Electrodynamic formation of astrophysical jets - Simulations

Details Electrodynamic formation of astrophysical jets - Simulations Electrodynamic formation of astrophysical jets - Simulations

Jul 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989apj...342..135g&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 342, July 1, 1989, p. 135-145. Research supported by DOE and Los Alamos Nat

Statistics

Computation

8

Accretion Disks, Black Holes (Astronomy), Computational Astrophysics, Electrodynamics, Radio Jets (Astronomy), Computer Programs, Maxwell Equation, Plasma Jets, Poynting Theorem, Relativistic Electron Beams

Scientific paper

Numerical simulations of electrodynamic models of astrophysical jets using the two and one-half dimensional, Maxwell-equation, special-relativistic particle-in-cell plasma code ISIS are described. Intense current-carrying, relativistic beams of particles are generated accompanied by an appreciable Poynting energy flux. The theory and simulations and related theory suggest a new regime of operation for laboratory foilless diodes in which generation of self-collimated plasma jets may be possible.

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