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Amplification of the Magnetic Fields in Astrophysical Jets- Screw Dynamo of a Nonneutral Beam-Plasma System |
MA Chunyu;HUANG Guangli |
Purple Mountain Observatory, Academia Sinica, Nanjing 210042 |
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Cite this article: |
MA Chunyu, HUANG Guangli 1995 Chin. Phys. Lett. 12 701-704 |
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Abstract When the relativistic electrons produced by in situ acceleration propagate through the plasma of jets, they will drive the fluid components to rotate around the cylindinal axis. The shear of rotation veiocity will amplify the magnetic fields through kinematic screw dynamo mechanism.
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Keywords:
98.60.Qs
52.25.Wz
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Published: 01 November 1995
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Abstract
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