with respect to each other

- Finalize the direct measurement at normal incidence

Images attached to this report
2816_20220201054403_90.jpg 2816_20220201054407_45.jpg 2816_20220201054411_135.jpg 2816_20220201054416_225.jpg 2816_20220201054420_270.jpg 2816_20220201054424_315.jpg 2816_20220201054428_45rotated.jpg 2816_20220201054432_135rotated.jpg 2816_20220201054439_225rotated.jpg 2816_20220201054443_270rotated.jpg 2816_20220201054446_315rotated.jpg 2816_20220201054929_dntheta.jpg 2816_20220201054935_dnthetaunwrap.jpg
Comments related to this report
MarcEisenmann - 09:45, Wednesday 02 February 2022 (2819)

For easier comparison with direct measurement with PCI (see elog 2755), I show here the absolute value of delta n flipped both horizontally and vertically .

It seems that the larger delta n area have somehow a close triangular shape.

R&D (FilterCavity)
Print this report.
RyutaroTakahashi - 22:46, Monday 31 January 2022 (2815)Get code to link to this report
Comment to Two magnets of end mirror fell down (Click here to view original report: 2812)

Picture of the mirror without magnets.

Images attached to this comment
2815_20220131144514_em2magnet.jpg
R&D (FilterCavity)
Print this report.
RyutaroTakahashi - 22:44, Monday 31 January 2022 (2814)Get code to link to this report
Comment to A magnet of input mirror fell down (Click here to view original report: 2800)

Pictures of gluing.

Images attached to this comment
2814_20220131144222_nm2gluing1.jpg 2814_20220131144240_nm2gluing2.jpg 2814_20220131144254_nm2gluingafter.jpg
R&D (FilterCavity)
Print this report.
NaokiAritomi - 14:48, Monday 31 January 2022 (2813)Get code to link to this report
Comment to END mirror oplev/actuation investigation (Click here to view original report: 2808)

Since the two magnets of end mirror fell down, this measurement does not make sense. I brought back the rotation angle for END oplev to 0 deg.

R&D (FilterCavity)
Print this report.
NaokiAritomi - 14:41, Monday 31 January 2022 (2812)Get code to link to this report
Two magnets of end mirror fell down

[Takahashi, Aritomi]

Since there is a new 6.35Hz peak in END oplev spectra as reported in elog2808, we opened the end chamber and checked the suspension. We found that two magnets of end mirror fell down! This is the reason why the Z correction does not work recently. Takahashi-san will glue the magnets next Monday.

Comments related to this report
RyutaroTakahashi - 22:46, Monday 31 January 2022 (2815)

Picture of the mirror without magnets.

RyutaroTakahashi - 22:36, Monday 07 February 2022 (2833)

One magnet (upper) was glued with the jig and released 3 hours later. The other magnet (left) is under gluing. It will be released on the 14th.

RyutaroTakahashi - 11:36, Monday 14 February 2022 (2837)

The other magnet (left) was released. The TM was released and the chamber was closed.

R&D (FilterCavity)
Print this report.
NaokiAritomi - 14:36, Monday 31 January 2022 (2811)Get code to link to this report
Comment to A magnet of input mirror fell down (Click here to view original report: 2800)

Takahashi-san glued the magnet to the input mirror and closed the input chamber. Since it takes one day for the glue to be fixed, we will evacuate the input chamber after tomorrow.

R&D (FilterCavity)
Print this report.
NaokiAritomi - 01:20, Monday 31 January 2022 (2810)Get code to link to this report
Comparison of CCFC error signal on 20210622 and 20211227

The attached figure shows the CCFC error signal on 20210622 and 20211227. The elogs on 20210622 and 20211227 are elog2597 and elog2770, respectively.

Images attached to this report
2810_20220130172047_ccfc202106221227.png
KAGRA MIR (Polarization)
Print this report.
MarcEisenmann - 19:18, Friday 28 January 2022 (2809)Get code to link to this report
stripes in polarization measurement

I checked the first measurement of the shinkosha 7 with s polarization at the input,

As shown in figure 1 there are some vertical stripes present in the measurement.

