Laboratory simulation of the astrophysical burst processes in non-uniform magnetised media

Details Laboratory simulation of the astrophysical burst processes in non-uniform magnetised media Laboratory simulation of the astrophysical burst processes in non-uniform magnetised media

Aug 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990esasp.311..189a&link_type=abstract

In ESA, Plasma Astrophysics p 189-190 (SEE N91-15046 06-90)

Astronomy and Astrophysics

Astrophysics

Bursts, Collisionless Plasmas, Laser Plasmas, Plasma Interactions, Simulation, Supernova Remnants, Barium Ion Clouds, Interstellar Magnetic Fields, Interstellar Matter, Magnetohydrodynamic Stability, Plasma Clouds, Solar Flares, Three Dimensional Models

Scientific paper

Under various astrophysical conditions the dynamics of nonstationary burst processes with mass and energy release may be defined by the inhomogeneity of the surrounding medium. In the presence of external magnetic field such a problem in general case becomes a three dimensional one and very complicated both from the observable and theoretical point of view (including the computer simulation method). The application of the laboratory simulation methods in such kinds of problems therefore seems to be rather promising and is demonstrated, mainly on the example of peculiar supernova.

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