  The eclipses seen in the radio emission of some pulsars can be invaluable to
study the properties of the material from the companion stripped away by the
pulsar. We present a study of six consecutive eclipses of PSR J0024-7204O in
the globular cluster 47 Tucanae as seen by the MeerKAT radio telescope in the
UHF (544-1088 MHz) band. A high scintillation state boosted the signal during
one of the orbits and allowed a detailed study of the eclipse properties. We
measure significant dispersion measure (DM) variations and detect strong
scattering that seems to be the dominating mechanism of the eclipses at these
frequencies. A complete drop in the linear polarization together with a small
increase in the rotation measure suggests the presence of a magnetic field of
$\sim 2$ mG. The study of multiple eclipses allowed us to measure difference in
the lengths of the eclipses and DM differences of $\sim 0.01$ pc cm$^{-3}$ in
consecutive orbits. One orbit in particular shows a delay in recovery of the
linear polarization and a visible delay in the arrival of the pulses caused by
a stronger scattering event. We suggest that these are caused by a higher
variance of density fluctuations during the event.
