I. Introduction
The ionosphere, an important part of the solar-terrestrial space environment, lies within a range of approximately 60–1000 km above the ground. The ionosphere exhibits long-term stable cyclic variations (solar cycle variations) and short-term unstable perturbation variations [1], [2] owing to various factors such as solar and geomagnetic activities. Perturbations in the ionosphere significantly affect the safety of spaceflights, high-frequency communication, positioning, and navigation. The total electron content (TEC), defined as the line integral of the electron density along the propagation path of a signal from the satellite to the receiver, is of great significance in the theoretical study of ionospheric physics and the applied study of ionospheric wave propagation [3]. Currently, various ionospheric models are available for obtaining the TEC, such as broadcast models, empirical ionospheric models, and global ionospheric maps (GIMs).