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

Table 5

Differences in percentage between the maximum and minimum proton intensities (Δ_max) as a function of the kinetic energy, using three values for the extension of the polar regions.

Energy range	Δmax (%)
	𝜃20^∘	𝜃25^∘	𝜃30^∘
0.35–0.98 GeV	−34^+5−5	−35^+4−4	−36^+4−3
0.76–2.09 GeV	−22^+6−7	−23^+5−4	−25^+3−3
2.09–200 GeV	−8^+4−3	−9^+3−3	−10^+2−2