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

<table class="table-group" id="tab2"><tr><td><table class="table"><tr><td class="thead-hr" colspan="2"><hr/></td></tr><tr class="thead"><td align="left">  HelMod Energy bin </td><td align="center"> KET channel</td></tr><tr><td class="thead-hr" colspan="2"><hr/></td></tr><tr><td align="left"> (0.35–0.98) GeV </td><td align="center"> (0.4–1.0) GeV</td></tr><tr><td align="left">(0.76–2.09) GeV </td><td align="center"> (0.8–2.0) GeV</td></tr><tr><td align="left">(2.09–200) GeV </td><td align="center"> &gt;2 GeV</td></tr><tr class="table-tr"><td colspan="2"><hr class="tbody-hr"/></td></tr></table></td></tr></table>

Kinetic energy bins (in GeV) selected with HelMod Code and the corresponding proton energy channel for KET instruments on board the Ulysses spacecraft [<a href="/journals/aa/2013/793072/#B8">8</a>].

Advances in Astronomy

tab2

Table 2

Table 2: Latitudinal Dependence of Cosmic Rays Modulation at 1 AU  and Interplanetary Magnetic Field Polar Correction 