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R&D (FilterCavity)
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EleonoraCapocasa - 18:32, Tuesday 10 December 2019 (1925)Get code to link to this report
PItch BS channel showing higher noise. Why?

PItch BS channel shows an excess of noise. Damp loops are open and even if I remove DC on coils for the aligment, noise is still there.

This was observed serveral times recently and after a while it goes back by itself. I think it is something electronic, but what?

 

Images attached to this report
1925_20191210103129_15.png
R&D (FilterCavity)
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YuhangZhao - 17:17, Tuesday 10 December 2019 (1924)Get code to link to this report
Remove of residual p-pol component from LO and BAB

Yaochin and Yuhang

As we reported in elog1867 and elog1857, we improved the matching between LO/BAB into AMC. However, we didn't care about the residual p-pol component after the optimization. And actually, it is really necessary to optimize them and remove the p-pol component.

LO part (The AMC spectrum before the change is attached as picture 2) (s-pol 11V, p-pol 14mV)

     Actually, I am confused that how can we have a p-pol component from LO. Because LO is provided by IRMC TEM00, TEM00 should provide a quite clean s-pol light. 

     1. We replaced the first mirror after IRMC with a PBS plate.

             After this, the p-pol peak is reduced from 14mV to 9mV(attached picture 3). (We also double-checked that total power doesn't change after the replacement of PBS, so this p-pol reduction is a real      reduction effect from PBS)

     2. We put an HWP just before homodyne BS.

            By rotating HWP, we could almost remove the p-pol component totally(attached picture 4).

BAB part (The AMC spectrum before the change is attached as picture 5) (s-pol 4V, p-pol 43.2mV)

     For the p-pol component inside BAB, it comes from the not optimized HWP. So we just rotate HWP. And then the p-pol is basically removed totally. (attached picture 6)

BAB HWP angle

286.5

LO HWP angle

178

We measured the squeezing spectrum before and after this change, but there is no obvious change.

Images attached to this report
1924_20191210084948_removeppol.png 1924_20191210091935_tek00086.png 1924_20191210092014_tek00089.png 1924_20191210092043_tek00095.png 1924_20191210092102_tek00090.png 1924_20191210092114_tek00091.png
R&D (FilterCavity)
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YuhangZhao - 16:23, Tuesday 10 December 2019 (1923)Get code to link to this report
About DC balance of homodyne

Yaochin and Yuhang

We found we could balance homodyne by aligning the flipping mirror and the lens before the far 'eye' of homodyne. (As shown in the attached figure)

By aligning pitch/yaw of flipping mirror and pitch of lens, we could also recover the balance of homodyne.

Images attached to this report
1923_20191210082340_alignhomodyne.png
R&D (FilterCavity)
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EleonoraCapocasa - 10:58, Tuesday 10 December 2019 (1922)Get code to link to this report
Python scripts from MEDM: issue solved!

Today Miyakawa-san managed to solve the long-lasting problem we had to run python script called by medm button (see entry #1656).  

He modified the command used by the medm desktop icon to call medm to: bash -c 'source /kagra/apps/etc/client-user-env_tama.sh && cd /opt/rtcds/kamioka/k1/medm && /opt/rtapps/epics/extensions/bin/linux-x86_64/medm -x sitemap.adl'

Now the command is also calling a script he made (/kagra/apps/etc/client-user-env_tama.sh) to include all the needed evironmental variables.

Somehow when opening MEDM with this command the PV info on the channel cannot be seen anymore. The icon MEDM (edit) was not changed so, by using that one, we can still read PV info ( but not run python scripts) 

Conlusion: we can now run python screep from MEDM screen open by desktop icon, and this should help to better manage control loops, while we wait for guardians.

R&D (FilterCavity)
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YuhangZhao - 10:40, Tuesday 10 December 2019 (1921)Get code to link to this report
Cable connection problem for CC1 loop

Yuhang and Yaochin

We reported sometimes the CC1 loop cannot be locked.

Today we found the cable which is sending error signal for the loop has some connection problem. When we shake the cable, the error signal sent to the loop got a lot of noise.

We have already replaced it with a new cable. We checked the new cable doesn't introduce noise when we shake it.

