I. Introduction
Geomagnetic storms, resulting from solar wind disturbances interacting with the Earth's magnetosphere, pose significant risks to satellite operations, communication systems, and power grids. The Disturbance Storm Time (Dst) Index serves as a critical measure in quantifying the intensity of these geomagnetic storms. Accurate and timely prediction of the Dst Index is therefore crucial in mitigating the potential impacts on technological systems and infrastructure.