  The Tully-Fisher Relation (TFR) links two fundamental properties of disk
galaxies: their luminosity and their rotation velocity (mass). The pioneering
work of Vogt et al. in the 1990's showed that it is possible to study the TFR
for spiral galaxies at considerable look-back-times, and use it as a powerful
probe of their evolution. In recent years, several groups have studied the TFR
for galaxies in different environments reaching redshifts beyond one. In this
brief review I summarise the main results of some of these studies and their
consequences for our understanding of the formation and evolution of disk
galaxies. Particular emphasis is placed on the possible environment-driven
differences in the behaviour of the TFR for field and cluster galaxies.
