Neutrino Oscillations in the Atmospheric Parameter Region: From the Early Experiments to the Present

<table>Reduction factor in the number of upgoing muons for different <svg height="20.0625" id="M193" style="vertical-align:-3.3907pt" version="1.1" viewbox="0 0 36.474998 20.0625" width="36.474998" xmlns="http://www.w3.org/2000/svg" xmlns:xlink="http://www.w3.org/1999/xlink">
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</svg> values for a muon detection threshold of 1 GeV (MC studies). Note the shape dependence vs the <svg height="20.0625" id="M194" style="vertical-align:-3.3907pt" version="1.1" viewbox="0 0 36.474998 20.0625" width="36.474998" xmlns="http://www.w3.org/2000/svg" xmlns:xlink="http://www.w3.org/1999/xlink">
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q56 202 87 347q7 33 -3 33q-8 0 -31.5 -17.5t-41.5 -35.5l-12 28q42 45 84 72t63 27q44 0 10 -124l-20 -75h2q92 121 193 178q36 21 64 21q62 0 28 -159l-8 -37h2q50 67 103.5 112t94.5 65q39 19 62 19q60 0 23 -156l-45 -189q-9 -39 2 -39q17 0 71 49z" id="x1D45A"></path></g>
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q0 45 -26.5 69.5t-68.5 24.5q-67 0 -120 -79l-20 20l43 63q51 56 127 56h1q66 0 107 -37t41 -95q0 -42 -31 -71q-22 -23 -68 -54z" id="x33"></path></g>
</svg> values.</table>

Advances in High Energy Physics

fig4

Figure 4

Figure 4: Neutrino Oscillations in the Atmospheric Parameter Region: From the Early Experiments to the Present 