LOG-IN
Displaying reports 1681-1700 of 3128.Go to page Start 81 82 83 84 85 86 87 88 89 End
KAGRA MIR (Absorption)
Print this report.
SimonZeidler - 19:48, Monday 07 October 2019 (1706)Get code to link to this report
Recalculation of Absorbance for the Sapphire Calibration Samples

Simon

I recalculated the absorbance values to take into account the small transmittances we got from the spectra taken at the ATC for all colored Sapphire samples.

The new spectra, now also with reference values at 633nm, can be found in the attachement.

Images attached to this report
1706_20191007124829_bs1.png 1706_20191007124833_bs2.png 1706_20191007124836_gs1.png 1706_20191007124839_gs2.png
KAGRA MIR (Absorption)
Print this report.
SimonZeidler - 19:45, Monday 07 October 2019 (1705)Get code to link to this report
Absorption Measurement on Small Sapphire Smaple from Shinkosha

Pengbo, Simon

We removed the OSTM and packed it again. It is now located in the small shelf inside the clean room.

After that, we recalibrated the system.
The calibration values are:

R_surf = 17.86 1/W
(AC = 0.54V, DC = 4.58V, P_in = 0.030W, abs_surfref = 0.22)

R_bulk = 0.8 cm/W
(DC = 0.105V, AC = 5.42V, P_in = 0.030W, abs_bulkref = 1.04/cm)

Then, we exchanged the calibration sample with the first of the 5 small Shinkosha Sapphire samples: S5 (2" x 20mm)
We located the center of the sample as [X,Y,Z] = [327.25, 122, 33.5].
The transmittance of the sample is T ~ 0.85

Since we cannot set 10W as an input power and leave it as it is while moving the sample into the beam and out again (the sample holder will cut the beam otherwise), we set the power to its minimum trough the polarizer while it is feeded with 7A current and used the beam-shutter for moving the sample holder. In the center position, we set the power to maximum. The transmitted beam power has been measured to be 8.4W.

Now the map is being taken with 15mm radius.

R&D (FilterCavity)
Print this report.
YuhangZhao - 11:28, Monday 07 October 2019 (1704)Get code to link to this report
Test of bias for AA's quadrant

Aritomi and Yuhang

We found the problem of the small RF signal of the AA's quadrant (elog1670). Matteo T suggested checking the bias. We turned on the button on the quadrant box and measured the voltage at the end of the power cable.  We checked with multi-meter and it shows 150V reached quadrant.

So bias seems not to be a problem.

Images attached to this report
1704_20191007042834_wechatimg548.jpeg
R&D (Cryogenic)
Print this report.
SatoshiTanioka - 22:59, Sunday 06 October 2019 (1703)Get code to link to this report
Installation of Mirrors

I installed 3 steering mirrors for HOMs beam paths to roughly decide where to put PDs for intensity stabilization.
2 HOM-beams are roughly alinged into STMs which are for the alignment for cryogenic cavity.

Attached is the picture of current situation of optical table.

Images attached to this report
1703_20191006155917_20191006.jpg
R&D (FilterCavity)
Print this report.
NaokiAritomi - 17:56, Sunday 06 October 2019 (1702)Get code to link to this report
Summary of current issues
  • fluctuation of IR transmission from filter cavity (entry 1701)
  • large CC2 phase noise from filter cavity (entry 1695)
  • large bump in shot noise spectrum at low frequency (entry 1529)
R&D (FilterCavity)
Print this report.
NaokiAritomi - 17:48, Sunday 06 October 2019 (1701)Get code to link to this report
IR alignment with dithering

[Aritomi, Yuhang]

We measured mode matching when filter cavity is aligned with pitch dithering. The result is as follows. Mode matching was around 90%. We found that when pitch dithering was engaged, pitch misalignment became less, but yaw misalignment became more.

Mode AOM frequency (MHz) IR transmission
TEM00 109.03607 3000
HG10 109.43128 350
HG01 109.43219 200
IG02 109.8288 115
offset   94

IR TEM00 transmission was fluctuating even when dithering was engaged (attached movie). Time scale of the movie is 2s and DC offset is 94.

We measured BAB reflection when BAB is on/off resonance. Off resonance reflectivity is 82% and the reflection might be still cutted.

