NAOJ GW Elog Logbook 3.2
* INPUT LP Filter: 36kHz
* OUTPUT 2nd order LP filter: 120 kHz - Q = 0.79
* OUTPUT LP filter: 155 kHz
* pole (LP filter R54-C54): 145 kHz
* Integrators:
- 1/f^4 : 4 zeros @ 1.55kHz
- 1/f : 1 zero @ 145 Hz
=> New servo: newservo.jpg
* INPUT LP Filter: 675kHz
* OUTPUT 2nd order LP filter: 375 kHz - Q = 0.74
* OUTPUT LP Filter: 330 kHz kHz
* pole (LP filter R54-C54): 660 kHz
* Integrators:
- 1/f^4 : 4 zeros @ 2.7kHz
- 1/f : 1 zero @ 145 Hz
* Differentiator (added compared to the old version):
- zero: 33 kHz
- pole: 725 kHz
Following the discussion we had offline, I upload a measurement that was done few years ago when I was in the Padova group. The measurement is a characterization of the laser PZT gain as function of the frequency.
The laser is a 1W Mephisto laser from Coherent.
Yesterday I measured power after the first BS on in-air bench. They are 16.84mW and 601.5mW seperatly. This means the ratio is 36:1 of this 2-inch BS.
And I also measured the power going into SHG, which is 413.3mW.
[Eleonora, Matteo L.]
In order to investigate the fluctuations of the IR reflected power during the lock-unlock measurement, we have plotted the histogram of the data both for a lock and for an unlocked period.
We observe that for the unlocked period the noise seems to be gaussian as we expected assuming that it is domated by input power fluctuations.
On the other hand the fluctuations during the locked period dosen't seem to be gaussian and shows a "longer tail' on the right side. This is compatible with fact that the mechanisms explaining such fluctuations (in addition to the input power one), that is misalignments and lock accuracy, are expected to act only increasing the reflected power.
We don't know which is the best distrution to use to fit the locked data. Up to now they have been treated as if they were gaussian.
The last plot shows the contour of the normalized histogram for different set of lock/unlock taken during the same measurement.
I have been doing a simulation of TAMA optical bench using OptoCAD. Here attached interim results. It has not been completed. You can convert an attached text file into a fortran source code by changing .txt to .f90 for eample (depending on your environment). For some unknown reason (probably a problem of windows OS), I couldn't divide code into multiple files (like a main program and some external files beside it) as is a common method to gain readability of a long code. Consequently, the source code got complete mess. Basically it is just a list of optical component so you caan just add components which will be placed later on. For a green beam part at least it is consistent to the actual situation. For an IR beam part it should be changed afterwards.
alignment of the imaging unit:
put the surface reference and aling the IU in order to have the blade sharp image on the pd. Do a scan and move the z axis to the central peak maximum Maximize the AC/DC signalas goog as possible. Do again the scan (see first screenshot). The imaging unit position is 65.5mm, set exactly at the distance that have to be moved to measure the 154mm thick kagra sapphire. To measure the substrate we have to move the IU to 0mm.
Calibration: bulk reference
pump power=32mW, DC=4.1V, IUposition=65.5mm, AC=60mV (see second screenshot)
Maps of KAGRA substrate shinkosha#7: 130mm diameter, 1mm resolution, z_stage=110mm,70mm,35mm
plot the maps with the same color scale
Loss measurement 28/03/18
Reflectivity: 89%+/- 2.5% => Losses: 44 +/- 12 ppm
Mismatching/misalignement considered in the estimation: 11% (worse than usual)
New did a new measurement of RTL with lock/unlock.
Reflectivity 84% +/- 2% => Losses 63±12 ppm
We considered that 7% of the input light is not coupled into the cavity.
We have measured the spectrum of the piezo correction, through the channel PZT mon.
In the plot we took into account the factor 100 of attuation of the channel PZT MON and we used the calibration 2 MHz/V.
The spectrum looks similar to that we measured in july. We fitted it with the curve 7.5 kHz/f, which is compatible with the expected free running laser noise.
I attach the .txt file with data not calibrated.
In order to increase the statistic yesterday we repeated the measurement of the round trip losses, with the lock unlock technique.
Since we did it in two different moments of the day the alignement conditions were likely to be different.
| reflectivity | losses | |
| #1 | 0.87±0.02 | 50±13 |
| #2 | 0.80±0.03 | 81±16 |
The reflectivity has been computed by taking the mean of the time series between a lock and an unlock period. The error is computed as the progagation of the standard deviation of these two set of data.
We estimated that 7% of the input light does not couple into the cavity.
Last week we measured the bandwidth of cavity. By using this data, we also did the extrapolation and got the losses.
We considered all the losses come from the increase of end mirror transmissivity. Then we did like this:
- Fix r1 as sqrt(1-T1) and T1=0.136%.
- Use the Airy distribution to fit EM transmission and get R2.
- Losses is calculated as 1-R2-T2. T2 is set as 3.9ppm.
| Velocity | Bandwidth | Finesse | Losses | r2 |
| 200Hz/s | 119Hz | 4191 | 134 | 0.999931 |
| 400Hz/s | 114Hz | 4355 | 78 | 0.999959 |
| 80Hz/s | 115Hz | 4312 | 92 | 0.999952 |
After measuring the Tama-mirror-size sapphire substrate Sample2 (see elog entry 678), I measured the Sample1. I upload the maps of Sample1.
