Charge-to-Mass Fractionation during Injection into First-order Fermi Acceleration of Suprathermal Ions at an Interplanetary Shock

Details Charge-to-Mass Fractionation during Injection into First-order Fermi Acceleration of Suprathermal Ions at an Interplanetary Shock Charge-to-Mass Fractionation during Injection into First-order Fermi Acceleration of Suprathermal Ions at an Interplanetary Shock

Dec 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001agufmsh31c..02k&link_type=abstract

American Geophysical Union, Fall Meeting 2001, abstract #SH31C-02

Physics

2114 Energetic Particles, Heliospheric (7514), 7509 Corona, 7513 Coronal Mass Ejections, 7514 Energetic Particles (2114), 7519 Flares

Scientific paper

A model for the injection of suprathermal ions into first-order Fermi acceleration at an interplanetary shock associated with a coronal mass ejection is presented. Three source populations are considered: 1) Ions that are pre-accelerated in the turbulence generated by the shock, 2) ions that are statistically accelerated in a magnetic cloud following the shock, and 3) solar energetic particles from impulsive solar flares.

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