THESE CALIBRATION FACTORS HAVE CHANGED

PS - Keita was able to enable the damping on the TMS even though it is not spectacular.  It looks like something is rubbing as the OSEMs are not well centered, but at least some damping will slow it in the event SEI needs that this weekend.

PUM drivealign P2P and Y2Y filters were installed.

In each of the attached, foton screen shot to the left shows the actual filter installed, matlab plot to the right shows the P2P or Y2Y measurement, fit, model, and the expected TF from PUM to the test mass after the new filter takes effect.

As you see I made the filters such that ITM and ETM looks as if they share the same low Q (Q=3) resonance at 0.51 Hz for PIT and 0.6Hz for YAW. There's also a roll of at 30Hz, which is not that aggressive. If necessary you can easily add more.

I ignored the DC calibration of the measurement. I'll handle them in the gain.

The filters relevant are FM1 of H1:SUS-ETMX_L2_DRIVEALIGN_P2P, Y2Y and corresponding ITMX filters.

Scripts used for the fit and inversion as well as the filter definition files generated by the scripts are:

~controls/keita.kawabe/fit/[EI]XPUM_[PY]2[PY]fit.m

~controls/keita.kawabe/fit/[EI]XPUM_[PY]2[PY]inversion_soscoeffs.txt

[Yuta Keita Arnaud]

ETMX ITMY ITMX top mass P2P drivealign filters installed

On friday, filters were designed the same way as Keita, in order to get a single pendulum transfer function from the top mass drive to the test mass displacement in pitch. The filters were installed in the top drivealign matrix in FM1 of the P2P bank filter. ITMX filter is a copy paste from ITMY, assuming they have the same P2P transfer function (both are wires). Attached are the plots showing the design of the filters and the foton version. The transfer function after filtering has its cut off frequency at 0.45Hz for ETMX and 0.55Hz for ITMY/ITMX.

ETMX Length to pitch decoupling was also designed and installed in L2P drivealign matrix. Plots of design pending.

Jim and Travis connected all of the TMS cables to the in-vacuum feedthrus.  This required completely rerouting 2 of the cables which were destined for feedthru's further away than where they were found mounted.  None of them are screwed in.  Although the ones that Corey mentions in the table above are missing hardware, they are a tight fit on the feedthru so I would advise just leaving them as is.  The task of adding the screws to the connectors is too risky for the cable this late in the game.  Adding the screws requires one to partially disassemble the cable which could cause a break inside of the connector.

And I enabled the damping and it's working.

However, it seems like LF coil is totally out, so TMSY might not be completely free.

On which sensor to use for your demodulated signal

In order to best balance the coils one wants a sensor that captures what affects the cavity alignment the best. This is typically some sensor measuring the optic motion. However, each suspension type tried thus far has had different options.

- H1 SUS BS, a BSFM (Balanced by Keita) has only an optical lever measuring the optic. So this was the obvious choice, and as such, the LOCKIN part is directly hooked up to it. Good.

- H1 SUS PRM, an HSTS (Balanced by Kiwamu) does not have an optical lever. However, it *does* have OSEMs on the bottom stage. These are hooked up to the LOCKIN as the optical levers are on the BS. HOWEVER, the OSEM sensors, which are in the same location as the actuators, so if the basis transformation from UL LL UR LR to Optic P and Y are imperfect, then that limits the precision to which you can balance the coils. As such, Kiwamu constructed a make-shift optical lever using the REFL WFS at DC, which act like a QPD and the light source is the transmitted light from the IMC: because PRM is a 3% transmission mirror, it reflects tons of light into HAM1 when the PRC is not locked. A rather expensive light source, but GENIUS! As Kiwamu mentioned however, this work-around wasn't hooked up to the demodulator, so he just used the ASD as his figure merit.

- H1 SUS PR2, which has also has no optical lever, and because of the transmissions of the mirrors in the PRC, one can't get enough light on any nearby WFS or QPD to pull the same Izumi trickery, so we're stuck with the imperfect OSEMs. 

Once we get cavities under stable lock, we can revisit these optics which have no lever (i.e. all HSTS), because then we'll have the full ASC system with light everywhere at our disposal. But in summary, PRM is the only mirror lucky enough to do this trickery. Thankfully, as shown above, the M3 OSEMs can get some of improvement by themselves (as reported by themselves; of course we should check the improvement with global control loops and interferometers).

*nudge*nudge* Integration Issue 461 *nudge*nudge*

On the signal processing filters and OSC frequency for the LKIN part

In the lock-in amplifier process, we want the average amplitude of the product of the oscillator and the response signal (filtered at that same frequency). This average value provides a metric of the linear coupling to the drive at the oscillator frequency which one can minimize, with the benefit of directionality. In order to isolate this DC, average value of the product from the bilinear term, we low-pass the output of the demodulator. The design metrics of this low-pass are a function of the oscillator frequency chosen and, in our case, the patience of the user:
(1) One wants a significant amount of isolation at twice the oscillation frequency, such that the 2f "noise" does not interfere with the average DC value, but
(2) The response time of the low-pass filter defines how many cycles which the average includes, and therefore the response time of your metric to the knobs you have to change it.
As such, one wants a high oscillation frequency with respect to the corner frequency of the low pass. 

