LOG-IN
Displaying reports 1901-1920 of 3128.Go to page Start 92 93 94 95 96 97 98 99 100 End
R&D (FilterCavity)
Print this report.
YuhangZhao - 00:21, Wednesday 10 July 2019 (1453)Get code to link to this report
Some 50Hz noisy becomes quite obvious now

Eleonora, Pierre, Aritomi, Yuhang

Recently we found 50 Hz presents everywhere. In the attached figures, we can see some examples of these 50Hz noises.

A part of noise level was identified that it comes from of ground loop between circuit and measurement device. This is identified by changing the power supply of the oscilloscope to different places. But we cannot eliminate this noise totally. (From figure 5 to figure 2, the change is the change of oscilloscope power supply)

We also identified that the 50Hz noise for GRMC transmission signal comes from the DDS board. At that moment, only DDS board output is connected to mixer and mixer IF channel is connected to the oscilloscope. We tried to change the connection with and without a lot of other components, and we found only DDS board gives this 50Hz noise.  (Figure 3)

We see a different shape with normal measurement 50Hz noise for GRMC transmission signal, so we think this noise coupled into control loop and affects the phase locking of GRMC a lot. (Figure 2)

Images attached to this report
1453_20190709171607_wechatimg454.jpeg 1453_20190709171617_wechatimg455.jpeg 1453_20190709171626_wechatimg456.jpeg 1453_20190709171634_wechatimg457.jpeg 1453_20190709171642_wechatimg458.jpeg
R&D (FilterCavity)
Print this report.
YuhangZhao - 00:00, Wednesday 10 July 2019 (1452)Get code to link to this report
The implementation of MZ/GRMC auto-locking

Pierre, Yuhang

After the design/talk/discuss with Matteo, Eleonora and us, Pierre redesign the circuit and we implemented it. Now the procedure is just to press 'reset' button and then MZ and GRMC will be locked in sequence. Please also remember to use 'auto' mode of GRMC and 'man' mode of MZ and put them both in 'lock' state.

Then we measured the open loop transfer function of MZ.

Images attached to this report
1452_20190710160305_grmc.png 1452_20190710160310_mz.png
KAGRA MIR (Absorption)
Print this report.
MatteoLeonardi - 22:12, Tuesday 09 July 2019 (1448)Get code to link to this report
Recovery of the absorption bench (Vol 2)

[Matteo, Simon]

Today we switched on the 1064nm pump laser for the first time after four months. We had some problem identifying the correct COM port (COM11) but solved that the laser could be successfully switched on and controlled from the PCI computer. One thing to be noticed is that the power cord of the pump laser seems to have connection instabilities, please remember to be careful and never touch the plug in into the power supply.

After the successful result on the pump laser we switched on the probe laser (633nm). No problems on that. We had to install a variable OD filter in front of the probe laser not to saturate the photodiode on the imaging unit. We aligned the probe on the imaging unit without any reference sample to have about 4V of DC output as read by the lock in. We then installed the surface reference sample and performed some z scan. NOTE: the written part present on the sample is facing the imaging unit. At this stage we aligned again the probe beam into the imaging unit photodiode maximizing the DC to compensate for the misalignment introduced by the reference sample, we then aligned the pump beam to maximize the AC signal at the crossing point.

MEMO: to align the probe on the IU photodiode we used the IU lens translation stage; to align the IR beam we used the translation stage on the last lens before the sample area.

Attached (1) the screenshot of the absorption measurement for surface reference sample (try one).

After speaking with Manuel, he told us that the written part of the surface reference sample should be facing the pump side and not the IU side. We flipped the surface reference sample and optimized again the alignment and performed again the z scan. Result is in attached figure (2).

In the end we substituted the surface reference sample with the bulk reference sample and measured the z scan. Result is in the attached figure (3).

From measurements shown in (2) and (3) we can obtain the calibration of the system.

R_surf = AC_surfref/(DC_surfref*P_in*abs_surfref) = 16 [1/W]
where AC_surfref = 0.42V, DC_surfref = 3.85V, P_in = 0.031W and abs_surfref = 0.22

R_bulk = AC_bulkref/(DC_bulkref*sqrt(T_bulkref)*P_in*abs_bulkref) = 0.604 [cm/W]
where AC_bulkref = 0.067V, DC_bulkref = 4.64V, T_bulkref = 0.55, P_in = 0.031W and abs_bulkref = 1.04/cm

The two calibration values are compatible with old calibrations.

