ملاحظ الحالة

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ملاحظ الحالة النمطي

The state of a physical discrete-time system is assumed to satisfy

x(k+1)=Ax(k)+Bu(k)
y(k)=Cx(k)+Du(k)



ملاحظ النمط المنزلق

x^˙=[H(x^)x]1M(x^)sgn(V(t)H(x^))

where:

  • The sgn() vector extends the scalar signum function to n dimensions. That is,
sgn(z)=[sgn(z1)sgn(z2)sgn(zi)sgn(zn)]
for the vector zn.
  • The vector H(x) has components that are the output function h(x) and its repeated Lie derivatives. In particular,
H(x)[h1(x)h2(x)h3(x)hn(x)][h(x)Lfh(x)Lf2h(x)Lfn1h(x)]
where Lfih is the ith Lie derivative of output function h along the vector field f (i.e., along x trajectories of the non-linear system). In the special case where the system has no input or has a relative degree of n, H(x(t)) is a collection of the output y(t)=h(x(t)) and its n1 derivatives. Because the inverse of the Jacobian linearization of H(x) must exist for this observer to be well defined, the transformation H(x) is guaranteed to be a local diffeomorphism.
M(x^)diag(m1(x^),m2(x^),,mn(x^))=[m1(x^)m2(x^)mi(x^)mn(x^)]
where, for each i{1,2,,n}, element mi(x^)>0 and suitably large to ensure reachability of the sliding mode.
  • The observer vector V(t) is such that
V(t)[v1(t)v2(t)v3(t)vi(t)vn(t)][y(t){m1(x^)sgn(v1(t)h1(x^(t)))}eq{m2(x^)sgn(v2(t)h2(x^(t)))}eq{mi1(x^)sgn(vi1(t)hi1(x^(t)))}eq{mn1(x^)sgn(vn1(t)hn1(x^(t)))}eq]
where sgn() here is the normal signum function defined for scalars, and {}eq denotes an "equivalent value operator" of a discontinuous function in sliding mode.


The modified observation error can be written in the transformed states e=H(x)H(x^). In particular,

e˙=ddtH(x)ddtH(x^)=ddtH(x)M(x^)sgn(V(t)H(x^(t))),

and so

[e˙1e˙2e˙ie˙n1e˙n]=[h˙1(x)h˙2(x)h˙i(x)h˙n1(x)h˙n(x)]ddtH(x)M(x^)sgn(V(t)H(x^(t)))ddtH(x^)=[h2(x)h3(x)hi+1(x)hn(x)Lfnh(x)][m1sgn(v1(t)h1(x^(t)))m2sgn(v2(t)h2(x^(t)))misgn(vi(t)hi(x^(t)))mn1sgn(vn1(t)hn1(x^(t)))mnsgn(vn(t)hn(x^(t)))]=[h2(x)m1(x^)sgn(v1(t)v1(t)=y(t)=h1(x)h1(x^(t))e1)h3(x)m2(x^)sgn(v2(t)h2(x^(t)))hi+1(x)mi(x^)sgn(vi(t)hi(x^(t)))hn(x)mn1(x^)sgn(vn1(t)hn1(x^(t)))Lfnh(x)mn(x^)sgn(vn(t)hn(x^(t)))].

وبذلك:

  1. ما دام m1(x^)|h2(x(t))|, the first row of the error dynamics, e˙1=h2(x^)m1(x^)sgn(e1), will meet sufficient conditions to enter the e1=0 sliding mode in finite time.
  2. Along the e1=0 surface, the corresponding v2(t)={m1(x^)sgn(e1)}eq equivalent control will be equal to h2(x), and so v2(t)h2(x^)=h2(x)h2(x^)=e2. Hence, so long as m2(x^)|h3(x(t))|, the second row of the error dynamics, e˙2=h3(x^)m2(x^)sgn(e2), will enter the e2=0 sliding mode in finite time.
  3. Along the ei=0 surface, the corresponding vi+1(t)={}eq equivalent control will be equal to hi+1(x). Hence, so long as mi+1(x^)|hi+2(x(t))|, the (i+1)th row of the error dynamics, e˙i+1=hi+2(x^)mi+1(x^)sgn(ei+1), will enter the ei+1=0 sliding mode in finite time.

So, for sufficiently large mi gains, all observer estimated states reach the actual states in finite time. In fact, increasing mi allows for convergence in any desired finite time so long as each |hi(x(0))| function can be bounded with certainty. Hence, the requirement that the map H:nn is a diffeomorphism (i.e., that its Jacobian linearization is invertible) asserts that convergence of the estimated output implies convergence of the estimated state. That is, the requirement is an observability condition.

In the case of the sliding mode observer for the system with the input, additional conditions are needed for the observation error to be independent of the input. For example, that

H(x)xB(x)

does not depend on time. The observer is then

x^˙=[H(x^)x]1M(x^)sgn(V(t)H(x^))+B(x^)u.

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هذه المقالة عبارة عن بذرة تحتاج للنمو والتحسين؛ فساهم في إثرائها بالمشاركة في تحريرها.