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R&D (Cryogenic)
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SatoshiTanioka - 19:47, Tuesday 30 July 2019 (1530)Get code to link to this report
Close cryostat chamber

So far I have worked with closed 80K shield, and without most outer shield of cryostat chamber.
Today I closed the most outer shield using crane.

Actually, it did not improve the PDH lock stability.
The viewport window on the most outer shield is detached in order to avoid scattered light.
So this may cause acoustic fluctuation.

R&D (FilterCavity)
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NaokiAritomi - 19:20, Tuesday 30 July 2019 (1529)Get code to link to this report
Large bump in shot noise spectrum at low frequency

We often have large bump in shot noise spectrum like an attached picture. Note that squeezing path is blocked.

Images attached to this report
1529_20190730122001_img7715.jpg
R&D (FilterCavity)
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YuhangZhao - 11:26, Tuesday 30 July 2019 (1528)Get code to link to this report
The effect of turbo pump for squeezing

Yuhang and Aritomi

It seems that the turbo pump just gives us a narrow peak at 600Hz. The on and off of it doesn't change squeezing level.

Images attached to this report
1528_20190730042544_turbopump.png
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YuhangZhao - 10:45, Tuesday 30 July 2019 (1527)Get code to link to this report
The measurement of coherence between squeezing and other signals

To see the contribution of noise at different frequencies, I performed the coherence measurement between squeezing and GRMC locking loop error signal/IRMC locking loop error signal/GRMC transmission signal/Green phase-locking error signal/IR phase-locking error signal.

The result is attached. From these results, we could have the following deduction:

  • GRMC locking loop is contributing the noise at 9.5kHz and 6.9kHz
  • The coherence between 3.7kHz and 6.9kHz shows up mainly in IR phase and IRMC locking.
  • It seems IR phase noise and IRMC locking loop has strong coherence. So I think we can improve IR phase behavior by improving IRMC locking.
  • 600Hz noise doesn't show up in the IRMC and GRMC locking loop.
  • Sometimes, the squeezing measurement is very good. For example, the one together with GRMC loop error signal. I attach the squeezing level at that time.

All the measurement is using averaging of the meachine of 200, I think we should use more average in the future.

Images attached to this report
1527_20190730034624_grmcloop.png 1527_20190730034630_irmcloop.png 1527_20190730034636_grmctransmission.png 1527_20190730034642_grphase.png 1527_20190730034649_irphase.png 1527_20190730040432_figure1.png
R&D (FilterCavity)
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EleonoraCapocasa - 10:40, Tuesday 30 July 2019 (1526)Get code to link to this report
Comment to Recovery of good squeezing (Click here to view original report: 1522)

The large increase of phase noise above 300 Hz when the CC2 is closed (pic 3) is very strange and we need to investigate it. The loop should have a UGF of few kHz, but it doesn't seem to work correctly.

Images attached to this comment
1526_20190730034152_cc2.png
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NaokiAritomi - 01:21, Tuesday 30 July 2019 (1523)Get code to link to this report
Squeezing and anti-squeezing with different green power

[Aritomi, Yuhang]

We measured squeezing and anti-squeezing with green power from 15 mW to 55 mW. Attached picture shows the result. Our case seems that loss is 25% and phase noise is 30 mrad. Note that this is not a fitting.

After this measurement, we checked visibility and found that visibility is 0.935 which means loss is 12.6%. (Note that when we calculated visibility, we didn't consider DC offset of PD. Visibility should be higher than this.) Then we aligned LO and BAB and visibility became 0.973 which means loss is 5.3%. However, squeeze level didn't increase.

green power (mW) MZ offset OPO temperature (kOhm) p pol PLL (MHz)
15 4.01 7.16 192
20 4.1 7.16 177
25 4.19 7.17 177
30 4.29 7.18 180
35 4.38 7.175 162
40 4.5 7.175 150
45 4.58 7.18 147
50 4.68 7.19 150
55 4.78 7.195 150
60 4.88 7.195 144
65 4.98 7.2 141
Images attached to this report
1523_20190730054246_sqzasqz20190729.png
R&D (FilterCavity)
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NaokiAritomi - 22:38, Monday 29 July 2019 (1522)Get code to link to this report
Recovery of good squeezing

