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Parametrization of Hankel-norm Approximants of Time-Varying Systems

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Parametrization of Hankel-norm approximants of

time-varying systems

Alle-Jan van der Veen and Patrick Dewilde Delft University of Technology

Department of Electrical Engineering 2628 CD Delft, The Netherlands

email: allejan@dutentb.et.tudelft.nl, dewilde@dutentb.et.tudelft.nl

The classical time-invariant Hankel-norm approximation problem is generalized to the time-varying context. The input-output operator of a time-varying bounded causal linear system acting in discrete time may be specified as a bounded upper-triangular operator T with block matrix entries Tij. For such an operator T, we will define the Hankel norm as a generalization of the time-invariant Hankel norm. Subsequently, we describe all operators T which are closer to T in (operator) norm than some prespecified error toleranceΓ, and whose upper triangular part admits a state realization of minimal dimensions. The upper triangular part of T can be regarded as the input-output operator of a causal time-varying system that approximates T in Hankel norm.

1. INTRODUCTION

For time-invariant systems, the Hankel norm approximation problem (its minimal degree version) reads as follows [1]. Let T(z) = t0+ t1z + t2z2+ be in the Hardy space H∞, and

define the Hankel operator HT= [ti+j+1]∞i,j=0. Then, for a predefined error tolerance γ, find a transfer function Ta(z) for which rank HTa is minimal, such that



HTTa



≤ γ. Recall that the rank of HT is the system order of T, i.e., the minimal number of states that are required in a state realization of T(z). A fundamental result, proven in [1], is that there exists an approximant Ta for which the state dimension is equal to the number of singular values of HT which are larger than γ. The generalization to time-varying systems was derived by the authors in [2]. In this presentation, we will emphasize one of the results in this paper, namely the fact that all Hankel-norm approximants are described by a certain chain-fraction representation.

2. DEFINITIONS AND PRELIMINARY RESULTS

Define the space of non-uniform  2-sequences as follows. Let Mi ∈ N|  ∞ , for all

integers i, and for each i define the vector space i =C|

Mi. Then

=  × i× is

a space of sequences whose entries are vectors of non-uniform dimensions, and

 2 =  x∈ :  x  2 < ∞

0In U. Helmke e.a., editor, Systems and Networks: Mathematical Theory and Applications (Proc. Int.

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is the space of such sequences with bounded two-norm. Such sequences will represent signals in our theory. The space of bounded operators T = [Tij]∞i,j=−∞ with entries Tijwhich are Mi ×Nj matrices acting on such sequences is

( , ) = [

2 →

2 ] .

We also define the space of upper operators as



( , ) =  T

: Tij = 0, i<j

and likewise, the space  of lower and  of diagonal operators is defined. An operator

T

( , ) can be regarded as the input-output operator of a time-varying system

acting on non-uniform sequences: an input sequence u ∈ 

2 is mapped by T to an

output sequence y = uT ∈ 



2 . The sequence [Tij]∞j=−∞ (the i-th row of T) is the impulse response to an impulse at time i, and hence, for an LTI system, T has a Toeplitz structure. In the present notation, a causal system has an input-output operator T



. An operator T∈

has a time-varying state realization  Ak, Bk, Ck, Dk

−∞ if its

block-entries are given by

Tij =    0 , i> j Di, i = j BiAi+1 Aj−1Cj, i< j

A realization is called strictly stable if limn→∞supi



Ai+1Ai+1  Ai+n



1/n <1 . In this case,

the multiplication y = uT, with u = [ u0 u1 ] and y = [ y0 y1 ] is

equivalent to the set of equations

xk+1 = xkAk + ukBk yk = xkCk+ ukDk

k =  , 0, 1,  ,

in which xk is introduced as the state. Note that state dimensions need not be constant. In order to determine realizations with minimal state dimensions, we associate to an operator T∈

(or T

) the collection of operators  Hk

−∞ which are submatrices of

T: Hk = [Tki−1,k+j]∞i,j=0 =    Tk1,k Tk1,k+1  Tk−2,k Tk−2,k+1 .. . . ..    .

The Hk play the same role as the Hankel operator of T in the time-invariant case, although they do not possess a Hankel structure. In particular,

Theorem 1 ([3]) Let T ∈ 

, dk := rank Hk < ∞ (all k). Then T admits a realization

 Ak, Bk, Ck, Dk

−∞ where Ak : dk×dk+1. This realization is minimal.

In view of this theorem, we define statedim(T) := [rank Hk]−∞. We call T locally finite if all entries of this sequence are finite.

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3. HANKEL NORM APPROXIMATION

The Hankel norm of T

is defined as  T  H := sup k  Hk  .

The Hankel norm is a seminorm, and weaker than the operator norm, as submatrices of a matrix have smaller norm than the matrix itself.

The time-varying Hankel-norm approximation problem can be formulated as follows. Given T ∈ 

and a diagonal parameter operator Γ ∈  (Γ > 0 and invertible), find

T ∈ such that (1)  Γ−1(TT ) ≤ 1 ,

(2) statedim(T ) is minimal (pointwise) .

Then Ta := (upper part of T ) can be called a Hankel-norm approximant of T of minimal state dimension, as  Γ−1(TT a)  H=  Γ−1(TT ) H≤  Γ−1(TT ) ≤1 . Theorem 2 ([2]) Let T ∈ 

be locally finite and have a strictly stable realization. Partition the singular values of (HΓ−1T)k as (σ+)i,k ≤ 1 , (σ−)i,k > 1 , and suppose that

supi,k(σ+)i,k < 1 , infi,k(σ−)i,k > 1 . Let Nk be the number of elements of the set  (σ−)i,k i.

