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B Y
D R . M AH D I D AM G H AN I
2 0 1 7 - 2 0 1 8
Structural Design and Inspection-
Finite Element Method (Beams)
1
Suggested Readings
Reference 1 Reference 2
2
Objective(s)
 Familiarisation with Finite Element equations for
beam structures;
 Ability to assemble global stiffness matrix for a beam
shape structure;
 Familiarisation with Finite Element Modelling (FEM)
of beam structures using ABAQUS CAE (Tutorial).
3
Introduction
4
Introduction
 Refer to chapter 6 of Reference 1;
 Refer to chapter 5 of Reference 2;
 This method is used in most of commercially
available FE based software to solve structural
problems;
 Some typical software in aerospace industry are;
 Altair HyperWorks (mostly for optimisation purposes)
 MSC Nastran (mostly for linear analysis)
 Abaqus (mostly for non-linear analysis)
 Ansys (mostly for non-linear analysis)
5
Introduction
6
 Unlike truss elements that are joined together by
hinges, beams are connected by welding so they
transfer both bending moment and forces across
each other;
 In this lecture, we would be using Euler-Bernoulli
beam theory that is applicable to thin beams.
Beam element
7
The length of element
Node 1 has only 2 DOF
(vertical displacement
and rotation)
Therefore, this
beam element has
4 DOFs in total
Node 2 has only 2 DOF
(vertical displacement
and rotation)
Local coordinate system with
origin at the middle of beam
This slide shows positive direction of
shear forces, bending moments,
displacements and rotations.
The Finite Element Analysis (FEA) process
8
Displacement in FEM
9
 In finite element methods, the displacement for an
element is written in the form;
e
h
xxu dN )()( 
Approximated displacement
within the element
Shape function Vectors of displacements at
the two nodes of the element
This function
approximates
displacements
within the element
by just having
displacements at
the two nodes, i.e.
de
Question:
What should
be N(x)???
Note
10
 It is convenient if the shape functions are derived from a
special set of local coordinates (natural coordinate system);
 The natural coordinate system is dimensionless, has its
origin at the centre of the element and is defined from −1 to
+1.
Note
11
 The relationship between the natural coordinate
system and the local coordinate system can simply
be given as a scaling function, i.e.
a
x

Shape function
12
 Since we have four DOFs for the element we need
to find 4 shape functions;
 We assume displacement within element has the
form where ;
Four unknowns
in the form of
4x1 matrix
Vector of polynomial
basis functions
This matrix is 1x4 because
we have a 4-DOF element
ax/
Shape function
13
 We also know;




x
v
  




 



axa
x
x
v
1








v
a
1
 2
321 32
1
 
a
a/2
Note
14






v
a
1
 2
321 32
1
 
a
 






3211
32101
32
1
)1(
)1(


a
v
 






3212
32102
32
1
)1(
)1(


a
v
a/2
Shape function
15
a/2
e
T
v dPP 1
)()( 
 
Shape function
16
Shape functions for
displacement are
functions of natural
coordinates
Shape functions for
displacement are
functions of natural
coordinates
Shape functions for
rotations are
functions of natural
coordinates and
length of element
Shape functions for
displacement are
functions of natural
coordinates

These cubic shape (or interpolation) functions are known as
Hermite cubic interpolation (or cubic spline) functions.
Shape functions
17
-0.2
0
0.2
0.4
0.6
0.8
1
-1 -0.8 -0.6 -0.4 -0.2 0 0.2 0.4 0.6 0.8 1
ξ
Shape functions along the length of beam element
N1 N2
N3 N4
Strain calculation
18
B is called
strain matrix
L is differential
operator
 
Note
19
 First derivative of the shape function is important as it will be
used to obtain rotations within each element (we will see this
in some examples);
 How first derivative of shape function (dN/dx) is obtained?



 d
d
adx
d
d
d
dx
d NNN 1

 21
1
4
3

adx
dN
 22
321
4
1
 
dx
dN
 23 3
1
4
dN
dx a
   24
321
4
1
 
dx
dN
Reminder
20
x
2x
1x
x
Fibre ST has shortened in
length whilst NQ increased
in length so they have gone
through strains
Remember that the length
of neutral axis does not
change and remains as x