[Aritomi, Yuhang]

Recently we turned off lasers when we leave. We accidentally kept lasers ON from last Friday and today we found that squeezing spectrum is very flat and phase noise is much less (attached pictures). Green power is 40 mW and error signal of CC1 and CC2 is 76 mVpp and 120 mVpp. Phase noise is smaller almost by a factor of 10. We guess large phase we had so far is due to unstable lasers. When we achieved good squeezing in May, lasers were always ON. We'll keep lasers on and see what happens.

Images attached to this report
1522_20190729153749_sqz20190729.png 1522_20190729153755_cc120190729.png 1522_20190729153759_cc220190729.png
Comments related to this report
EleonoraCapocasa - 10:40, Tuesday 30 July 2019 (1526)

The large increase of phase noise above 300 Hz when the CC2 is closed (pic 3) is very strange and we need to investigate it. The loop should have a UGF of few kHz, but it doesn't seem to work correctly.

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EleonoraCapocasa - 16:16, Monday 29 July 2019 (1521)Get code to link to this report
DGS failure: still not recovered

[Yuhang, Matteo, Eleonora, Miyakawa (remotely)]

Last Friday,  just before going home, we noticed that the DGS system was not working anymore and no signal can be read from ADC.

This happend suddenly since we used it up to one hour before and it was perfectly working.

Since me and Matteo were doing some cabling around the rack at that moment, we suspected we had accidentaly disconnected some cable but after a carefull checking it seemed that everything was fine.

On Saturday I contacted Miyakawa-san which accessed remotely the PC and told me it seemed a timing problem. On Saturday afternoon and also this morning we have carefully checked the timing signal.

Following the advice of Miyakawa-san, we change it from square wave of +/-5 V to 0-5V. It didn't solve the problem.

We tried to restart the models and reboot the PC countless times.

I tried to use only one time adapter (and switch it from one to the other) to check if one of the two was broken, but it didn't solve the problem

I tried to double the amplitude of the timing signal, to disconnect and reconnect the cables between AA, time adapter and I/O chassis. It didn't change the situation.

Pic.1 and 2 show the errors that appear in the DGS_TP screen for K1x01 (master model) and K1FDS (slave model), respectively.

We really need the help of an expert.

 

On top of that it seems the screen connected to the standalone doesn't work properly. Sometimes it gets black and we need to switch it on and off to recover it (but it usually last few seconds and then gets black again!) 

Images attached to this report
1521_20190729091317_k1x01.png 1521_20190729091335_k1fds.png
R&D (FilterCavity)
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EleonoraCapocasa - 15:53, Monday 29 July 2019 (1520)Get code to link to this report
More DGS hardware installation

[Matteo, Eleonora]

On Friday 19/08 we recived from Kamioka one AA module and two BNCtoDsub converters. 

Last week we have installed the AA into the DGS rack and did some cabling from this rack to the cleenrrom as we blan to install the BNCtoDsub converters into the clean room rack.

We took a power supply from ATC and use it to power a KAGRA DC power strip (also taken from ATC). We use the strip to power all the two AA, the AI and the DAC dSub->BNC converter (not that ADC BNC-> dSub converters don't need power.)

We reorganize the cables behind the DGS rack to make them more tidy.

We also removed one ADC PCiexpress card from the new DGS computer (the one we couldn't make work) and installed it into the standalone PC we are currently using.

The standalone can host up to 4 card and we have currently installed two ADC an one DAC. The slots are piled up in vertical. From the bottom we have 

1) ADC 1 (used for local controls)

2) ADC 2 ( not used, it will be used for AA signal)

3) DAC

4) empty

In the future we can decide to put another DAC or another ADC in the empty slot. According to Miyakawa-san all the possible combinations of 4 PCie among ADC and DAC are fine with the excepion of 4 DAC.