R&D (Cryogenic)
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SatoshiTanioka - 21:00, Monday 09 December 2019 (1920)Get code to link to this report
Log on Dec. 9th

[Optics]
I adjusted the lenses' positions for mode matching.
I tried to measure the beam profile inside the cryostat chamber, but it was too difficult to measure the distance.
Fortunately, some amount of the beam was reflected by a PBS in front of the chamber due to the imcomplete alignment of FI and it propagets on the optical table.
The profile of this kicked beam is almost same as the beam which incoming to the chamber.
Therfore I will use this beam to measure the beam profile.

[Cryostat]
I assembled another window for 80K shield as attached picture.
I am planning to use two 80K shield windows for my experiment.

[Next Step]
Measure the beam profile.
Install a FP cavity to characterize fused silica mirrors.

Images attached to this report
1920_20191209124923_20191208window.jpg
KAGRA MIR (Absorption)
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SimonZeidler - 19:12, Monday 09 December 2019 (1919)Get code to link to this report
Reflectance Measurement Bench in TAMA

Simon

I have set up a measurement bench in TAMA to easily and fastly take reflection data of a 1064nm laser on samples (mostly optics, I guess) as a function of the angle of incidence (from 0 to 90 degrees) and input polarization.
The system works fine but it still not entirely finished. For example, we plan to install a rotation-gear on the angular rotator to compensate the 2*AoI effect, so that a manual change of the PD won't be necessary anymore.

Especially today, I was trying to further understand the laser. I recognized that the used PD cannot measure powers more than 8mW (which is strange as there is a threshold of 50mW written on it...). But putting the laser at such low power-gains, the stability of the laser is not good at all. Therefoe, I was inserting a ND-filter in front of the laser and increased the gain so that the laser-power is stable (change of power after 10 minutes <1%).

After setting up the laser, I tested the system with a Brewster-polarizer (TFP-1064-pw-2037-uv) which we use for the PCI. The input power for the measurements was set for both S and P polarization to 6.53mW.
Please see the attached graphic which illustrates the results. For P-pol, a minimum at 63 degrees was found (R = 3.5%), while for S-pol, the reflectance did not change much at all over the entire measured range (which is somehow expected, I guess).

Please note that the data taken at 80 degrees AoI are probably not very accurate, since I believe that the beam was clipped (I need to check this further, maybe installing a lens is better).

Images attached to this report
1919_20191209112831_reflectionplot.png
R&D (Cryogenic)
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SatoshiTanioka - 17:01, Sunday 08 December 2019 (1917)Get code to link to this report
80K shield window assembling

Today I assembled a window for 80K shield with 1~1.5 um broadband AR coated glass.
After that I found that a washer for M4 screw cannot go through the though hole, and it is a little bit difficult to install on 80K shield.
I will ask Ueda-san (KEK) about this.

Images attached to this report
1917_20191208085715_20191208window.jpg
R&D (FilterCavity)
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YuhangZhao - 00:24, Sunday 08 December 2019 (1916)Get code to link to this report
Measurement of loss and phase noise(SQZ and ASQZ @20191206)

Yuhang and Yaochin

Firstly, we checked the amplification of BAB with 60mW. The factor is around 30. While the characterization we did last year shows amplification of roughly 60.

Then we measured SQZ and ASQZ at different green power

Green power(mW)

OPO T (kOhm)

PLL-pol (MHz)

CC1 error signal pk-pk (mV)

CC2 demodulation phase (SQZ)

CC2 demodulation phase (ASQZ)

60mW

7.23

170

49.2

124

130

55mW

7.227

170

40

118

138

50mW

7.217

170

37.5

115

139

45mW

7.211

170

31.2

110

145

40mW

7.205

175

30.8

110

150

35mW

7.201

180

26.4

105

155

30mW

7.196

185

23.2

100

155

25mW

7.189

185

21.6

90

155

From the above data, loss is 25.1% and phase noise is 19.4mrad. The loss is consistent with Aritomi-san's result. While the phase noise is a bit reduced.

We also measured the CC2 phase noise. The measurement is done with a 40mW green power and 110deg CC2 demodulation phase. Then we got CC2 pk-pk 62.4mV. We use this for calibration and got a phase noise of 4.25mrad.

Images attached to this report
1916_20191207162401_sqzfit.png 1916_20191210120428_phasenoise.png
R&D (FilterCavity)
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EleonoraCapocasa - 14:59, Friday 06 December 2019 (1915)Get code to link to this report
Seismic noise comparison Kagra, Virgo, TAMA (day and night)

[Camilla, Irene Federico]

Images attached to this report
1915_20191206065937_dayvsnightkagratamavirgo.png
R&D (FilterCavity)
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AyakaShoda - 12:55, Friday 06 December 2019 (1914)Get code to link to this report
PR Pitch local control updated

I updated the control filter for the PR PIT.

