Reference documentation

• Interface Specifications
  • Introduction
  • Stellar Dynamics Interface Definition
  • Stellar Evolution Interface Definition
  • Hydrodynamics Interface Definition
  • Radiative Transfer Interface Definition
• Message protocol between python and community codes
  • Introduction
  • Overall Operation
  • Message format
  • Examples
• Support code for AMUSE framework
• Support code for the community code interfaces
• Currently supported Community Codes
  • Introduction
  • Stellar Dynamics
  • Stellar Evolution
  • Hydrodynamics
  • Radiative Transfer
• Supported File Formats
  • Introduction
  • Use
  • Exceptions
  • Text files
  • Starlab
  • NEMO
  • Gadget
• Reporting during a run
• Quantities and Units
  • Introduction
  • Quantities
  • Units
  • Unit systems and converters
• Datamodel
  • Introduction
  • Identity
  • Sets of particles
• Particle Attributes
• From Codes to Data
  • Introduction
  • The first level
• Sets and Grids in Codes
• Stopping Conditions
  • Introduction
  • Using stopping conditions
  • Implementing stopping conditions
  • Using the stopping conditions library
• Input / Output Framework
  • Introduction
  • Extending
• Options
  • Introduction
  • Configuration file location
  • Configuration file format
  • Option values
  • Sections lookup
  • Use
• Directory Structure
  • The src directories
  • The test directories
  • The support directories
• Setting up GPGPU with CUDA
  • Introduction
  • Self-help script
  • Step-by-step
• Distributed AMUSE
  • Installation
  • Specifying resources using Jungle files
  • Starting Ibis Deploy
  • Running workers remotely
• AMUSE Style Guide
  • Python Code
  • C / C++ code
  • Fortran code
• Source Code Management
  • Commiting Code
  • SVN repository location
• Glossary