LengthOriginal
LengthinChange
xx
  


x


RyR
xx
 
R
y
R
RyR
xx 





Positive y gives negative
strain, i.e. compression
  


x


xyR
xx
Reminder
21
 How did the following come about?
 Euler-Bernoulli beam curvature (1/R) is used for this
formula;
e
N
B
e
e
Bdd
NNd
 



























xx
dx
d
y
xx
dx
d
y
dx
d
y
dx
yd
y
R
y

2
2
2
2
2
2
2
2
Reminder
22
A
a2
dx
aAVVolume 2 dAdxdV 
dA
Element local stiffness matrix
23
Element stiffness matrix
(see chapter 3 of Ref. 2)
Ec  dAdxdV 
Aiscrosssectional
area
Eismodulusof
elasticity(material
constant)
Further elaboration
24
 Some might ask where did the following come from?
 See below;
 
''111
1
22
2
2
2
2
NNN
NNN
aaxa
xaxxxxx
N




















































Further elaboration
25












 V
T
e dxdA
a
y
E
a
y
'''' 22
NNk
''2
NB
a
y

     



 adx
d
ax
a
a
T
A
e dxdAy
a
E
1
,/
2
4
''''


NNk












 


1
1
2
2
2
2
4




ad
d
Nd
d
Nd
I
a
E
T
zek    



1
1
3
''''


dNNI
a
E T
zek
Element local stiffness matrix
26
Elements mass matrix
27
 Following similar procedure as stiffness matrix;
 Students are advised to familiarise themselves with chapter 3
of ref. 2
Fs1
Fs2
Ms1 Ms2fy
Nodal forces
28
Surface force (applied
at the node)
Surface force (applied
at the node)
Body forces (applied
between nodes)
Note that in FEA, body forces are always
transferred to the nodes
Nodal forces
29
Example 1
30
 Obtain tip deflection and rotation of the beam shown
below using FEA. (E=69.0 GPa and Poisson’s ratio
is 0.33)
Solution
31
 For practical purposes, a beam must be divided into
more than 1 element to obtain precise enough
results;
 However, for the sake of showing the process and
simplicity, let’s divide the beam into one element
only.
Solution
32
29
/106969
25.05.02
mNGPaE
mama


Solution
33
eedKF 
Reaction forces at clamped
boundary that are unknown
Applying BC, i.e.
v1 =0 and θ1=0
Solution
34
 The reduced stiffness matrix becomes;
Example 2
35
 In previous example, what are the deflection and
rotation at mid-point of beam structure?
3
1.0064 10
 
3
1.0064 10
 
Tutorials 3a
36
 See T3a.pdf
Tutorial 3b
37
 Model beam problem of example 1 in Abaqus and
extract deflection and rotation at the tip and mid
point of the structure.
Tutorial 3c
38
 See T3c.pdf

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Lec9 finite element_beam_structures 1