We took an additional timing adaptor from ATC which we used to provide the timing signal to the new ADC card.

We haven't tested the new ADC but the system seemed to work fine after these modifications. We didn't experienced any trouble until the failure of last friday (26/07).

R&D (Cryogenic)
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SatoshiTanioka - 18:31, Sunday 28 July 2019 (1519)Get code to link to this report
PDH error signal

I checked PDH error signal (green line) with low-pass filter.
Though the time resolution is higher than before, still the error signal is spike-ish structure.
This may be due to too high finesse of silicon cavity.
At this moment, I did not use frequency scan by laser PZT, but temperature fluctuation of laser induced frequency fluctuation.
Thus I could see error signal without scanning laser frequency.

It needs temp. control loop for stable lock.
Anyway, I will consider cotrol loops for TEM00 lock.

Images attached to this report
1519_20190728112341_20190728.jpg
R&D (FilterCavity)
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EleonoraCapocasa - 16:50, Sunday 28 July 2019 (1517)Get code to link to this report
Feedback to the FC end mirror: preliminary implementation

I tried to feedback a part of the PZT correction (sent to the main laser to lock it to the FC) to the end mirror. The goal is to reduce the cavity motion at the logitudial resonance frequency (around 1Hz),  acting on the mirror in order to reduce the correction sent to the laser. In fact in this region, the correction increases the frequency noise of the main laser, inducing higher PLL noise.

The PZT correction is taken from the channel  "pzt mon" of the rampeauto (which is 100 times smaller that the real correction), it is sent to the ADC of the DGS where it is digially filtered and then the correction is summed to the one already sent to the end mirror coils (from anguar damping).

We observed that the signal seen by DGS has a very strong 50 Hz, which is not present when locking at it with the oscilloscope.

In order to select the part of the spectrum aroun the 1Hz, I used a filter like this:

  Freq (Hz) Q
zero 0 simple
pole 1 simple
pole 20 simple
pole 20 simple

The simulated openloop TF is shown in pic1. Where as a mechanical TF I used the one measured in entry #1506

Pic.2 show the spectrum of the PZT correction with (bue curve) and without (red curve) test mass feedback engaged. It can be seen that the correction to PZT is reduced by a factor ~10 in the 1Hz region when the feedback is engaged (blu curve).

To be done:

- Amplify the signal before the ADC with a stanford to better exploit the ADC dynamics.

- Check the RMS improvement and optimize the correction filter (an overshoot is now visible at 2-3 Hz).

- Add a notch filter to avoid feeding back the 50 Hz and to be able to check the signal improvemt in time (currently it is fully dominated by the 50 Hz).

- Check wheather the PLL noise is reduce when the loop is engaged.

Images attached to this report
1517_20190728094006_zcorrtf.jpeg 1517_20190728094018_zcorr.png
R&D (FilterCavity)
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NaokiAritomi - 09:04, Friday 26 July 2019 (1516)Get code to link to this report
Phase noise at high frequency is limiting squeezing

[Aritomi, Yuhang]

First we moved position of green phase shifter closer to GRMC since effect of misalignment of green phase shifter was large due to rubber and also there was no space to put additional clamp to fix green phase shifter.

Then we measured free running and closed loop phase noise of CC1,2 (attached pictures). We measured EPS2 of servo as error signal. Note that EPS2 of servo is larger than real error signal by a factor of 15.

calibration factor from EPS2 signal [V] to phase noise [rad]
CC1 error signal: 80.8 mVpp, calibration factor: pi/0.0808/15 = 2.6 rad/V 
CC2 error signal: 116 mVpp calibration factor: pi/0.116/15 = 1.8 rad/V

As you can see, phase noise above 400Hz is very large and rms phase noise is mostly accumulated at high frequency where phase noise is not suppressed by CC loop. When we close the CC loop, phase noise at high frequency becomes larger and rms phase noise becomes even larger. This measurement is consistent with recent noisy squeezing measurement.

