The thermal analysis of a satellite by an in-house computer code based on Thermal Network Method and Monte Carlo Ray Tracing Technique

H. Isik, A. B. Uygur, Cem Omur, Erhan Solakoğlu
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引用次数: 3

Abstract

In this paper, the development of an in-house computer code for the thermal analysis of satellites is discussed. The code is based on Thermal Network Method (TNM) in conjunction with Method of Lines (MOL) for the solution of energy equation. The view factors required for the computation of radiative exchange factors which are used in TNM are calculated by a newly developed module based on Monte-Carlo Ray Tracing Technique. The predictive accuracy of the code including the new module was assessed on a realistic test problem involving a satellite orbiting the earth at an altitude of 700 km. Comparison of transient results obtained by the in-house code and a commercial thermal analysis software package (Thermica-SINDA/G) has shown that the in-house code predictions mimic the ones obtained by Thermica-SINDA/G very accurately.
基于热网络法和蒙特卡罗光线追踪技术的卫星热分析
本文讨论了卫星热分析内部计算机代码的开发。该代码基于热网络法(TNM)结合线法(MOL)求解能量方程。采用基于蒙特卡罗射线追踪技术的新开发模块,计算了TNM中辐射交换因子计算所需的视点因子。对包含新模块的代码的预测精度进行了评估,该预测精度是在一个涉及地球轨道高度700公里的卫星的实际测试问题上进行的。通过与商业热分析软件包(Thermica-SINDA/G)的瞬态结果比较,表明内部代码的预测结果与Thermica-SINDA/G的预测结果非常接近。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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