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RyutaroTakahashi - 08:53, Tuesday 12 April 2022 (2924)Get code to link to this report
Comment to Input H4, End H1,H3 magnets fell down as expected (Click here to view original report: 2900)

Some pictures of the gluing.

Images attached to this comment
2924_20220412015241_em2gluingafter.jpg 2924_20220412015252_nm2gluing3.jpg 2924_20220412015301_nm2gluingafter2.jpg
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YuhangZhao - 20:39, Monday 11 April 2022 (2923)Get code to link to this report
Squeezing and anti-squeezing measurement @2022/04/11

After optimizing homodyne balance, alignment and checking parametric gain, I performed some sqz-asqz measurements. The result is shown in the attached figures. The measurement seems not stable enough to match the theoretical prediction curve in Fig.2. New measurements should be done.

6.19dB squeezing was observed

Images attached to this report
2923_20220411133939_figure2.png 2923_20220411133943_figure3.png
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MichaelPage - 19:41, Monday 11 April 2022 (2922)Get code to link to this report
TAMA DGS upgrade - frontend PC installation

Following on from the previous report, I ignored the Kerberos prompt since it is not used at NAOJ. When it asked me for the hostname and admin password changing server I just left both options blank. After that, the package installation completed.

I am now working on 1.3 of T2012111 (Installation procedure of new workstations (Debian10)). I'm a bit stuck on mounting the folders as shown. The instruction page doesn't seem to match the format accepted by /etc/fstb (figure 1) so I added some spaces that seem consistent with how the mount command works - i.e. device directory filesystem options 0 0. My guess is that the device 10.68.10.100:/opt/rtcds is being mounted to the director /etc/opt/rtcds but maybe I should understand which device this actually is. I get the error shown in figure 2, so something is wrong here.

Images attached to this report
2922_20220411123333_20220411185001fstb.jpg 2922_20220411123336_20220411185038mount.jpg
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NaokiAritomi - 17:05, Monday 11 April 2022 (2921)Get code to link to this report
Comment to Input H4, End H1,H3 magnets fell down as expected (Click here to view original report: 2900)

Takahashi-san glued the magnet of input mirror and released the input/end mirrors. We will start the evacuation of input/end chambers tomorrow.

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YuhangZhao - 15:43, Monday 11 April 2022 (2920)Get code to link to this report
A rough check and optimization of parametric gain before squeezing measurement @2022/04/11

MZ offset: 4.3

Pump power: 29.4mW

Parametric gain: 504/51.6 = 9.8 (Done by scanning OPO and check BAB transmission. The gain is the ratio of Airy peaks for BAB without pump and BAB with 29.4mW pump. The pump phase was continuously scanned.)

This parametric gain is consistent with old measurement.

Images attached to this report
2920_20220411084511_2449420449222702925520220411154500.jpg 2920_20220411084516_2449420449222702925520220411154447.jpg
KAGRA MIR (Absorption)
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MatteoLeonardi - 11:13, Monday 11 April 2022 (2919)Get code to link to this report
AZTEC #1 (KAGRA size)

During the weekend the first two XY maps.

The maps are attached.

Here the position and average.
Z= 71.075 (center), mean absorption: (42.4 +/- 16.8)
Z= 36.85, mean absorption: (40.8 +/- 9.7)

Images attached to this report
2919_20220411041248_075.png 2919_20220411041259_85.png
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MatteoLeonardi - 16:55, Tuesday 19 April 2022 (2933)

Additional maps.

Here the position and average.
Z=105.3, mean absorption: (61.6 +/- 13.95)
XZ map, mean absorption: (50.1 +/- 18.1)
YZ map, mean absorption: (56.8 +/- 19.1)

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YuhangZhao - 10:55, Monday 11 April 2022 (2918)Get code to link to this report
Recover of OPO locking servo

Michael and Yuhang

After pointing out the place where issue appears in elog2916, we followed the suggestion from Pierre and checked the resistor connect through J10.

1. We disconnected three pins of J10.

2. We put resistor meter between these pins. It was found that the resistor between blue and black wires becomes infinity after touching wires.

3. We peeled off the heat shrinkable tubing for black wire at the place of connecting to potentiometer. But no issue was found.