Then there exists an operator T

satisfying (1)  Γ−1(TT ) ≤ 1 , (2) statedim(T )[Nk]−∞.

It is possible to show that statedim(T )k < Nk cannot occur. A suitable T can be con-structed by the following recipe [2]:

1. Determine an inner system U ∈

(satisfying UU= I, UU = I) such that UT∗ ∈

. 2. Interpolation: construct a J-unitary operator Θ ∈ 

(satisfying Θ∗J= J2,

ΘJ2Θ∗ = J1 for certain signature operators J1,2 ∈ ) such that

[U∗ −T∗Γ−1]Θ =: [AB ]∈[ 

] .

3. Define T = ΓΘ−∗22B= T− Γ(Θ12Θ−122)∗U.

To outline the proof that this T satisfies the two conditions in the theorem, let us remark that under the posed conditions onΓ−1T one can construct the operators U andΘ. In

ad-dition, one can show that

 Θ12Θ−122  <1 so that  Γ−1(TT )

≤ 1. Finally, it is not hard to see from T =ΓΘ−∗22B ∗ with Θ−∗22

and B ∗ ∈ that statedim(T )≤statedim(Θ

−∗ 22).

With more effort, one shows that there exists aΘ for which statedim(Θ−∗22)k = Nk, so that also the second requirement of the theorem is fulfilled.

U and Θ can be computed using state space techniques, and in this way a state realization of Ta can be obtained [2]. A suitable Θ can also be computed by a recursive generalized Schur procedure [4].

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4. ALL APPROXIMANTS

The next issue is to determine all T

satisfying the two conditions in theorem 2. The solution will be that all such T are given by T = T +ΓSU, where S is given by a linear fractional transformation of Θ and a free parameter SL, which is upper and contractive (the previous solution is obtained by setting SL = 0). In particular, the following two theorems hold true, showing that more, resp. all approximants are obtained.

Theorem 3 ([2]) Let T∈

, Γ ∈ be as in theorem 2 and define U, Θas before, where

statedim(Θ−∗22)k = Nk. Let SL∈  ,  SL  ≤1. Put S = (Θ11SL− Θ12)(Θ22− Θ21SL)−1. Then T := T +ΓSU satisfies (1)  Γ−1(TT )  ≤ 1 , (2) statedim(T ) = [Nk]∞−∞.

Theorem 4 ([2]) Let T,Γ, U,Θbe as in theorem 3. Let T

be any operator satisfying (1)



Γ−1(TT )

1 , (2) statedim(T )[Nk]−∞. Define S = U(T∗−T∗)Γ−1 and SL= (Θ

11S +Θ12)(Θ21S +Θ22)−1. Then SL ∈  ,  SL  ≤ 1 , S = (Θ11SL− Θ12)(Θ22− Θ21SL)−1.

In fact, statedim(T ) = [Nk]∞−∞, so that there are no approximants of order less than [Nk]∞−∞. In this paper, we will only provide an outline of the proofs. It is straightforward to show that, in both theorems,

 SL  ≤1 ⇔  S  ≤ 1 ⇔ Γ−1(TT )  ≤ 1. The main point to prove in the first theorem is that T has state dimensions as specified and in the second theorem that SL



. These proofs are related; the line of reasoning is as in [5], although the winding number argument is to be replaced by the following proposition:

Proposition 1 ([2]) Let A∈  , A−1 ∈ ; X,  X  <1. Let Nk = statedim(lower part of A−1)∗k. Then

statedim(lower part of (IX)−1A−1)∗k = Nk + pk iff statedim(lower part of A(IX))k = pk.

The application of this proposition to theorem 3 is as follows. Put A = Θ22, X =

Θ−1 22Θ21SL, for any SL∈  ,  SL  ≤1. Then (IX)−1A−1 = (Θ22− Θ21SL)−1. Hence

statedim(lower part of Θ−122)∗k = Nk and Θ22− Θ21SL



⇒ statedim(lower part of (Θ22− Θ21SL)−1)∗k = Nk.

This implies that T ∗Γ−1 = (A SL+ B )(Θ22−Θ21SL)−1has statedim(lower part of T ∗Γ−1)∗kNk. A similar argument gives equality.

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REFERENCES

[1] V.M. Adamjan, D.Z. Arov, and M.G. Krein, “Analytic properties of Schmidt pairs for a Hankel operator and the generalized Schur-Takagi problem,” Math. USSR Sbornik, vol. 15, no. 1, pp. 31–73, 1971. (transl. of Iz. Akad. Nauk Armjan. SSR Ser. Mat. 6 (1971)).

[2] P.M. Dewilde and A.J. van der Veen, “On the Hankel-norm approximation of upper-triangular operators and matrices,” Integral Equations and Operator Theory, vol. 17, no. 1, pp. 1–45, 1993.

[3] A.J. van der Veen and P.M. Dewilde, “Time-varying system theory for computa-tional networks,” in Algorithms and Parallel VLSI Architectures, II (P. Quinton and Y. Robert, eds.), pp. 103–127, Elsevier, 1991.

[4] A.J. van der Veen and P.M. Dewilde, “On low-complexity approximation of matrices,” subm. Linear Algebra and its Applications, 1992.

[5] J.A. Ball, I. Gohberg, and L. Rodman, Interpolation of Rational Matrix Functions, vol. 45 of Operator Theory: Advances and Applications. Birkh¨auser Verlag, 1990.

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