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Coronal Magnetic Fields and Energetic Particles

Published online by Cambridge University Press:  25 May 2016

Gordon Newkirk Jr.*
Affiliation:
High Altitude Observatory, National Center for Atmospheric Research*, Boulder, Colo., U.S.A.

Abstract

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**Magnetic fields in coronal and interplanetary space play a critical role in the propagation and storage of energetic particles from the flare site to 1 AU. The current investigation is designed to determine if the detailed configuration of the coronal magnetic fields below 2.5 R has a measurable influence on the escape of particles to 1 AU, can account for the observed broad longitudinal distribution of proton flares, and can provide a realistic site for storage of energetic particles.

Type
Part IV Acceleration, Containement and Emission of High-Energy Flare Particles
Copyright
Copyright © Reidel 1974