Abstract:We propose a physical approach to reconstruct the ultimate spectrum of solar/stellar cosmic rays (SCR) in a given point in the heliosphere (stellar sphere) basing on maximal value of magnetic field strength in active region and its characteristic linear dimension. An accelerator of given dimensions and magnetic field strength may accelerate to some finite energy for a given time (a maximal energy of SCR). We use the spectrum of SCR proposed by Syrovatsky (1961) for relativistic and non-relativistic energies no… Show more
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