The old filter is in ASC2G and notches.

The new filter works with the filters, test and boost2, with the gain of 1.0. The residual decreases more than 10 times wink

Images attached to this report
1914_20191206045502_speprp191206.png
Comments related to this report
AyakaShoda - 22:24, Tuesday 10 December 2019 (1928)

Attached is the designed OLTF of the previous and the new servoes on Dec 6th.

The phase mergin is about 40 deg. The difference of gain at above the UGF is about 10 dB.

Also, I have tried to look up the time the PR was resonating (at around 6/12/2019 6:00 UTC), but I could not find any DAQ signal for PR local damping loop.
Why don't we add some (if the storage allows)?

R&D (FilterCavity)
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YuhangZhao - 11:56, Friday 06 December 2019 (1913)Get code to link to this report
one of the reasons for AMC misalignment

Yuhang and Yaochin

We should put AMC offset always at 150V, because different offset will result in different alignment condition.

Attached three pictures show the situation of AMC's offset as 40V, 150V and 240V. We could see quite different alignment situation.

Images attached to this report
1913_20191206035620_img20191206112912.jpg 1913_20191206035625_img20191206112942.jpg 1913_20191206035629_img20191206113029.jpg
R&D (FilterCavity)
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EleonoraCapocasa - 13:55, Thursday 05 December 2019 (1912)Get code to link to this report
Seismic noise results from trillium seismomenter placed on TAMA floor
 
[Irene, Camilla, Federico]
 
Some conclusion drawn from data taken with a trillium seismomenter placed on TAMA floor (behind squeezing clean room, below mode cleaner pipe).
 
1) Figures 1, 2, 3 show spectrograms (GPS is in UTC). Only for the day 21/11 we have 24h of data.
 
2) Noise between 1-30 Hz changes between day and night. Figure 4 highlights it.
 
3) There is a device that turns off/off every ~ 8 minutes, which produces the peaks at 24.5 Hz (fan? air conditioning? pump?). See plot 5.
 
4) Figure 6 shows the percentiles calculated on a day. Some other non-stationary peaks, in addition to that at 24.5 Hz, are clearly visible
 
5) Comparing trillium spectrum with the TEAC seismometer we have in TAMA it seems the TEAC is useful only between 10Hz and 50 Hz. Its own noise dominates below 10Hz, while ADC noise dominates above 50Hz (To Be Confirmed) - Plot to be posted.
 
 
Good face to face!Figures 1, 2, 3 are spectrograms (GPS is in UTC). Only for the
November 21 we have 24h of data.
 
1) you see the peak around 10 Hz that you told us about. In reality
it is very wide, between 1-30 Hz, and from the spectrograms we see that it "breathes"
between day and night. Figure 4 highlights it, they are two spectra:
one by day, the other by night.
 
2) There is a device that turns off / on every 8 minutes or so, which makes the
peaks at 24.5 Hz (one fan? air conditioning? pump?). See plot 5.
 
3) Figure 6 is the percentiles calculated on a day. They look good
some non-stationary peaks, beyond that at 24.5 Hz.
 
That's all. We have no more precise conclusions, it should be understood
which are the devices that generate the peaks, but we have had no way
to analyze the data in time to do so. :)
 
Good face to face!
Images attached to this report
1912_20191205054737_191120trilliumzspectrogram.png 1912_20191205054743_191121trilliumzspectrogram.png 1912_20191205054749_191122trilliumzspectrogram.png 1912_20191205054912_seismometerdayvsnightfftz.png 1912_20191205054946_peak24hz.png 1912_20191205055022_percentiles21nov.png
R&D (FilterCavity)
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EleonoraCapocasa - 13:22, Thursday 05 December 2019 (1911)Get code to link to this report
FC lock not stable

[Yuhang, Matteo, Eleonora]

On Tue 3/12 morning we found the FC has difficulties to acquire the lock and to keep it, while in the past months lock was very robust and easy to get.

After some investigation (and having tweeked the gain of ramepeato) we found the input power was reduced from 12 mW to 9 mW, due to temperature change of SHG.

