- Conference date: 5-9 Oct 1998
- Location: Nantucket, Massachusetts (USA)
A summary of the new model of the heliospheric magnetic field and its observational implications is presented. We first introduce a global model for the steady-state configuration in the low corona and discuss solar and heliospheric implications of the resulting field configuration. Finally, we compare the effects of this model with random transport of field-lines due to reconnection on the solar surface and to the dynamic turbulent transport of magnetic field-lines.
- Magnetic fields
- Solar magnetic fields
- Turbulence simulations
- Turbulent transport processes
- Magnetic reconnection
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