When a group of spins is placed in a magnetic field, each spin aligns in one of the two possible orientations. The relative numbers of spins with different
alignments will be given by the Boltzmann distribution.
Definition: if a system of particles, which are able to exchange
energy in collisions is in
thermal equilibrium, then the relative number (
population) of particles, N1 and N2, in two particular
energy levels with corresponding energies, E1 and E2, is given by N1/N2 = exp [-(E1 - E2)/kT] where k is the Boltzmann constant and T is the absolute temperature.
For example, in
NMR of protons at room temperature in a
magnetic field of 0.25
tesla, the difference in relative numbers of spins aligned with the
magnetic field and against the field is about one part in a million; the small excess of nuclei in the lower
energy state is the basis of the net
magnetization and the
resonance phenomenon.