Astronomy and Astrophysics – Astronomy
Scientific paper
Dec 2006
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aspc..359..190p&link_type=abstract
Numerical Modeling of Space Plasma Flows: Astronum-2006 ASP Conference Series, Volume 359, Proceedings of the Conference Held 26
Astronomy and Astrophysics
Astronomy
Scientific paper
The propagation of a reconnection-generated plasma flow into a magnetic
dipole-dominated region is investigated using 3-D PIC simulations. The
front of the jet is found to filament due to an interchange instability
with a wavelength determined by k_y ρ_{iz} ˜ 3.
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