WINDMI is a family of dynamical models of the magnetotail that use different closure schemes to derive truncated descriptions of the collisionless microscopic energy transfer processes occurring in the quasineutral layer. The six-dimensional systems are both Kirchhoffian and Hamiltonian in structure, ensuring that the power input from the solar wind is divided into physically realizable energy sub-components. Model parameters are defined analytically as volume integrals of physically identifiable quantities. Particle simulations are used to calculate the parameters for the various models, giving a direct comparison of the relative advantages of different closure schemes. A collisionless kinetic closure scheme that includes the heat flux gives better agreement with observations by allowing for a rapid non-adiabatic cooling of the central plasma sheet (CPS).
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