The day before the air conditiong was switched from summer to winter mode by Yuhang.

The injected power was put back to 12mW and the gains were tuned to get UGF ~ 15 kHz.  (See pic 1 and 2). Anyway it seems a loop oscillation happened from time to time and error signal looks noisier than usual. It was quite late and we coudn't keep investingating any longer. We haven't been in TAMA yesterday and today because of F2F.  Will check the situation tomorrow.

Images attached to this report
1911_20191205051708_tf.jpeg 1911_20191205051734_gain.jpeg
R&D (FilterCavity)
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EleonoraCapocasa - 11:47, Thursday 05 December 2019 (1910)Get code to link to this report
Comment to Mode mis-matching between filter cavity(FC) and local oscillator(LO) (Click here to view original report: 1905)

The main effect causing degradation of the overlap between LO and reflected beam form FC when it is ON and OFF resonance is the relative phase change between TEM 00 (resonating the cavity) and HOM (not resoanting). Raffaele did a quick calculation to show this and the numbers he found are in rough agreement with those we observed. I attached a pdf with a similar calulation and a plot that shows the overlap degradation as a function of the not coupled power into FC. 

Non-image files attached to this comment
R&D (General)
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EleonoraCapocasa - 11:35, Thursday 05 December 2019 (1909)Get code to link to this report
FC dithering loops implemented for YAW

[Eleonora, Matteo, Raffaele]

On 29/11 dIthering was implemented also in Yaw, with the same scheme used for pitch.

Dithering lines are injected on INPUT and END mirrors at a frequency of 16.5 Hz and 17.5 Hz respectively. Each error signal obtained from transmitted power demodulation is filtered with a simple integrator and fed back to its own mirror.

From the time taken by the loop to recover the alignemnt after misalignig a mirror on purpose, the UGF seems smaller 50 mHz. I tried to measure openloop TF with a swep sine injection at very low frequency but coherence was not good, no matter the excitation amplitude.

Note that with the current filter configuration (simple integrator) the UGF of dithering is limited by the interaction with the damping loops. See attached simulation. We discussed the possibiliy to shape the filter to avod the instabilty. Anyway since damping UGF is quite high ~1 Hz. in the present configuration the sum of the two loops is stable. Another possibility would be to go back to DC controlled optical lever and add the dithering DC correction to the set point of this loop. I think this is what is done in Virgo.

Images attached to this report
1909_20191205033454_tfcross.png
R&D (Cryogenic)
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SatoshiTanioka - 18:56, Tuesday 03 December 2019 (1908)Get code to link to this report
Log on Dec. 3rd

I put fused silica mirrors inside the cryostat chamber in order to construct a FP cavity with cavity length od 9.9cm.
Then I injected a laser into the cavity and tried to see the flash with PD which is located at transmission port.
So far I could not see any transmitted beam.

I will improve the alignment and mode matching with two lenses.

R&D (FilterCavity)
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YuhangZhao - 10:11, Tuesday 03 December 2019 (1907)Get code to link to this report
FDS (anti-squeezing~9dB rotates to squeezing~1dB in filter cavity) @ 2kHz

Yaochin and Yuhang

We see anti-squeezing rotates to squeezing @2kHz. But the filter cavity was really unstable.

average: 50 times

Setting of hand-fit parameters:

sqz_dB = 9.5;                      % produced SQZ

L_rt = 105e-6;                    % FC losses

L_inj = 0.17;                     % Injection losses

L_ro = 0.1;                      % Readout losses

A0 = 0.05;                         % Squeezed field/filter cavity mode mismatch losses

C0 = 0.03;                        % Squeezed field/local oscillator mode mismatch losses

ERR_L =   5e-12;                   % Lock accuracy [m]

ERR_csi = 50e-3;                  % Phase noise[rad]

phi_Hom = [-1/180*pi, -11/180*pi, -75/180*pi];         % Homodyne angle [rad] (you can input a vector of values)

det =  2e3;                       % detuning frequency 

int = 0.8e3;                         % frequency range = det+/-int 

 

Setting of shot noise level/detuning error parameters:

 

semilogx(fd+34, d_a1+133.5,'k','LineWidth',3) %squeezing to anti-squeezing

hold on

semilogx(fd+32, d_a2+133.5,'LineWidth',3) %anti-squeezing to squeezing

hold on

semilogx(fd+150, d_a3+133.5,'LineWidth',3) %intermediate

Images attached to this report
1907_20191203021515_fds.png
R&D (FilterCavity)
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NaokiAritomi - 15:06, Saturday 30 November 2019 (1906)Get code to link to this report
FDS on 20191129

[Aritomi, Yuhang, Yaochin, Eleonora]

First we measured frequency independent squeezing with filter cavity (Pic. 1). We had 3.5dB squeezing down to 80Hz with filter cavity.

