Particles from the Sun

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Feb 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006nwap.conf..177m&link_type=abstract

NEW WORLDS IN ASTROPARTICLE PHYSICS. Proceedings of the Fifth International Workshop. Held 8-10 January 2005 in Faro, Portugal.

Physics

Scientific paper

Particle acceleration is ubiquitous in all forms of coronal activity. The question is where, when, and how are those particles accelerated? In the Sun this question can be answered by using spatially resolved observations of the electromagnetic emissions and in-situ measures of plasmas in the heliosphere. In order to relate the remote and the in-situ observations one needs to consider both the problem of the origin of the particles, and of the propagation of those particles. We present here the details of a kinematic approach to the particle propagation problem that allows us to infer the particle injection profile at the Sun from in-situ measures at any point in the heliosphere.

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