Magnetic and Velocity Shear Driven Instabilities in the Heliospheric Plasma

We have addressed the problem of combined magnetic and velocity shear driven instabilities in the context of the heliospheric plasma. New high-order numerical methods have been used to analyze the instability dynamics of the heliospheric current-sheet interacting with the structure determined by the...

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Veröffentlicht in:Earth, moon, and planets moon, and planets, 2009-04, Vol.104 (1-4), p.135-137
Hauptverfasser: Bettarini, L., Landi, S., Velli, M., Londrillo, P.
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container_end_page 137
container_issue 1-4
container_start_page 135
container_title Earth, moon, and planets
container_volume 104
creator Bettarini, L.
Landi, S.
Velli, M.
Londrillo, P.
description We have addressed the problem of combined magnetic and velocity shear driven instabilities in the context of the heliospheric plasma. New high-order numerical methods have been used to analyze the instability dynamics of the heliospheric current-sheet interacting with the structure determined by the slow component of the solar wind on the solar equatorial plane above the helmet streamers. Preliminary results are presented.
doi_str_mv 10.1007/s11038-008-9270-y
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source EZB-FREE-00999 freely available EZB journals
subjects Astronomy
Astrophysics
Astrophysics and Astroparticles
Dynamic stability
Dynamic structural analysis
Heliosphere
Magnetic fields
Numerical methods
Observations and Techniques
Physics
Physics and Astronomy
Planetology
Protective equipment
Simulation
Solar wind
Space Exploration and Astronautics
Space Sciences (including Extraterrestrial Physics
Stability analysis
Sun
Velocity
title Magnetic and Velocity Shear Driven Instabilities in the Heliospheric Plasma
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