  By resorting to the Burgers model for hurricanes, we study the molecular
motion involved in the hurricane dynamics. We show that the Lagrangian
canonical formalism requires the inclusion of the environment degrees of
freedom. This also allows the description of the motion of charged particles.
In view of the role played by moist convection, cumulus and cloud water
droplets in the hurricane dynamics, we discuss on the basis of symmetry
considerations the role played by the molecular electrical dipoles and the
formation of topologically non-trivial structures. The mechanism of energy
storage and dissipation, the non-stationary time dependent Ginzburg-Landau
equation and the vortex equation are studied. Finally, we discuss the fractal
self-similarity properties of hurricanes.
