Finite difference multi-resolution trigonometric function WENO format simulation method
A technology of trigonometric functions and finite differences, which is applied in the simulation field of WENO format of finite difference multiple resolution trigonometric functions, and can solve problems such as reduced precision
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[0144] Example 1. Solving the one-dimensional Euler equation
[0145]
[0146] where ρ is the density, u is the velocity in the x direction, E is the total energy, and p is the pressure. The initial conditions are ① ρ(x,0)=1+0.99sin(x); ②ρ(x,0)=1+0.999sin(x); ③ρ(x,0)=1+0.99999sin(x); and u(x,0)1=, p(x,0)=1, γ=1.4. The calculation area of x is [0,2π], which satisfies the periodic boundary conditions. The exact solution of the density is ① ρ(x,t)=1+0.99sin(x-t); ②ρ(x,t)=1+0.999sin(x-t); ③ρ(x,t)=1+0.99999sin(x-t ). Numerically calculate the solutions when ①t=0.1; ②t=0.01; ③t=0.0001. The classic WENO-JS format does not work for the third case, because the density calculated with it produces negative values. The error and numerical accuracy of the density obtained by numerical simulation using the new finite-difference multiple-resolution trigonometric function WENO scheme and the classical WENO-JS scheme are shown in Tables 1 and 2. Obviously, both the trigonometric func...
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