The Compressible Euler Equations

Collaboration diagram for The Compressible Euler Equations:

Classes
struct	ryujin::Euler::HyperbolicDescription
class	ryujin::Euler::HyperbolicSystem
class	ryujin::Euler::HyperbolicSystemView< dim, Number, MemorySpace >
class	ryujin::Euler::Indicator< ScalarNumber >
class	ryujin::Euler::IndicatorView< dim, Number, MemorySpace >
class	ryujin::EulerInitialStates::AstroJet< Description, dim, Number >
class	ryujin::EulerInitialStates::BeckerSolution< Description, dim, Number >
class	ryujin::EulerInitialStates::Contrast< Description, dim, Number >
class	ryujin::EulerInitialStates::ExactRiemannSolution< Description, dim, Number >
class	ryujin::EulerInitialStates::FourStateContrast< Description, dim, Number >
class	ryujin::EulerInitialStates::Function< Description, dim, Number >
class	ryujin::EulerInitialStates::ICFLike< Description, dim, Number >
class	ryujin::EulerInitialStates::IsentropicVortex< Description, dim, Number >
class	ryujin::EulerInitialStates::LeBlanc< Description, dim, Number >
class	ryujin::EulerInitialStates::Noh< Description, dim, Number >
class	ryujin::EulerInitialStates::RadialContrast< Description, dim, Number >
class	ryujin::EulerInitialStates::RampUp< Description, dim, Number >
class	ryujin::EulerInitialStates::Rarefaction< Description, dim, Number >
class	ryujin::EulerInitialStates::ShockFront< Description, dim, Number >
class	ryujin::EulerInitialStates::SmoothWave< Description, dim, Number >
class	ryujin::EulerInitialStates::ThreeStateContrast< Description, dim, Number >
class	ryujin::EulerInitialStates::Uniform< Description, dim, Number >
class	ryujin::Euler::Limiter< ScalarNumber >
class	ryujin::Euler::LimiterView< dim, Number, MemorySpace >
class	ryujin::Euler::WaveSpeedEstimator< ScalarNumber >
class	ryujin::Euler::WaveSpeedEstimatorView< dim, Number, MemorySpace >

Detailed Description

This module contains classes and functions related to solving the compressible Euler equations of gas dynamics with a polytropic gas equation of state (include/ryujin/euler).