However, we have further design constraints: 
(3) Given that the SUS actuators are weak and the particular, off-diagonal, mechanical response to our excitation is so small at high-frequency, signal-to-noise and/or coherence limit how high we can push of oscillator frequency to roughly 5 [Hz]. 
(4) Ideally, the SUS response to pringle excitation should be frequency-independent, if we've done a proper job of digitally compensating for the analog frequency response of the actuation chain. But, if one chooses a low oscillator frequency -- say 0.1 [Hz] -- then the averaging low-pass filter will have to be much lower, and the response time becomes unbearably slow -- hundreds of seconds.
(5) In the middle, between ~0.5 [Hz] and ~5 [Hz] is a forest of SUS resonances, which, if excited, might result in all sorts of unexpected coupling to degrees of freedom not of interest, saturations of sensors, etc.

This leaves a tiny region between the given suspensions' resonant forest and where coherence drops off to stick the oscillation frequency. Keita chose 2.9 [Hz] on H1 SUS BS, and Kiwamu chose 4.1 [Hz] on H1 SUS PRM after considering these constraints, and because H1 SUS PR2 was the same SUS type as H1 SUS PRM, I stuck with Kiwamu's frequency of 4.1 [Hz].

Once the oscillation frequency is chosen, and the response signal, band-pass filter can be designed. Here, you want to isolate the response signal at the given oscillator frequency, but you need to be mindful that the impulse response of the band-pass filter is shorter than of the demodulated signal's low-pass filter. Here's how we each designed our filters:

Keita's approach (for H1 SUS BS): Lots of isolation on both the response signal band-pass and demodulated low-pass, and forgo patience. With a sharp cut-off, elliptic, band-pass the response time was greater than 5 seconds. The a sharp cut-off, elliptic low-pass, the averaging time was more than 100 sec.

Kiwamu's approach (for H1 SUS PRM): Less isolation for the less patient. Reduce the sharpness of the cutoff of both the band-pass to second order Butterworth filters, and increase the corner frequency of the low=pass to 300 mHz to reduce the averaging time to ~20 seconds. Note that he had started with an oscillator frequency of 10 [Hz] (hence the center frequency of his band-pass), but found the could not get enough coherence, reduced the oscillator frequency, and got enough response signal at 4.1 [Hz] to leak through to make a viable demodulated signal, so he didn't bother to change the design of the band-pass.

Since I just learned all of this today, and had Kiwamu, Stefan, and Keita telling me different metrics for their design, I chose what made sense to me (for H1 SUS PR2): Compromise. Move the center frequency of Kiwamu's band-pass to the oscillator frequency, but leave the shallow isolation in order to preserve the short impulse response time. Take the happy medium regarding patience and move the corner frequency of the demodulated low-pass to 50 [mHz]. This gave me plenty of SNR, lots of averages, and a impulse response time of the demodulated signal metric similar to Kiwamu's; about 10-20 seconds.

I attach bode plots and impulse response times for each of the three filters, color coded as above, with H1 SUS BS, H1 SUS PRM, and H1 SUS PR2.

Measurement Technique Expanded

Though Keita did a fairly good job explaining the principles of the technique in LHO aLOG 9079, I expand on his instructions with a little more detail below for the non-Jedi, and such that we might one day automate the process.

(A) Install the signal band-pass and demodulated I & Q filters; the same BPs in both oscillators' SIG bank, and the same LPs in both oscillators' I and Q banks.
SIG band pass: BP4.1Hz = butter("BandPass",2,3.5,4.5)
DEMOD I & Q low-pass: CLP50mHz = cheby1("LowPass",2,3,0.05)

(B) Turn on both the Pitch and Yaw Oscillators. 
As Keita mentions,
   (i) Only the amplitude of the oscillator you send out the coils matters, but the other must at least be *on* in order for the demodulation to happen,
   (ii) For each oscillator, the amplitude of the sin and cos don't matter, as long as they're the same,
   (iii) You want to demodulate both oscillators at the same frequency, so the oscillator frequency should be the same for both.
For sanity's sake, I just made both oscillators have exactly the same parameters
OSC     Frequency [Hz]     Amplitude [ct]     Sin [ct]      Cos [ct]
 P         4.1              200000 (2e6)       1000           1000
 Y         4.1              200000 (2e6)       1000           1000

(C) Turn on the EXC_SW for the stage you wish to balance, and filling out the associated stage's LKIN2OSEM matrix such that only one oscillator drives in a pringle configuration (I, like Keita, chose to use the Pitch oscillator),
     P   Y
UL  +1   0
LL  -1   0
UR  -1   0
LR  +1   0

(D) Open up two StripTool charts, one for each oscillator. Put the output of the I & Q demodulator banks for each oscillator on each tool, (e.g. H1:SUS-PR2_LKIN_Y_DEMOD_I_OUTPUT and H1:SUS-PR2_LKIN_Y_DEMOD_Q_OUTPUT). Be sure to set the y-scale for each channel to be consistent (+/- 10 [ct] worked for me, and then I zoomed in and out as necessary).