Images attached to this report
1448_20190709092550_201907091.png 1448_20190709145617_201907092.png 1448_20190709145631_201907093.png
R&D (FilterCavity)
Print this report.
NaokiAritomi - 20:31, Tuesday 09 July 2019 (1451)Get code to link to this report
RF amplifier is fixed

[Pierre, Aritomi]

Pierre fixed RF amplifier and measured amplification factor for AOM which is 34dB. Since we should have 23dBm for AOM, RF signal before RF amplifier should be -11dBm.

R&D (FilterCavity)
Print this report.
NaokiAritomi - 20:29, Tuesday 09 July 2019 (1450)Get code to link to this report
Replacement of IR phase shifter

I replaced IR phase shifter with a new one (Pic 1) and aligned IRMC and locked it with Pierre's servo. Tomorrow we'll measure transfer function of CC2.

Images attached to this report
1450_20190709132932_img7666.jpg
R&D (FilterCavity)
Print this report.
NaokiAritomi - 22:25, Monday 08 July 2019 (1447)Get code to link to this report
Back reflection of IR from filter cavity

[Aritomi, Yuhang, Eleonora, Matteo]

Recently we had a problem that when BAB is injected into filter cavity, we cannot lock green phase with p pol leakage of BAB transmission. Today we found that back reflection of IR from filter cavity makes green phase error signal unstable. When we block IR injected into filter cavity, green phase error signal is stable, but when we open it and IR is aligned to filter cavity, green phase error signal fluctuates a lot. We guess that back reflection of IR from filter cavity goes back to OPO and amplified and becomes p pol leakage.

To reduce back reflection, we put faraday (IO-3-1064-VHP) after OPO on the bench (Pic 1,2). BAB transmission without green before faraday is 103mV and 100mV after faraday, which means transmissivity is 97%. 

After installation of faraday, IR is totally misaligned. We'll try to align faraday tomorrow.

Images attached to this report
1447_20190708152506_12.png 1447_20190708152513_img7660.jpeg
R&D (FilterCavity)
Print this report.
NaokiAritomi - 19:44, Monday 08 July 2019 (1446)Get code to link to this report
How to connect remote desktop from cleanroom

To connect the DGS remote desktop from cleanroom, please use Remote Desktop Connection, not Microsoft Remote Desktop. I put Remote Desktop Connection to taskbar in computer in clean room.

KAGRA MIR (Absorption)
Print this report.
SimonZeidler - 19:44, Monday 08 July 2019 (1445)Get code to link to this report
Recovery of the absorption bench 1

Matteo, Simon

We tried to start recovering the absorption bench today by reactivating the translation-stage. For this step it is necessary to reset the position of the stage, but unfortunately we got problems with this especially for the vertical axis of the stage.
After some time of an unsuccessful try and error approach, we called Manuel and tried to redo the steps he was doing usually.

In the end, we could reactivate the whole stage by tricking the Zaber console (the PC program controlling the stage) which turned out to be the main burden for a proper reset since the predefined limits for the vertical axis made it impossible reach the "home" position manually.

Actually, I added a more particular description of what we have done in the GWPO wiki: here and here

R&D (Cryogenic)
Print this report.
SatoshiTanioka - 15:00, Monday 08 July 2019 (1444)Get code to link to this report
Comment to Dip of reflected beam (Click here to view original report: 1440)

By rough estimation, the reflected power dropped ~0.3mW, though I could not see any transmitted flash.

The reflected beam power was ~3mW with 3.5V.
The dip was ~0.4V.
3mW * 0.4V / 3.5V ~ 0.3mW

The loss and high reflectivity may cause too small transmitted power.

R&D (Cryogenic)
Print this report.
SatoshiTanioka - 14:07, Monday 08 July 2019 (1443)Get code to link to this report
Input optical layout

I updated the input optical layout as attached figure.
HOMs pahts are under construction now.

Images attached to this report
1443_20190708070715_layoutinputv3.png
R&D (FilterCavity)
Print this report.
NaokiAritomi - 19:18, Sunday 07 July 2019 (1442)Get code to link to this report
Further improvement of IR alignment

[Aritomi, Eleonora P&C, Yuhang]

This is work on July 5th.

We scanned green phase at 1kHz and scanned AOM again. The result of AOM scan and TEM00 are attached. With 1kHz green phase scan, TEM00 peak isn't measured properly. After AOM scan, we locked IR on TEM00 and HG01,10 and measured each power with dataviewer.

AOM frequency (MHz) IR transmission mode
109.03643 500 - 1200 TEM00
109.43154 100 - 200 HG10
109.43199 150 - 400 HG01

Then we tried to improve the alignment of IR. TEM00 and HG10,01 with 10 Hz green phase scan after the alignment is as follows.

