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Institute of Structural Engineering Page 1
Method of Finite Elements I
Chapter 2
The Direct Stiffness Method
Method of Finite Elements I
Institute of Structural Engineering Page 2
Method of Finite Elements I
Direct Stiffness Method (DSM)• Computational method for structural analysis• Matrix method for computing the member forces
and displacements in structures• DSM implementation is the basis of most commercial
and open-source finite element software• Based on the displacement method (classical hand
method for structural analysis)• Formulated in the 1950s by Turner at Boeing and
started a revolution in structural engineering
Institute of Structural Engineering Page 3
Method of Finite Elements I
Learning Goals of this Chapter• DSM formulation• DSM software workflow for …
• linear static analysis (1st order)• 2nd order linear static analysis• linear stability analysis
Lecture 2b
Institute of Structural Engineering Page 4
Method of Finite Elements I
Computational Structural Analysis
Modelling is the most important step in the process of a structural analysis !
X
Y
Physical problem Continuousmathematical model
Discretecomputational model
strong form weak form
Institute of Structural Engineering Page 5
Method of Finite Elements I
System Identification (Modelling)
Global Coordinate SystemNodesElementsBoundary conditionsLoads
X
Y
1
3 4
25
6
1 2
3
4
Element numbersand orientation
Node numbers
5 6
Institute of Structural Engineering Page 6
Method of Finite Elements I
Deformations – Degrees of Freedom
System Deformations
System identification
Nodal Displacements
nodes, elements, loads and supportsdeformed shape
(deformational, nodal)degrees of freedom = dofs
Institute of Structural Engineering Page 7
Method of Finite Elements I
Degrees of Freedom
7 * 2 = 14 dof
Frame Structure
8 * 3 = 24 dof
Truss Structure
ui = ( udx , udy )
uiui
ui = ( udx , udy , urz )dof per node
dof of structure
Institute of Structural Engineering Page 8
Method of Finite Elements I
Elements: Truss
compatibility
ux = displacement in directionof local axis X
ε =𝐷𝐷𝐷𝐷𝐿𝐿
σ = 𝐸𝐸 εconst. equation
equilibrium
𝑁𝑁 = 𝐴𝐴σ=𝐴𝐴𝐸𝐸 ε =𝐴𝐴𝐸𝐸𝐿𝐿𝐷𝐷𝐷𝐷
𝐹𝐹2 = −𝐹𝐹1 = 𝑁𝑁
𝐷𝐷𝐷𝐷 = (u2 −u1)
F2F1
𝐹𝐹1 =𝐴𝐴𝐸𝐸𝐿𝐿
(u1 −u2)
𝐹𝐹2 =𝐴𝐴𝐸𝐸𝐿𝐿
(−u1 + u2)
f = k uk : (element) stiffness matrixf : (element) nodal forcesu : (element) displacement vector
1 dof per nodeDX
𝐿𝐿,𝐸𝐸,𝐴𝐴N
F1 F2
ux
X/Y = local coordinate system
DX = displacement of truss end1 1
2 2
EA EAF uL LF uEA EA
L L
− =
−
Institute of Structural Engineering Page 9
Method of Finite Elements I
Elements: Beam3 dof per node
DX
DY
RZ
𝐿𝐿,𝐸𝐸,𝐴𝐴uy
uy
ux
k u
ux = displacement in directionof local axis X
uy = displacement in directionof local axis Y
3 2 3 2
2
0 0 0 0
12 6 12 6 0 0
6 4 0 0
EA EAL L
EI EI EI EIL L L LEI EI
LL
−
−
2
3 2 3 2
2
6 2
0 0 0 0
12 6 12 6 0 0
6 2 0
EI EILL
EA EAL L
EI EI EI EIL L L LEI EI
LL
−
−
− − −
1
2
3
4
5
26
6 4 0
u
u
u
u
uEI EI
uLL
−
Institute of Structural Engineering Page 10
Method of Finite Elements I
The Beam Stiffness Matrix
B
A´
B´
υA
υB
MAB
VAB
VBA
MBA
φB
φA
A
3 2 3 2
2 2
3 2 3 2
2 2
12 6 12 6
6 4 6 2
12 6 12 6
6 2 6 4
AB
AB
BA
BA
EI EI EI EIL L L L
V EI EI EI EIM L L L LV EI EI EI EI
L L L LMEI EI EI EIL L L L
− − = − − −
−
A
A
B
B
υϕυϕ
υA υBφA φB
4 DOFs φA, φB, υA, υΒ
Institute of Structural Engineering Page 11
Method of Finite Elements I
υA
3 2 3 2
2 2
