Helically symmetric astrophysical jets

Details Helically symmetric astrophysical jets Helically symmetric astrophysical jets

Dec 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000phrve..62.8616b&link_type=abstract

Physical Review E (Statistical Physics, Plasmas, Fluids, and Related Interdisciplinary Topics), Volume 62, Issue 6, December 200

Physics

13

Plasma Dynamics And Flow, Applied Classical Electromagnetism

Scientific paper

Astrophysical jets are modeled outside of their accretion disks by the helically symmetric MHD equilibria. The derived equilibria are smooth, have no current sheets, and no discontinuities. The obtained exact solutions to the MHD equilibrium equations generalize the Chandrasekhar equipartition solution and depend upon two arbitrary functions, α(ψ) and the plasma density ρ(ψ)>=0, and 2K+2 arbitrary parameters γ,aN,amn,bmn. The total kinetic and magnetic energy of the jet and its mass are finite in any layer c1

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