M. Barta, M. Karlicky
Astronomical Institute of the Academy of Sciences of the Czech
Republic, 25165 Ondrejov, Czech Republic
Using the test-particle/PIC simulations over the underlying global MHD model of solar flare reconnection the spatial and energetic distributions of accelerated particles are estimated in various sub-domains of the reconnection region (jet, ejected plasmoid, collapsing arcade of loops). Based on the results of these simulations the radio and X-ray emissions are then estimated under some plausible assumptions. Resulting spectra and/or brightness distributions are finally related to observations. Diagnostics of some plasma/magnetic field parameters based on the model is proposed.