An Unsplit Godunov Method for Ideal MHD via Constrained Transport in Three Dimensions
arXiv:0712.2634 · doi:10.1016/j.jcp.2007.12.017
Abstract
We present a single step, second-order accurate Godunov scheme for ideal MHD which is an extension of the method described by Gardiner & Stone (2005) to three dimensions. This algorithm combines the corner transport upwind (CTU) method of Colella for multidimensional integration, and the constrained transport (CT) algorithm for preserving the divergence-free constraint on the magnetic field. We describe the calculation of the PPM interface states for 3D ideal MHD which must include multidimensional ``MHD source terms'' and naturally respect the balance implicit in these terms by the condition. We compare two different forms for the CTU integration algorithm which require either 6- or 12-solutions of the Riemann problem per cell per time-step, and present a detailed description of the 6-solve algorithm. Finally, we present solutions for test problems to demonstrate the accuracy and robustness of the algorithm.
arXiv commentExtended version of the paper accepted for publication in JCP
References in corpus (7)
- An Unsplit Godunov Method for Ideal MHD via Constrained Transport
- On the Divergence-Free Condition in Godunov-Type Schemes for Ideal Magnetohydrodynamics: the Upwind Constrained Transport Method
- Numerical Magnetohydrodynamics in Astrophysics: Algorithm and Tests for One-Dimensional Flow
- High Order Upwind Schemes for Multidimensional Magnetohydrodynamics
- Nonlinear Evolution of the Magnetohydrodynamic Rayleigh-Taylor Instability
- A Free, Fast, Simple and Efficient TVD MHD Code
- Magnetic helicity evolution in a periodic domain with imposed field
Cited by in corpus (176)
- GIZMO: A New Class of Accurate, Mesh-Free Hydrodynamic Simulation Methods
- Athena: A New Code for Astrophysical MHD
- The Athena++ Adaptive Mesh Refinement Framework: Design and Magnetohydrodynamic Solvers
- The PLUTO Code for Adaptive Mesh Computations in Astrophysical Fluid Dynamics
- Linear and nonlinear evolution of the vertical shear instability in accretion discs
- The Mass and Size Distribution of Planetesimals Formed by the Streaming Instability. I. The Role of Self-Gravity
- Maximally Star-Forming Galactic Disks I. Starburst Regulation Via Feedback-Driven Turbulence
- Sustained Magnetorotational Turbulence in Local Simulations of Stratified Disks with Zero Net Magnetic Flux
- A Characteristic Scale for Cold Gas
- The Interaction of High-Speed Turbulence with Flames: Global Properties and Internal Flame Structure
- Magnetized Gas Clouds can Survive Acceleration by a Hot Wind
- An Extension of the Athena++ Code Framework for GRMHD Based on Advanced Riemann Solvers and Staggered-Mesh Constrained Transport
- The Structure of Spiral Shocks Excited by Planetary-mass Companions
- Effect of Ambipolar Diffusion on the Non-linear Evolution of Magnetorotational Instability in Weakly Ionized Disks
- Turbulence In the Outer Regions of Protoplanetary Disks. II. Strong Accretion Driven by a Vertical Magnetic Field
- Global Simulations of the Inner Regions of Protoplanetary Disks with Comprehensive Disk Microphysics
- The Impact of Star Formation Feedback on the Circumgalactic Medium
- Global Evolution of an Accretion Disk with Net Vertical Field: Coronal Accretion, Flux Transport, and Disk Winds
- How cold gas continuously entrains mass and momentum from a hot wind
- A Solution Accurate, Efficient and Stable Unsplit Staggered Mesh Scheme for Three Dimensional Magnetohydrodynamics
- Hall-effect Controlled Gas Dynamics in Protoplanetary Disks: I. Wind Solutions at the Inner Disk
- Particle Concentration At Planet Induced Gap Edges and Vortices: I. Inviscid 3-D Hydro Disks
- The Interaction of High-Speed Turbulence with Flames: Turbulent Flame Speed
- Spontaneous Transition of Turbulent Flames to Detonations in Unconfined Media
- Implementation of the Shearing Box Approximation in Athena