Images attached to this report
1516_20190726020445_cc120190725.png 1516_20190726020450_cc220190725.png
R&D (Cryogenic)
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SatoshiTanioka - 20:36, Thursday 25 July 2019 (1515)Get code to link to this report
Installation of double pass AOM

So far, I installed an AOM and some mirrors which consist double pass AOM configuration.
I install a lens in order to avoid clipping at AOM.
Then I adjusted the alignment, and double-passed light can be picked off by PBS now.

Although I have not driven the AOM, the first rough alignment has been done.

Images attached to this report
1515_20190725114445_20190725.jpg
R&D (FilterCavity)
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YuhangZhao - 13:07, Thursday 25 July 2019 (1514)Get code to link to this report
Comment to Investigation of squeezing spectrum (Click here to view original report: 1504)

Here I attach the measurement of SHG and GRMC transmission noise spectrum. 

The difference is I measured the noise spectrum of SHG transmission at a wrong place. (Actually, I was measuring the locking noise of SHG in the entry 1501)

However, we really have a worse GRMC transmission noise. Especially, there are peaks from the 4-10kHz region. They are responsible for the region where we have more noise in the squeezing measurement.

I will try to understand why there is a factor between the old and new measurement.

Images attached to this comment
1514_20190725060914_shgn.png 1514_20190726035743_150120190723050014mz.png
R&D (FilterCavity)
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YuhangZhao - 11:12, Thursday 25 July 2019 (1513)Get code to link to this report
Locking noise of filter cavity by green (RMS)

The measurement done last week shows RMS locking noise is much lower than we expect(entry 1486). It was almost 50 times lower than the measurement done last year(entry 642). So we decide to double-check by using time series.

I did the measurement of RMS locking noise when the gain is 7 and 10. The result is shown in the attached figure 1. However, I just realized the gain of 10 sometimes brought some resonance(I didn't find this resonance last week). Now the gain of filter cavity lock should be 7.

Then I measured the time series of the error signal. And the calibration result is attached in figure 2.

The measurement of time series shows RMS as 4.33Hz while FFT shows 1.5Hz. Basically, they are very similar.

Images attached to this report
1513_20190725040753_figure1.png 1513_20190725041228_together.png
KAGRA MIR (Polarization)
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SimonZeidler - 09:54, Thursday 25 July 2019 (1512)Get code to link to this report
Polarization measurements now possible

Matteo, Eleonora, Simon

We have changed the setup of the absorption bench so to be able to measure S and P polarization of the transmitted beam.
The basic point in the new setup is that we are using two photo-sensors (PSDs, to be more specific) and a PBS together with a lens to focus and split the beam.
Since the measurements are very sensible to the setup, we needed to take several aspects into account:

  • Incoming beam needs a good initial alignment in terms of polarization
    •  another PBS and a HWP were installed
  • The PSDs are too sensitive for the pure transmitted beam
    • A stack of ND filters were installed between lens and PBS in the outcoming beam-path
  • The setup is extremly sensitive to stray-light
    • A beam-tube is covering the PSD in the lateral beam-path from the PBS (S - polarization)
    • A beam-dump (Vantablack) is catching the reflected beams from the ND-filters
    • A razor-blade beam-dump is covering the space btw. beam-tube and ND-filters (catching scattered light)
    • A couple of obligued ND-filters is placed at the blind-side of the PBS
    • A black light-cover is placed on top of the lens to catch some ghost-beam reflections coming from the top of the sample

Especially the stray-light suppression is challenging as there are a lot of possibilities where scattered light can enter the sensors and it may be that we still find new sources.
For example, one main source of stray-light was a ghost beam created by a probe-prism which is reflected by a lens for the incoming pump-beam, and this reflection is entering the test-mass and internally reflected on the upper boundary and eventually entered the P-pol sensor from above (shielded now - see pictures)

