Table 6: Average values (last three columns) of (in percentage, %) as a function of () and , for BESS1997, AMS1998, PAMELA2006/08, obtained from (17) without enhancement of the diffusion tensor along the polar direction (), using “R” and “L” models for the tilt angle and No Drift approximation. The differential intensities were calculated accounting for particles inside the heliospheric regions for which solar latitudes are lower than .  
