340 research outputs found

    Cesaro mean distribution of group automata starting from measures with summable decay

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    Consider a finite Abelian group (G,+), with |G|=p^r, p a prime number, and F: G^N -> G^N the cellular automaton given by {F(x)}_n= A x_n + B x_{n+1} for any n in N, where A and B are integers relatively primes to p. We prove that if P is a translation invariant probability measure on G^Z determining a chain with complete connections and summable decay of correlations, then for any w= (w_i:i<0) the Cesaro mean distribution of the time iterates of the automaton with initial distribution P_w --the law P conditioned to w on the left of the origin-- converges to the uniform product measure on G^N. The proof uses a regeneration representation of P

    Error analysis for filtered back projection reconstructions in Besov spaces

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    Filtered back projection (FBP) methods are the most widely used reconstruction algorithms in computerized tomography (CT). The ill-posedness of this inverse problem allows only an approximate reconstruction for given noisy data. Studying the resulting reconstruction error has been a most active field of research in the 1990s and has recently been revived in terms of optimal filter design and estimating the FBP approximation errors in general Sobolev spaces. However, the choice of Sobolev spaces is suboptimal for characterizing typical CT reconstructions. A widely used model are sums of characteristic functions, which are better modelled in terms of Besov spaces Bqα,p(R2)\mathrm{B}^{\alpha,p}_q(\mathbb{R}^2). In particular B1α,1(R2)\mathrm{B}^{\alpha,1}_1(\mathbb{R}^2) with α≈1\alpha \approx 1 is a preferred model in image analysis for describing natural images. In case of noisy Radon data the total FBP reconstruction error ∥f−fLδ∥≤∥f−fL∥+∥fL−fLδ∥\|f-f_L^\delta\| \le \|f-f_L\|+ \|f_L - f_L^\delta\| splits into an approximation error and a data error, where LL serves as regularization parameter. In this paper, we study the approximation error of FBP reconstructions for target functions f∈L1(R2)∩Bqα,p(R2)f \in \mathrm{L}^1(\mathbb{R}^2) \cap \mathrm{B}^{\alpha,p}_q(\mathbb{R}^2) with positive α∉N\alpha \not\in \mathbb{N} and 1≤p,q≤∞1 \leq p,q \leq \infty. We prove that the Lp\mathrm{L}^p-norm of the inherent FBP approximation error f−fLf-f_L can be bounded above by \begin{equation*} \|f - f_L\|_{\mathrm{L}^p(\mathbb{R}^2)} \leq c_{\alpha,q,W} \, L^{-\alpha} \, |f|_{\mathrm{B}^{\alpha,p}_q(\mathbb{R}^2)} \end{equation*} under suitable assumptions on the utilized low-pass filter's window function WW. This then extends by classical methods to estimates for the total reconstruction error.Comment: 32 pages, 8 figure

    Observer design for non-linear networked control systems with persistently exciting protocols

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    International audienceWe study the design of state observers for non-linear networked control systems (NCSs) affected by disturbances and measurement noise, via an emulation-like approach. That is, given an observer designed with a specific stability property in the absence of communication constraints, we implement it over a network and we provide sufficient conditions on the latter to preserve the stability property of the observer. In particular, we provide a bound on the maximum allowable transmission interval (MATI) that guarantees an input-to-state stability (ISS) property for the corresponding estimation error system. The stability analysis is trajectory-based, utilises small-gain arguments, and exploits a persistently exciting (PE) property of the scheduling protocols. This property is key in our analysis and allows us to obtain significantly larger MATI bounds in comparison to the ones found in the literature. Our results hold for a general class of NCSs, however, we show that these results are also applicable to NCSs implemented over a specific physical network called WirelessHART (WH). The latter is mainly characterised by its multi-hop structure, slotted communication cycles, and the possibility to simultaneously transmit over different frequencies. We show that our results can be further improved by taking into account the intrinsic structure of the WH-NCS model. That is, we explicitly exploit the model structure in our analysis to obtain an even tighter MATI bound that guarantees the same ISS property for the estimation error system. Finally, to illustrate our results, we present analysis and numerical simulations for a class of Lipschitz non-linear systems and high-gain observers
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