I. Introduction
Gravity and magnetic exploration facilitate resource detection and geological research by revealing density variations and magnetic structures within the Earth [1], [2], [3]. The observed gravity and magnetic fields represent the collective physical responses of rocks, structures, and fluids at various depths and contain a wealth of geological information [4]. This versatility allows gravity and magnetic data to be applied to a wide range of geological problems. However, the observed gravity and magnetic fields not only contain useful signals caused by detection targets but also include potential field signals caused by coherent sources, periodic signals resulting from regular variations in the observational environment, and abrupt signals induced by human activities and/or solar wind [5], [6], [7], [8], [9]. Redundant information increases the uncertainty of inversions and interferes with interpretations. Therefore, extracting gravity and magnetic anomalies induced by target sources from superimposed data is crucial to accurately reconstructing the density or magnetization spatial distribution of target sources.