The Mechanical Design of the Second and third Antarctic Survey Telescope Wen Haikun Outline • • • • 1. The Tube Design 2. The Drive System Design 3. The Low temperature test 4.The AST3-3 Mechanical Design http://www.niaot.ac.cn The Tube Structure Design Sealing Structure Temperature compensation Structure Titanium alloy http://www.niaot.ac.cn Bending angle • Corrector mirror:2.84″ • Primary Mirror:2.12″ http://www.niaot.ac.cn Primary Mirror Supporting Structure • 9 point whiffle tree structure • Fixed position in the middle hole. • Flexure supporting structure http://www.niaot.ac.cn The stress and the deformation of the Mirror shape • The max stress value :0.425Mpa • The defromation of the mirror surface shape: PV Value :43.7nm, RMS Value:7.2nm。 http://www.niaot.ac.cn The focal plane System • Switch the filter • Auto-focus system • Thermal dissipation http://www.niaot.ac.cn Deformation of the drive system Deformation in the east-west direction Max displacement: 0.935e-04mm Deformation in the north-south direction Max displacement :0.884-04mm http://www.niaot.ac.cn http://www.niaot.ac.cn Buffer and limit position structure http://www.niaot.ac.cn Reducer improvement • Increase the rigidity of the reducer • The lowest frequency :14.8Hz http://www.niaot.ac.cn The Low temperature Test http://www.niaot.ac.cn Mo He winter test http://www.niaot.ac.cn Picture in the Anatarctic http://www.niaot.ac.cn The tube of the third telescope • Move the CCD to the outside of the tube • Solve the heat problem • easy to install and maintain http://www.niaot.ac.cn The drive system of the third telescope • Adjust the gaps of the gear • Increase the rigidity of the reducer http://www.niaot.ac.cn Thankyou http://www.niaot.ac.cn
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