Euler equations of Gas Dynamics

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Euler equations of Euler equations of Gas Dynamics Gas Dynamics Hailiang Liu Hailiang Liu Math517@ISU Math517@ISU October 15, 2004 October 15, 2004

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Euler equations of Gas Dynamics. Hailiang Liu Math517@ISU October 15, 2004. Simulated Gas Flow. Nonlinear Conservation Laws: of great practical importance since they govern a variety of physical phenomena that appear in fluid mechanics, - PowerPoint PPT Presentation

Transcript of Euler equations of Gas Dynamics

Page 1: Euler equations of Gas Dynamics

Euler equations of Gas Euler equations of Gas Dynamics Dynamics

Hailiang LiuHailiang Liu

Math517@ISUMath517@ISU

October 15, 2004October 15, 2004

Page 2: Euler equations of Gas Dynamics

Simulated Gas FlowSimulated Gas Flow

0)( ufu xt

vmvEp

pEv

pv

m

f

E

mu

)5.0)(1(

)(

22

Where u has components of density, momentum and energy.

Nonlinear Conservation Laws: of great practical importance since they govern a variety of physical phenomena that appear in fluid mechanics, astrophysics, groundwater flow, meterology, semiconductors, and reactive flows

Euler equation: Modeling inviscid non-heat conducting ( ideal polytropic) gases

Page 3: Euler equations of Gas Dynamics

Eigen-structureEigen-structure

cpc

pccpccR

cppcR

cvvcv

iii

ii

ttss

ti

i

1-

1 vs, v,

1-

1 vs,

invariants

Riemann 0

)0,,(),0,()0,,(

321

Here c^2=\gamma p/\rho=dh/dp, and c is called the sound speed.

Page 4: Euler equations of Gas Dynamics

Numerical Test by SodNumerical Test by Sod

Riemann problem proposed by Sod (1978)

Tr

Tl

r

l

u

u

xu

xuxu

)25.0,0,125.0(

)5.2,0,1(

0

0)0,(

Page 5: Euler equations of Gas Dynamics

Numerical Test by LaxNumerical Test by LaxRiemann problem proposed by Lax (1974)

Tr

Tl uu )4275.1,0,5.0()928.8,311.0,445.0(

Page 6: Euler equations of Gas Dynamics

Woodward-Collela’s testWoodward-Collela’s test

• Woodward-Collela proposed this test in 1984

)100,0,1()01.0,0,1()100,0,1(),,(

.19.0

9.01.0

1.00

)0,(

,,

rml

r

m

l

pm

xu

xu

xu

xu

Page 7: Euler equations of Gas Dynamics

The shock InteractionThe shock Interaction

A model of the interaction of a sinusoidal disturbance and a shock wave due to the initial conditions

8.0),1,0),5sin(2.01(

8.0),629369.2,333333.10,857143.3()0,)(,,(

xx

xxpv

A density wave will emerge behind the shock discontinuity, its fine structure makes the current problem a suitable test case for high order methods.

Page 8: Euler equations of Gas Dynamics

Test I--requiredTest I--required

• The first order central non-staggered LxF scheme (1954)

• The staggered NT scheme (4.2), (4.4a), (4.5).• The non-staggered NT second order accurate

central scheme, (2.18), (4.4a), (4.5).• Ref: Paper by Nessyahu and Tadmor(1990).

Page 9: Euler equations of Gas Dynamics

Test II--optionalTest II--optional

• The first order accurate Godunov-type scheme of Roe (1983)

• The ENO second order accurate scheme (1988)