Modeling of the Near-Earth Low-Energy Antiproton Fluxes

<table>The <svg height="10.325" id="M109" style="vertical-align:-0.0pt" version="1.1" viewbox="0 0 11.1875 10.325" width="11.1875" xmlns="http://www.w3.org/2000/svg">
<g transform="matrix(1.25,0,0,-1.25,0,10.325)">
<g transform="translate(72,-63.74)">
<text transform="matrix(1,0,0,-1,-71.95,63.79)">
<tspan style="font-size: 12.50px; " x="0" y="0">𝐿</tspan>
</text>
</g>
</g>
</svg>-dependence of the trapped antiproton flux spectra for various energies of antiprotons. The horizontal segments of the curves correspond to the direct penetration of the cosmic ray flux to the magnetosphere.</table>

Advances in Astronomy

fig6

Figure 6

Figure 6: Modeling of the Near-Earth Low-Energy Antiproton Fluxes 