"Fremdionen" in the solar wind

Physics

Scientific paper

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Solar Wind, Ions

Scientific paper

This chapter starts out by discussing how non-solar wind ions in a solar plasma stream can be identified. The concepts needed to describe the motion of charged particles in electromagnetic field configurations are presented and the basic equations which govern their motion in heliospheric space are reviewed. The notion of pickup ions (PUIs) is introduced and their characteristics discussed. A brief introduction into the calculation of their fluxes and the modeling of their distribution function is given. The question of how PUIs couple with the solar wind and interact with waves is addressed. The chapter closes with an outline of what we can learn by studying PUIs.

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