Shape adjustment of "FAST" active reflector

Yuanchao Zhu, Dazhao Zhang, Yanlin Lai, Huabiao Yan
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Abstract

Abstract. In this paper, the relevant working principle of "FAST" Chinese Eye is studied, and a mathematical model is established to solve the equation of the ideal paraboloid. The ideal paraboloid model is obtained by rotating the paraboloid around the axis in the two-dimensional plane. On this basis, the specific solutions of each question are discussed, and the parabolic equation, the receiving ratio of the feed cabin to the reflected signal, the numbering information and coordinates of the main cable node and other parameters are obtained. This paper for solving directly above the benchmark of spherical observation of celestial bodies when ideal parabolic equation, according to the geometrical optics to knowledge should be clear all the signals of the incoming signal after the ideal parabolic will converge to the focal point of basic rules, then through converting ideal parabolic model of ideal parabolic equation in a two-dimensional plane, An optimization model was established to minimize the absolute value of the difference between the arc length and the arc length of the parabola in the diameter of 300 meters. The known conditions were substituted into Matlab to solve the equation of the ideal parabola by rotating the parabola around the axis: . In order to determine the ideal paraboloid of the celestial body, a new spatial cartesian coordinate system is first established with the line direction between the celestial body and the spherical center as the axis, so that the observed object is located directly above the new coordinate system. The same model in question 1 is established to obtain the vertex coordinates of the ideal paraboloid at this time. Then the vertex coordinates are converted to the coordinates in the original space cartesian coordinate system by rotation transformation between space cartesian coordinate systems. The solution of its vertex coordinates (-49.5287, -37.0203, -294.1763).
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“FAST”有源反射镜的形状调整
摘要本文研究了“FAST”中国眼的相关工作原理,建立了求解理想抛物面方程的数学模型。通过在二维平面上绕轴旋转抛物面,得到理想的抛物面模型。在此基础上,讨论了各问题的具体解,得到了抛物线方程、馈源舱对反射信号的接收比、主电缆节点的编号信息和坐标等参数。本文为求解直接在天体球面观测基准上方的理想抛物方程,根据几何光学的知识,应明确所有信号的入射信号经过理想抛物会向焦点收敛的基本规律,然后通过将理想抛物模型转换为理想抛物方程在二维平面上的形式;建立了直径为300 m的抛物线弧长与弧长之差绝对值最小的优化模型。将已知条件代入Matlab中,通过将抛物线绕轴旋转求解理想抛物线方程:。为了确定天体的理想抛物面,首先以天体与球心之间的直线方向为轴,建立一个新的空间笛卡尔坐标系,使被观测物体位于新坐标系的正上方。建立与问题1相同的模型,得到此时理想抛物面的顶点坐标。然后通过空间直角坐标系之间的旋转变换,将顶点坐标转换为原空间直角坐标系中的坐标。其顶点坐标(-49.5287,-37.0203,-294.1763)的解。
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