NAOJ GW Elog Logbook 3.2


we found the pd DET10A for the 633nm probe didn't give any output. Replacing the power supply with a 12V battery solved the problem. We checked the power supply with a multimeter and it looks fine (9V of output). We figured out that it's the adaptor bad contact. We continue working using the battery.
We made a scan of the surf ref sample and maximized the AC signal adjusting the pump alignment.
Current experimental parameters:
Laser current 1.3A Power meter value: 31mW (without sample)
DC signal: 3.26 (with sample) (3.4V at the max of the scan)
AC signal max: 0.2V


After doing that we have put to zero the local control error signals and we have closed all the local controls loops. Then, we could fine tune the alignment with the local controls and lock the cavity stably.
We took pictures of each local control panel while the cavity was locked (See figure from 1 to 4: END, INPUT, BS, PR). The lock can last for more than 30 minutes (we had to unlock on purpose before going away). See figure 5 for the transmitted beam during the lock. We took photos of the oscilloscope showing the transmitted power just after achieving the lock (pic 6) and after 30 min of locking (pic 7). In the best alignment condition it is about 1 V.

So I did experiment today. Fortunately, I found a PBS without costing a lot of time. Although yuefan told me that the most consuming part of job in TAMA is finding something.
Then I improvised the testing set-up. I found most of the light is reflected by the PBS. However, I didn't know the ratio between s and p polarization should be around 1000, which I learnt from Matteo latter on. But this can explain why the energy doesn't conserve if I put half-wave plate in-between. You can refer to attached picture 1. I will take the picture of weak light and measure it next time. As Matteo suggested, the weak signal will have less fluctuation which is important for measurement.
The power evolution is shown as attached picture 2. The attached picture 3 is about the diffraction angle.
I will do the measurement of green soon and compare it with this one. Before that we will refine the alignment of some wave plates.

I use the holes on the bench to estimate the incident angle. The test are divided by two sorts. For the first one, the incident beam is aligned with the arrow on the grating. For the second one, it is opposite.
I also test it by using a wave plate. It is used to see if polarization can affect the diffraction and if so, how it can affect.

In the entry 613, I made a miscalculation. This entry is a correct one.
I re-calculated optimal lens pairs for a telescope for the mode cleaner (green) with accurate dimensions (see here for the drawing). Figures attached show lens pairs that seem acceptable and the parameters I used.
In the case of the first figure, the mode matching factors are 99.718% and 99.601% for vertical and horizontal axes, respectively.
In the case of the second figure, the mode matching factors are 100% and 99.727% for vertical and horizontal axes, respectively.
The lens with 75.6 mm focal length that we already have is one without any surface coating thus low transmissivity. So I think the first case is preferable.

Figures were missed in the entry. They are shown here.

Open-loop transfer function
On 12/21, we measured open-loop transfer function of SHG control, because a new servo was designed and installed by Matteo Leonardi. For the previous situation, please refer to an entry 585.Fig.1 shows open loop transfer function of the SHG control. We have three switches on the new servo, each of them is corresponding to a different integrator. Measurements were conducted for three combinations of these integrators. Noise level inserted were different depending on the conditions in order to keep the cavity being locked. PZT resonance point is located aroun 25 kHz. Unity gain frequency is shown on each graph by a black line (770 Hz, 1380 Hz, and 1610 Hz). You can see a high phase margin (approx. 90 degree) when the mid integrator ON.
We also measured power spectra of an error signal on the loop and DC signal from the photo detector which is monitoring transimitted light from the SHG (Fig.2). You can see a spike around 600 Hz. I am not sure what it means.
All spectra were taken by Agilent 36540A.
Output power stability
Fig.3 shows a long term (1000 second) stability of the SHG output. Stability of the SHG is much better than before. In this moment, we do not find a large fluctuation in the SHG output (532 nm) as we did so far.

A comment on the local controls large output: the voltage range at the output of the DAC is +/- 10 Volts. So If the correction signal is out of this range (as in the case of picture 1) the output is saturating and the control loop is likely not to be working properly (as can be seen from the large RMS in picture1).
More in general, looking at the error singnal, it seems to me that we are still affected by the "spikes issue". It could be useful to compare the open loop rms with the reference values in the absence of spikes.

We know for PDH control, the local oscillator phase and signal phase must match. But the cable length can affect this phase. So after changing cables, we need to set the phase of signal generator again.
Firstly, we need to close the loop for local control to make the light beam interferes well inside the cavity. However, I found the local control goes oscillation even with the previous value. The previous value means the value we used for locking yesterday. I should mention this abnormal case happened the day before yesterday.
After a very long time of adjusting, I found the the local can be fairly stable while the output of local is large(Fig 1). I adjusted it a little and make the output much smaller(but it is still around 40). Then I could find the beam through the end room camera.
Secondly, I took the photo of beam on the first iris(Fig 2,3) and the second iris(Fig 4).
Thirdly, I went to set the PDH phase. I set different value to see how the error signal looks like. I took three pictures(Fig 5,6,7) for this processes. We can deduce from them the worst case should between 80 and 90 degrees. So I set the phase as 175 degrees.
Finally, I found the transmitted signal decreases from 1V to 0.6V(Fig 8). And I found this is not caused by the SHG. Now the SHG locking is pretty pretty good! This is caused by the bad local control. The position of mirror drifts away fast. However, this maybe also caused by the large output of local control. Besides, I and Matteo measured the TF of BS pitch. Matteo said it is not a good control system according to this TF. So the local control definitely should be improved.
A comment on the local controls large output: the voltage range at the output of the DAC is +/- 10 Volts. So If the correction signal is out of this range (as in the case of picture 1) the output is saturating and the control loop is likely not to be working properly (as can be seen from the large RMS in picture1).
More in general, looking at the error singnal, it seems to me that we are still affected by the "spikes issue". It could be useful to compare the open loop rms with the reference values in the absence of spikes.


see the attached document

While I check the first iris, I find the pattern on it is really similar with the pattern we get from infrared. So I think the problem should come from the bench. Refer to figure 2.
But the locking is not stable enough, I will check the phase of two signals sending to EOM. Refer to figure 3.