3 2 3 2
2 2
12 6 12 6
6 4 6 2
12 6 12 6
6 2 6 4
AB
AB
BA
BA
EI EI EI EIL L L L
V EI EI EI EIM L LL LV EI EI EI EI
L L L LMEI EI EI EI
L LL L
− − − − = − − − −
A
A
B
B
υϕυϕ
υB
* υΑ
* υB
The Beam Stiffness Matrix
Institute of Structural Engineering Page 12
Method of Finite Elements I
* φA
φA
3 2 3 2
2 2
3 2 3 2
2 2
12 6 12 6
6 4 6 2
12 6 12 6
6 2 6 4
AB
AB
BA
BA
EI EI EI EIL L L L
V EI EI EI EIM L L L LV EI EI EI EI
L L L LMEI EI EI EIL L L L
− − = − − −
−
A
A
B
B
υϕυϕ
* φB BφBA
4EI L
26EL L2EI L
26EL L
φB
The Beam Stiffness Matrix
Institute of Structural Engineering Page 13
Method of Finite Elements I
3 2 3 2
2 2
3 2 3 2
2 2
12 6 12 6
6 4 6 2
12 6 12 6
6 2 6 4
AB
AB
BA
BA
EI EI EI EIL L L L
V EI EI EI EIM L L L LV EI EI EI EI
L L L LMEI EI EI EIL L L L
− − = − − −
−
A
A
B
B
υϕυϕ
direct
: Moment/Shear in that occurs for a rotation/displacement / acting on node : Moment/Shear in that occurs for a rotation/displacement / acting on node
ik k k
ki i i
t i kt k i
ϕ δ
ϕ δ
Coupling Stiffness Terms
coupling
: Moment/Shear in that is required for inducing in a rotation/displacement / 1 : Moment/Shear in that is required for inducing in a rotation/displacement / 1
ik i i
ki k k
s i is k k
ϕ δ =
ϕ δ =
Direct Stiffness Terms
The Beam Stiffness Matrix
Institute of Structural Engineering Page 14
Method of Finite Elements I
Elements: Global Orientation
local
global
uloc = R uglob
uglob = u = RT uloc
𝜃𝜃
kglob = k = RT kloc R
cos sin 0 0 0 0sin cos 0 0 0 00 0 1 0 0 00 0 0 cos sin 00 0 0 sin cos 00 0 0 0 0 1
R
θ θθ θ
θ θθ θ
−
= −
Institute of Structural Engineering Page 15
Method of Finite Elements I
Beam Stiffness Matrixe.g. k24 =
reactionin global direction Yat start node S
due to a
unit displacementin global direction Xat end node E
UXE=1
FYS
S
EFXS =
FYS =
MS =
FXS =
FYS =
ME =
UXS UYS RS UXE UYE RE
k14 k15 k16
k24 k25 k26
k34 k35 k36
k44 k45 k46
k55 k56
k66
k11 k12 k13
k22 k23
k33
symm.
Element stiffness matrixin global orientation
[ ] [ ][ ] [ ]
iS iSSS SE
iE iEES EE
f uf u
=
i i
i i
k kk k
f = k u
Institute of Structural Engineering Page 16
Method of Finite Elements I
Nodal Equilibrum
3 4
2
5
6
f4r4: Vector of all forces acting at node 4
r4 = - k6ES u3 + contribution of element 6 due tostart node displacement u3
- k6EE u4 + contribution of element 6 due toend node displacement u4
- k5EE u4 + contribution of element 5 due toend node displacement u4
- k5ES u2 + contribution of element 5 due tostart node displacement u2
f4 external load
Equilibrum at node 4: r4 = - k5SE u2 -k6ES u3 - k5EE u4 - k6EE u4 + f4 = 0
Institute of Structural Engineering Page 17
Method of Finite Elements I
Global System of Equations
r1 = -
u1
r2 = -
r3 = -
r4 = -
u2 u3 u4
k5ES k6ES k5EE+k6EE
1
3 4
25
6
1 2
34
k1EE+k3SS+k4SS
k3SE k4SE
k3ES k2EE+k3EE+k5SS
k5SE
k4ES k4EE+k6SS
k6SE
+ f1 = 0
+ f2 = 0
+ f3 = 0
+ f4 = 0
- K U + F = 0 F = K U
Institute of Structural Engineering Page 18
Method of Finite Elements I
K = global stiffness matrix = Assembly of all ke
F = K U
Global System of Equations
= equilibrium at every node of the structure
F = global load vector = Assembly of all fe
U = global displacement vector = unknown
Institute of Structural Engineering Page 19
Method of Finite Elements I
Solving the Equation System
K U = F
U = K-1 F
What are the nodal displacements fora given structure (= stiffness matrix K )due to a given load (= load vector F ) ?