Injection: 334uW
Reflection: 273uW (off resonance)
Reflection: 190-250uW (on resonance)
 
However, after one hour, IR was misaligned even though green was aligned well with dithering. We guess that it is because green and IR is not overlapping well.
Non-image files attached to this report
R&D (FilterCavity)
Print this report.
EleonoraCapocasa - 17:04, Sunday 06 October 2019 (1699)Get code to link to this report
Preparation for CC2 feedback to the INPUT mirror

I modified the simulink model to include the possibility to feedback the CC2 correction signal to the length d.o.f. of the input mass.

The ADC channel where to inject the CC2 signal is the n 13 in the top BNCtoDsub converter in the clean room (named ADC0 Ch16-32).

I modified the medm screen accordingly. Next step will be to optimize the length driving of the input mirror.

R&D (FilterCavity)
Print this report.
EleonoraCapocasa - 16:54, Sunday 06 October 2019 (1698)Get code to link to this report
Time-out error on diaggui.

On Wed 02/10 we had another timed-out error on diaggui. It was solved by restarting the standalone. It happened ~13 days after the previous one. (entry #1650).

KAGRA MIR (Absorption)
Print this report.
SimonZeidler - 12:20, Saturday 05 October 2019 (1697)Get code to link to this report
OSTM HR coating absorption

Pengbo, Simon

We have started to analyze the coated OSTM from Shinkosha regading the absorption of the HR side.

First, we took out the OSTM and inspected the mirror visually. We found pencil marks on the barrel and among them an arrow that indicates the thicker side of the wedged substrate and shows toward the HR side of the mirror (see attached photos).
The actual orientation of the sample inside the sample holder was a little bit tricky mainly because of the wedge and the size of the sample-holder which is basically too large for such a mirror.

  • At first, we tried to put the thicker side upside to have a somewhat parallel orientation between sample-holder and mirror-plane (as can be seen from the pictures, we are using a - with optical tissue - covered ruler as a spacer). However, we recognized that this will distract the pump-beam so that it cannot be measured anymore regarding its power.
  • Therefore, secondly, we rotated the mirror by 90 degrees so that the distraction of both pump and probe beam is only parallel to the optical table which can be counter measured by a respective relocalisation of the IU and the photometer. However, with this position, the HR coating is facing the pump but also the spacer, which we originally wanted to avoid
  • Especially regarding the probe, we had to change the IU position by ~3mm less than it would have been the case for a wedge-free substrate

After the alignment of the sample, we looked for the exact position of the HR-coating by applying Z-scans. We carefully increased the laser power to take care that the coating is not damaged (initially, we did this on the outer edges of the mirror of course).

Then, we ran a map-scan in the center with 15mm radius in the position were we identified the coating (Z = 48.8). The results of that scan can be seen also in the pictures attached. Our main result is a quite homogeneous mean absorption of 16 ppm (+/- 3ppm) with some point-like excesses indicating the positions of either dust or defects within the coating, most likely.

Images attached to this report
1697_20191005051902_30.jpg 1697_20191005051912_49.jpg 1697_20191005051931_27.jpg 1697_20191005051939_19.jpg 1697_20191005051953_map20191003coatingz488.png 1697_20191005051959_dist20191003coatingz488.png
R&D (FilterCavity)
Print this report.
YuhangZhao - 00:17, Saturday 05 October 2019 (1696)Get code to link to this report
Measurement of CC2 phase noise by using different gain of CC2 loop

Now we could lock CC2 loop with unity gain frequency of 2kHz. To see the difference of CC2 phase noise with different gain. We measured phase noise with different gain.

As expected, higher gain make noise lower at low frequency. But also the higher gain excites resonance at higher frequency.

From the measurement, it seems the gain of 0.2 is the best case. (Although they are all quite similar)

Images attached to this report
1696_20191004171722_phasenoise.png
R&D (FilterCavity)
Print this report.
NaokiAritomi - 22:47, Friday 04 October 2019 (1695)Get code to link to this report
CC2 free running phase noise when filter cavity is locked and aligned with dithering

[Aritomi, Yuhang]

We measured CC2 free running phase noise when filter cavity is locked and aligned with dithering (attached picture). We cannot lock CC2 stably since piezo actuation range is not enough. We'll try to feedback CC2 error signal at low frequency to input mirror of filter cavity.

