and evaluating the correlation coefficients ^(Ref,Adr,Xo), and corresponding regression coefficients A(Ref, Adr, Xo) which determine the CR intensity out of the
Heliosphere, and B(Ref, Adr, Xo) characterizing the effective diffusion coefficient in the interplanetary space. The values of correlation coefficient ^(Ref, Adr, Xo)
are shown in Fig. 2.46.15 for different values of Adr obtained for the period of solar cycle 22 which is totally covered by the used GOES data on alpha-particle fluxes.
Xo, AVERAGE MONTHS
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