(E) Tune drive amplitude. I was initially scared of the large drive amplitudes Kiwamu had chosen, so I crept up on 200000. However, this meant when I started out with 10000 [ct], I got very little response when I began to tune the oscillator phase. So, crank up the drive to where you get lots of response to changing the oscillator phase, while making sure not to saturate the DAC. 

(F) Tune the oscillator phase
    (i) Again, drive hard enough that the separation between the I & Q phase is much larger than the noise (noise = wiggles around the DC value)
    (ii) Spin through the DEMOD Phase until you get the Q phase near zero
    (iii) Use Kiwamu's script mentioned in the main entry, perturbcoilbalance_fourosem.py, to put a *large* coil imbalance into the COILOUTF bank. This should cause a step in both the I & Q signals. The arctangent of the ratio between the the step sizes gives you the remaining distance you are away from the ideal phase:
             dPhi = 180/pi * atan( (Q_DC^{before} - Q_DC^{after}) / (I_DC^{before} - I_DC^{after}) )
The sign with which you add this to the current oscillator phase is unclear, so try both. A well-tuned oscillator phase means that abs(Q) is close to zero, and it doesn't respond [it's DC value doesn't change] to coil imbalance changes. Note, any offset the Q phase has from zero is noise that you can't tune away with the COILOUTF gain knobs. As mentioned in the above comments, this can be a result of, for example, imperfect sensors. As long as Q doesn't respond to coil unbalancing, then it's OK -- it's just one of limits on how well you can balance the coils. You'll need to tune the phase of each oscillator independently. 

(G) Set COILOUTF gains back to +/-1. Open up a DTT session (like the templates shown in the main entry), and set up a rolling averaged transfer function between the oscillator and the response sensor input. For PR2, that's H1:SUS-PR2_LKIN_P_LO (as the A channel) and H1:SUS-PR2_M3_WIT_P_DQ, H1:SUS-PR2_M3_WIT_Y_DQ. Take a reference measurement of 10-15 averages to show how badly the pringle excitation causes pitch and yaw in your response sensor. 
Remember: (as Keita says) A Pitch imbalance shows up in the Yaw oscillator's I phase, and a Yaw imbalance shows up in the the Pitch oscillator's I phase.

(H) Begin tweaking the COILOUTF bank gains (using perturbcoilbalance_fourosem.py) until the abs(I) phase goes to zero. You should stop when the noise is larger than the distance between the DC value ad zero. For the M2 and M3 stages of PR2, a perturbation of +/- 0.0005 was the precision I was able to achieve. If your oscillator phase is tuned correctly, a PIT imbalance should not affect the Pitch I phase, and Yaw imbalance should not affect the Yaw I phase. Therefore, you can do these degrees of freedom in succession, and not have to worry about going back and fourth.

(I) Because perturbcoilbalance_fourosem.py was quickly written, the perturbation increments are not exactly what you request. So by then end of the tuning process for both DOFs you'll have overly precise gains (check by caget-ing the gains in a terminal). Round off these gains to the nearest 1000th for reasons mentioned in the main entry.

(J) Making sure to have captured the "before" measurement as a reference, take a new DTT spectra to prove how well you've done!

Demod Phases and Resulting I & Q Values

After balancing the coils, I took a 300 second tds average of each I and Q channel just so I'd have a quantifiable number of "how good" I tuned the balancing. Unfortunately, there's no command line standard deviation tool, so I don't have a number for how much noise was on each channel. It was roughly +/- 0.5 [ct].
PR2 M2
     Demod Phase [deg]         Balanced Value
P       165              I         -0.017
                         Q         -0.088
Y       90               I          0.14
                         Q          0.52

PR2 M3
     Demod Phase [deg]         Balanced Value
P       160              I         0.15
                         Q         1.91
Y       87               I         0.11
                         Q         3.14

As one can see, the residual offset in the Q phase was much larger on the M3 stage than on M2. Unclear why this is, but this most probably is the reason why the results for M3 are not nearly as good as those for M2. It would be nice to have an independent sensor to verify the results, but we'll have to wait for resonant cavities and the full ASC system.

Here're a few screenshots of the StripTool session during the tuning process. They're attached in chronological order, showing
(1) Aligning the optical lever, to show the difference between junk signal and plenty of signal, then after hand-tuning the demod phase to get the Q phases close to zero
(2) Before and after the big perturnations to gather the tweak needed in the demod phase, as determined by math
(3) The process of balancing the coils once the demod phase is perfect, bringing the I phases to zero as well, with little perturbations to the balance
(4) What balanced coils look like (strikingly similar to junk signal, but just signal doesn't respond to perturbations), also what it looks like to have saturations (sudden increase in I and Q phase signal amplitude).

You should be able to get a good amount of SNR exciting with an oscillator amplitude between 115000 and 125000, depending on the strength of your driver, and how much you've imbalanced the coils.