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- W2083480334 abstract "Many quasars and active galactic nuclei are connected with long, thin jets. When observed with high angular resolution, these jets show a structure with bright knots separated by relatively dark regions. We consider magnetic collimation, connected with torsional oscillations of a cylinder with elongated magnetic field, and periodically distributed initial rotation around the cylinder axis. The stabilizing azimuthal magnetic field is created here by torsional oscillations. An approximate, simplified model is developed. The parameters for which jets may be stabilized by torsional oscillations are estimated quantitatively." @default.
- W2083480334 created "2016-06-24" @default.
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- W2083480334 date "2008-09-01" @default.
- W2083480334 modified "2023-10-18" @default.
- W2083480334 title "JET CONFINEMENT BY NONLINEAR MAGNETO-TORSIONAL OSCILLATIONS" @default.
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- W2083480334 doi "https://doi.org/10.1142/s0218271808013315" @default.
- W2083480334 hasPublicationYear "2008" @default.
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