Cosmic Rays and the Global Heliospheric Magnetic Field: Meridional Motion of Footpoints

Physics

Scientific paper

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Scientific paper

We consider cosmic ray transport in magnetic field models where a meridional motion of the fo otp oints leads to organized meridional field components. We have developed a 3-D numerical code of cosmic-ray transport, incorporating a meridional HMF component. The fully time-dep endent code includes the complete 3-D time-varying magnetic field. We use this code to study a Fisk-like field, as well as the effects of a dynamically changing current sheet. Preliminary results are discussed.

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