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2.092/2.093 — Finite Element Analysis of Solids & Fluids I Fall ‘09 
Lecture 20 -Wave Propagation Response 
Prof. K. J. Bathe MIT OpenCourseWare 
Quiz #2: Closed book, 6 pages of notes, no calculators. Covers all materials including this week’s lectures. 
Lw 
C = tw (C depends on material properties) 
For this system, C is the wave speed (given), Lw is the critical wavelength to be represented, tw is the total time for this wave to travel past a point, Le is the “effective length” of a finite element, and is equivalent to Ln w (given). To solve, we should use Δt = LC e . 
Mesh 
Le should be smaller than the shortest wave length we want to pick up. To establish a mesh, we use low-order 
elements (4-node elements in 2D, 8-node elements in 3D). We use the central difference method, which requires stability. We need to ensure that Δt ≤ Δtcr = ω2 n . Recall that in nonlinear analysis, the wave speed changes. 
We know that no ωn ≤ max ωn (m) 
m 
where ωn is the largest frequency of an assembled finite element mesh and max ωn (m) is the largest element 
m 
frequency of all elements in the mesh. Then we can use 
2 
Δt = no 
(m) 
max ωn 
m 
and conservatively, we use a slightly smaller value. 
1
Lecture 20 Wave Propagation Response 2.092/2.093, Fall ‘09 
(m) 
How to Find ωn 
For lower-order elements, we have bounds for ωn (m) . (See Sections 9.3/9.4 and Table 9.5 that gives formulae for ωn (m).) Proof: We know  
φT ΣK(m) φn 
n ω2 = m  (a) 
n φTn ΣM(m) φn 
m 
Σ (m) 
ωn 2 = mU(b) 
Σ 
mJ (m) 
U(m) = φT K(m)φnn 
J (m) = φT M (m)φnn 
Note that K(m) is of the same size as K. Also, for an element (m), since φn is not an eigenvector for K(m): 
φT K(m)φn 2 n ω(m) φT M (m)φn ≤ n n 
2 
U(m) ≤J (m) ω(m) (c) n 
Plug (c) into (b) and we have 
2 
Σ (m) ωn (m)  2  
ω2 mJ mJ (m) ≤ max ω(m) 
nn 
≤ Σ m 
In practice, wave propagation problems are very difficult to solve, due to reflections, absorptions, and the many different wave types (shear waves, etc.). As mentioned, the central difference method is almost always used for wave propagation solutions, because wave propagation modeling needs fine meshes. 
In beams, rotational DOFs result in high frequencies, so rotational mass is frequently set to zero. If we have zero masses in the model, we need to use static condensation. 
      
Kaa Kab φa = ω2 Ma 0 φa 
Kba Kbb φb 00 φb 
No mass on b-DOFs 
Use the 2nd equation to eliminate φb from the 1st equation. 
Kbaφa + Kbbφb = 0 
φb = −K−1 
bb Kbaφa 
We obtain  
Kaa − KabK−1Kba φa = ω2Maφa 
bb 
It is the same as Gauss elimination on b-DOFs. Hence, if there are zero masses, we use static condensation prior to the use of the central difference method. 
All we have discussed regarding transient/dynamic analysis is also applicable (with modifications!) in heat transfer  fluid flow analysis. 
2
Lecture 20 Wave Propagation Response 2.092/2.093, Fall ‘09 
Transient Heat Transfer Analysis 
The governing finite element equation is Cθ˙ + Kθ = Q (given 0θ) (A) where C is the heat capacity matrix, K is the conductivity matrix, and Q is the heat flow input vector. 
I. Mode Superposition Frequently, heat transfer solutions can be obtained with coarser meshes. Let’s examine the system 
Cθ˙ + Kθ = 0 (no heat flow input) 
Assume 
θ = e−λtφ e−λtφ = 0 
e−λtCφ + K� 
−λ� 
→ 
Kφ = λCφ (B) 
n×n 
The eigenvalues are 0 ≤ λ1 ≤ λ2 ≤ ... ≤ λn, and the eigenvectors are φ1,φ2,...,φn. For constant temperature over the mesh, we have λ1 = 0. Also: 
φTi Cφj = δij 
φTi Kφj = λiδij We obtain the n decoupled equations. η˙i + λiηi = qi (i =1,...,n); 0ηi (C) n 
θ =Σ φiηi 
i=1 
ΦT CΦ = I ; Φ = 
φ1 ... φn 
→ ⎡ 
θ = Φη 0η = ΦT C 0θ 
⎤ 
ΦT KΦ = 
⎢⎢⎣ 
. 
