Replenishment of the ring current in the recovery phase

Physics

Scientific paper

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Geomagnetic Pulsations, Magnetic Disturbances, Magnetospheric Instability, Ring Currents, Solar Terrestrial Interactions, Magnetic Variations, Solar Flares, Solar Wind, Space Plasmas

Scientific paper

A theoretical analysis of the replenishment phenomenon for M-type geomagnetic disturbances and flare-related disturbances is presented. It is shown that the replenishment of the ring current in the recovery phase has a significant effect on the course of the disturbance. This phenomenon gives to Dst variations an irregular (often wavy) shape. As for flare-related disturbances, the replenishment has a more modest (though still appreciable) effect, usually leaving the Dst variation curve unchanged.

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