  • 1. B Y D R . M AH D I D AM G H AN I 2 0 1 7 - 2 0 1 8 Structural Design and Inspection- Finite Element Method (Beams) 1
  • 3. Objective(s)  Familiarisation with Finite Element equations for beam structures;  Ability to assemble global stiffness matrix for a beam shape structure;  Familiarisation with Finite Element Modelling (FEM) of beam structures using ABAQUS CAE (Tutorial). 3
  • 5. Introduction  Refer to chapter 6 of Reference 1;  Refer to chapter 5 of Reference 2;  This method is used in most of commercially available FE based software to solve structural problems;  Some typical software in aerospace industry are;  Altair HyperWorks (mostly for optimisation purposes)  MSC Nastran (mostly for linear analysis)  Abaqus (mostly for non-linear analysis)  Ansys (mostly for non-linear analysis) 5
  • 6. Introduction 6  Unlike truss elements that are joined together by hinges, beams are connected by welding so they transfer both bending moment and forces across each other;  In this lecture, we would be using Euler-Bernoulli beam theory that is applicable to thin beams.
  • 7. Beam element 7 The length of element Node 1 has only 2 DOF (vertical displacement and rotation) Therefore, this beam element has 4 DOFs in total Node 2 has only 2 DOF (vertical displacement and rotation) Local coordinate system with origin at the middle of beam This slide shows positive direction of shear forces, bending moments, displacements and rotations.
  • 8. The Finite Element Analysis (FEA) process 8
  • 9. Displacement in FEM 9  In finite element methods, the displacement for an element is written in the form; e h xxu dN )()(  Approximated displacement within the element Shape function Vectors of displacements at the two nodes of the element This function approximates displacements within the element by just having displacements at the two nodes, i.e. de Question: What should be N(x)???
  • 10. Note 10  It is convenient if the shape functions are derived from a special set of local coordinates (natural coordinate system);  The natural coordinate system is dimensionless, has its origin at the centre of the element and is defined from −1 to +1.
  • 11. Note 11  The relationship between the natural coordinate system and the local coordinate system can simply be given as a scaling function, i.e. a x 
  • 12. Shape function 12  Since we have four DOFs for the element we need to find 4 shape functions;  We assume displacement within element has the form where ; Four unknowns in the form of 4x1 matrix Vector of polynomial basis functions This matrix is 1x4 because we have a 4-DOF element ax/
  • 13. Shape function 13  We also know;     x v             axa x x v 1         v a 1  2 321 32 1   a a/2
  • 14. Note 14       v a 1  2 321 32 1   a         3211 32101 32 1 )1( )1(   a v         3212 32102 32 1 )1( )1(   a v a/2
  • 15. Shape function 15 a/2 e T v dPP 1 )()(   
  • 16. Shape function 16 Shape functions for displacement are functions of natural coordinates Shape functions for displacement are functions of natural coordinates Shape functions for rotations are functions of natural coordinates and length of element Shape functions for displacement are functions of natural coordinates  These cubic shape (or interpolation) functions are known as Hermite cubic interpolation (or cubic spline) functions.
  • 17. Shape functions 17 -0.2 0 0.2 0.4 0.6 0.8 1 -1 -0.8 -0.6 -0.4 -0.2 0 0.2 0.4 0.6 0.8 1 ξ Shape functions along the length of beam element N1 N2 N3 N4
  • 18. Strain calculation 18 B is called strain matrix L is differential operator  
  • 19. Note 19  First derivative of the shape function is important as it will be used to obtain rotations within each element (we will see this in some examples);  How first derivative of shape function (dN/dx) is obtained?     d d adx d d d dx d NNN 1   21 1 4 3  adx dN  22 321 4 1   dx dN  23 3 1 4 dN dx a    24 321 4 1   dx dN
  • 20. Reminder 20 x 2x 1x x Fibre ST has shortened in length whilst NQ increased in length so they have gone through strains Remember that the length of neutral axis does not change and remains as x  LengthOriginal LengthinChange xx      x   RyR xx   R y R RyR xx       Positive y gives negative strain, i.e. compression      x   xyR xx
  • 21. Reminder 21  How did the following come about?  Euler-Bernoulli beam curvature (1/R) is used for this formula; e N B e e Bdd NNd                              xx dx d y xx dx d y dx d y dx yd y R y  2 2 2 2 2 2 2 2
  • 23. Element local stiffness matrix 23 Element stiffness matrix (see chapter 3 of Ref. 2) Ec  dAdxdV  Aiscrosssectional area Eismodulusof elasticity(material constant)
  • 24. Further elaboration 24  Some might ask where did the following come from?  See below;   ''111 1 22 2 2 2 2 NNN NNN aaxa xaxxxxx N                                                    
  • 25. Further elaboration 25              V T e dxdA a y E a y '''' 22 NNk ''2 NB a y            adx d ax a a T A e dxdAy a E 1 ,/ 2 4 ''''   NNk                 1 1 2 2 2 2 4     ad d Nd d Nd I a E T zek        1 1 3 ''''   dNNI a E T zek
  • 27. Elements mass matrix 27  Following similar procedure as stiffness matrix;  Students are advised to familiarise themselves with chapter 3 of ref. 2
  • 28. Fs1 Fs2 Ms1 Ms2fy Nodal forces 28 Surface force (applied at the node) Surface force (applied at the node) Body forces (applied between nodes) Note that in FEA, body forces are always transferred to the nodes
  • 30. Example 1 30  Obtain tip deflection and rotation of the beam shown below using FEA. (E=69.0 GPa and Poisson’s ratio is 0.33)
  • 31. Solution 31  For practical purposes, a beam must be divided into more than 1 element to obtain precise enough results;  However, for the sake of showing the process and simplicity, let’s divide the beam into one element only.
  • 33. Solution 33 eedKF  Reaction forces at clamped boundary that are unknown Applying BC, i.e. v1 =0 and θ1=0
  • 34. Solution 34  The reduced stiffness matrix becomes;
  • 35. Example 2 35  In previous example, what are the deflection and rotation at mid-point of beam structure? 3 1.0064 10   3 1.0064 10  
  • 37. Tutorial 3b 37  Model beam problem of example 1 in Abaqus and extract deflection and rotation at the tip and mid point of the structure.

Editor's Notes

  • #13: The complete cubic displacement function is appropriate because there are four total degrees of freedom (a transverse displacement and a small rotation at each node). The cubic function also satisfies the basic beam differential equation (y’’=M/EI and Eiy’’’’=0)— further justifying its selection. In addition, the cubic function also satisfies the conditions of displacement and slope continuity at nodes shared by two elements.