4. We peeled off the heat shrinkable tubing for blue wire at the place of connecting to potentiometer. We found the inner steel part of the wire has broken.

5. We soldered the broken blue wire.

6. We tested OPO locking servo and found it worked again. But we will see if it always work in the next week or so to confirm its recovery.

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YuhangZhao - 01:23, Friday 08 April 2022 (2917)Get code to link to this report
Comment to Mode matching from BAB to AMC after optimizing BAB matching to OPO (Click here to view original report: 2899)

Michael and Yuhang

We found the new way of fixing lens causes the problem of BAB OPO transmission to drift. This is the second lens we have in the transmission of OPO along the FIS measurement path. So we need to find a new way to fix this lens.

Now we put it on a pedestal pillar. After doing so, a large portion of p-polarization appears. Before removing this p-pol, it composes of ~5% of total power. However, we found that we could convert p-polarization completely to s-polarization by tilting HWP. 

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YuhangZhao - 00:17, Friday 08 April 2022 (2916)Get code to link to this report
Issue of OPO locking servo

Marc, Michael, Yuhang

It was reported in elog2627 that we have problem of OPO locking servo, which works from time to time.

To solve this problem, we contacted Pierre for suggestions. Now, it becomes clear where the problem is from.

Firstly, we need to notice that we should check the OPO locking servo circuit when 'servo output' is just an offset. The test result reported in this elog is in this situation.

We found a triangular wave at J10 Pin3 but not at J10 Pin2. According to Pierre, this is related to the 'amplitude' potentiometer. We will check the impedance between J10 pin1/pin2/pin3. According to Pierre, the total impedance should be about 2k. If not, we need to buy a new one and replace it: Bourns (3590S-2-503L). We should make sure there is no issue for this potentiometer soldering.

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MarcEisenmann - 19:48, Thursday 07 April 2022 (2915)Get code to link to this report
os/software installation for Front End PC in central building

Marc, Michael, Yuhang

Today we installed Debian 10 on the Front End PC of the central building (and during this process removed the 2 previously installed os).

Yamamoto-san kindly gave us instructions for this (and also future) installation.

Documentations can be find from these links or inside KAGRA dropbox (folder Subsystem/FKC/TAMA_DGS/Reference documents) :

[1] https://dcc.ligo.org/LIGO-T1600055/public

[2] https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=12111

 
 
Some additional informations :
We used the amd64 installer of Debian 10 together with Rufus software on a pink usb key for the installation
We set up the debian partition to fill the entire 1TB hard-disk with separated /home, /var and /tmp partitioning (recommended for server installation to avoid flooding the /home partition with temporary data during data transfer)
The /temp and /var partitions were left at the default values (1 and 2 GB respectively?)
The /swap partition size was increased to 32 GB. This is a standard recommendation to avoid RAM saturation. But currently we have not seen recommended /temp, /var, /swap sizes in any DGS related documentation.
The network hostname is FEcentral.
The user name is ops and we then setted up the controls user (so that controls user ID is 1001 as recommended by Yamamoto-san)
We gave sudo authorization to ops and controls user.
The root, ops and controls passwords are the same as for the standalone pc
 
We install the version 1.0.6 of the ligo repository (see [2]) which seems to be the latest one.
When trying to install the cds-workstation package, we were asked to 'configure Kerberos authentification' (see fig 1)
We are not sure about this step so we are asking details to Yamamoto-san.
Images attached to this report
2915_20220407124804_dgskerberos.jpeg
KAGRA MIR (General)
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MarcEisenmann - 13:56, Thursday 07 April 2022 (2914)Get code to link to this report
cleaning of repolished AZTEC mirrors

Marc, Matteo

Today we received 2 25 kg substrates grown by AZTEC and repolished by Sigma Koki.

We applied first contact on one of their surfaces and will apply on their other surfaces later today.

On each mirror barrel there is written 'top' followed by some characters.

We added the mirror number (1 or 2) as well as an arrow pointing towards the 'top' sign.

We will use this as our reference for the top part of the mirror during measurement.

