Geoscience Reference
In-Depth Information
Using the following notation
/
D
z
2
z
3
z
n
.
T
f.
z
/
z
2
4
3
5
010
00
001
00
:
:
:
:
:
:
:
:
:
:
:
:
:
:
:
A
D
C
D
10
0
the observer has the form
z
D
f.
z
/
S
1
C.C
z
y/
where
S
is the solution of the equation
A
T
S
S A
C
C
T
C
D
0
S
where
is a constant. It is proved in
Gauthier et al.
(
1992
) that the error of the
observer
e.t/
D
z
z
approaches zero if
is large enough (thus the name “high gain observer”). While
the proof is carried out in the
z
-space, the observer can be constructed in the original
state space
@
1
z
@x
x
D
f.x/
S
1
C.h.x/
y/
The simplicity in the construction of a high gain observer makes it a convenient
tool for nonlinear systems (
Gauthier and Kupka 1994
). However, in the presence
of noise, a high gain observer should be used with caution. It may significantly
enlarge the impact of the noise and result in large estimation errors. In addition,
the “homomorphism” requirement for (
1.17
) limits the region in the state space in
which the observer is applicable. In
Krener and Kang
(
2003
), a nonlinear observer is
constructed without a global homomorphism requirement. In addition, the observer
gain depends on the state of the system so that it is not constantly high. Global or
semi-global observers can also be derived based on Lyapunove functions for systems
with a triangular structure or bounded nonlinear terms in its differential equations
(
Lei et al. 2007
;
Krener and Kang 2003
;
Tsinias 1989
). Deriving Lyapunov
functions for nonlinear systems is always difficult. An alternative is to directly apply
convergent numerical algorithms in nonlinear observers. For instance, an Euler-
Newton observer is introduced in
Kang
(
2006
). Moving horizon observers are also
computational based methodologies (
Findeisen et al. 2002
;
Michalska and Mayne
1995
).
The sliding mode observer is another Lyapunov function based approach. It has
the capability of handling unknown inputs or unknown parameters (
Floquet and
Barbot 2007
). A survey of various types of sliding mode observers can be found in
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