The Characteristics of Cosmic Rays in a Fractal Medium

<table>The intensity (arb. Units) of CRs as a function of galactic radial distance assuming a supernova origin with CRs propagating in various fractal media (for different values of the parameter <svg height="7.1750002" id="M37" style="vertical-align:-0.1254pt" version="1.1" viewbox="0 0 8.9375 7.1750002" width="8.9375" xmlns="http://www.w3.org/2000/svg">
<g transform="matrix(1.25,0,0,-1.25,0,7.175)">
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<text transform="matrix(1,0,0,-1,-71.95,66.44)">
<tspan style="font-size: 12.50px; " x="0" y="0">𝛼</tspan>
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</svg>, see text).</table>

International Scholarly Research Notices

fig1

Figure 1

Figure 1: The Characteristics of Cosmic Rays in a Fractal Medium 