Semiempirical modeling of thermospheric magnetic storms

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Atmospheric Composition, Atmospheric Heating, Atmospheric Models, Magnetic Effects, Magnetic Storms, Thermosphere, Atmospheric Energy Sources, Atmospheric Temperature, Mathematical Models

Scientific paper

An improved formulation for empirical modeling of magnetic storm effects in neutral thermospheric composition and temperature is utilized in a study of two disturbed periods. The formulation, which incorporates the prior history of the heat input rather than a single phase delay, is based on a Fourier integral representation of an existing theoretical model. This results in an improved representation of the detailed time variations and a better carry-over of model parameters from one storm to the other and provides a basis for theoretical interpretation.

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