We examine the physics capabilities of known flavor neutrino beams from int
ense muon sources. We find that long-baseline neutrino experiments based on
such beams can provide precise measurements of neutrino oscillation mass a
nd mixing parameters. Furthermore, they can test whether the dominant atmos
pheric neutrino oscillations are nu(mu) --> nu(tau) and/or nu(mu) --> nu(s)
, determine the nu(mu) --> nu(e) content of atmospheric neutrino oscillatio
ns, and measure nu(e) --> nu(tau) appearance. Depending on the oscillation
parameters, they may be able to detect Earth matter and CP violation effect
s and to determine the ordering of some of the mass eigenstates.