Electronics
We are using basically the same system as already given by the absorption-bench setup.
However, we had to do some modifications:

  • As we have only one channel to demodulate an AC signal on the lock-in, we have installed another lock-in to demodulate the signal from the second PSD (using the same reference signal)
  • The power for the measurements is reduced to be in the mW region (2A input current)
  • Of course more cables and power-sources needed for the sensors
Images attached to this report
1512_20190725025855_48.jpg 1512_20190725025905_38.jpg 1512_20190725025912_29.jpg
R&D (FilterCavity)
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YuhangZhao - 09:49, Thursday 25 July 2019 (1511)Get code to link to this report
open-loop transfer function of filter cavity now

I upload here the open-loop transfer function of the filter cavity. The situation now we are operating with.

(gain of 7, attenuation of 7)

Images attached to this report
1511_20190725042026_figure1.png
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YuhangZhao - 23:30, Wednesday 24 July 2019 (1510)Get code to link to this report
Improvement of phase shifter behavior by putting rubber(2)

Aritomi and Yuhang

After seeing the effect of rubber in entry 1508, we tried to put it at another position. Considering what we reported in entry 1471, we found the resonance of 500Hz/600Hz is due to different base plate we put for phase shifter. So it seems to be an overall resonance of the mirror mount.(flag pole mode) So we decided to put a piece of rubber under the whole mirror mount. We thought it will damp the resonance of 500Hz/600Hz. The rubber and the position we put for CC1 and CC2 is shown in the attached figure 1 and 2.

After put them we increase gain little by little, we couldn't find the resonance of 500Hz/600Hz. It makes a big difference. The measurement of the optomechanical transfer function is attached.

Images attached to this report
1510_20190724162825_wechatimg480.jpeg 1510_20190724162830_wechatimg481.jpeg 1510_20190725044101_cc1.png 1510_20190725044106_cc2.png
R&D (FilterCavity)
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NaokiAritomi - 23:10, Wednesday 24 July 2019 (1509)Get code to link to this report
Squeezing with high bandwidth phase control

[Aritomi, Yuhang]

First we put rubber under phase shifter to damp 500Hz resonance. 500Hz resonance almost disappeared with rubber and finally we could lock CC1 with 4kHz bandwidth and CC2 with 1.5kHz bandwidth. CC2 is still a bit unstable and maybe integrator is necessary for CC2.

Then we measured squeezing spectrum, but the spectrum is similar with before... 

Tomorrow we'll measure free running and closed loop phase noise of CC1,2 to estimate phase noise.

Images attached to this report
1509_20190724161041_sqz20190724.png
R&D (FilterCavity)
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YuhangZhao - 23:10, Wednesday 24 July 2019 (1508)Get code to link to this report
Improvement of phase shifter behavior by putting rubber(1)

Yuhang and Aritomi

We tried to put a rubber at the place where we think it can be related to resonance. First, we tried to put it between mirror/PZT holder and mirror mount. See attached figure 1 and 2.

In the measurement shown in entry 1503, CC1 has already been installed with this rubber while not for CC2. In this entry, I put a comparison of OLTF for CC2 with and without the rubber.

In the attached figure 3, it is shown the measurement with and without the rubber. We can see 4kHz resonance is damped.

In the attached figure 4, I add 12dB to measurement with rubber. The reason is we were locking with different unity gain frequency. In this case, we could compare better. From this comparison, we could see that the reduction of resonance at 4kHz gives energy to the peak at 600Hz and 7kHz and makes them higher.

Considering the position we put rubber, we think 4kHz corresponds to resonance along the direction of mirror/PZT holder axis.

Images attached to this report
1508_20190724161037_wechatimg478.jpeg 1508_20190724161042_wechatimg479.jpeg 1508_20190724161207_cc22.png 1508_20190724161212_ccc.png