The MINOS experiment ran from 2003 until 2012 and collected a data sample
including 10.71x10^20 protons-on-target (POT) of beam neutrinos, 3.36x10^20 POT
of beam antineutrinos and an atmospheric neutrino exposure of 37.88 kt-yrs. The
final measurement of the atmospheric neutrino oscillation parameters, dm^2_32
and theta_23, came from a full three flavour oscillation analysis of the
combined CC nu_mu and CC anti-nu_mu beam and atmospheric samples and the CC
nu_e and CC anti-nu_e appearance samples. This analysis yielded the most
precise measurement of the atmospheric mass splitting dm^2_32 performed to
date. The results are |dm^2_32|=[2.28 - 2.46]x10^-3 eV^2 (68\%) and
sin^{2}theta_23=0.35-0.65$ (90\%) in the normal hierarchy, and |dm^2_32|=[2.32
- 2.53]x10^-3 eV^2 (68\%) and sin^{2}theta_23=0.34-0.67 (90\%) in the inverted
hierarchy. The successor to MINOS in the NOvA era at FNAL, MINOS+, is now
collecting data mostly in the 3-10 GeV region, and an analysis of nu_mu
disappearance using the first 2.99x10^20 POT of data produced results very
consistent with those from MINOS. Future data will further test the standard
neutrino oscillation paradigm and allow for improved searches for exotic
phenomena including sterile neutrinos, large extra dimensions and non-standard
interactions.Comment: 18 pages, 12 figures. Accepted to Nucl. Phys.