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LIU Quan, ZHAO Weisong, XIAO Na, SONG Yanjun, ZHOU Meng, ZHANG Zhili, WANG Jinhai, WANG Lichong. Co-Frequency Interference Analysis and Dynamic Simulation Validation of Satellite-Direct-to-Device Systems Against Terrestrial IMT Networks in Cross-Border Scenarios[J]. Journal of Electronics & Information Technology. doi: 10.11999/JEIT260263
Citation: LIU Quan, ZHAO Weisong, XIAO Na, SONG Yanjun, ZHOU Meng, ZHANG Zhili, WANG Jinhai, WANG Lichong. Co-Frequency Interference Analysis and Dynamic Simulation Validation of Satellite-Direct-to-Device Systems Against Terrestrial IMT Networks in Cross-Border Scenarios[J]. Journal of Electronics & Information Technology. doi: 10.11999/JEIT260263

Co-Frequency Interference Analysis and Dynamic Simulation Validation of Satellite-Direct-to-Device Systems Against Terrestrial IMT Networks in Cross-Border Scenarios

doi: 10.11999/JEIT260263 cstr: 32379.14.JEIT260263
Funds:  The Key Project of the National Natural Science Foundation of China (62231012), the National Science and Technology Major Project of the Ministry of Industry and Information Technology (MIIT) for Mobile Information Networks (2024ZD1300800)
  • Received Date: 2026-03-09
  • Accepted Date: 2026-06-24
  • Rev Recd Date: 2026-06-17
  • Available Online: 2026-07-02
  •   Objective   Satellite-Direct-to-Device (SD2D) systems that reuse terrestrial IMT spectrum may generate harmful downlink interference to incumbent IMT networks in adjacent administrations, especially in cross-border deployments where SD2D downlinks overlap the receiver bands of both IMT user equipment (UEs) and IMT base stations (BSs). Therefore, a practical coexistence methodology is needed to (i) translate IMT receiver protection criteria into explicit power-flux-density (PFD) or equivalent-power-flux-density (EPFD) constraints and (ii) validate these constraints under realistic spatiotemporal dynamics so that they can be mapped to enforceable geographic coordination measures such as border isolation distances. The study focuses on the dominant interference path (SD2D downlink to IMT receivers) and establishes a traceable workflow from deterministic PFD/EPFD limits to dynamic Monte Carlo validation and the resulting minimum border isolation distances.  Methods   A cross-border scenario is modeled where Country A deploys an SD2D system and Country B operates a terrestrial IMT network. Two representative downlink frequencies, 1995 MHz and 2190 MHz, are evaluated for two SpaceX-related configurations, Starlink-1 and Starlink-2. The IMT network is modeled with ITU-R/3GPP-compliant characteristics, using I/N protection criteria with a threshold of −6 dB and a target percentile κ (baseline κ=99.5%) for both IMT UEs and BSs. Satellite transmit antennas use the ITU-R S.1528 reference pattern; IMT-BS receive antennas use the ITU-R F.1336 sector pattern; IMT-UEs are modeled as omnidirectional. A back-lobe blocking attenuation model is applied to both satellite and BS patterns to capture rear-side shielding. Propagation follows the ITU-R P.619 model with free-space loss as a conservative baseline, and an optional clutter-loss term is introduced via a shielding probability. Deterministic protection limits are obtained by back-calculating the maximum permissible aggregate PFD for IMT-UE protection and the maximum permissible aggregate EPFD for IMT-BS protection. A dynamic simulator then validates these limits and searches for the required minimum border isolation distances (Fig.4). Co-channel beam isolation is optimized through the C/I complementary cumulative distribution function (CCDF), and a segmented-search algorithm determines the minimum UE- and BS-side isolation distances together with κ-percentile PFD/EPFD statistics.  Results and Discussions   The deterministic-limit derivation yields a maximum permissible aggregate PFD of −102.72 dBW/m2/MHz at 2190 MHz (IMT-UE) and a maximum permissible aggregate EPFD of −129.53 dBW/m2/MHz at 1995 MHz (IMT-BS) (Fig.3). For Starlink-1, the C/I design target gives a minimum beam-isolation angle pair of (12°, 12°) (Fig.5). Dynamic simulation shows that under the representative baseline setting and the I/N threshold of −6 dB and κ=99.5%, the minimum isolation distance is 195 km for UE-protection and 290 km for BS-protection (Fig.6, Fig.7, Table 4). The coordination distance is therefore 290 km, and the κ-percentile simulated PFD/EPFD matches the deterministic limits with a residual margin below 0.5 dB. For Starlink-2, the optimized isolation angles increase to (15°, 15°), and under the same baseline setting, the required distances rise to 272 km (UE) and 420 km (BS) (Table 5). The baseline distances reported above should be interpreted as representative values under the specified simulation configuration, rather than strictly converged unique results. Stability verification shows that, under different sampling intervals, simulation durations, and random seeds, the UE/BS-side distances mainly fall within 195–210 km/290–300 km for Starlink-1 and 266–290 km/370–420 km for Starlink-2 (Table 7). Sensitivity results for Starlink-1 further show that the isolation distance is governed by the upper tail of the aggregate I/N distribution (Table 6). Tightening κ from 99.5% to 100% increases the UE/BS-side distances from 195/290 km to 304/560 km. Clutter shielding substantially reduces the UE-side distance, e.g., to 173 km at a shielding probability of 0.5, but has little effect on BS protection. Polarization reuse increases the UE/BS-side distances to 222/360 km, while increasing the number of co-channel beams to 16 raises the BS-side distance to 330 km. The minimum service elevation and link-establishment strategy are dominant operational factors: changing the elevation threshold from 10° to 35° shifts the required distances from 340/460 km to 101/150 km, while switching from Sat-MaxElevation to UE-MaxElevation reduces them to 80/180 km.  Conclusions   The proposed workflow converts IMT receiver protection criteria into deterministic PFD/EPFD limits and validates them with a spatiotemporal simulator. Under the I/N threshold of −6 dB and κ=99.5%, the baseline and stability tests jointly indicate representative UE/BS coordination-distance ranges of 195–210 km/290–300 km for Starlink-1 and 266–290 km/370–420 km for Starlink-2, rather than unique, strictly converged values. Sensitivity tests further show that the κ-percentile only changes the statistical criteria for extracting "tail events" from the samples, and clutter shielding mainly benefits UEs, whereas minimum elevation, polarization reuse, co-channel-beam number, and link-establishment strategy can reshape worst-case geometry and drive large (sometimes non-monotonic) changes in the required distances. The framework provides a traceable bridge from receiver criteria to enforceable border coordination measures.
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