Space weather refers to the time-varying conditions in near-Earth space and throughout the heliosphere driven primarily by solar activity, including the solar wind, coronal mass ejections (CMEs), solar flares, and variations in the interplanetary magnetic field. As a physical phenomenon, it encompasses the coupling of solar outputs with Earth’s magnetosphere, ionosphere, and thermosphere, producing geomagnetic storms, substorms, ionospheric disturbances, and energetic particle events. These processes are governed by magnetohydrodynamic and plasma-physical interactions, including magnetic reconnection, wave–particle interactions, and particle acceleration, and are quantitatively characterized using indices such as Kp, Dst, AE, and measures of solar wind and IMF parameters.
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