  Expected atmospheric ${\bar \nu_e}$ fluxes will result in a significant
number of resonantly produced low mass hadronic vector states, as the $\rho$,
in large volume neutrino telescopes. The existence of sources of higher energy
neutrinos will result in the production of higher mass states, as the $D_s^*$
and the $({\bar t}b)_{J=1}$. We calculate the rates of production of these
states and discuss their signals. Independent of theoretical flux
determinations, the detection of these states will be a tool for experimentally
determining these fluxes.