K-1left multiply
K-1 K U = K-1 F
Inversion possible only if K is non-singular(i.e. the structure is sufficiently supported = stable)
Institute of Structural Engineering Page 20
Method of Finite Elements I
Beam Element Results
2. Element end forcesCalculate element end forces = f = k u
4. Element deformations along axis
1. Element nodal displacementsDisassemble u (indiv. element displacement vectors) from resulting global displacements U
3. Element stress and strain along axisCalculate moment/shear from end forces (equilibrium equation)Calculate curvature/axial strain from moments/axial force
Calculate displacements from strain (direct integration)
Institute of Structural Engineering Page 22
Method of Finite Elements I
PP/2
PL/8 P/2
PL/8
l/2 l/2
P/2
PL/8P/2
PL/8
DSM Gleichung
Pfx1 fy2
1 2P/2
PL/8
P/2
PL/8
ux1
uy1
ux2
uy2
φ2φ1
intu + PK = ffx1
fy2
Special Considerations
Treatment of Loads acting within Elements
In this case, we need to transfer the loads within the element to equivalent nodal loads, and accordingly modify the DSM equation:
Institute of Structural Engineering Page 23
Method of Finite Elements I
PP/2
PL/8 P/2
PL/8
l/2 l/2
P/2
PL/8P/2
PL/8
P/2
PL/8
P/2
PL/8
ux1
uy2
ux2
uy2
φ2φ1
= int+ Pf Ku
fx1fy2Lokale Elementkräfte
0
2
80
2
8
P
Pl
P
Pl
= −
intP
Special Considerations
Treatment of Loads acting within Elements
In this case, we need to transfer the loads within the element to equivalent nodal loads, and accordingly modify the DSM equation:
Institute of Structural Engineering Page 24
Method of Finite Elements I
ql/2
qL2/12 ql/2l/2 l/2
ql/2
ql/2
ql/2 ql/2
qL2/12
ux1
uy2
ux2
uy2
φ2φ1fx1
fy2Lokale Elementkräfte
2
2
0
2
120
2
12
ql
ql
ql
ql
= −
intP
q
qL2/12
qL2/12 qL2/12
qL2/12
= int+ Pf Ku
Special Considerations
Treatment of Loads acting within Elements
In this case, we need to transfer the loads within the element to equivalent nodal loads, and accordingly modify the DSM equation:
Institute of Structural Engineering Page 25
Method of Finite Elements I
- Discretization- Individualization/Localization- Member Formulation
- Global Coordinates- Assembly- Boundary Conditions- Solution for Displacements- Element Moment/Shears
The DSM-Steps
Institute of Structural Engineering Page 26
Method of Finite Elements I
Illustrative Example: Truss System
Step # 0: Idealized System with Loads and Supports
1 2
3
fy3=1
fx3=2
Loads
Supports
The DSM-Steps
Institute of Structural Engineering Page 27
Method of Finite Elements I@C. Felippa, Uni Colorado
Step #1: Define a global coordinate SystemEnumerate the Nodes, Elements and Degrees of Freedom
1 2
3
(3)(2)
(1)ux2, fx2
uy2, fy2
ux3, fx3
uy3, fy3
ux1, fx1
uy1, fy1
DOFs on the global system
x
y3
3 3
10 2
200 2
L
E A
=
=
2
2 2
1050
LE A
==
1
1 1
10100
LE A==
Illustrative Example: Truss System
The DSM-Steps
Institute of Structural Engineering Page 28
Method of Finite Elements I@C. Felippa, Uni Colorado
Step #2: Decomposition and definition of Local Systems
1 2
3
(3) (2)
(1)
In this step we ignore external loads and supports and wedefine the local coordinate systems for every element