CC error signal
CC1: 35.6mV
CC2: 162mV
Images attached to this report
1695_20191004154718_cc220191004.png
KAGRA MIR (Absorption)
Print this report.
MatteoLeonardi - 13:52, Friday 04 October 2019 (1694)Get code to link to this report
Calibration check performed on Oct 2nd
[Simon, Pengbo]

R_surf = AC_surfref/(DC_surfref*P_in*abs_surfref) = 18.1 [1/W]
where AC_surfref = 0.425V, DC_surfref = 3.55V, P_in = 0.030W and abs_surfref = 0.22

R_bulk = AC_bulkref/(DC_bulkref*sqrt(T_bulkref)*P_in*abs_bulkref) = 0.741 [cm/W]
where AC_bulkref = 0.072V, DC_bulkref = 4.2V, T_bulkref = 0.55, P_in = 0.030W and abs_bulkref = 1.04/cm
Images attached to this report
1694_20191004065344_15.png 1694_20191004065358_47.png
R&D (FilterCavity)
Print this report.
YuhangZhao - 10:49, Friday 04 October 2019 (1693)Get code to link to this report
Characterization of IRMC after power check

Aritomi and Yuhang

We checked power at several points this Monday and make IRMC transmission set at 1.7mW.

Actually, this means we increased also the error signal(or increase gain). Today we checked the error signal, and actually, it was quite close to oscillation. So we adjusted the gain while looking at the error signal and measured transfer function again. In the end, we put the gain value of the control board from 1.3 to 0.8.

The open-loop transfer function now is as the attached figure 1.

We also measured the IRMC error signal spectrum while IRMC is unlocked and locked. As shown in the attached figure 2. From this locking performance, we could see that the loop suppresses the even harmonics of a fundamental 9Hz oscillation while there are still some odd harmonics left. Also, the 50Hz and its harmonics are introduced after closing the loop. So the PD doesn't introduce any 50Hz noise.

Images attached to this report
1693_20191004034934_irmcoltf.png 1693_20191004034940_irmcerr.png
R&D (FilterCavity)
Print this report.
YuhangZhao - 00:50, Friday 04 October 2019 (1692)Get code to link to this report
Implementation of damping for phase shifter spring (reduction of resonance at 1 and 2 kHz)

Aritomi and Yuhang

Since the unity gain frequency of CC2 was only ~400Hz because of some resonance. We decide to put some more damping material. 

So we put some double layers bent rubber(as shown in the attached photo1) in the position where there may be some spring resonance(as shown in attached photos 2 and 3).

Then we measured OLTF, which is shown in the attached photo 4. And it is shown that the unity gain frequency is around 2kHz now. We also tried to increase the gain, we measured the resonance frequency when there is oscillation. As shown in the attached photo5, the oscillation is at ~23kHz. 

We also measured OMTF. By comparing the measurement we did before putting this new damping rubber, we found the peak around 1 and 2kHz disappeared(as shown in the attached figure 6).

Images attached to this report
1692_20191003174400_wechatimg544.jpeg 1692_20191003174739_wechatimg542.jpeg 1692_20191003174744_wechatimg543.jpeg 1692_20191003174808_oltf.png 1692_20191003174824_wechatimg541.jpeg 1692_20191003175010_comparison.jpg
R&D (FilterCavity)
Print this report.
NaokiAritomi - 22:17, Thursday 03 October 2019 (1691)Get code to link to this report
Squeezing and phase noise when filter cavity is locked

[Aritomi, Yuhang]

First we measured squeezing when filter cavity is locked/unlocked (Pic. 1). We expected more squeezing since we improved reflectivity of dichroic mirror by 4%, but squeezing level is still around 6.1dB when filter cavity is unlocked. Squeezing level when filter cavity is locked/unlocked is similar, but phase noise seems suppressed when filter cavity is locked.

Here are some information of this measurement.

green power (mW) OPO temperature (kOhm) p pol PLL (MHz) Demodulation phase of CC2 (SQZ) (deg) Demodulation phase of CC2 (ASQZ) (deg)
40 7.19 165 105 135
 
CC error signal
CC1: 87.2mVpp
CC2: 144mVpp
 
Then we measured CC1,2 phase noise when FC is locked/unlocked (Pic. 2,3). CC1 phase noise doesn't change so much, but CC2 phase noise is suppressed at high frequency when filter cavity is locked. One problem is that 70kHz large peak appears when filter cavity is locked. It might come from piezo of main laser.
 
