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ივანე ჯავახიშვილის სახელობის
თბილისის სახელმწიფო უნივერსიტეტი ლექცია 9
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Shock Waves
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Water Waves Small amplitude waves Large amplitude waves
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Shock Development Wave front steepening Transverse waves
Longitudinal waves
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Jumps Discontinuous solutions obeying conservation laws
Jumps in (P, Rho, V, T); Continuous (E,M)
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Rankine-Hugoniot Equation
1D Euler equations:
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Rankine-Hugoniot Equation
Jump conditions:
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3D Euler equation in the conservative form:
3D Shocks 3D Euler equation in the conservative form:
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Shock Consequences Viscous Heating Bow shock produced
by a neutron star Supernova envelope Supernova remnant
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HD Linear Spectrum Fourier Analysis: ( V, P, r ) ~ exp(i k r – i w t)
Dispersion Equation: w2 (w2 - Cs2 k2)=0 Solutions: Vortices: w2 = 0 Sound waves: w2 = Cs2 k2
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HD Discontinuities Sound waves -> Shocks
(P1,r1,Vn1) -> (P2,r2,Vn2) ; Vt1=Vt2 Vortex -> Contact Discontinuity Vt1 -> Vt2 ; (P1, r1,Vn1)= (P2,r2,Vn2) Vt Vn
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MHD modes - Fast magnetosonic waves; - Slow magnetosonic waves;
- Alfven waves; - Fast shocks; - Slow shocks; - Contact shocks;
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MHD shocks
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Riemann Shock Tube Problem
1D: Shock tube problem Method of characteristics:
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Riemann Shock Tube Problem
Shock wave Rarefaction wave
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Riemann Problem Shocks in Euler equations
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Godunov Method Godunov 1959 Grid: Cell interface
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Godunov scheme Find cell interface jumps ¯ Solve Riemann Problem
(for every cell) Find cell center values (conservative interpolation) integration step
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Riemann stepping
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Interpolation
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Conservative Interpolation
Rho = Rho(P,S) Rho<0
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Approximations Riemann Solver: Interpolation
- Linear Riemann solver (ROE) Fast, medium accuracy - Harten-Laxvan-Leer solver (HLL) Problems with contact discontinuities - Two-Shock Rieman Solver Problems with entropy waves Interpolation Linear (numerical stability) Parabolic (ppm) High order
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Riemann Solvers Linear Riemann solver (Roe, 1981)
Formulate approximate linear problem d/dt Ut + A(UL,UR) d/dx U = 0
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Interpolations Linear (numerical stability) Parabolic (ppm) High order
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+/- + Best accuracy + Shock capturing
+ study of the Heating, viscosity, … Slow Turbulence Complicated
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