Non-steady astrophysical spiral jets driven by magnetic collapse and pressure

Details Non-steady astrophysical spiral jets driven by magnetic collapse and pressure Non-steady astrophysical spiral jets driven by magnetic collapse and pressure

Jan 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989plap.work...69s&link_type=abstract

In ESA, Proceedings of an International School and Workshop on Plasma Astrophysics, Volume 1 p 69-75(SEE N89-24910 18-75)

Astronomy and Astrophysics

Astronomy

Astronomical Models, Magnetohydrodynamic Waves, Particle Acceleration, Radio Jets (Astronomy), Magnetic Compression, Plasma Pinch, Plasma Pressure

Scientific paper

A theoretical model of nonsteady, astrophysical, spiral, two sided jets is investigated by means of the ideal MHD equations with the adiabatic law for both cases; gamma = 5/3 (ion dominated plasma) and gamma = 4/3 (radiation dominated plasma). It is shown that the combined effects of the radial magnetic pinch (magnetic collapse) and anisotropic plasma pressure can explosively produce super-Alfvenic two sided jets with the spiral structure. The high energy particle acceleration during explosive jet formation is also discussed.

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