  Giant flares from soft gamma-ray repeaters (SGRs) are one of the most violent
phenomena in neutron stars. Quasi-periodic oscillations (QPOs) with frequencies
ranging from 18 to 1840 Hz have been discovered in the tails of giant flares
from two SGRs, and were ascribed to be seismic vibrations or torsional
oscillations of magnetars. Here we propose an alternative explanation for the
QPOs in terms of standing sausage mode oscillations of flux tubes in the
magnetar coronae. We show that most of the QPOs observed in SGR giant flares
could be well accounted for except for those with very high frequencies (625
and 1840 Hz).
