Latitudinal Dependence of Cosmic Rays Modulation at 1 AU and Interplanetary Magnetic Field Polar Correction

Figure 2

Latitudinal relative intensity at 𝑟=1AU, obtained at different solar colatitudes for protons in the energy range defined in the Table 2 and using three definitions of polar regions: 𝜃₂₀^∘, 𝜃₂₅^∘, and 𝜃₃₀^∘.