  I give an overview of the rich phenomenology of dwarf nova oscillations
(DNOs) and Quasi-periodic Oscillations (QPOs) observed in cataclysmic variable
stars (CVs). The favoured interpretation of these rapid brightness modulations
(3 - >1000 s time scales) is that they are magnetic in nature - magnetically
channelled accretion from the inner accretion disc for DNOs and possible
magnetically excited travelling waves in the disc for QPOs. There is increasing
evidence for the magnetic aspects, which extend to lower field the well known
properties of strong field (polars) and intermediate strength field
(intermediate polars) CVs. The result is that almost all CVs show the presence
of magnetic fields on their white dwarf primaries - though for many the
intrinsic field may be locally enhanced by the accretion process itself. There
are many parallel behaviours with the QPOs seen in X-Ray binaries, with high
and low frequency X-Ray QPOs resembling respectively the DNOs and QPOs in CVs.
