Kinematic MHD Models of Collapsing Magnetic Traps: Extension to 3D

Details Kinematic MHD Models of Collapsing Magnetic Traps: Extension to 3D Kinematic MHD Models of Collapsing Magnetic Traps: Extension to 3D

Feb 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aipc.1094..740g&link_type=abstract

COOL STARS, STELLAR SYSTEMS AND THE SUN: Proceedings of the 15th Cambridge Workshop on Cool Stars, Stellar Systems and the Sun.

Physics

Magnetic Mirrors, Gas Dynamic Traps, Particle Acceleration, Corona

Scientific paper

We show how fully 3D kinematic MHD models of collapsing magnetic traps (CMTs) can be constructed, thus extending previous work on 2D trap models. CMTs are thought to form in the relaxing magnetic field lines in solar flares and it has been proposed that they play an important role in the acceleration of high-energy particles. This work is a first step to understanding the physics of CMTs better.

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