Fig. 1

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Dependences on time of the forward-shock radius Rf (thin solid line), the reverse-shock radius Rb (thin dashedline), the forward-shock velocity Vf (thick solid line), the reverse-shock velocity |Vb| (thick dashed line), the ratio of CR energy and energy of supernova explosion Ecr ∕Esn (thick dotted line), and the magnetic field strength (thick dash-dotted line) in the shock radius (r = Rf).
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