Images attached to this report
1691_20191003151712_sqz20191003.png 1691_20191003151717_cc120191003.png 1691_20191003151723_cc220191003.png
R&D (FilterCavity)
Print this report.
EleonoraCapocasa - 21:23, Thursday 03 October 2019 (1690)Get code to link to this report
A first encouraging result on dithering

[Eleonora, Matteo]

Today we did good progress on the dithering.

We gave up on measuring the sensing matrix and we tried to close the loops by simply feeding back each demodulated signal to "its" mirror. 

This seemed to work surprisingly well. (See pic 1-2). The transmitted power increased and became quite stable as well as the lock.

I tried to move one by one the BS, the INPUT mirror and the END mirror when dithering is engaged and the loops seem able to move the cavity mirrors to recover the good alignment. (See pic 3, 4, 5)

From the last two plots we can also check the level of coupling of our error signals, and possibly improve the driving.

The main problem I see is that the error signals are not oscillating around zero but they have an offset and the dithering lines are still well visible in transmission. It shouldn't be like this but I'm not sure about the reason.

Currently the corrector filter is a simple pole at 0.001 Hz. Maybe we should move it to zero. I will also try to put a offset in the loops and see if it can improve the transmission and reduce the dithering line in transmission.

Even if the transmitted power is very stable because we were mostly affected by pitch misalignment, I also tried to close the loops in yaw. They seem not to work well. The error signal is always around zero, so it is not easy to tell the difference when I close the loops, but when tried to misalign the BS in yaw they didn't recover. I didn't spend much time to investigate the problem but I will do it soon.

Since the error signals get crazy if the cavity unlocks I decided it was safer to stop the lock for the night. The cavity kept the lock for more than 5 hours (best record ever) and the lock was stopped on purpose before I go to sleep. It will be good to implement some kind of guardian that will open the dithering loops when the cavity unlocks.

Some details:

- The gain of the input and end loops are respectively -1 and -0.5.

- I reduced the amplitude of both dithering lines from 10000 to 5000 counts.

Images attached to this report
1690_20191003142407_dit1.png 1690_20191003142412_dit2.png 1690_20191003142416_bs.png 1690_20191003142422_input.png 1690_20191003142426_end.png
R&D (Cryogenic)
Print this report.
SatoshiTanioka - 20:31, Thursday 03 October 2019 (1688)Get code to link to this report
Fixing AOM driver

The wire inside the AOM driver box for supplying DC voltage was disconnected.
I fixed it by soldering, then it was conducting.

Also I soldered the power supply cable with 2 capacitors.

I forgot to take pictures.
I will upload them tomorrow.

R&D (Cryogenic)
Print this report.
SatoshiTanioka - 17:28, Thursday 03 October 2019 (1687)Get code to link to this report
Note on Silicon Sample Mirror

We have one flat silicon mirror which will be used for measurement.
It has a wedge, 50arcmin.

On the other hand, fused silica input and output mirrors' wedge are 30min.
We have to take it into account to make a mirror cap.

R&D (FilterCavity)
Print this report.
YuhangZhao - 00:28, Thursday 03 October 2019 (1686)Get code to link to this report
Green reflected by quadrant(used for AA)

Aritomi and Yuhang

We measured the green power reflected from the quadrant(used for the AA system). The incident power is measured as 1.2mW while the reflected power is measured as 0.46mW.

Almost 40% of power is reflected from it.

R&D (FilterCavity)
Print this report.
YuhangZhao - 00:19, Thursday 03 October 2019 (1685)Get code to link to this report
The green beam seen from filter cavity transmission camera (comparison on several days)

I took a picture of the green beam shape from the filter cavity transmission more than one week ago (11 days ago). Shown in attached figure 1.

I took the same picture last Thursday after the flatting of green beam height. Shown in attached figure 2. 

I also took the same picture again today after correcting the beam cut issue on AOM/iris. Shown in attached figure 3.

I think it is clear that the filter cavity transmission has less astigmatism.

Images attached to this report
1685_20191002171834_wechatimg536.jpeg 1685_20191002171902_wechatimg538.jpeg 1685_20191002171913_wechatimg535.jpeg