Author Affiliations
1Nanjing Institute of Astronomical Optical & Technology, CAS, Nanjing, Jiangsu 210042, China2CAS Key Laboratory of Astronomical Optics & Technology, Nanjing Institute of Astronomical Optics & Technology, Nanjing, Jiangsu 210042, Chinashow less
Fig. 1. Rendered images for the extremely large telescopes. (a) Thirty Meter Telescope; (b) Extremely Large Telescope; (c) Giant Magellan Telescope
Fig. 2. Design and optimization of trussed supporting structure for the primary mirror of TMT
Fig. 3. Steel frame bridge supporting structure for the primary mirror of E-ELT
Fig. 4. Sheet metal welding support structure for the primary mirror of GMT
Fig. 5. Concept design for the main truss structure of 30 m CFGT
Fig. 6. Concept design for the primary M1 cell structure of 30 m CFGT telescope
Fig. 7. Mode shapes for pointing to zenith. (a) Mode 1, 2.3 Hz; (b) Mode 2, 2.4 Hz; (c) Mode 3, 2.5 Hz
Fig. 8. Mode shapes for pointing to horizon. (a) Mode 1, 2.1 Hz; (b) Mode 2, 2.2 Hz; (c) Mode 3, 2.4 Hz
Fig. 9. Original elevation lateral bearings hydraulic whiffletree
Fig. 10. Latest elevation lateral bearings hydraulic whiffletree arrangement
Fig. 11. Gravitational deformation distributions pointing at zenith and horizon. (a) Pointing to zenith; (b) Pointing to horizon
Fig. 12. Relative deformation along Z-axis and equivalent stress for the trussed supporting structure of the primary mirror M1. (a) Relative deformation along the Z-axis; (b) Equivalent stress
Fig. 13. Displacement distribution due to temperature and static wind for configuration. (a) Temperature gradient of 0.12 °C/m along the Z-axis; (b) Static wind 10 m/s
弹簧类型 | 弹簧方向 | 刚度/(N/m) | 静压油垫 | 方位轴轴向 | 2.65×1010 | 方位径向 | 1.67×109 | 高度径向 | 1.25×1010 | 高度轴向 | 1.55×109 | 直线驱动 | 方位切向 | 1.75×108 | 高度切向 | 1.49×108 |
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Table 1. Spring stiffnesses used in finite element model
模态 | 频率/Hz | 状态 | 1 | 2.3 | M1桁架中心扭转 | 2 | 2.4 | M2 spider 弯曲 | 3 | 2.5 | M2 spider 扭转 |
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Table 2. Eigenfrequencies for the CFGT telescope pointing at zenith
模态 | 频率/Hz | 状态 | 1 | 2.1 | M2 spider 弯曲 | 2 | 2.2 | M1桁架中心扭转 | 3 | 2.4 | M2 spider 扭转 |
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Table 3. Eigenfrequencies for the CFGT telescope pointing at horizon
描述 | GMT | TMT | E-ELT | 本设计 | 主模态频率范围/Hz | 3~12 | 2~5 | 1.56~6.0 | 2~5 |
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Table 4. Comparison about dominant modal eigenfrequencies for the extremely large telescopes