Solar storms, particularly coronal mass ejections (CMEs), pose significant threats to Earth’s technological infrastructure. These events can induce geomagnetic storms, leading to widespread power outages, satellite malfunctions, and communication disruptions. The increasing reliance on technology amplifies the potential impact of such solar phenomena. Historical instances, like the 1859 Carrington Event, demonstrate the catastrophic effects of severe solar storms. Modern society’s dependence on interconnected systems makes it vulnerable to similar events, which could result in global technological meltdowns. Mitigation strategies, including improved forecasting and infrastructure resilience, are essential to prepare for future solar activity.
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