. 
. 
λi 
. 
. 
. 
⎥⎥⎦ 
q = ΦT Q 
qi = φiT Q 
To solve Eq. (C) or perform direct integration on Eq. (A), we can use the Euler backward method or the Euler forward method. 
II. The Euler Backward Method 
Reading assignment: Section 9.6 
t+Δtθ˙ = t+Δtθ − tθ 
Δt Use Eq. (A) at time t +Δt to solve for t+Δtθ. This is an implicit method, and is unconditionally stable. Δt only needs to be selected for accuracy. 
3
Lecture 20 Wave Propagation Response 2.092/2.093, Fall ‘09 
III. The Euler Forward Method 
tθ˙ = t+Δtθ − tθ 
Δt 
Then, use Eq. (A) at time t. 
C tθ˙ + K tθ = tQ 1  1 
C t+Δtθ = C tθ − K tθ + tQ 
Δt Δt If C is a diagonal matrix, then no factorization is involved. The Euler forward method results in: 
1 
C t+Δtθ = tQˆ 
Δt 
The method is conditionally stable, and Δt must satisfy 
2 
Δt ≤ Δtcr = 
λn 
Recall: 
MU ¨+ KU = 0 
U = φ sin ω (t − τ) 
U ¨= −ω2φ sin ω (t − τ ) 
−Mω2φ((((� sin ω (t − τ )=0 
sin ω (t − τ )+ Kφ((((� Hence, Kφ = ω2Mφ is the eigenvalue problem. 
2 
η˙i + λiηi = qi Δtcr = 
→ λn 
2 
x¨i + ωi 2 xi = ri → Δtcr = ωn 
The explicit method uses the governing equations at time t to obtain the solution at t +Δt. The implicit method uses the governing equations at time t +Δt to obtain the solution at t +Δt. 
4
MIT OpenCourseWare 
http://ocw.mit.edu 
2.092 / 2.093 Finite Element Analysis of Solids and Fluids I 
Fall 2009 
For information about citing these materials or our Terms of Use, visit: http://ocw.mit.edu/terms.

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Mit2 092 f09_lec20

  • 1. n o 2.092/2.093 — Finite Element Analysis of Solids & Fluids I Fall ‘09 Lecture 20 -Wave Propagation Response Prof. K. J. Bathe MIT OpenCourseWare Quiz #2: Closed book, 6 pages of notes, no calculators. Covers all materials including this week’s lectures. Lw C = tw (C depends on material properties) For this system, C is the wave speed (given), Lw is the critical wavelength to be represented, tw is the total time for this wave to travel past a point, Le is the “effective length” of a finite element, and is equivalent to Ln w (given). To solve, we should use Δt = LC e . Mesh Le should be smaller than the shortest wave length we want to pick up. To establish a mesh, we use low-order elements (4-node elements in 2D, 8-node elements in 3D). We use the central difference method, which requires stability. We need to ensure that Δt ≤ Δtcr = ω2 n . Recall that in nonlinear analysis, the wave speed changes. We know that no ωn ≤ max ωn (m) m where ωn is the largest frequency of an assembled finite element mesh and max ωn (m) is the largest element m frequency of all elements in the mesh. Then we can use 2 Δt = no (m) max ωn m and conservatively, we use a slightly smaller value. 1
  • 2. Lecture 20 Wave Propagation Response 2.092/2.093, Fall ‘09 (m) How to Find ωn For lower-order elements, we have bounds for ωn (m) . (See Sections 9.3/9.4 and Table 9.5 that gives formulae for ωn (m).) Proof: We know φT ΣK(m) φn n ω2 = m (a) n φTn ΣM(m) φn m Σ (m) ωn 2 = mU(b) Σ mJ (m) U(m) = φT K(m)φnn J (m) = φT M (m)φnn Note that K(m) is of the same size as K. Also, for an element (m), since φn is not an eigenvector for K(m): φT K(m)φn 2 n ω(m) φT M (m)φn ≤ n n 2 U(m) ≤J (m) ω(m) (c) n Plug (c) into (b) and we have 2 Σ (m) ωn (m) 2 ω2 mJ mJ (m) ≤ max ω(m) nn ≤ Σ m In practice, wave propagation problems are very difficult to solve, due to reflections, absorptions, and the many different wave types (shear waves, etc.). As mentioned, the central difference method is almost always used for wave propagation solutions, because wave propagation modeling needs fine meshes. In beams, rotational DOFs result in high frequencies, so rotational mass is frequently set to zero. If we have zero masses in the model, we need to use static condensation. Kaa Kab φa = ω2 Ma 0 φa Kba Kbb φb 00 φb No mass on b-DOFs Use the 2nd equation to eliminate φb from the 1st equation. Kbaφa + Kbbφb = 0 φb = −K−1 bb Kbaφa We obtain Kaa − KabK−1Kba φa = ω2Maφa bb It is the same as Gauss elimination on b-DOFs. Hence, if there are zero masses, we use static condensation prior to the use of the central difference method. All we have discussed regarding transient/dynamic analysis is also applicable (with modifications!) in heat transfer fluid flow analysis. 2
  • 3. Lecture 20 Wave Propagation Response 2.092/2.093, Fall ‘09 Transient Heat Transfer Analysis The governing finite element equation is Cθ˙ + Kθ = Q (given 0θ) (A) where C is the heat capacity matrix, K is the conductivity matrix, and Q is the heat flow input vector. I. Mode Superposition Frequently, heat transfer solutions can be obtained with coarser meshes. Let’s examine the system Cθ˙ + Kθ = 0 (no heat flow input) Assume θ = e−λtφ e−λtφ = 0 e−λtCφ + K� −λ� → Kφ = λCφ (B) n×n The eigenvalues are 0 ≤ λ1 ≤ λ2 ≤ ... ≤ λn, and the eigenvectors are φ1,φ2,...,φn. For constant temperature over the mesh, we have λ1 = 0. Also: φTi Cφj = δij φTi Kφj = λiδij We obtain the n decoupled equations. η˙i + λiηi = qi (i =1,...,n); 0ηi (C) n θ =Σ φiηi i=1 ΦT CΦ = I ; Φ = φ1 ... φn → ⎡ θ = Φη 0η = ΦT C 0θ ⎤ ΦT KΦ = ⎢⎢⎣ . . . λi . . . ⎥⎥⎦ q = ΦT Q qi = φiT Q To solve Eq. (C) or perform direct integration on Eq. (A), we can use the Euler backward method or the Euler forward method. II. The Euler Backward Method Reading assignment: Section 9.6 t+Δtθ˙ = t+Δtθ − tθ Δt Use Eq. (A) at time t +Δt to solve for t+Δtθ. This is an implicit method, and is unconditionally stable. Δt only needs to be selected for accuracy. 3
  • 4. Lecture 20 Wave Propagation Response 2.092/2.093, Fall ‘09 III. The Euler Forward Method tθ˙ = t+Δtθ − tθ Δt Then, use Eq. (A) at time t. C tθ˙ + K tθ = tQ 1 1 C t+Δtθ = C tθ − K tθ + tQ Δt Δt If C is a diagonal matrix, then no factorization is involved. The Euler forward method results in: 1 C t+Δtθ = tQˆ Δt The method is conditionally stable, and Δt must satisfy 2 Δt ≤ Δtcr = λn Recall: MU ¨+ KU = 0 U = φ sin ω (t − τ) U ¨= −ω2φ sin ω (t − τ ) −Mω2φ((((� sin ω (t − τ )=0 sin ω (t − τ )+ Kφ((((� Hence, Kφ = ω2Mφ is the eigenvalue problem. 2 η˙i + λiηi = qi Δtcr = → λn 2 x¨i + ωi 2 xi = ri → Δtcr = ωn The explicit method uses the governing equations at time t to obtain the solution at t +Δt. The implicit method uses the governing equations at time t +Δt to obtain the solution at t +Δt. 4
  • 5. MIT OpenCourseWare http://ocw.mit.edu 2.092 / 2.093 Finite Element Analysis of Solids and Fluids I Fall 2009 For information about citing these materials or our Terms of Use, visit: http://ocw.mit.edu/terms.