Images attached to this report
2914_20220407065649_repolishedaztecsign.jpeg 2914_20220407065653_repolishedaztecfc.jpeg
KAGRA MIR (Absorption)
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MarcEisenmann - 20:09, Wednesday 06 April 2022 (2913)Get code to link to this report
quick annealed AZTEC measurements

Because new substrates should arrive soon, we decided to pursue our investigation of the annealing of the AZTEC samples by taking several XY measurements with 1 mm step size (instead of 0.25 mm for the previous ones).

The results are reported in the attached entry where only z changes as : 45, 47 49 51 53 56 mm (same order as in picture).

Because of the large step size, it was not so obvious to draw conclusion on the improved/degraded homogeneity with annealing so we decided to start again measurements with 0.5 mm step size.

We are not so sure why the measurement at z = 45 mm (fig 1) has so many values at 0 ppm/cm (the surface should be around 41 mm)

Images attached to this report
2913_20220406130745_z45.png 2913_20220406130750_z47.png 2913_20220406130757_z49.png 2913_20220406130801_z51.png 2913_20220406130805_z53.png 2913_20220406130811_z56.png
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MichaelPage - 16:01, Tuesday 05 April 2022 (2911)Get code to link to this report
Squeezing - local oscillator alignment

Yuhang and Michael,

We would like to characterise frequency independent squeezing at the best performance we can manage before replacing the OPO. One task is to optimise the alignment of the local oscillator to the alignment mode cleaner, and same for squeezing (i.e. bright alignment beam). Here we checked the alignment of the LO to AMC. We found that the mode matching was still quite good, but there was some undesirable polarization that was leaking. So we added a half wave plate in the LO path just before the homodyne beam splitter. We adjusted the HWP polarization rotation, as well as the tilt and transverse displacement, to remove the unwanted transmission peaks. Then we aligned the LO to reduce higher order modes. The result is shown in figures 1 (TEM00) and 2 (others).

Also we noticed it was quite hot in the clean room. Checking the air conditioning gave a temperature of 25.9 C and humidity 32.8%. Given that it was cold leading up to this measurement we increased the cooling to the cleanroom air conditioner. Some alignment may be affected.

Images attached to this report
2911_20220405090143_20220404171124.jpg 2911_20220405090148_20220404171003.jpg
KAGRA MIR (General)
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MarcEisenmann - 15:48, Tuesday 05 April 2022 (2912)Get code to link to this report
Preparation of absorption measurements

Marc, Matteo

We removed the AZTEC sample and installed the 2 razor blades on the translation stage.

We tuned the input polarization of the pump beam to s polarization (ie hwp angle of 45 deg)

With the translation stage set at z = 20 mm, we measured the distance between the edge of the injection breadboard and the blades to be 92 mm (horizontal one) and 97 mm (vertical one).

We measured the beam parameters as presented in fig 1 (again the z = 0 mm position is the same as in Manuel PhD) and got w0 = 36.24 um at z = 59.24 mm ie 2 mm further away than previous calibration.

By measuring the distance between the last lens of the inejction breadboard and the blades we tried to improve the vertical incidence angle at better than -0.248 deg.

Using the other blade we confirmed that the horizontal angle of incidence is about 2.7 deg.

For previous surface calibration we used z = 35 mm and z_IU = 68 mm. We did few scans at z = 35 mm and 37 mm but found out that the best calibration was obtained at z = 35 mm.

We measured R_surface = 16.12 /W and R_bulk = 0.6718 cm/W (where z_IU = 67.34 mm).

We reinstalled the AZTEC sample (orientation should be the same as previous measurements) and using the drop in the DC power we measured X_center = 327.293 mm and Y_center = 122.55 mm.

We reinstalled the black cover, all the required beam dumps and increased the laser power to about 7 W.

We started long z scans to find the 2 surfaces of the sample.

At first we found out some strange drop of the dc signal with z about 80 mm. It was because the translation stage was hitting the imaging unit black cover.

After moving it a bit further away we recovered the expected situation and started several measurements in the XY plane with 1 mm step size.

Images attached to this report
2912_20220405083944_20220404verticalsize.png
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RyutaroTakahashi - 17:05, Monday 04 April 2022 (2910)Get code to link to this report
Comment to Input H4, End H1,H3 magnets fell down as expected (Click here to view original report: 2900)

Pictures in the gluing today.

