A phenomenological study of the DST storm variation

Mathematics – Dynamical Systems

Scientific paper

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Earth Magnetosphere, Geomagnetic Pulsations, Magnetic Storms, Phenomenology, Dynamical Systems, Energy Transfer, Interplanetary Medium, Stochastic Processes

Scientific paper

Possible modifications and generalizations of the phenomenological model of the Dst storm variation proposed by Burton et al. (1975) are analyzed. The Dst storm variation is considered to be an output signal of some dynamic system. Stochastic generalizations are discussed with due account of additive and multiplicative noise. A method of modeling the dst variation of a magnetospheric storm using data on the regime of different types of geomagnetic pulsations at midlatitudes is proposed. The analysis is carried out in terms of the theory of fluctuation and critical phenomena. The model's tenability indicates the important role played by the pulsations in energy accumulation and dissipation processes during a geomagnetic storm.

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