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YANG Boyu, QIU Kun, CHEN Zhe, ZHAO Jin, GAO Yue. Research on LEO Constellation Interference Prediction and Detection Algorithm Driven by Collaborative Spatial Feature Mapping and Temporal Transformer[J]. Journal of Electronics & Information Technology. doi: 10.11999/JEIT260368
Citation: YANG Boyu, QIU Kun, CHEN Zhe, ZHAO Jin, GAO Yue. Research on LEO Constellation Interference Prediction and Detection Algorithm Driven by Collaborative Spatial Feature Mapping and Temporal Transformer[J]. Journal of Electronics & Information Technology. doi: 10.11999/JEIT260368

Research on LEO Constellation Interference Prediction and Detection Algorithm Driven by Collaborative Spatial Feature Mapping and Temporal Transformer

doi: 10.11999/JEIT260368 cstr: 32379.14.JEIT260368
Funds:  The Natural Science Foundation of China (U25A20396)
  • Accepted Date: 2026-07-29
  • Rev Recd Date: 2026-07-29
  • Available Online: 2026-08-08
  •   Objective  The continuous putting into use of large-scale low Earth orbit (LEO) satellite constellation groups has caused a serious crowding of orbital space resources. The wide employment of frequency repeating technique by satellite operation persons has seriously brought challenges to the frequency spectrum resources of current LEO satellite network systems. At the same time, the inner quick motion and changing topological structure of LEO satellites bring about violent changes in satellite electric power lead to serious co-frequency interference between satellites. Existing detection methods for interference between satellites mainly depend on compulsory rules formulated by the International Telecommunication Union (ITU), which employ the Interference-to-Noise Ratio (I/N) to serve as the primary indicator. Nevertheless, the link attenuation formulae and satellite position computations that are contained in the calculation procedure bring about a sharp rise in total calculation cost, hence it is hard to satisfy the real-time interference check demands of large-scale satellite constellation working. The recent interference detection algorithms which are based on deep learning are still limited to taking all visible satellites as input, thus they cannot carry out constraint on the spatial sparsity of interference feature distribution. For solving these problems, this paper puts forward a LEO constellation interference prediction and detection method which is based on spatial feature mapping and temporal Transformer, therefore it greatly decreases calculation complexity while it realizes high-efficiency interference prediction and detection.  Methods  The proposed spatial-temporal Transformer framework efficiently models dynamic co-frequency interference in large-scale heterogeneous multi-constellation LEO networks. By analyzing ITU interference formulations, we extract three core physical properties: permutation invariance, spatial sparsity, and temporal continuity. Consequently, the traditional physical iteration is reframed as a spatio-temporally decoupled feature mapping problem. A dedicated spatial mapping module, leveraging attention and parallel pooling mechanisms, compresses raw satellite parameters into robust permutation-invariant features. This effectively highlights key interference sources while filtering redundant background nodes. Finally, a temporal Transformer captures the dynamics of interference trajectories, achieving high-accuracy prediction and significantly reducing computational complexity for real-time monitoring applications.  Results and Discussions  The interference prediction and detection algorithm for LEO constellation uses space feature mapping and a time Transformer to carry out interference detection and forecast by making use of high-fidelity data. According to ITU regulations, one high-mobility LEO satellite scene has been simulated, which includes thousands of real satellites from Starlink and OneWeb constellations. Parameter analysis results show that setting reasonable feature dimensions and encoder layers can achieve an optimal balance between feature extraction accuracy and computational cost (Fig. 4 and Fig. 5). By setting model parameters such as sampling step size, prediction accuracy and engineering real-time performance can be comprehensively considered (Fig. 6 and Fig. 7). Simulation results show that compared to baseline methods, the predicted trajectory of the proposed method closely matches the baseline ground truth (Fig. 8), with the absolute deviation controlled within 0.5 dB at a 90% cumulative probability (Fig. 9). Furthermore, the algorithm maintains an extremely high interference detection rate with low false alarms (Fig. 10), and the Root Mean Square Error (RMSE) remains stable at 0.45 dB within a 20.0 s prediction window, significantly outperforming traditional regression and neural network models (Fig. 11). In terms of computational efficiency, the algorithm in this paper takes 14.2 ms for a single inference, which is only 4.1% of the time required by the traditional ITU-based physical iteration method (Table 3), effectively decoupling computational overhead and constellation scale.  Conclusions  For the problem that LEO satellite network topology has extremely strong dynamic property, and traditional physical iteration interference checking methods have limitations brought by sharply risen computation complexity, this paper puts forward a low-Earth orbit constellation interference checking algorithm which combines spatial feature mapping and temporal Transformer, therefore it effectively makes computation cost and constellation size decouple. The results of simulation show that, when the comparison is made with baseline methods, this algorithm possesses fine long-term dynamic tracking capabilities, and at the same time it keeps conformity with ITU evaluation rules. Experiments which carry on equipment analysis with different parameters have proven that the algorithm we put forward can obtain a balance between feature extraction accuracy and computation spending. By utilizing the long-distance dependence modeling ability of time-domain Transformer, the RMSE still keeps steady at 0.45 dB at identical time step. Through the method of eliminating unnecessary background satellite nodes, the single inference time has been reduced to 14.2 ms. By means of manifold experiments, which contain error distribution assessment and model parameter analysis, the algorithm put forward by us obtains the best precision and full decoupling of calculation cost from constellation scale, hence it gives a highly flexible engineering scheme for future super-large constellation arrangements.
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