  In this paper we present the elementary assumptions of our research on the
role of the magnetic field in modelling the quiescence-outbursts cycle in
Cataclysmic Variables (CVs). The behaviour of the magnetic field is crucial not
only to integrate the disk instability model (Osaki 1974), but also to
determine the cause and effect nexus among parameters affecting the behavior of
complex systems. On the ground of our interpretation of the results emerging
from the literature, we suggest that in models describing DNe outbursts, such
as the disk instability model, the secondary instability model (Bath 1973) and
the thermonuclear runaway model (Mitrofanov 1978), the role of the magnetic
field is at least twofold. On the one hand, it activates a specific dynamic
pathway for the accreting matter by channelling it. On the other hand, it could
be indirectly responsible for switching a particular outburst modality. In
order to represent these two roles of the magnetic field, we need to integrate
the disk instability model by looking at the global behaviour of the system
under analysis. Stochastic resonance in dynamo models, we believe, is a
suitable candidate for accomplishing this task. We shall present the MHD model
including this mechanism elsewhere.
