Magnetic and Velocity Shear Driven Instabilities in the Heliospheric Plasma

Details Magnetic and Velocity Shear Driven Instabilities in the Heliospheric Plasma Magnetic and Velocity Shear Driven Instabilities in the Heliospheric Plasma

Apr 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009em%26p..104..135b&link_type=abstract

Earth, Moon, and Planets, Volume 104, Issue 1-4, pp. 135-137

Computer Science

Solar Wind, Ideal And Resistive Instabilities, Magnetic Reconnection, 3D Mhd Numerical Simulations Introduction

Scientific paper

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.

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