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Software design for the control system of Small LAMOST

机译:小型LAMOST控制系统的软件设计

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The Large Sky Area Multi-Object Fiber Spectroscopic Telescope , LAMOST hereafter, will become an astronomical telescope with largest field of view and most efficient observation in 4-m aperture telescopes in the world by its completion in 2008. In June 2007, Small System for LAMOST was completed successfully. Small LAMOST is composed of mirror with aperture of 3 meter(effective aperture of 2 meter), 250 fibers, one spectrograph, two 4kx4k CCD camera, tracking and controlling system. This paper presents the study in Small LAMOST. It comprises three main parts. First, it introduces the software design for the control system of Small LAMOST, including Mount tracking, Focal Plane tracking, GPS time ticking and time synchronization between computers, auto-guiding, etc. The design has proved correct and feasible. Second, it describes some technical solutions to the requirements of precision, real time and open architecture for Small LAMOST. Lastly, some experimental data and curves are given to show the tracking precision of Small LAMOST.
机译:此后,大型天空多目标光纤光谱望远镜LAMOST将于2008年建成,届时将成为世界上最大的视场和4 m口径望远镜最高效观察的天文望远镜。2007年6月,Small System LAMOST已成功完成。小型LAMOST由孔径为3米(有效孔径为2米)的反射镜,250根光纤,一台光谱仪,两台4kx4k CCD摄像机,跟踪和控制系统组成。本文介绍了Small LAMOST中的研究。它包括三个主要部分。首先,介绍了小型LAMOST控制系统的软件设计,包括坐骑跟踪,焦平面跟踪,GPS时间刻度和计算机之间的时间同步,自动导航等。该设计被证明是正确可行的。其次,它描述了一些针对小型LAMOST的精度,实时性和开放架构要求的技术解决方案。最后,给出了一些实验数据和曲线,表明了小型LAMOST的跟踪精度。

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