Abstract
A dynamical time-dependent model of particle acceleration at coronal
mass ejection (CME) driven shock waves is presented. We consider first a
one-dimensional model applicable to shock waves of arbitrary strength.
The model includes the determination of the particle's injection energy,
the maximum energy of particles accelerated at the shock, energetic
particle spectra at all spatial and temporal locations, and the
dynamical distribution of particles that are trapped in the post shock
flow and those that escape upstream and downstream of the evolving shock
complex. We then consider the extension of this model to two dimensions.
The 2-dimensional model computes the variation of the shock strength
both temporally and spatially and illustrates how this effects the
evolution of the energetic particle spectra and intensities.
| Original language | English |
|---|---|
| Pages (from-to) | 901-906 |
| Journal | Advances in Space Research |
| Volume | 31 |
| Publication status | Published - 2003 |