( ),i ix y
3x3y
2x
2y
1x1y
Illustrative Example: Truss System
The DSM-Steps
Institute of Structural Engineering Page 29
Method of Finite Elements I@C. Felippa, Uni Colorado
Step #3: Definition of DOFs on the Local System
i j(e)
In this step, we define the DOFs for each element in their local system (according to each element type, e.g. beam or truss)
exey
, yyi iu f
, xxi iu f, yyj ju f
, xxj ju f
Illustrative Example: Truss System
The DSM-Steps
Institute of Structural Engineering Page 30
Method of Finite Elements I
Step #4: Define the Local Stifness Matrix
For a Truss Element:
@C. Felippa, Uni Colorado
1 0 1 00 0 0 01 0 1 0
0 0 0 0
xixi
yiyi
xjxj
yjyj
ufuf EAuf Luf
− = −
1 0 1 00 0 0 01 0 1 0
0 0 0 0
eEAL
− = −
KTruss Stiffness Matrix:
xiu yiu xju yju
xiu yiu xju yju
xiu
yiu
xju
yju
Illustrative Example: Truss System
The DSM-Steps
Institute of Structural Engineering Page 31
Method of Finite Elements I
Step #5: Global Coordinates – Rotation & Translation
@C. Felippa, Uni Coloradoi
j
exey
, yyi iu f
, xxi iu f
, yyj ju f , xxj ju f
xiu
yiu
xju
yju
( ) ( ), ,e ex y x y→
ϕ
cos sin 0 0sin cos 0 00 0 cos sin0 0 sin cos
xi xi
yi yi
xj xj
yj yj
u uu uu uu u
ϕ ϕϕ ϕ
ϕ ϕϕ ϕ
− =
−
& Te e e e e e= =
⇓
u R u u R u
Global
Local
Example: The truss element
In this step, we move from the local to the global coordinate system using the Rotation Matrix
The DSM-Steps
Institute of Structural Engineering Page 32
Method of Finite Elements I
Step #5: Global Coordinates – Rotation & Translation
0 90
1 2
1 0 0 0 0 1 0 00 1 0 0 1 0 0 0
, 0 0 1 0 0 0 0 10 0 0 1 0 0 1 0
oϕ ϕ= =
− = =
−
R R
45
3
2 2 2 2 0 0
2 2 2 2 0 0
0 0 2 2 2 2
0 0 2 2 2 2
oϕ=
−
= −
R
For the elements of our simple example:
Example: The truss element
The DSM-Steps
Institute of Structural Engineering Page 33
Method of Finite Elements I
Step #6: Transform the local stiffness matrix to global coordinates
@C. Felippa, Uni Colorado
1
e e e
e e e
Te e
e e e e e e e e
Te e e e e
Te e e e
−
==
=
= → =
→ = ⇒
=
u R uf R f
R R
K u f K R u R f
R K R u f
K R K R
Example: The truss element
The DSM-Steps
Institute of Structural Engineering Page 34
Method of Finite Elements I
For our example:
@C. Felippa, Uni Colorado
1 2
3
(3) (2)
(1)
ux2, fx2
uy2, fy2
ux3, fx3
uy3, fy3
ux1, fx1
uy1, fy1
x
y
3
3 3
10 2
200 2
L
E A
=
=2
2 2
1050
LE A
==
1
1 1
10100
LE A==
Step #6: Transform the local stiffness matrix to global coordinates
Example: The truss element
The DSM-Steps
Institute of Structural Engineering Page 35
Method of Finite Elements I@C.
Fel
ippa
, Uni
Col
orad
o
Example:
1 =T1 1 1K R K R
2 2 2 2= TK R K R
3 3 3 3= TK R K R
Step #6: Transform the local stiffness matrix to global coordinates
Example: The truss element
The DSM-Steps
Institute of Structural Engineering Page 36
Method of Finite Elements I
DisassemblyIndividualization/LocalizationMember Formulation
Global CoordinatesAssemblyApplication of BCsSolutionResponse Quantities
Back to the Summary – DSM Steps
@C. Felippa, Uni Colorado
What have we done so far?