AOM frequeny (MHz) IR transmission mode
109.03646 100 - 5500 TEM00
109.43156 100 - 300 HG10
109.43204 100 - 400 HG01

We haven't measured all the higer order modes, but mode matching should be around 90% now.

Images attached to this report
1442_20190707121914_20190705scan.png 1442_20190707122105_20190705tem00.png
R&D (Cryogenic)
Print this report.
SatoshiTanioka - 15:47, Sunday 07 July 2019 (1441)Get code to link to this report
Transmittance of silicon mirror

I measured the transmittance of one of the silicon mirrors using power meter.
When I injected 10mW power laser, the transmitted power was about 0.2uW.
This corresponds to T=20ppm.
If the loss is zero, this transmittance corresponds to finesse~150,000.

So it seemes that the coating is not what we wanted.

R&D (Cryogenic)
Print this report.
SatoshiTanioka - 19:36, Friday 05 July 2019 (1440)Get code to link to this report
Dip of reflected beam

Yesterday, I measured the beam profile, and the beam had its waist around 1250mm distance from FI with ~60um beam radius.
Then I adjusted the beam height to achieve ''straight'' beam.

Next, I scaned the laser freq. using both temp. control and PZT of the laser.
During scanning the freq., I monitored both transmitted beam, and reflected beam.

I could see some dips in reflection, though I could not see any transmitted beam.
I have not checked the error signal yet, it may be possible to lock the laser, but it seemes difficult to see transmitted beam.

Images attached to this report
1440_20190705121349_dipt.jpg 1440_20190705121353_dipp.jpg
Comments related to this report
SatoshiTanioka - 15:00, Monday 08 July 2019 (1444)

By rough estimation, the reflected power dropped ~0.3mW, though I could not see any transmitted flash.

The reflected beam power was ~3mW with 3.5V.
The dip was ~0.4V.
3mW * 0.4V / 3.5V ~ 0.3mW

The loss and high reflectivity may cause too small transmitted power.

R&D (FilterCavity)
Print this report.
NaokiAritomi - 00:56, Friday 05 July 2019 (1439)Get code to link to this report
Improvement of IR alignment

[Aritomi, Eleonora P&C, Yuhang]

Today we tried to improve IR alignment into filter cavity.

First we increased green power to 68mW. OPO temperature is 7.2 kOhm and p pol PLL frequency is 150 MHz. IR injected into filter cavity is around 13mW. Then we locked IR on TEM00 and maximized TEM00 by aligning two steering mirrors for IR. During IR alignment, green transmission was above 5000.

Since lock of green phase is not stable, we scanned green phase with 10Hz and 1.3Vpp. Then we scanned AOM frequency at 2 mHz. After the scan, we locked IR on TEM00 and HG10,01 and measured each power with dataviewer. We repeated alignment of IR and AOM scan twice. Attached pictures show cavity scan. IR transmission when IR is locked on TEM00 and HG10,01 is as follows.

After scan 1

AOM frequency (MHz) IR transmission  mode
109.036 100 - 2000 TEM00
109.43 100 - 400 HG10

After scan 2

AOM frequency (MHz) IR transmission mode
109.03646 100 - 3800 TEM00
109.43133 100 - 270 HG10
109.432 100 - 400 HG01

This scan seems strange and is not compliant with measurement when IR is locked due to green phase scan. Pic 3 shows TEM00 in scan 2. Given that linewidth of filter cavity is 100Hz and AOM scan speed is 8kHz/s, frequency of green phase scan should be higher than 80Hz. Actually we tried 1kHz once, but TEM00 peak hight became smaller.

Anyway now TEM00 is 10 times larger than highest HOM. It seems that mode mismatch is small. We'll continue the alignment tomorrow.

Note
I found that there is time difference between time in diaggui and movie even though we start measurement and movie at the same time. It seems that diaggui starts measurement around 40 s after we push start button.
Images attached to this report
1439_20190704175556_screenshotfrom20190704201412scan1.png 1439_20190704175604_screenshotfrom20190704201321scan2.png 1439_20190705061253_tem00.png
R&D (Cryogenic)
Print this report.
SatoshiTanioka - 21:24, Thursday 04 July 2019 (1438)Get code to link to this report
Beam Profile measurement

This afternoon, Matteo checked my experimental setup, and gave me some advices.

Following his advice, I measured beam profile.
I will upload the results tomorrow...

R&D (Cryogenic)
Print this report.
SatoshiTanioka - 21:17, Thursday 04 July 2019 (1437)Get code to link to this report
Spec of silicon mirror

Today, Aso-san pointed out that the silicon mirrors may have higher finesse than we expected.
Therefore, I checked the spec sheet of mirrors, and the designed reflectance is more than 99.997%, which corresponds to more than 100,000 finesse, though we ordered as 50,000 finesse.
The manufacturer may assume that the loss (probably ~30ppm) reduces the finesse from ~100,000 to 50,000.
However, it may be almost impossible to see transmitted beam with such high finesse and loss...

