diff --git a/figs/h-infinity-2-blocs-constrains.pdf b/figs/h-infinity-2-blocs-constrains.pdf index df7064a..6d23172 100644 Binary files a/figs/h-infinity-2-blocs-constrains.pdf and b/figs/h-infinity-2-blocs-constrains.pdf differ diff --git a/figs/h-infinity-2-blocs-constrains.png b/figs/h-infinity-2-blocs-constrains.png index 786cd70..07e8069 100644 Binary files a/figs/h-infinity-2-blocs-constrains.png and b/figs/h-infinity-2-blocs-constrains.png differ diff --git a/index.html b/index.html index 4497f64..a7656b0 100644 --- a/index.html +++ b/index.html @@ -4,7 +4,7 @@ "http://www.w3.org/TR/xhtml1/DTD/xhtml1-strict.dtd">
- +-To understand the design challenges of such system, a short introduction to Feedback control is provided in Section 1. +To understand the design challenges of such system, a short introduction to Feedback control is provided in Section 1. The mathematical tools (Power Spectral Density, Noise Budgeting, …) that will be used throughout this study are also introduced.
@@ -108,60 +114,131 @@ The mathematical tools (Power Spectral Density, Noise Budgeting, …) that To be able to develop both the nano-hexapod and the control architecture in an optimal way, we need a good estimation of:We then develop a model of the system that must represent all the important physical effects in play. -Such model is presented in Section 4. +Such model is presented in Section 4.
A modular model of the nano-hexapod is then included in the system. The effects of the nano-hexapod characteristics on the dynamics are then studied. -Based on that, an optimal choice of the nano-hexapod stiffness is made (Section 5). +Based on that, an optimal choice of the nano-hexapod stiffness is made (Section 5).
Finally, using the optimally designed nano-hexapod, a robust control architecture is developed. -Simulations are performed to show that this design gives acceptable performance and the required robustness (Section 6). +Simulations are performed to show that this design gives acceptable performance and the required robustness (Section 6).
-+In this section, we first introduce some basics of feedback systems (Section 1.1). +This should highlight the challenges in terms of combined performance and robustness. +
+ + ++In Section 1.2 is introduced the dynamic error budgeting which is a powerful tool that allows to derive the total error in a dynamic system from multiple disturbance sources. +This tool will be widely used throughout this study to both predict the performances and identify the effects that do limit the performances.
-We usually analyze dynamical systems in the frequency domain using the Laplace transform. +
- - -+
+The use of feedback control as several advantages and pitfalls that are listed below (taken from schmidt14_desig_high_perfor_mechat_revis_edition):
-Figure 1: Figure caption
-+Let’s consider the block diagram shown in Figure 1 where the signals are: +
++And the dynamical blocks are: +
++
+Figure 1: Block Diagram of a simple feedback system
++Without the use of feedback (i.e. nano-hexapod), the disturbances will induce a sample motion error equal to: +
+\begin{equation} + y = G_d d \label{eq:open_loop_error} +\end{equation} ++which is out of the specifications (micro-meter range compare to the required \(\approx 10nm\)). +
+ ++In the next section, we see how the use of the feedback system permits to lower the effect of the disturbances \(d\) on the sample motion error. +
++If we write down the position error signal \(\epsilon = r - y\) as a function of the reference signal \(r\), the disturbances \(d\) and the measurement noise \(n\) (using the feedback diagram in Figure 1), we obtain: \[ \epsilon = \frac{1}{1 + GK} r + \frac{GK}{1 + GK} n - \frac{G_d}{1 + GK} d \]
@@ -172,83 +249,203 @@ We usually note: S &= \frac{1}{1 + GK} \\ T &= \frac{GK}{1 + GK} \end{align} --\(S\) is called the sensibility transfer function and \(T\) the transmissibility transfer function. +where \(S\) is called the sensibility transfer function and \(T\) the transmissibility transfer function.
