基于ZED-F9P低成本接收机的电离层闪烁监测技术研究

Research on low-cost navigation receiver for BDS ionospheric scintillation monitoring and impact assessment in UAVs

  • 摘要: 电离层闪烁是影响北斗卫星导航系统(BeiDou Navigation Satellite System, BDS)定位精度与信号稳定性的关键因素,然而,目前市场上专用的电离层闪烁监测设备成本较高. 为实现电离层闪烁的实时准确低成本监测与威胁评估,本文设计了一种基于低成本接收机的北斗电离层闪烁监测与影响评估方法. 系统采用ZED-F9P高精度GNSS接收机模块与树莓派微型处理器构建硬件平台,利用Python与RTKLIB实现数据采集、预处理及幅度闪烁指数 S_4 的计算. 通过实验室半实物仿真平台,将低成本接收机与专业电离层闪烁监测接收机对比分析,结果表明两者监测的 S_4 曲线在时序变化上高度一致,均方根误差(root mean square error,RMSE)仅为0.048,验证了低成本接收机在闪烁监测精度和稳定性方面的可行性. 此外,基于精密单点定位(precise point positioning, PPP)方法的闪烁影响下导航性能评估结果显示,闪烁期间载波相位残差显著增大,验证了系统电离层闪烁监测能力的有效性. 研究成果可为构建低成本、可扩展空间天气监测网络提供技术支撑.

     

    Abstract: Ionospheric scintillation represents a critical factor affecting the positioning accuracy and signal stability of the BeiDou Navigation Satellite System (BDS). However, dedicated ionospheric scintillation monitoring equipment currently available on the market is costly. To achieve real-time, accurate, and low-cost monitoring of ionospheric scintillation and assessment of its impacts, this paper presents a BDS ionospheric scintillation monitoring and impact assessment method based on low-cost receivers. The system employs a ZED-F9P high-precision GNSS module coupled with a Raspberry Pi microprocessor to construct the hardware platform, utilizing Python and RTKLIB for data acquisition, preprocessing, and automated calculation of the amplitude scintillation index S_4 . Through a laboratory hardware-in-the-loop simulation platform, comparative analysis between the low-cost receiver and professional ionospheric scintillation monitor receiver (ISMR) was conducted. Results demonstrate high temporal consistency between the S_4 curves monitored by both systems, with a root mean square error (RMSE) of only 0.048, validating the feasibility of the low-cost receiver in terms of scintillation monitoring accuracy and stability. Furthermore, navigation performance assessment under scintillation conditions based on the precise point positioning (PPP) method reveals significant increases in carrier phase residuals during scintillation events, confirming the effectiveness of the system’s ionospheric scintillation monitoring capability. The results of this study can provide technical support for the construction of a low-cost and scalable space weather monitoring network.

     

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