Visintin Monica, Schiavone Riccardo, Garello Roberto
Department of Electronics and Telecommunications (DET), Politecnico di Torino, 10129 Torino, Italy.
Sensors (Basel). 2024 Oct 26;24(21):6879. doi: 10.3390/s24216879.
This paper studies the performance of the communication link between a ground station and the satellites of a LEO constellation, employing code division multiplexing and a non-linear high-power amplifier. The analysis shows that the input power selection at the high-power amplifier of the ground station has a significant impact on overall system performance. The results concerning output power, the challenge of adjusting the back-off with a continuously changing number of satellites, and improved energy efficiency suggest operating in saturation. In this scenario, we can choose to transmit directly the sign of the sum of the signals directed to individual satellites. Analytical exact and simplified results are derived, enabling the estimation of performance as a function of the number of satellites being served when the amplifier operates at saturation. These analytic results are further validated through simulations. A formula to compute the loss across different numbers of satellites is also presented. The performance under saturated amplifier conditions is evaluated, compared, and discussed, providing valuable insights for simplifying the design and operation of satellite uplink communication systems under power amplifier constraints.
本文研究了地面站与低地球轨道(LEO)星座卫星之间通信链路的性能,采用了码分复用和非线性高功率放大器。分析表明,地面站高功率放大器的输入功率选择对整个系统性能有重大影响。关于输出功率、随着卫星数量不断变化调整回退的挑战以及提高能源效率的结果表明应在饱和状态下运行。在这种情况下,我们可以选择直接传输指向各个卫星的信号之和的符号。得出了精确的解析结果和简化结果,能够在放大器处于饱和状态时根据所服务卫星的数量估计性能。这些解析结果通过仿真进一步得到验证。还给出了一个计算不同卫星数量下损耗的公式。对饱和放大器条件下的性能进行了评估、比较和讨论,为在功率放大器约束下简化卫星上行链路通信系统的设计和运行提供了有价值的见解。