-And we have: -\[ \epsilon = S r + T n - G_d S d \] +And the position error can be rewritten as:
+\begin{equation} + \epsilon = S r + T n - G_d S d \label{eq:closed_loop_error} +\end{equation} +-Thus, we usually want \(|S|\) small such that the effect of disturbances are reduced down to acceptable levels and such that the system is able to follow the change of reference with only small tracking errors. -
- --However, when \(|S|\) is small, \(|T| \approx 1\) and all the sensor noise is transmitted to the position error. -
- - --
-Figure 2: Figure caption
--The nano-hexapod characteristics will change both \(G\) and \(G_d\). -
--The Power Spectral Density (PSD) \(S_{xx}(f)\) of the time domain \(x(t)\) (in \([m]\)) can be computed using the following equation: -\[ S_{xx}(f) = \frac{1}{f_s} \sum_{m=-\infty}^{\infty} R_{xx}(m) e^{-j 2 \pi m f / f_s} \ \left[\frac{m^2}{\text{Hz}}\right] \] -where +From Eq. \eqref{eq:closed_loop_error} representing the closed-loop system behavior, we can see that:
+Ideally, we would like to design the controller \(K\) such that: +
++As shown in the next section, there is a trade-off between the disturbance reduction and the noise injection. +
++We have from the definition of \(S\) and \(T\) that: +
+\begin{equation} + S + T = \frac{1}{1 + GK} + \frac{GK}{1 + GK} = 1 +\end{equation} ++meaning that we cannot have \(|S|\) and \(|T|\) small at the same time. +
+ ++There is therefore a trade-off between the disturbance rejection and the measurement noise filtering. +
+ + ++Typical shapes of \(|S|\) and \(|T|\) as a function of frequency are shown in Figure 2. +We can observe that \(|S|\) and \(|T|\) exhibit different behaviors depending on the frequency band: +
++
+Figure 2: Typical shapes and constrain of the Sensibility and Transmibility closed-loop transfer functions
+-The PSD \(S_{xx}(f)\) represents the distribution of the (average) signal power over frequency. + +
+ ++As shown in the previous section, the effect of disturbances is reduced inside the control bandwidth. +
+ ++Moreover, the slope of \(|S(j\omega)|\) is limited for stability reasons (not explained here), and therefore a large control bandwidth is required to obtain sufficient disturbance rejection at lower frequencies (where the disturbances have large effects). +
+ ++The next important question is what effects do limit the attainable control bandwidth? +
+ + ++The main issue it that for stability reasons, the behavior of the mechanical system must be known with only small uncertainty in the vicinity of the crossover frequency. +
+ ++For mechanical systems, this generally means that control bandwidth should take place before any appearing of flexible dynamics (Right part of Figure 3). +
+ + ++
+Figure 3: Envisaged developments in motion systems. In traditional motion systems, the control bandwidth takes place in the rigid-body region. In the next generation systemes, flexible dynamics are foreseen to occur within the control bandwidth. oomen18_advan_motion_contr_precis_mechat
++This also means that any possible change in the system should have a small impact on the system dynamics in the vicinity of the crossover. +
+ ++For the NASS, the possible changes in the system are: +
++The nano-hexapod and the control architecture have to be developed such that the feedback system remains stable and exhibit acceptable performance for all these possible changes in the system. +
+ ++This problem of robustness represent one of the main challenge for the design of the NASS. +
++The dynamic error budgeting is a powerful tool to study the effect of multiple error sources and to see how the feedback system does reduce the effect +
+ ++To understand how to use and understand it, the Power Spectral Density and the Cumulative Power Spectrum are first introduced. +Then, is shown how does multiple error sources are combined and modified by dynamical systems. +
+ ++Finally, +
++The Power Spectral Density (PSD) \(S_{xx}(f)\) of the time domain signal \(x(t)\) is defined as the Fourier transform of the autocorrelation function: +\[ S_{xx}(\omega) = \int_{-\infty}^{\infty} R_{xx}(\tau) e^{-j \omega \tau} d\tau \ \frac{[\text{unit of } x]^2}{\text{Hz}} \] +
+ ++The PSD \(S_{xx}(\omega)\) represents the distribution of the (average) signal power over frequency.