In the entry 613, I made a miscalculation. This entry is a correct one.
I re-calculated optimal lens pairs for a telescope for the mode cleaner (green) with accurate dimensions (see here for the drawing). Figures attached show lens pairs that seem acceptable and the parameters I used.
In the case of the first figure, the mode matching factors are 99.718% and 99.601% for vertical and horizontal axes, respectively.
In the case of the second figure, the mode matching factors are 100% and 99.727% for vertical and horizontal axes, respectively.
The lens with 75.6 mm focal length that we already have is one without any surface coating thus low transmissivity. So I think the first case is preferable.

After the installation of the coverage on optical bench, we are now checking the situation.
Note that our AOM is very easily misaligned by touching the cable.
Temporarily, I put a post right next to the cable in order not to make it move a lot (see a figure attached).

In order to allow their work all the cables from the bench were disconnected and the racks were moved away.
After the company work the cables are being reconnected (ongoing).

1. For leaving space for the shield case, we moved two irises close to PR. Due to one of them is used to fix the lens rail, so we need to adjust the lens again to get good mode matching. Adjusting that lens costed a period of time, and then we can lock the cavity as it before.
2. Then we improvised a tripod to hold the camera, which is used for the near iris in the vacuum tube. Then we adjusted its position. Note that the camera we used here if found on the optical bench in the central room.
3. While we can see the EM transmitted signal, we rise up both of two irises one by one. And we cannot see a clear infrared on the iris. At the same time, the transmitted signal was blocked partly.
By the way, I found the transmitted signal of EM is on the edge of EM chamber view port.
(You can see the infrared checking video by clicking the following link.)
https://drive.google.com/open?id=1CqVLnQrDSaECMgJzHP2Fivabp3ip_E8T
https://drive.google.com/open?id=18AbcXlJ9LMBlW7SOZ7-MdkWTKyISZRya

Firstly, I checked the camera for the second iris. I brought two cameras and one cable around the second iris back. We have a PR's camera, so I used it to check. The method is to replace one thing at a time. In this way, we can diagnose the replaced component. I found the cable is fine but two cameras are broken.
Broken camera 1: SONY NO.92980
Broken camera 2:SONY NO.161274
Secondly, I found the drifting of SHG is really serious.(with the driven voltage set around 50V). Within only 30 min or less, the power decreased from 50mW to 30mW and final 10mW. The measurement point is ahead of filter cavity's EOM.
Finally, I took a picture of the beam which is sent to our filter cavity. You can see from the attached photo. The beam is a combination of a large bright beam point and a small weak point. I cannot make it a rough circle by just adjusting the turing mirror or local control offset.

Firstly, about the losing of the camera of the second target(or irises or aperture). I checked the link and cable. I also changed the driver for this camera. All of them didn't bring back our camera. But I found there was a gap on the case of camera.(As you can see in the figure one.) Maybe this is one reason, so I will check its capability further more.(Since we can see the scattered light or halo, I think there is no need to use the second irises. But brining it back will be a good thing for the future.)
Secondly, about the cable in the end room. I almost stumble because of the cable around the end room's bench. The reason is one of the cables is really short, which makes it suspended away the ground. And this happened on Thursday. On Friday, I cannot find the transmitted signal from the end mirror. I checked many things and finally realized where the problem would be. If you read previous part carefully, you can see the problem comes from the short cable. It causes the misalignment of the QPD. So I think we should do something to avoid this happens again.
Thirdly, I can find something really similar with yuefan's previous infrared beam gazing. You can find the video I took from the link in the bracket. But I tried to change the local control offset for each mirror, finding it's really different from the behavior of green beam. For example, the changing of this possible infrared beam does't follow the changing of the local control offset very well. Sometimes it looks really like the halo after changing the local control offset. I need to confirm this strictly, but the signal here is really weak! I feel the confirmation is really difficult.
(https://drive.google.com/file/d/12OmtNB93hNnNigcgu_0SNxJNy5pxSIPq/view?usp=sharing)
Fourthly, Tomura-san found we can use the sensor card to sense the infrared beam in the end room. I used it to check the light from EM chamber output port to the camera. I found almost one third of the beam is lost because the alignment on the end room bench. So I changed the alignment a little bit. The change includes one lens, one 45 degree mirror(Actually I don't know what this mirror for) and the camera. Now we can see the whole two half of halos by changing the angle and height of camera. You can see the video by clicking the attached link as following.
(https://drive.google.com/file/d/1MsWtaURQJLrXH1PSE4-g_qudrmI73w9c/view?usp=sharing)
Fifthly, Tomura-san suggested there is possibility that something is blocking on the infrared. Because you can see a black line in the spot of reference infrared beam. But I check the layout of our experiment, it's not the beam sending to cavity. However, the reference which is sending to cavity has also something like defect. The defect is the combination of a small spot and a larger spot. It's really like the scenario we can see from the infrared transmitted signal of EM, where there is a bright halo and a darker halo.(You can see this combination from the second video)
Sixthly, I checked the bright halo by changing the local control offset. As you can see from the attached second and third photo, there is angle changing of halo. And the halo is flashing. I suspect this halo can be the what we want to find. I will try to figure it out soon.
In the end, I can ride the bicycle very well now! I need to go to end room and go back many times to find the signal, which drives me to ride bicycle many times. This is really an useful skill and a good way to calm down or feel balance. &( ^___^ )&