研究目的
To analyze the rules of the solar array output current accurately for satellites in sun synchronous orbit by comprehensively researching influential factors and establishing a model.
研究成果
The model accurately fits the output current of the solar array, with a mean error of -0.3711 A and standard deviation of 2.6208 A. The temperature of the solar wing has a significant influence on output current, and more attention should be paid to temperature changes in satellite management for optimization.
研究不足
The model shows a sharp increase in error at a temperature point of 55°C, which is considered noise. The confidence interval is 98.83% (3σ), but fluctuations and potential noise in data may affect accuracy. The study is specific to sun synchronous orbit satellites and may not generalize to other orbits.
1:Experimental Design and Method Selection:
The study uses Poisson series fitting to model the relationship between output current and variables such as incidence angle of the sun, temperature, earth-sun distance factor, attenuation factor, and fixed offset angle. The least square method is employed for fitting coefficients.
2:Sample Selection and Data Sources:
256 sets of in-orbit data from a satellite that has been working normally for eighteen months are used, collected over two months.
3:List of Experimental Equipment and Materials:
Not specified in the paper.
4:Experimental Procedures and Operational Workflow:
Data on output current, incidence angle, temperature, earth-sun distance factor, attenuation factor, and fixed offset angle are collected and analyzed. The Poisson series model is applied and verified against the data.
5:Data Analysis Methods:
The least square method is used to minimize the objective function for fitting Poisson coefficients. Statistical analysis includes mean error and standard deviation calculations.
独家科研数据包,助您复现前沿成果,加速创新突破
获取完整内容