- High-order conservative finite difference GLM-MHD schemes for cell-centered MHD
- Accretion disc dynamo activity in local simulations spanning weak-to-strong net vertical magnetic flux regimes
- Hydrodynamical Coupling of Mass and Momentum in Multiphase Galactic Winds
- Magnetic Field Amplification in Galaxy Clusters and its Simulation
- Turbulence In the Outer Regions of Protoplanetary Disks. I. Weak Accretion with No Vertical Magnetic Flux
- A Unified Mechanism for Unconfined Deflagration-to-Detonation Transition in Terrestrial Chemical Systems and Type Ia Supernovae
- Emergent Mesoscale Phenomena in Magnetized Accretion Disc Turbulence
- Magnetohydrodynamic-Particle-in-Cell Method for Coupling Cosmic Rays with a Thermal Plasma: Application to Non-relativistic Shocks
- Star Formation Efficiency and Dispersal of Giant Molecular Clouds with UV Radiation Feedback: Dependence on Gravitational Boundedness and Magnetic Fields
- A Radiation Transfer Solver for Athena using Short Characteristics
- Simulating Magnetohydrodynamical Flow with Constrained Transport and Adaptive Mesh Refinement; Algorithms & Tests of the AstroBEAR Code
- A Second Order Godunov Method for Multidimensional Relativistic Magnetohydrodynamics
- Resistivity-driven State Changes in Vertically Stratified Accretion Disks
- Adiabatic Heating of Contracting Turbulent Fluids
- A Two-moment Radiation Hydrodynamics Module in Athena Using a Time-explicit Godunov Method
- Turbulent resistivity driven by the magnetorotational instability
- Anisotropic Thermal Conduction and the Cooling Flow Problem in Galaxy Clusters
- A Constrained-Gradient Method to Control Divergence Errors in Numerical MHD
- The Mass and Size Distribution of Planetesimals Formed by the Streaming Instability. II. The Effect of the Radial Gas Pressure Gradient
- A Second-Order Unsplit Godunov Scheme for Cell-Centered MHD: the CTU-GLM scheme
- Dense core formation in supersonic turbulent converging flows
- The Magnetohydrodynamics of Shock-Cloud Interaction in Three Dimensions
- Survival and mass growth of cold gas in a turbulent, multiphase medium
- Density Waves Excited by Low-Mass Planets in Protoplanetary Disks II: High-Resolution Simulations of the Nonlinear Regime
- A Validated Nonlinear Kelvin-Helmholtz Benchmark for Numerical Hydrodynamics
- Computational Eulerian Hydrodynamics and Galilean Invariance
- Cholla : A New Massively-Parallel Hydrodynamics Code For Astrophysical Simulation
- Hall-effect Mediated Magnetic Flux Transport in Protoplanetary Disks
- Inclined Massive Planets in a Protoplanetary Disc: Gap Opening, Disc Breaking, and Observational Signatures
- Density Probability Distribution Functions in Supersonic Hydrodynamic and MHD Turbulence
- Detecting the orientation of magnetic fields in galaxy clusters
- Dissipation and Heating in Supersonic Hydrodynamic and MHD Turbulence
- Effects of Magnetic Field Strength and Orientation on Molecular Cloud Formation
- Protoplanetary Disk Rings as Sites for Planetesimal Formation
- A conservative orbital advection scheme for simulations of magnetized shear flows with the PLUTO code
- Simulations of Magnetorotational Turbulence with a Higher-Order Godunov Scheme
- Filament formation in wind-cloud interactions. I. Spherical clouds in uniform magnetic fields
- Pegasus: A New Hybrid-Kinetic Particle-in-Cell Code for Astrophysical Plasma Dynamics
- An Unstaggered Constrained Transport Method for the 3D Ideal Magnetohydrodynamic Equations
- Pulsating instability and self-acceleration of fast turbulent flames
- On the dynamics of planetesimals embedded in turbulent protoplanetary discs
- Density Waves Excited by Low-Mass Planets in Protoplanetary Disks I: Linear Regime
- Global Hydromagnetic Simulations of Protoplanetary Disks with Stellar Irradiation and Simplified Thermochemistry
- Numerical Simulations of Optically Thick Accretion onto a Black Hole - I. Spherical Case
- Is Multiphase Gas Cloudy or Misty?
