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Astrophysical MHD Simulation and Visualization

  • Bertil Dorch
Conference paper
Part of the Lecture Notes in Computational Science and Engineering book series (LNCSE, volume 13)

Abstract

The combination of numerical simulations, interactive data-mining, and visualization has proven to be very powerful when attempting to understand complex astrophysical systems. The present contribution aims at illustrating this by discussing examples from numerical magneto-hydrodynamical simulations within the context of astrophysical dynamos. Two qualitatively different simulations are discussed: A study of the magnetic field topology in a kinematic dynamo model, and a model of the buoyant rise of a twisted magnetic flux rope through a stellar convection zone.

Keywords

Stagnation Point Flux Tube Magnetic Field Line Convection Zone Flux Rope 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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Copyright information

© Springer-Verlag Berlin Heidelberg 2000

Authors and Affiliations

  • Bertil Dorch
    • 1
  1. 1.Stockholm ObservatoryThe Royal Swedish Academy of SciencesSaltsjöbadenSweden

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