Electronic Performance-Oriented Mold Sharing Method and Application in QTT 110 m Large Radio Telescope

The reflector surface of a large reflector antenna may even consist of thousands of panels, and if the panel molds with high-precision requirements are fabricated uniquely for each ring, the overall cost will be very high. Therefore, from a perspective of reducing the cost, the mold sharing design is of particular significance. In order to obtain the minimum number of molds satisfying the given electronic performance index, the electronic performance-oriented mold sharing design is suggested, in which the effective surface accuracy is used to evaluate electrical performance. The smaller the combined effective root-mean-square (rms) error value introduced after sharing the mold, the more preferential these rings should share the mold to reduce the number of molds. Based on such idea, a fast mold reduction process is presented, which can give the minimum number of molds quickly according to the electrical performance requirements. During this process, a combined effective rms value matrix and a mold sharing discriminant matrix are defined and used. To construct these two matrices, the panel normal error induced by mold sharing is derived, and the optimal mold position is determined first. As a test problem, application of the proposed method to mold reduction of a 110 m radio telescope is presented, and the discussions of the results are given.

[1]  Qian Xu Challenges for QTT structure , 2016, Astronomical Telescopes + Instrumentation.

[2]  Jingli Du,et al.  Shape Control of Cable-Network Antennas Considering the RF Performance , 2016, IEEE Transactions on Antennas and Propagation.

[3]  J. Baars The Paraboloidal Reflector Antenna in Radio Astronomy and Communication , 2007 .

[4]  J. Ruze Antenna tolerance theory—A review , 1966 .

[5]  Z.-Q. Shen Shanghai 65m radio telescope , 2011, 2011 XXXth URSI General Assembly and Scientific Symposium.

[6]  R. Wielebinski The effelsberg 100-m radio telescope , 2004, Naturwissenschaften.

[7]  Wang Qiming,et al.  The Five-hundred-meter Aperture Spherical radio Telescope (FAST) project , 2015 .

[8]  H. Kärcher,et al.  Radio Telescope Reflectors: Historical Development of Design and Construction , 2017 .

[9]  Stephen Padin Design considerations for a highly segmented mirror. , 2003, Applied optics.

[10]  Na Wang,et al.  Xinjiang Qitai 110 m radio telescope , 2014 .

[11]  Yan Wang,et al.  A method for representation of component geometry using discrete pin for reconfigurable moulds , 2011, Adv. Eng. Softw..

[12]  Tuanjie Li,et al.  Preliminary design of paraboloidal reflectors with flat facets , 2013 .

[13]  A. Greve,et al.  Quality evaluation of radio reflector surfaces , 1981 .

[14]  Todd R. Hunter,et al.  The Green Bank Telescope , 2009, Proceedings of the IEEE.

[15]  Daniel Kirk,et al.  Development of a reconfigurable tool for forming aircraft body panels , 1998 .

[16]  Joseph Antebi,et al.  RF-mechanical performance for the Haystack radio telescope , 2011, Optical Engineering + Applications.

[17]  Yahya Rahmat-Samii,et al.  Reflector Antenna Developments: A Perspective on the Past, Present and Future , 2015, IEEE Antennas and Propagation Magazine.

[18]  Terry S. Mast,et al.  Construction of the Keck Observatory , 1990, Astronomical Telescopes and Instrumentation.

[19]  Yahya Rahmat-Samii,et al.  An efficient computational method for characterizing the effects of random surface errors on the average power pattern of reflectors , 1983 .

[20]  Baoyan Duan,et al.  Design of tipping structure for 110 m high-precision radio telescope , 2017 .

[21]  Roy Levy,et al.  Structural engineering of microwave antennas : for electrical, mechanical, and civil engineers , 1996 .