Thus, the total power in the signal can be obtained by integrating these infinitesimal contributions, the Root Mean Square (RMS) value of the signal \(x(t)\) is then:
\begin{equation} - x_{\text{rms}} = \sqrt{\int_{0}^{\infty} S_{xx}(f) df} \ [m,\text{rms}] + x_{\text{rms}} = \sqrt{\int_{0}^{\infty} S_{xx}(\omega) d\omega} \end{equation}-One can also integrate the infinitesimal power \(S_{xx}(f)df\) over a finite frequency band to obtain the power of the signal \(x\) in that frequency band: +One can also integrate the infinitesimal power \(S_{xx}(\omega)d\omega\) over a finite frequency band to obtain the power of the signal \(x\) in that frequency band:
\begin{equation} - P_{f_1,f_2} = \int_{f_1}^{f_2} S_{xx}(f) df \quad [m^2] + P_{f_1,f_2} = \int_{f_1}^{f_2} S_{xx}(\omega) d\omega \quad [\text{unit of } x]^2 \end{equation}The Cumulative Power Spectrum is the cumulative integral of the Power Spectral Density starting from \(0\ \text{Hz}\) with increasing frequency:
\begin{equation} - CPS_x(f) = \int_0^f S_{xx}(\nu) d\nu \quad [\text{unit}^2] + CPS_x(f) = \int_0^f S_{xx}(\nu) d\nu \quad [\text{unit of } x]^2 \end{equation}The Cumulative Power Spectrum taken at frequency \(f\) thus represent the power in the signal in the frequency band \(0\) to \(f\). @@ -259,7 +456,7 @@ The Cumulative Power Spectrum taken at frequency \(f\) thus represent the power An alternative definition of the Cumulative Power Spectrum can be used where the PSD is integrated from \(f\) to \(\infty\):
\begin{equation} - CPS_x(f) = \int_f^\infty S_{xx}(\nu) d\nu \quad [\text{unit}^2] + CPS_x(f) = \int_f^\infty S_{xx}(\nu) d\nu \quad [\text{unit of } x]^2 \end{equation}And thus \(CPS_x(f)\) represents the power in the signal \(x\) for frequencies above \(f\). @@ -267,22 +464,23 @@ And thus \(CPS_x(f)\) represents the power in the signal \(x\) for frequencies a
-The Cumulative Power Spectrum can be used to determine in which frequency band the effect of disturbances should be reduced and the approximated required control bandwidth in order to obtained some specified vibration amplitude. +The Cumulative Power Spectrum will be used to determine in which frequency band the effect of disturbances should be reduced, and thus the approximate required control bandwidth.
-Let’s consider a signal \(u\) with a PSD \(S_{uu}\) going through a LTI system \(G(s)\) that outputs a signal \(y\) with a PSD (Figure 3). +Let’s consider a signal \(u\) with a PSD \(S_{uu}\) going through a LTI system \(G(s)\) that outputs a signal \(y\) with a PSD (Figure 4).
-+
Figure 4: LTI dynamical system \(G(s)\) with input signal \(u\) and output signal \(y\)
@@ -294,135 +492,73 @@ The Power Spectral Density of the output signal \(y\) can be computed using:
-Let’s consider a signal \(y\) that is the sum of two uncorrelated signals \(u\) and \(v\). +Let’s consider a signal \(y\) that is the sum of two uncorrelated signals \(u\) and \(v\) (Figure 5).
