Non-homogeneous charge-consistent model for the acceleration of iron in the solar corona

Details Non-homogeneous charge-consistent model for the acceleration of iron in the solar corona Non-homogeneous charge-consistent model for the acceleration of iron in the solar corona

Dec 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002esasp.506..359s&link_type=abstract

In: Solar variability: from core to outer frontiers. The 10th European Solar Physics Meeting, 9 - 14 September 2002, Prague, Cze

Physics

Solar Corona: Particle Acceleration, Iron

Scientific paper

Acceleration of Fe ions by a spherical shock wave moving through non-homogeneous solar corona is considered in a charge-consistent way. The energy dependence of the mean charge is determined by the characteristic acceleration time and time for charge changes. The latter varies along with plasma number density during the propagation of the shock wave at its given velocity. Adiabatic energy changes and shock broadening are shown to insufficiently influence the dependence of the mean charge on energy.

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