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摘要:
1.8 m×0.5 m口径的长条形主反射镜是某空间离轴三反光学系统的重要光学元件，其面形精度的好坏是决定光学系统在轨成像质量的关键。为保证主镜组件结构的稳定性、可靠性及反射镜的面形精度，提出一种适用于大尺寸长条形反射镜的双轴柔性支撑结构。首先，基于运动学等效原理提出双轴柔性支撑的初始结构，建立了柔性环节刚度数学模型并研究了其刚度特性。然后，对柔性支撑的安装位置进行了参数化研究并对柔性支撑的关键尺寸进行了优化设计。最后，确定了反射镜组件的最终设计方案。仿真与试验结果表明，反射镜组件一阶固有频率为104 Hz。
X /Y 两个光轴分别对径向施加1 G重力时面形精度RMS值分别为4.81 nm、6.09 nm，优于λ /50（λ =632.8 nm），均满足设计要求。组件正样动力学环境试验表明，反射镜组件的动力学特性良好，柔性支撑系统稳定可靠，与仿真结果一致。目前反射镜全口径面形精度已加工至λ /30 RMS，并在此精度下进行了自重0°/180°的±1 G面形检测试验，结果显示其稳定性良好。Abstract:The rectangular primary mirror with aperture of 1.8 m×0.5 m is the crucial component of an off-axis Three Mirror Anastigmat (TMA) space optical system. In order to guaranty the structural stability and reliability of the Primary Mirror Assembly (PMA) and the surface figure error (RMS value) of the mirror, a bi-axial flexural support has been proposed for the large-size rectangular mirror. First, based on the principle of kinematic equivalent, the initial structure of the bi-axial flexural support was designed and the analytical formula for stiffness and its characteristic was studied as well. Then the mounting position and the key dimensions of the flexural supports were studied and optimized. Finally, the final optimization design scheme of the PMA was determined. Experimental results indicate that the surface figure error (RMS value) of the PMA under 1 G gravity in
X andY directions are 4.81 nm and 6.09 nm respectively when the optical axis is placed horizontally, which are less thanλ /50 (λ =632.8 nm). The first-order natural frequency is 104 Hz, which can satisfy the design requirements. The dynamic tests have shown that the dynamic characteristics of the mirror assembly are good, and the flexural support system is stable and reliable. Now the mirror has been polished to have a surface figure better than λ/30 RMS. Zero Gravity optical testing has been performed under ±1 G respectively, which shows good coincidence with the analytical results. -
图 1大尺寸长条形反射镜的支撑结构原理示意图
Figure 1.Schematic diagram of mounting structure of a rectangular mirror with large aperture
图 2典型的反射镜约束方式。（a）“2-2-2”约束方式；（b）“3-2-1”约束方式
Figure 2.Typical constraints for a mirror. (a) 2-2-2 Constraint; (b) 3-2-1 Constraint
图 3基于运动学等效原理的双轴柔性铰链
Figure 3.A bi-axial flexural hinge based on kinematic equivalence principle
图 6kx与短直梁的高度a、厚度t、宽度w的关系图
Figure 6.Relationship betweenkxand heighta, thicknesst, widthwof the short straight beam
图 12ε1（a）和ε2（b）对反射镜组件一阶固有频率的影响
Figure 12.Effect ofε1(a) andε2(b) on the first-order natural frequency of PMA
图 14不同θ1值1 G自重作用下的镜面变形(去除刚体位移)
Figure 14.Surface deformation at differentθ1values under 1 G gravity (removed rigid-body displacement)
图 15θ2对RMS和一阶固有频率的影响
Figure 15.Effect of differentθ2values on the RMS and first-order natural frequency
图 16柔性支撑的不同尺寸对面形精度的影响
Figure 16.Effect of different sizes of flexural support on the RMS value
图 17柔性支撑不同尺寸对一阶固有频率的影响
Figure 17.Effect of different sizes of flexural supports on the first-order natural frequency
图 19镜面在x、y向自重作用下的变形(去除刚体位移)
Figure 19.Surface deformation under 1 G gravity inxandydirections (rigid-body displacement removed)
图 25反射镜非球面干涉检验原理图
Figure 25.Schematic diagram of mirror aspheric interferometry optical testing layout
图 27反射镜180°方向的面形检测结果
Figure 27.The surface figure of the mirror tested in 180° direction
表 1典型反射镜约束方式各支撑点的自由度
Table 1.Degree of freedom at each support point for mirror's typical constraints
（a）“2-2-2”约束方式 支撑点 约束自由度 释放自由度 A Tx、Rx Ty、Tz、Ry、Rz B Ty、Ry Tx、Tz、Rx、Rz C Tz、Rz Tx、Ty、Rx、Ry （b）“3-2-1”约束方式 支撑点 约束自由度 释放自由度 A Tx、Ty、Tz Rx、Ry、Rz B Ty、Rz Tx、Ty、Tz、Rx C Rx Tx、Ty、Tz、Ry、Rz 
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表 2短直梁的尺寸初值
Table 2.Initial size values of the short straight beam
尺寸变量 初值/mm 尺寸范围/mm a 20 15~25 t 8 5~10 w 12 7~15 下载:
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表 3柔性支撑1在不同安装角度下的镜面面形值
Table 3.Surface figure error of flexural support No.1 at different mounting angles
角度θ/° x向RMS/nm y向RMS/nm 一阶固有频率/Hz 0 10.1 28.5 108.75 90 3.97 5.34 106.36 下载:
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