- Dust Transport in MRI Turbulent Disks: Ideal and Non-ideal MHD with Ambipolar Diffusion
- Global Three-Dimensional Simulations of Outer Protoplanetary Disks with Ambipolar Diffusion
- Local simulations of the magnetized Kelvin-Helmholtz instability in neutron-star mergers
- A fourth-order accurate finite volume method for ideal MHD via upwind constrained transport
- Implementation of Sink Particles in the Athena Code
- First results from SMAUG: Uncovering the Origin of the Multiphase Circumgalactic Medium with a Comparative Analysis of Idealized and Cosmological Simulations
- Viscous and Resistive Effects on the MRI with a Net Toroidal Field
- Self-consistent picture of the mass ejection from a one second-long binary neutron star merger leaving a short-lived remnant in general-relativistic neutrino-radiation magnetohydrodynamic simulation
- Buoyancy Instabilities in a Weakly Collisional Intracluster Medium
- The Magnetothermal Instability in the Intracluster Medium
- The Athena Astrophysical MHD Code in Cylindrical Geometry
- Signatures of MRI-Driven Turbulence in Protoplanetary Disks: Predictions for ALMA Observations
- Buoyant Bubbles in Intracluster Gas: Effects of Magnetic Fields and Anisotropic Viscosity
- Surround & Squash: The Interstellar Medium around Scorpius Centaurus OB2
- Efficiency of Particle Trapping in the Outer Regions of Protoplanetary Disks
- Can conduction induce convection? The non-linear saturation of buoyancy instabilities in dilute plasmas
- Global 3-D Radiation Magnetohydrodynamic Simulations for FU Ori's Accretion Disk and Observational Signatures of Magnetic Fields
- Magnetohydrodynamic-Particle-in-Cell Simulations of the Cosmic-Ray Streaming Instability: Linear Growth and Quasi-linear Evolution
- The Effects of Anisotropic Viscosity on Turbulence and Heat Transport in the Intracluster Medium
- Introducing TIGRESS-NCR: I. Co-Regulation of the Multiphase Interstellar Medium and Star Formation Rates
- Filament formation in wind-cloud interactions. II. Clouds with turbulent density, velocity, and magnetic fields
- Tidal Disruption and Magnetic Flux Capture: Powering a Jet from a Quiescent Black Hole
- A Stable, Accurate Methodology for High Mach Number, Strong Magnetic Field MHD Turbulence with Adaptive Mesh Refinement: Resolution and Refinement Studies
- Shock-driven Accretion in Circumplanetary Disks: Observables and Satellite Formation
- Local Simulations of Instabilities in Relativistic Jets I: Morphology and Energetics of the Current-Driven Instability
- Three-Dimensional Relativistic Magnetohydrodynamic Simulations of Current-Driven Instability with A Sub-Alfvenic Jet: Temporal Properties
- Simulations of Magnetic Fields in Tidally-Disrupted Stars
- MHD simulations of the magnetorotational instability in a shearing box with zero net flux: the case Pm=4
- Global Simulations of the Vertical Shear Instability with Non-ideal Magnetohydrodynamical Effects
- Evolution of the Relativistic Plasmoid-Chain in the Poynting-Dominated Plasma
- A Subluminal Relativistic Magnetohydrodynamics Scheme with ADER-WENO Predictor and Multidimensional Riemann Solver-Based Corrector
- A Discontinuous Galerkin Method for Ideal Two-Fluid Plasma Equations
- A high-order positivity-preserving single-stage single-step method for the ideal magnetohydrodynamic equations
- Irradiation of Astrophysical Objects - SED and Flux Effects on Thermally Driven Winds
- Photoionization calculations of the radiation force due to spectral lines in AGNs
- Isotropically Driven versus Outflow Driven Turbulence: Observational Consequences for Molecular Clouds
- Interdependence of Electric Discharge and The Magnetorotational Instability in Protoplanetary Disks
- Dust Settling and Clumping in MRI Turbulent Outer Protoplanetary Disks
- Turbulent Linewidths in Protoplanetary Disks: Predictions from Numerical Simulations
- Constrained-Transport Magnetohydrodynamics with Adaptive-Mesh-Refinement in CHARM
- Strongly magnetized accretion discs require poloidal flux
- Systematic construction of upwind constrained transport schemes for MHD
- On the Kelvin-Helmholtz instability with smooth initial conditions -- Linear theory and simulations
- On the structure and stability of magnetic tower jets
- Implementation of advanced Riemann solvers in a neutrino-radiation magnetohydrodynamics code in numerical relativity and its application to a binary neutron star merger
- Dust segregation in Hall-dominated turbulent protoplanetary disks
- The CRONOS Code for Astrophysical Magnetohydrodynamics
- Global simulations of magnetorotational turbulence I: convergence and the quasi-steady state
- Low-mass planets in nearly inviscid disks: Numerical treatment
- Parallel grid library for rapid and flexible simulation development
- Global 3D Radiation Hydrodynamic Simulations of Proto-Jupiter's Convective Envelope
