Kinetic Modeling of Heavy Ions and Atoms in the Heliosphere

Details Kinetic Modeling of Heavy Ions and Atoms in the Heliosphere Kinetic Modeling of Heavy Ions and Atoms in the Heliosphere

Dec 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aspc..359..276m&link_type=abstract

Numerical Modeling of Space Plasma Flows: Astronum-2006 ASP Conference Series, Volume 359, Proceedings of the Conference Held 26

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Scientific paper

Interstellar hydrogen and heavier neutral atoms have access to the inner heliosphere, and they, together with secondary products after charge exchange interactions, are important messengers of the local interstellar medium and of remote heliospheric regions. This forms part of the motivation for the IBEX mission. The neutral atom populations are out of equilibrium, which warrants a kinetic modeling approach. Some of the issues of this type of modeling are detailed, including particle injection at the boundaries and improvements of particle statistics.

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