Numerical modeling of particle transport and acceleration of solar flare particles in a coronal loop

Details Numerical modeling of particle transport and acceleration of solar flare particles in a coronal loop Numerical modeling of particle transport and acceleration of solar flare particles in a coronal loop

Dec 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994aipc..294..118b&link_type=abstract

High-energy solar phenomena-A new era of spacecraft measurements. AIP Conference Proceedings, Volume 294, pp. 118-123 (1994).

Physics

1

Scientific paper

We examine the behavior of energetic particles in a flaring solar coronal loop under the assumption that a uniform turbulent MHD wave field causes the particles to diffuse in momentum and real space. The analytical formulation of these processes, presented in a previously published work, is restricted by the choice of a simple energy and spatial dependence of the diffusion coefficients and the collisional energy loss term. Although good agreement is evident between the predicted and the observed time profiles when the model is applied to the 1982 June 3 flare, we have constructed a numerical model which will allow us to relax the constraints inherent in the analytical version. Progress in applying this numerical model is presented.

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