The Relativistic Filamentation Instability in Magnetized Plasmas

Details The Relativistic Filamentation Instability in Magnetized Plasmas The Relativistic Filamentation Instability in Magnetized Plasmas

Apr 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007apj...659..419s&link_type=abstract

The Astrophysical Journal, Volume 659, Issue 1, pp. 419-425.

Astronomy and Astrophysics

Astronomy

14

Instabilities, Ism: General, Magnetic Fields, Plasmas

Scientific paper

The instability of perpendicular aperiodic fluctuations in a magnetized overall-neutral two-stream distribution function with relativistic speeds is investigated. It is demonstrated that there exists a critical magnetic field strength, above which the filamentation instability is not excited. The theory is applied to relativistic jets in AGNs, microquasars, and radio lobes in large radio galaxies.

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