I tuned both the hwp and qwp in the injection and found out that when injecting s polarization, the p polarization readout is minimized for hwp = 0.1 deg instead of previously 1.3 deg.

Then, I also added beam dump to catch the PSD reflections and a small wall to isolate the imaging unit from the injection part.

The beam dump were removed because they are supposed to be used for visible light...

In any case the good news is that we can recognize similar patterns to the previous measurement with tilted beam.

Finally I restarted the s polarization measurement.

Images attached to this report
2809_20220128111810_shinkosha7stripes.png
Comments related to this report
MarcEisenmann - 14:03, Tuesday 01 February 2022 (2817)

I had a look at the normalized Is and Ip data.

As seen in figures 1 and 2 which show respectively the s and p polarizations normalized intensities the stripes are mainly present in s polarization.

This was not the case for the previous measurements (see figures 3 and 4) were stripes were actually visibles in both s and p polarizations...

Also it seems that p polarization is saturating..

MarcEisenmann - 09:53, Wednesday 02 February 2022 (2820)

I have now taken 3 measurements with s polarization at the input that saturated the lockin amplifier..

It seems that we can really easily saturates the p polarization.

Indeed, it is connected to the old lockin amplifier where the range (0 to 1 V) is changed depending on the sensitivity setting we are using.

Now I'm injecting about 160 uW of power but when doing the measurement with s polarization it seems that the p polarization power changes by more than a factor 14...

I'm starting hopefully the last measurement with s polarization at the input where the sensitivity of the old lockin is set to 100 mV despite the value at the center being 0.2 mV.

It would be convenient to have a new lockin amplifier to avoid this issue...

R&D (FilterCavity)
Print this report.
NaokiAritomi - 19:06, Friday 28 January 2022 (2808)Get code to link to this report
END mirror oplev/actuation investigation

Recently, a 6.35Hz peak is visible in END pitch and yaw oplev spectra (Fig 1). For END oplev diagonalization, I changed the rotation angle for END oplev so that the 6.35Hz peak disappears in oplev yaw spectrum, assuming that the 6.35Hz peak is a natural pitch peak. I changed the oplev rotation angle from 0 deg to 1 deg. The END oplev spectra before/after this rotation are shown in Fig 2 (red, blue: after rotation, green, brown: before rotation).

To check END actuation, I put an excitation (12 Hz, amplitude 1000, sine wave) in END length (K1:FDS-END_LEN_ex2). The 12 Hz peak is visible in both pitch and yaw oplev spectra (Fig 3). The 12 Hz peak height was 13.5 and 20.8 for pitch and yaw, respectively. The current EUL2COIL matrix is shown in Fig 4. This matrix might not be optimized for L2P, L2Y coupling.

Images attached to this report
2808_20220128110635_20220124end.png 2808_20220128110647_20220128end.png 2808_20220128110652_20220128endexc.png 2808_20220128110656_20220128endeul2coiloriginal.png
Comments related to this report
NaokiAritomi - 14:48, Monday 31 January 2022 (2813)

Since the two magnets of end mirror fell down, this measurement does not make sense. I brought back the rotation angle for END oplev to 0 deg.

R&D (FilterCavity)
Print this report.
YuhangZhao - 13:28, Friday 28 January 2022 (2807)Get code to link to this report
An estimation of new OPO internal losses

In the case of a rigid cavity, we can estimate internal losses without locking. We just need to scan cavity and look for the reflection signal as shows in Fig.1.

1. We scan cavity and know that about gamma = 5% power is not coupled to cavity for TEM00 resonance.

2. We take the reflected power when cavity is on resonance for TEM00 (33.2mV) and off resonance (36.6mV)

3. We get Rcav = ((33.2/36.6)-gamma)/(1-gamma)

4. RTL = T1*(1-Rcav)/2/(1+Rcav) = 0.206%, here T1 = 0.08. Note: the polishing/coating company (LASEROPTIK) specifies AR coating reflectivity is less than 0.1%.

5. escape efficiency is T1/(T1+L)

In this way, we get escape efficiency of 97.5% for the new OPO.

Images attached to this report
2807_20220128051742_wechatimg781.jpeg