Auroral expansion refers to the broadening of the auroral oval, which is the area of the sky where auroras are typically visible, often occurring during geomagnetic storms. This phenomenon is closely linked to substorm dynamics, as energy is released from the magnetosphere and redistributed into the ionosphere, leading to increased intensity and visibility of auroras. The process of auroral expansion can be indicative of changes in the magnetosphere's current systems and is crucial for understanding the energy transfer during substorms.
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