- A high-order Godunov scheme for global 3D MHD accretion disks simulations. I. The linear growth regime of the magneto-rotational instability
- A New MHD Code with Adaptive Mesh Refinement and Parallelization for Astrophysics
- Galactic Spiral Shocks with Thermal Instability in Vertically Stratified Galactic Disks
- The Effect of Anisotropic Conduction on the Thermal Instability in the Interstellar Medium
- FISH: A 3D parallel MHD code for astrophysical applications
- Disk Accretion Driven by Spiral Shocks
- WOMBAT: A Scalable and High Performance Astrophysical MHD Code
- Cooling driven coagulation
- The Early Stage of Molecular Cloud Formation by Compression of Two-phase Atomic Gases
- The Effects of Inhomogeneities within Colliding Flows on the Formation and Evolution of Molecular Clouds
- A -order accurate finite volume method for ideal classical and special relativistic MHD based on pointwise reconstructions
- MOCMC: Method of Characteristics Moment Closure, a Numerical Method for Covariant Radiation Magnetohydrodynamics
- Annihilation of Magnetic Islands at the Top of Solar Flare Loops
- Multi-scale Pressure-balanced Structures in Three-dimensional Magnetohydrodynamic Turbulence
- Non-Axisymmetric Line Driven Disc Winds II - Full Velocity Gradient
- Dense Regions in Supersonic Isothermal Turbulence
- Quantifying energetics and dissipation in magnetohydrodynamic turbulence
- A high-order weighted finite difference scheme with a multi-state approximate Riemann solver for divergence-free magnetohydrodynamic simulations
- Dynamics Near the Inner Dead-Zone Edges in a Proprotoplanetary Disk
- Non-Axisymmetric Line Driven Disc Winds I - Disc Perturbations
- The Piecewise Cubic Method (PCM) for Computational Fluid Dynamics
- The Magnetohydrodynamic-Particle-In-Cell Module in Athena++: Implementation and Code Tests
- Radial Transport and Meridional Circulation in Accretion Disks
- Evolution of 3-dimensional Relativistic Current Sheets and Development of Self-Generated Turbulence
- A finite-volume scheme for modeling compressible magnetohydrodynamic flows at low Mach numbers in stellar interiors
- Magnetically Arrested Circumbinary Accretion Flows
- Equilibrium disks, MRI mode excitation, and steady state turbulence in global accretion disk simulations
- An Extension of the Athena++ Framework for Fully Conservative Self-Gravitating Hydrodynamics
- Cosmic Ray Transport in the Ionized and Neutral ISM: MHD-PIC Simulations and Effective Fluid Treatments
- Performance-Portable Binary Neutron Star Mergers with AthenaK
- General relativistic magnetized Bondi-Hoyle-Lyttleton accretion with a spin-field misalignment: Jet nutation, polarity reversals, and Magnus drag
- Investigating the influence of magnetic fields upon structure formation with AMIGA - a C code for cosmological magnetohydrodynamics
- Turbulence, Transport and Waves in Ohmic Dead Zones
- Smoothed particle magnetohydrodynamics with the geometric density average force expression
- HOW-MHD: A High-Order WENO-Based Magnetohydrodynamic Code with a High-Order Constrained Transport Algorithm for Astrophysical Applications
- Stratified Global MHD Models of Accretion Disks in Semi-Detached Binaries
- The Dynamics of Rayleigh-Taylor Stable and Unstable Contact Discontinuities with Anisotropic Thermal Conduction
- 2-D Magnetohydrodynamic Simulations of Induced Plasma Dynamics in the Near-Core Region of a Galaxy Cluster
- Metallicity Dependence of Molecular Cloud Hierarchical Structure at Early Evolutionary Stages
- Simulations of Tidal Disruption Events
- Stability and Ly emission of Cold Stream in the Circumgalactic Medium: impact of magnetic fields and thermal conduction
- Theoretical X-ray light curves of young SNe II: the example of SN 2013ej
- Simulation of Head-on Collisions Between Filamentary Molecular Clouds Threaded by a Lateral Magnetic Field and Subsequent Evolution
- WENO-Wombat: Scalable Fifth-Order Constrained-Transport Magnetohydrodynamics for Astrophysical Applications
- Divergence-Free Magnetohydrodynamics on Conformally Moving, Adaptive Meshes Using a Vector Potential Method
- Resistive and multi-fluid RMHD on graphics processing units
- Effects of Radiation Field Geometry on Line Driven Disc Winds
- Directionally Unsplit Hydrodynamic Schemes with Hybrid MPI/OpenMP/GPU Parallelization in AMR
- Effects of Opacity Temperature Dependence on Radiatively Accelerated Clouds
- Instability and Evolution of Shocked Clouds Formed by Orthogonal Collisions between Magnetized Filamentary Molecular Clouds
- The Nature of Turbulence in the Outer Regions of Protoplanetary Disks
- Development and Application of Numerical Techniques for General-Relativistic Magnetohydrodynamics Simulations of Black Hole Accretion
- Turbulence in Magnetised Neutron Stars
- Evolution of compressed clouds formed by filament coalescence. I. Oblique collisions
- Towards Exascale Simulations of the ICM Dynamo with WENO-Wombat