Numerical observations of a simulated jet with a passive helical magnetic field

Details Numerical observations of a simulated jet with a passive helical magnetic field Numerical observations of a simulated jet with a passive helical magnetic field

Jul 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989apj...342..700c&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 342, July 15, 1989, p. 700-717.

Statistics

Computation

75

Computational Astrophysics, Magnetic Field Configurations, Magnetohydrodynamics, Radio Jets (Astronomy), Circular Polarization, Computerized Simulation, Extragalactic Radio Sources, Force-Free Magnetic Fields, Very Large Array (Vla)

Scientific paper

The first computations of the Stokes I, Q, and U parameters from a self-consistent MHD simulation of a jet with a passive helical magnetic field are presented. The results can be compared directly with astronomical observations of real extragalactic radio sources. Once the structures associated with passive fields are well understood, the polarization properties of jets with active magnetic fields can be studied.

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