-We have that the PSD of \(y\) is equal to sum of the PSD and \(u\) and the PSD of \(v\): +We have that the PSD of \(y\) is equal to sum of the PSD and \(u\) and the PSD of \(v\) (can be easily shown from the definition of the PSD): \[ S_{yy} = S_{uu} + S_{vv} \]
-+
Figure 5: \(y\) as the sum of two signals \(u\) and \(v\)
-Let’s consider the Feedback architecture, -
- --The position error \(\epsilon\) is equal to: +Let’s consider the Feedback architecture in Figure 1 where the position error \(\epsilon\) is equal to: \[ \epsilon = S r + T n - G_d S d \]
-If we suppose that the signals \(r\), \(n\) and \(d\) are uncorrelated, the PSD of \(\epsilon\) is: +If we suppose that the signals \(r\), \(n\) and \(d\) are uncorrelated (which is a good approximation in our case), the PSD of \(\epsilon\) is: \[ S_{\epsilon \epsilon}(\omega) = |S(j\omega)|^2 S_{rr}(\omega) + |T(j\omega)|^2 S_{nn}(\omega) + |G_d(j\omega) S(j\omega)|^2 S_{dd}(\omega) \]
-And the RMS residual motion is equal to: +And we can compute the RMS value of the residual motion using:
\begin{align*} \epsilon_\text{rms} &= \sqrt{ \int_0^\infty S_{\epsilon\epsilon}(\omega) d\omega} \\ - &= \sqrt{ \int_0^\infty |S(j\omega)|^2 S_{rr}(\omega) + |T(j\omega)|^2 S_{nn}(\omega) + |G_d(j\omega) S(j\omega)|^2 S_{dd}(\omega) d\omega } + &= \sqrt{ \int_0^\infty \Big( |S(j\omega)|^2 S_{rr}(\omega) + |T(j\omega)|^2 S_{nn}(\omega) + |G_d(j\omega) S(j\omega)|^2 S_{dd}(\omega) \Big) d\omega } \end{align*} +-To estimate the PSD of the position error \(\epsilon\) and thus the RMS residual motion, we need: +To estimate the PSD of the position error \(\epsilon\) and thus the RMS residual motion (in closed-loop), we need to determine:
-If we want high level of performance, the experimental conditions should be carefully controlled. -
- - --
-Figure 5: Envisaged developments in motion systems. In traditional motion systems, the control bandwidth takes place in the rigid-body region. In the next generation systemes, flexible dynamics are foreseen to occur within the control bandwidth. oomen18_advan_motion_contr_precis_mechat
-Limitation of feedback control: -
--Predictible system. -
- --For instance, ASML, everything is calibrated (wafer, some size, mass, etc…) -
- --Here, the main difficulty is that we want a very high performance system that is robust to change of: -
--When applying feedback in a system, it is much more convenient to look at things in the frequency domain. -
- - -[ ]
Add a-we will generally decrease the effect of the disturbances -
- -[ ]
Find the citation where it is said that the bandwidth is the consequence of the wanted disturbance rejection at some lower frequencyhttps://tdehaeze.github.io/meas-analysis/ @@ -437,8 +573,8 @@ The obtained dynamics will allows us to compare the dynamics of the model.
In order to perform to Modal Analysis and to obtain first a response model, the following devices were used: @@ -453,13 +589,13 @@ In order to perform to Modal Analysis and to obtain first a response mode The measurement thus consists of:
Figure 6: Figure caption
@@ -479,7 +615,7 @@ In total, 69 degrees of freedom are measured (23 tri axis accelerometers). -
Figure 7: Figure caption
@@ -487,8 +623,8 @@ In total, 69 degrees of freedom are measured (23 tri axis accelerometers).From the measurements, we obtain @@ -501,14 +637,14 @@ From the measurements, we obtain -
Figure 8: Figure caption
Figure 9: Figure caption
@@ -516,8 +652,8 @@ From the measurements, we obtainThe reduction of the number of degrees of freedom from 69 (23 accelerometers with each 3DOF) to 36 (6 solid bodies with 6 DOF) seems to work well. @@ -530,11 +666,11 @@ This confirms the fact that the stages are indeed behaving as a solid body in th
https://tdehaeze.github.io/meas-analysis/ @@ -558,22 +694,22 @@ The problem are on the high frequency disturbances
Figure 10: Amplitude Spectral Density fo the motion error due to disturbances
@@ -618,7 +754,7 @@ We consider: -
Figure 11: Cumulative Amplitude Spectrum of the motion error due to disturbances
@@ -631,8 +767,8 @@ Expected required bandwidthHere, the measurement were made with inertial sensors. @@ -659,16 +795,16 @@ Detector Requirement:
https://tdehaeze.github.io/nass-simscape/ @@ -679,8 +815,8 @@ Multi-Body model
The mass/inertia of each stage is automatically computed from the geometry and the density of the materials. @@ -704,7 +840,7 @@ Comparison model - measurements : +