  The flow structure in magnetic cataclysmic variables was investigated taking
into account the effects of strong magnetic field and fast rotation of the
white dwarf. We modeled the AE Aqr system as a unique object that has the
rotation period of the white dwarf is about 1000 times shorter than the orbital
period of the binary system. Observations show that in spite of fast rotation
of the white dwarf some part of the stream from the inner Lagrange point comes
into the Roche lobe region. We analyzed possible mechanisms preventing material
to outflow from the system.

Solar and Stellar Astrophysics