Three-dimensional Modeling of Physical Processes in the Outer Heliosphere

Details Three-dimensional Modeling of Physical Processes in the Outer Heliosphere Three-dimensional Modeling of Physical Processes in the Outer Heliosphere

Aug 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aipc.1039..410p&link_type=abstract

PARTICLE ACCELERATION AND TRANSPORT IN THE HELIOSPHERE AND BEYOND: 7th Annual International Astrophysics Conference. AIP Confer

Astronomy and Astrophysics

Astrophysics

4

Magnetohydrodynamics And Plasmas, Interplanetary Magnetic Fields, Heliopause And Solar Wind Termination, Plasma Waves And Instabilities, Flares

Scientific paper

We discuss the influence of magnetic fields on the distribution of parameters in the outer heliosphere. The physical model acknowledges the crucial importance of charge exchange and collisions between neutral and charged particles in the partially ionized plasma and takes into account both the interstellar and interplanetary magnetic fields (ISMF and IMF). We summarize the results obtained for different ISMF orientations and discuss possible consequences of increasing the ISMF magnitude for both the 2-3 kHz radio emission and the deflection of the flow of neutral hydrogen in the inner heliosheath from its original direction in the unperturbed interstellar medium.

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