Next Steps:
Institute of Structural Engineering Page 37
Method of Finite Elements I
Step #7: Assembly - Bring together the individual element stiffness matrices Keinto the System's stiffness Matrix Ksys
In our example we have 6 DOFs
1 =K
2 =K
3 =K
ux1 uy1 ux2 uy2
ux2 uy2 ux3 uy3
ux1 uy1 ux3 uy3
Stiffness Matrix remains Symmetrical!(Maxwell-Betti Prinzip)
U = [ux1 uy1 ux2 uy2 ux3 uy3]T
1 2 3 4 5 6
u1 u2 u3 u4
u3 u4 u5 u6
u1 u2 u5 u6
u1 u2u3u4
u3 u4u5u6
u1 u2u5u6
Example: The truss element
The DSM-Steps
Institute of Structural Engineering Page 38
Method of Finite Elements I
1 1 1 111 21 31 411 1 1 121 22 32 42
1 1 1 1 131 32 33 431 1 1 141 42 43 44
k k k kk k k kk k k kk k k k
=
K
ux2 uy2 ux3 uy3
ux1 uy1 ux3 uy3
2 2 2 233 43 53 632 2 2 243 44 54 64
2 2 2 2 253 54 55 652 2 2 263 64 65 66
k k k kk k k kk k k kk k k k
=
K
3 3 3 311 21 51 613 3 3 321 22 52 62
3 3 3 3 351 52 55 653 3 3 361 62 65 66
k k k kk k k kk k k kk k k k
=
K
U = [ux1 uy1 ux2 uy2 ux3 uy3]T
1 2 3 4 5 6ux1 uy1 ux2 uy2
Step #7: Assembly - Bring together the individual element stiffness matrices Keinto the System's stiffness Matrix Ksys
In our example we have 6 DOFs
Example: The truss element
The DSM-Steps
Stiffness Matrix remains Symmetrical!(Maxwell-Betti Prinzip)
Institute of Structural Engineering Page 39
Method of Finite Elements I
1 3 1 3 1 1 3 311 11 21 21 31 41 51 611 3 1 3 1 1 3 321 21 22 22 32 42 52 62
1 1 1 2 1 2 2 231 32 33 33 43 43 53 631 1 1 2 1 2 2 241 42 43 43 44 44 54 643 3 2 2 2 3 2 351 52 53 54 55 55 65 653 3 2 2 2 361 62 63 64 65 65
sys
k k k k k k k kk k k k k k k k
k k k k k k k kk k k k k k k kk k k k k k k kk k k k k k
+ ++ +
+ +=
+ ++ ++
K
2 366 66k k
+
ux1 uy1 ux2 uy2 ux3 uy3
1 2 3 4 5 6
U = [ux1 uy1 ux2 uy2 ux3 uy3]T
Stiffness Matrix remains Symmetrical! (Maxwell-Betti Prinzip)
Step #7: Assembly - Bring together the individual element stiffness matrices Keinto the System's stiffness Matrix Ksys
In our example we have 6 DOFs
Example: The truss element
The DSM-Steps
Institute of Structural Engineering Page 40
Method of Finite Elements I
10 10 0 10 10 0 10 100 10 0 10 0 0 10 10
10 0 10 0 0 0 00 0 0 0 5 0 510 10 0 0 0 10 0 1010 10 0 5 0 10 5 10
sys
+ + − − − + + − − − +
= + −
− − + + − − − + +
K
ux1 uy1 ux2 uy2 ux3 uy3
where sys sys=K u f
Step #7: Assembly - Bring together the individual element stiffness matrices Keinto the System's stiffness Matrix Ksys
In our example we have 6 DOFs
Example: The truss element
The DSM-Steps
Stiffness Matrix remains Symmetrical! (Maxwell-Betti Prinzip)
Institute of Structural Engineering Page 41
Method of Finite Elements I
1
1
2
2
21
x
y
xsys
y
RRR
fR
=
Step #8: Assemnle the nodal loads Fi into the System-Load Vektor Fsys
1 2
3
fy3=1
fx3=2
ux3
uy3
ux2
uy2ux1
uy1
Rx2
Ry2Ry1
Rx1
ux1
uy1
ux2
uy2
ux3
uy3
Example: The truss element
The DSM-Steps
Institute of Structural Engineering Page 42
Method of Finite Elements I
Step #9: Impose the Boundar Conditions by eliminating the corresponding Rows and Columns of the fixed (restrained) DOFs from the system‘s Stiffness Matrix, and the system load vector.
ff fs f f
sys sys sys fs ss s s
= ⇒ =
K K u fK u f
K K u f
Why can we do this?
Denote with s the fixed DOFs and with f the fre DOFs, then theglbal equilibrium equations can be rewritten as:.
