It is difficult for the
standard numerical algorithms currently adopted by the plasma physics community to meet the long - term accuracy and fidelity requirement in large -
scale numerical studies of multi-
scale, complex dynamics of plasmas in space and laboratory.
In this model the
standard set of equations plus some additional
numerical schemes are combined to find the dependence of some variable of interest (in this case, hurricane velocity V) on other variables and parameters, of which one is the turbulence length
scale hl.