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The IceCube Neutrino Observatory detects neutrinos at energies orders ofmagnitude higher than those available to current accelerators. Above 40 TeV,neutrinos traveling through the Earth will be absorbed as they interact viacharged current interactions with nuclei, creating a deficit of Earth-crossingneutrinos detected at IceCube. The previous published results showed the crosssection to be consistent with Standard Model predictions for 1 year of IceCubedata. We present a new analysis that uses 8 years of IceCube data to fit the$\nu_\mu$ absorption in the Earth, with statistics an order of magnitude betterthan previous analyses, and with an improved treatment of systematicuncertainties. It will measure the cross section in three energy bins that spanthe range 1 TeV to 100 PeV. We will present Monte Carlo studies thatdemonstrate its sensitivity.

Measuring the Neutrino Cross Section Using 8 years of Upgoing Muon Neutrinos Observed with IceCube