[A Predictive Model for the Magnetic Field in the Heliosphere and Acceleration of Suprathermal Particles in the Solar Wind]

Details [A Predictive Model for the Magnetic Field in the Heliosphere and Acceleration of Suprathermal Particles in the Solar Wind] [A Predictive Model for the Magnetic Field in the Heliosphere and Acceleration of Suprathermal Particles in the Solar Wind]

Jan 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005stin...0523614f&link_type=abstract

Technical Report,

Mathematics

Mathematical Models, Heliosphere, Solar Corona, Magnetic Field Configurations, Magnetic Flux, Solar Wind

Scientific paper

The purpose of this grant was to develop a theoretical understanding of
the processes by which open magnetic flux undergoes large-scale
transport in the solar corona, and to use this understanding to develop
a predictive model for the heliospheric magnetic field, the
configuration for which is determined by such motions.

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