High-order shock-capturing methods for modeling dynamics of the solar atmosphere

DOI10.1016/J.PHYSD.2004.12.006zbMath1067.85503OpenAlexW2115139367MaRDI QIDQ1776973

Steve Bryson, Alexander Kosovichev, Doron Levy

Publication date: 12 May 2005

Published in: Physica D (Search for Journal in Brave)

Full work available at URL: http://hdl.handle.net/2060/20040086888

zbMATH Keywords

Conservation lawsSource termsBalance lawsCoronal oscillationsHigh-order central-upwind schemesRebound-shock modelsSpicules

Mathematics Subject Classification ID

Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Galactic and stellar structure (85A15)

Cites Work

• Efficient implementation of essentially nonoscillatory shock-capturing schemes
• Semidiscrete Central-Upwind Schemes for Hyperbolic Conservation Laws and Hamilton--Jacobi Equations
• High Resolution Schemes Using Flux Limiters for Hyperbolic Conservation Laws
• Nonoscillatory High Order Accurate Self-Similar Maximum Principle Satisfying Shock Capturing Schemes I
• A third-order semi-discrete genuinely multidimensional central scheme for hyperbolic conservation laws and related problems

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