  We discuss the possibility that the IceCube neutrino telescope might be
observing the Fermi Bubbles. If the bubbles discovered in gamma rays originate
from accelerated protons, they should be strong emitters of high energy (> GeV)
neutrinos. These neutrinos are detectable as shower- or track-like events at a
Km^3 neutrino observatory. For a primary cosmic ray cutoff energy at or above
10 PeV, the Fermi Bubble flux substantially exceeds the atmospheric background,
and could account for up to ~ 4-5 of the 28 events detected above ~ 30 TeV at
IceCube. Running the detector for ~ 5-7 more years should be sufficient to
discover this flux at high significance. For a primary cosmic ray flux with
steeper spectrum, and/or lower cutoff energy, longer running times will be
required to overcome the background.
