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首页> 外文期刊>SIAM journal on applied dynamical systems >Evaluation of solar temperature field under different wind speeds for Shanghai 65 m radio telescope
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Evaluation of solar temperature field under different wind speeds for Shanghai 65 m radio telescope

机译:上海65米广播望远镜不同风速下的太阳能温度场评价

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The Shanghai 65 m radio telescope is currently the largest full range rotatable radio telescope in Asia. Gravity, wind and temperature are the three main factors which may have a bad effect on the reflector's surface precision. To study the effect of the thermal deformation caused by daily non-uniform temperature fields on the surface precision of the main reflector, both the temperature field and its effect were studied in detail for two typical days (January 15th and July 15th). The method to simulate temperature fields was studied initially, considering heat conduction, solar radiation, shadowing, air convection, sky radiation and ground radiation. Then, an integral parametric thermal finite element model (FEM) of the telescope was established using the ANSYS thermal analysis module. Finally, the effect of non-uniform temperature fields on the surface precision of the main reflector was estimated in terms of the Root Mean Square (RMS) deformation based on temperature transient analysis. The proposed methods and conclusions drawn can provide valuable information for thermal design, thermal monitoring and thermal control of the Shanghai 65 m radio telescope and other similar giant antenna structures.
机译:上海65米广播望远镜目前是亚洲最大的全系列旋转式电台望远镜。重力,风和温度是可能对反射器表面精度产生不良影响的三个主要因素。为研究每日非均匀温度场引起的热变形对主反射器的表面精度引起的,对温度场及其效果进行了详细研究了两个典型的日子(1月15日和7月15日)。考虑导热,太阳辐射,阴影,空气对流,天空辐射和地面辐射,研究了模拟温度场的方法。然后,使用ANSYS热分析模块建立望远镜的一体式参数热有限元模型(FEM)。最后,根据基于温度瞬态分析的根均线(RMS)变形,估计了非均匀温度场对主反射器的表面精度的影响。所提出的方法和结论可以为上海65米射频望远镜和其他类似的巨型天线结构提供有价值的热设计,热监测和热控制。

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