Acceleration of iron in gradual SEP events: nonhomogeneous plasma

Details Acceleration of iron in gradual SEP events: nonhomogeneous plasma Acceleration of iron in gradual SEP events: nonhomogeneous plasma

Aug 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001icrc....8.3112o&link_type=abstract

Proceedings of the 27th International Cosmic Ray Conference. 07-15 August, 2001. Hamburg, Germany. Under the auspices of the Int

Physics

Scientific paper

Acceleration of iron ions by a spherical shock wave moving through the solar corona is considered. The energy dependence of the mean charge, (?) is determined by the characteristic acceleration time, Ta, and time for charge changes, Tq. The latter varies along with plasma number density during the propagation of the shock wave. An account of adiabatic energy changes and shock broadening is shown to insufficiently influence the dependence (?). According to our estimations the photoionizing processes do not affect the ionic states of the accelerated iron in gradual events in most cases.

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