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The Analysis of Solar Energetic Particles

The Analysis of Solar Energetic Particles - NOA

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Taken fromJ.-I. Sakai andC. de Jager,1996Stochastic acceleration – diffusion in themomentum space. dE/dt ∝ (v c /v) 2 , where E and vare energy and velocity <strong>of</strong> the particle and v c isvelocity <strong>of</strong> magnetic compression.Model <strong>of</strong> the flare(Aschwandenet al.,1995): reconnection inthe X-point X point is followedby a downwarddirected shocks andMHD turbulence.(Selective He 3acceleration may occuhere) . Timing is sec –min, , E is up to GeV,spectrum is a powerlaw (Bessel function folower energy).

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