Images attached to this report
1437_20190704141706_unko.jpg
R&D (Cryogenic)
Print this report.
SatoshiTanioka - 20:19, Wednesday 03 July 2019 (1436)Get code to link to this report
Installation for double-pass AOM

Today, I re-started the installation of optics for double-pass AOM which is used in HOMs paths.
The beam is aligned roughly.

In addition, I cleaned silicon mirrors using First Contact.
Then I installed them inside the chamber, but still cannot see any flash.

Also I re-designing the cavity in order to make another set of mirrors which have lower finesse and high coating quality.

Images attached to this report
1436_20190703130845_img9682.jpg
R&D (FilterCavity)
Print this report.
Pierre Prat - 18:57, Wednesday 03 July 2019 (1435)Get code to link to this report
GRMC servo repair and modification
The GRMC servo was modified and repaired.

Firstly after the new measurement of the mechanical transfer funtion of GRMC, the notch filter 2 was modified as below:
The center frequency of the notch filter was tune to 9,47kHz without changing the Q factor (1 as previously).
C60; C63; C61; C62; : 560 pF (unchanged)
R79; R80; R81; R82: 30 kOhm (instead of 24 kOhm previously)

We didn't succeed to lock the GRMC, so I checked completely the filter section of the servo: it appears after measurement of the transfer function of the 1/f filter, that the corner frequency was displaced from 2,2 kHz to 9 kHz.
It appears that the C38 capacitor was damaged. The C38 capacitor was replaced by a 33nF capacitor and the transfers function was restablished.

We always didn't succeed to lock the GRMC. It appears that the error signal in scan mode has an amplitude of -20mv / + 30mV which is weak for the current design of the servo. So the hysteresis of the detection comparator (U23 - LM311DR) was reduced drastically from 10mV to 0.5mV (largely less than the amplitude of the error signal in scan mode).
The R108 resistor was changed to a 10 MOhm resistor (instead of 470 Kohm previously).

After this modification, the GRMC locking was succesfull and robust.

We tuned the gain (position 3 of the gain potentiometer) in order to have a gain margin of 10dB (at phase 0 deg) and a unity gain frequency of 1.6kHz (more than 50 degree of phase margin).

So the GRMC servo is now functional and we can go on the modification of GRMC and MZ servos for synchronized locking.
R&D (FilterCavity)
Print this report.
NaokiAritomi - 12:35, Wednesday 03 July 2019 (1434)Get code to link to this report
Comment to Replace the AC channel op-amp with a high speed one for CC1 locking PD (Click here to view original report: 1432)

Error signal is 30 mVpp and conversion factor from V to rad is pi/0.03 = 105 rad/V.

R&D (FilterCavity)
Print this report.
NaokiAritomi - 09:34, Wednesday 03 July 2019 (1433)Get code to link to this report
AOM frequency scan

[Aritomi, Eleonora P&C, Yuhang]

This is work on July 2nd.

First we increased green power to 60mW. OPO temperature and p pol PLL are as follows

green power (mW) OPO temperature (kOhm) P pol PLL (MHz)
60 7.19 150

Then we scanned AOM frequency and measured green and IR transmission with diaggui. Note that this data is slow channel and sampled at 16Hz. Setting of AOM is shown in Pic 1. FM is 2 mHz and deviation is 1 MHz (peak to peak: 2MHz). During this measurement, we scanned green phase with 2kHz, 700mVpp. We also took a movie of green and IR camera to characterize higher order modes. Starting time is 19-07-02-07-08-57 UTC. Pic 2 shows transmission of green and IR. Higher order mode is as follows.

time (s) mode
22.75 TEM00
46.81 pitch HOM
72.5 HG10,01
97.94 HOM
147.4 TEM00
197.1 HG10,01
248.6 HG11,02
347.8 HG10,01
423.2 TEM00
472.8 HG10,01

Note that speed of scan is 2 MHz / 250 s = 8 kHz/s and measured FSR is 147.4 - 22.75 = 124.65 s which means FSR is 0.9972 MHz in AOM.

As you can see, green transmission is also scanned by AOM since AOM scan changes alignment of green injected into filter cavity. But this shouldn't be a problem as long as alignment of filter cavity is fixed. When you look at TEM00 closely (Pic 3), sampling rate seems not enough. We'll try with oscilloscope today.

Images attached to this report
1433_20190703023406_aom.jpg 1433_20190703023415_scan.png 1433_20190703023420_scantem00.png