Then we alined BAB to AMC with 1kHz filter cavity detuning and measured FDS (Pic. 2). Fitting parameters are follows. It seems that detuning changed for squeezing and anti squeezing measurement.

CC2 demodulation phase
sqz: 75 deg, asqz: 130 deg, intermediate: 100 deg
 

sqz_dB = 13;                      % produced SQZ

L_rt = 100e-6;                    % FC losses

L_inj = 0.20;                     % Injection losses

L_ro = 0.11;                      % Readout losses

A0 = 0.1;                         % Squeezed field/filter cavity mode mismatch losses

C0 = 0.1;                         % Squeezed field/local oscillator mode mismatch losses

ERR_L =   5e-12;                  % Lock accuracy [m]

ERR_csi = 80e-3;                  % Phase noise[rad]

phi_Hom = [-5/180*pi, pi/2];      % Homodyne angle [rad] 

det =  [1074 1004];               % detuning frequency [Hz]

cavity_pole = 59.6;               % cavity pole (Hz)

 

We measured FDS again with smaller frequency span (Pic. 3). Fitting parameters are follows. This time, it seems that produced SQZ also changed in addition to detuning.

 

sqz_dB = [13.5 11 13.5];          % produced SQZ

L_rt = 100e-6;                    % FC losses

L_inj = 0.20;                     % Injection losses

L_ro = 0.11;                      % Readout losses

A0 = 0.05;                        % Squeezed field/filter cavity mode mismatch losses

C0 = 0.1;                         % Squeezed field/local oscillator mode mismatch losses

ERR_L =   5e-12;                  % Lock accuracy [m]

ERR_csi = 80e-3;                  % Phase noise[rad]

phi_Hom = [-3/180*pi 70/180*pi 7/180*pi];       % Homodyne angle [rad] 

det =  [970 1005 965];                          % detuning frequency [Hz]

cavity_pole = 59.6;               % cavity pole (Hz)

Images attached to this report
1906_20191130070637_sqz20191129.png 1906_20191130070643_fds20191129.png 1906_20191130074217_fds20191129expand.png
R&D (FilterCavity)
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YuhangZhao - 02:19, Saturday 30 November 2019 (1905)Get code to link to this report
Mode mis-matching between filter cavity(FC) and local oscillator(LO)

Aritomi, Eleonora, Yaochin, and Yuhang

For the adjustment of OPO/FC matching and FC/LO matching, we always do the following.

1. Send BAB into the filter cavity. Align IR into the filter cavity while filter cavity alignment is kept in the best condition. Check IR 0/1/2 order modes by changing AOM frequency.

2. Align BAB reflection into AMC while the filter cavity is locked.

However, we found that the matching from BAB_ref into AMC is quite different when the filter cavity is locked and detuned. And we know that we measure FDS while FC is detuned, so we decide to align BAB_ref into AMC while FC is detuned. So now the procedure is as follows.

1. Send BAB into the filter cavity. Align IR into the filter cavity while filter cavity alignment is kept in the best condition. Check IR 0/1/2 order modes by changing AOM frequency.

2. Align BAB reflection into AMC while the filter cavity is detuned.

However, we are not very sure why the matching can be so different when FC is locked and detuned. Because I think the BAB_ref should be quite similar in both cases of lock and detuned since we had 94% of matching from OPO/FC. I put the reason for my thought as following. Please correct me if there is something wrong.

Images attached to this report
1905_20191129181900_wechatimg602.jpeg
Comments related to this report
EleonoraCapocasa - 11:47, Thursday 05 December 2019 (1910)

The main effect causing degradation of the overlap between LO and reflected beam form FC when it is ON and OFF resonance is the relative phase change between TEM 00 (resonating the cavity) and HOM (not resoanting). Raffaele did a quick calculation to show this and the numbers he found are in rough agreement with those we observed. I attached a pdf with a similar calulation and a plot that shows the overlap degradation as a function of the not coupled power into FC.