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into the unknown nodal displacement vector
w
a
=− w a
θ
a
v
=
(4.42)
w
b
=− w b
θ
b
The assumed series is then referred to as an interpolation or shape function . The derivative of
w
, which is needed to form Eq. (4.42), is given by
w 1
w 2
w 3
w 4
=
w =
3 x 2 ]
N u
w T
N u )
T
[012 x
w
=
(
(4.43)
θ =− w
Now, evaluate
w
and
at x
=
a and x
=
b, giving
w a
θ a
w b
θ b
)
w (
w(
0
10
0
0
w 1
w 2
w 3
w 4
=
=
0
)
0
10
0
(4.44)
2
3
w()
w ()
1
2
0
1
2
3
N u
v
=
w
The constants
w are found in terms of the (unknown) displacements at a and b by using
the inverse of N u ,
= N 1
u
w
v
=
Gv
(4.45)
where
1
0
0
0
0
1
0
0
= N 1
u
G
=
3
/
2
2
/
3
/
2
1
/
/
3
/
2
/
3
/
2
2
1
2
1
The relationship between
w
and v , i.e., between the deflection
w
and the values of dis-
placements
w
and
θ
at the ends of the element, is
w =
N u
w
=
N u Gv
=
Nv
(4.46a)
or
1
3 x 2
x 2
3 x 2
2 x 3
2 x 2
x 3
2 x 3
x 3
w(
x
) =
2 +
w a +
x
+
θ a +
2
w b +
θ b
3
2
3
2
(4.46b)
where N
This expression is the desired form of the assumed series, where the
matrix N , which is often called a shape function matrix , characterizes the “interpolation”
or “shape” between the nodes. The components of this expression are often referred to as
shape, basis ,or interpolation functions .
=
N u G
.
Interpolation Functions Based on a Normalized Coordinate
Some mathematical handbooks tabulate various interpolation functions. The Hermitian 2
interpolation polynomials of Fig. 4.8 can be employed when derivatives of the displace-
ments at the nodes are involved, as with beams. The Hermitian polynomials can be derived
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