But for restrained DOFs we have: s =u 0
0
ff fs f f ff f f
sf ss s sf f s
== ⇒ =
K K u f K u fK K f K u f
This means we can solve the equation only for the free DOFs
Example: The truss element
The DSM-Steps
Institute of Structural Engineering Page 43
Method of Finite Elements I
1
1
2
2
21
x
y
xsys
y
RRRR
=
f
1
1
2
2
3
3
x
y
xsys
y
x
y
uuuuuu
=
u
10 10 0 10 10 0 10 100 10 0 10 0 0 10 10
10 0 10 0 0 0 00 0 0 0 5 0 510 10 0 0 0 10 0 1010 10 0 5 0 10 5 10
sys
+ + − − − + + − − − +
= + −
− − + + − − − + +
K
ux1 = uy1 = ux2 = uy2 = 0
ffKfsK
sfKssK
Step #9: Impose the Boundar Conditions by eliminating the corresponding Rows and Columns of the fixed (restrained) DOFs from the system‘s Stiffness Matrix, and the system load vector.
Example: The truss element
The DSM-Steps
Institute of Structural Engineering Page 44
Method of Finite Elements I
1
1
2
2
21
x
y
xsys
y
RRRR
=
f
1
1
2
2
3
3
x
y
xsys
y
x
y
uuuuuu
=
u
10 10 0 10 10 0 10 100 10 0 10 0 0 10 10
10 0 10 0 0 0 00 0 0 0 5 0 510 10 0 0 0 10 0 1010 10 0 5 0 10 5 10
sys
+ + − − − + + − − − +
= + −
− − + + − − − + +
K
ux1 = uy1 = ux2 = uy2 = 0
Step #9: Impose the Boundar Conditions by eliminating the corresponding Rows and Columns of the fixed (restrained) DOFs from the system‘s Stiffness Matrix, and the system load vector.
Example: The truss element
The DSM-Steps
Institute of Structural Engineering Page 45
Method of Finite Elements I
21f
=
f
Step #10: Solution: Solve for the unknow displacements uff :
3
3
xf
y
uu
=
u 10 1010 15ff
= ⇒
K 1ff f f f ff f
−= ⇒ =K u f u K f
1 1für a b d bc d c aad bc
− − = ⇒ = −−
A AReminder: Inverse of a 2x2 Matrix:
Hence 1
3
3
15 10 2110 10 1150 100
0.40.2
f ff f
xf
y
uu
− − = = −−
⇒ = =
u K f
u
0000
0.40.2
sys
⇒ =
u
Example: The truss element
The DSM-Steps
Institute of Structural Engineering Page 46
Method of Finite Elements I
Step #11: Back-Calculate the Individual Element forces(a) Reorganize the system (global) displacements usys into the respective elemental vectors ue
1 2 1
1 2 11 2 3
2 3 3
2 3 3
0 0 00 0 0
, , ,0 0.4 0.40 0.2 0.2
x x x
y y y
x x x
y y y
u u uu u uu u uu u u
= = = = = =
u u u
Example: The truss element
The DSM-Steps
Institute of Structural Engineering Page 47
Method of Finite Elements I
Example: The truss element
The DSM-Steps
Step #11: Back Calculate the Element Forces(b) Rotation from global back to local coordinates
e e e=u R u
1 1 1 2 2 2
3 3 3
0 0 1 0 0 0 00 1 0 0 0 0 0
, 0 0 0 0 1 0.4 0.20 0 0 1 0 0.2 0.4
2 2 2 2 0 0 0 02 2 2 2 0 0 0 0
0.4 0.420 0 2 2 2 20.2 0.140 0 2 2 2 2
− = = = = =
− − − = = = − −
u R u u R u
u R u
Institute of Structural Engineering Page 48
Method of Finite Elements I
Step #11: Back Calculate the Element Forces(b) Calculate the element forces
1 1 1
2 2 2
3 3 3
01 0 1 0 0 10 0 0 0 0 0
51 0 1 0 0.2 1
0 0 0 0 0.4 0
1 0 1 0 0 8.40 0 0 0 0 0
201 0 1 0 0.42 8.4
0 0 0 0 0.14 0
= =
− − = = = −
− − −
= = = −
−
F K u
F K u
F K u
eF
Example: The truss element
The DSM-Steps
Institute of Structural Engineering Page 49
Method of Finite Elements I
Summary: Linear Static Analysis (1st order)
Workflow of computer program
1. System identification: Elements, nodes, support and loads2. Build element stiffness matrices and load vectors3. Assemble global stiffness matrix and load vector4. Solve global system of equations (=> displacements)5. Calculate element results
Exact solution for displacements and stresses