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2910_20220404100418_magnetonem25.jpg 2910_20220404100443_magnetonem26.jpg
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NaokiAritomi - 15:03, Monday 04 April 2022 (2909)Get code to link to this report
Comment to Input H4, End H1,H3 magnets fell down as expected (Click here to view original report: 2900)

Today Takahashi-san glued the two magnets of end mirror. We will glue the magnet of input mirror and release the input/end mirrors next Monday. 

KAGRA MIR (Polarization)
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HomareAbe - 17:54, Friday 01 April 2022 (2908)Get code to link to this report
Calibration of laser to measure compensator
I checked the beam property outside clean room.
beam waist w_0 = 2.71627188e-05 [m]
waist position z_0 =8.28865994e-02 [m].
I will put lens to put the laser into PD.
Images attached to this report
2908_20220401105322_calibrationlaseroutsidecleanroom.png
KAGRA MIR (Polarization)
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MarcEisenmann - 12:07, Friday 01 April 2022 (2907)Get code to link to this report
birefringence measurements of annealed AZTEC sample

This entry reports the birefringence measurements of annealed AZTEC sample.

Note that here I normalized the s and p polarization power by their sum (see fig 1) so to be independent on the power fluctuations.

This does not affect the results much as we were considering the ratio of these power in any case.

Images attached to this report
2907_20220401050659_power15.png 2907_20220401050703_pola0.png 2907_20220401050708_pola11.png 2907_20220401050711_pola23.png 2907_20220401050715_pola36.png 2907_20220401050718_pola50.png 2907_20220401050723_pola70.png 2907_20220401050727_stress.png 2907_20220401050731_deltan.png
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MarcEisenmann - 20:56, Thursday 31 March 2022 (2906)Get code to link to this report
Comment to Assembly of the new DGS rack (Click here to view original report: 2905)

Marc, Yuhang

We installed the GPS cable on the top of all the cables going around the central building up to the new dgs rack.

During this operation, we found the lightning arrester (HP 58505A). It is now installed above the bottom end of the stairs. We still need to connect it to the ground.

We also found out that the gps receiver had the led 'Alarm' on. But because we now have the lightning arrester we are confident that we could connect the gps cable directly to the irig-b card.

We turned on the 2 pc and during the boot we could saw the hardware that we previously installed. The os 'CentOS' is already installed but we don't know the pcs password so we could not investigate more.

We connected the tcp-ip switch to the switch used by the standalone pc with a 10 m long ethernet cable and connected the 2 pcs to this switch.

While turning off the front end pc (offline) it updated some drivers.

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MarcEisenmann - 19:53, Wednesday 30 March 2022 (2905)Get code to link to this report
Assembly of the new DGS rack

Marc, Yuhang

Today we installed all the required pcs and switches for the new DGS in the rack close to the input chamber.

From top to bottom there is :

  • dolphin switch
  • front end pc for central building
  • myrinet switch
  • tcp-ip switch
  • data concentrator pc
  • gps receiver
  • camera server
  • smart ups

We put label on each component but did not connected anything yet.

The key of the data concentrator pc is on the blue plastic container on the right side of the rack

Images attached to this report
2905_20220330125237_newdgsrack.jpeg
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MarcEisenmann - 20:56, Thursday 31 March 2022 (2906)

Marc, Yuhang

We installed the GPS cable on the top of all the cables going around the central building up to the new dgs rack.

During this operation, we found the lightning arrester (HP 58505A). It is now installed above the bottom end of the stairs. We still need to connect it to the ground.

We also found out that the gps receiver had the led 'Alarm' on. But because we now have the lightning arrester we are confident that we could connect the gps cable directly to the irig-b card.

We turned on the 2 pc and during the boot we could saw the hardware that we previously installed. The os 'CentOS' is already installed but we don't know the pcs password so we could not investigate more.

We connected the tcp-ip switch to the switch used by the standalone pc with a 10 m long ethernet cable and connected the 2 pcs to this switch.

While turning off the front end pc (offline) it updated some drivers.