Figures of Merit Analysis for Over-the-Air Testing of the Non-Terrestrial Network Direct-to-Smartphone Handsets
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https://doi.org/10.13052/2026.ACES.J.410210关键词:
Direct-to-Smartphone (DTS), Figures of Merit (FoMs), Non-Terrestrial Network (NTN), Over-the-Air (OTA) testing摘要
The Non-Terrestrial Network (NTN) is a critical component of the 6G integrated space-air-ground-sea network. The comprehensive Over-the-Air (OTA) performance evaluation of NTN terminals is essential for ensuring wireless connection reliability and quality of experience. However, major international standards bodies including 3rd Generation Partnership Project (3GPP) and Cellular Telecommunications and Internet Association (CTIA) remain in the preliminary stages of developing their OTA specifications for mobile terminals supporting NTN communications. Accordingly, the objective of this paper is to investigate key Figures of Merit (FoMs) for OTA testing of NTN handsets from the perspective of satellite coverage multiplicity, to better characterize, distinguish, and rank OTA performance of different NTN handsets for future testing methodology development. During the analysis, coverage models are created for Low Earth Orbit (LEO) and Geosynchronous Orbit (GEO) constellations separately, based on which the coverage multiplicity for Starlink Direct-to-Cell (DTC) and TianTong-1 constellations is evaluated and determined for different target regions quantitatively. By comparing the coverage multiplicity and usage scenarios with those of the Global Positioning System (GPS), whose OTA FoMs and testing methods have been clearly defined in specifications, the FoMs for OTA testing of NTN handsets are recommended, including integrated FoMs for LEO (e.g., Total Isotropic Sensitivity [TIS] and Upper Hemisphere Isotropic Sensitivity [UHIS] metrics for receiver performance, and Total Radiated Power [TRP] and new Upper Hemisphere Radiated Power [UHRP] metric [corresponding to the UHIS] for radiation performance evaluation) as well as directional FoMs (e.g., requiring the average or minimum of Effective Isotropic Radiated Power [EIRP] and Effective Isotropic Sensitivity [EIS] values within a specific zenith angular range to exceed the limit) for GEO constellations, respectively.
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