I plot the maps of the small sapphire sample we measured.
The first is the overall picture of the clean booth, from this picture you can see the three different parts Yuhang mentioned, the clean level increase from the closest to the furtherst.
The second and the third pictures was where we put the clean suits and gloves in the first clean booth, we are going to add another drawers next to the present one.
The fourth one is the shelf we put in the middle clean booth.
The last picture is the tube between the bench clean booth and the PR tank. We cut the wall of the clean booth with a cross-cutting from inside, the tube is fixed on the view port with a metal ring. Between the tube and the clean booth, we didn't put anything.
Last Thursday, the company came here to install our clean booth(three parts).
1. The first part is for in-air bench, it is high level clean.
2. The second part is for electronics and control.
3. The third one is for changing cllean suit.
After this installment, we cleaned everything would be put in and already in the room. We made also other changes.
1. We connected everything need to be connected. All the cables are gonging under the steps around the in-air bench.(Fig 1).
2. The Laser switch boxes are all under the in-air bench now.(Fig 2)
3. The control computer and transmission camera monitor are in the second part clean room now.(Fig 3)
Finally, we brought back the locking of our filter cavity both for green and infrared.
The first is the overall picture of the clean booth, from this picture you can see the three different parts Yuhang mentioned, the clean level increase from the closest to the furtherst.
The second and the third pictures was where we put the clean suits and gloves in the first clean booth, we are going to add another drawers next to the present one.
The fourth one is the shelf we put in the middle clean booth.
The last picture is the tube between the bench clean booth and the PR tank. We cut the wall of the clean booth with a cross-cutting from inside, the tube is fixed on the view port with a metal ring. Between the tube and the clean booth, we didn't put anything.
I put some other parameters of fitting here.
| velocity | bandwith | r1(r2 is assumed as 1) | Finesse |
| 200Hz/s | 119Hz | 0.999251 | 4190 |
| 400Hz/s | 114Hz | 0.999279 | 4355 |
| 80Hz/s | 115Hz | 0.999272 | 4311 |
r1=0.9992673 +/- 1.19e-5
Finesse=4285.3 +/- 69.7
I have compared the transfer function measured in entry #693 and the error signals measured in the entry #699 with the Matlab model of the servo.
#1 plot: TF measured vs model. Eleonora's thesis model (PZT pole of 30 kHz).
#2 plot: TF measured vs model, where I changed the high frequency part of the TF in order ot fit the measurements. In particular, I have moved to higher frequency the frequency of the PTZ pole. This can be explained due to the fact that the PZT transfer fucntion is not really known, even if this is strange that we have to change the model vs Eleonora's thesis measurements.
#3 plot: TF measured vs model. I changed the high frequency part and also changed the frequency of the zeros at 1540 Hz to 1000 Hz. This is strange, since the frequency of these poles is given by the electronics, but maybe the coherence of the TF measuremnt around 1 kHz is not very high.
#4 plot: error signals measured vs model. In the model I have used a laser frequency noise of 7.5 kHz/f /sqrt(Hz), as measured during Eleonora's thesis. We remark that the error signals are higher than the model.
#5 plot: error signals divided by 2.5 vs model. The factor 2.5 is not explained. A wrong calibration factor? Some problems with data acquisition? An higher input noise?
As further measurement, I would suggest to save the correction signal of the PZT and maybe try to have a better measurement of the TF below 1 kHz.
We have measured the spectrum of the piezo correction, through the channel PZT mon.
In the plot we took into account the factor 100 of attuation of the channel PZT MON and we used the calibration 2 MHz/V.
The spectrum looks similar to that we measured in july. We fitted it with the curve 7.5 kHz/f, which is compatible with the expected free running laser noise.
I attach the .txt file with data not calibrated.
After using the correct Airy function, we can get a better fit of our filter cavity. It gives us the results as below.
| velocity | bandwith |
| 200Hz/s | 119Hz |
| 400Hz/s | 114Hz |
| 80Hz/s | 115Hz |
According to this result, we can say our filter cavity's Bandwidth(for infrared) is 116 +/- 2.16Hz.
I put some other parameters of fitting here.
| velocity | bandwith | r1(r2 is assumed as 1) | Finesse |
| 200Hz/s | 119Hz | 0.999251 | 4190 |
| 400Hz/s | 114Hz | 0.999279 | 4355 |
| 80Hz/s | 115Hz | 0.999272 | 4311 |
r1=0.9992673 +/- 1.19e-5
Finesse=4285.3 +/- 69.7
Actually, there is a factor 2 to take into accunt in the definition of the decay time we used, that is P = P0*exp(-2*t/tau)
(see https://www.osapublishing.org/oe/abstract.cfm?uri=oe-21-24-30114 )
So the decay time from the "hand cutting" fit should be: 2/tau = 3149 => tau = 0.6 ms. Anyway, since I used this definition also for computing the filter cavity decay time (about 2.7ms) if I'm not wrong we have a factor 5 of difference between the two, in any case.
According to the fit the decay time is 0.3msec that is a factor of 10 smaller than the cavity decay time.
For the purpose of getting a better estimation of cavity bandwidth, we want to fit the transmission of End Mirror.
I tried three model, including gaussian function, generalized normal distribution and airy pattern function. However, none of them seems fit very well. Before proceeding to next step, I would like to ask for some suggestions.
