Design and application of an autonomous Master Control System for a multi-layer magnetic and helioseismic telescope
作者机构:National Astronomical ObservatoriesChinese Academy of SciencesBeijing 100101China Key Laboratory of Solar Activity and Space WeatherNational Space Science CenterChinese Academy of SciencesBeijing 100190China School of Astronomy and Space ScienceUniversity of Chinese Academy of SciencesBeijing 100049China School of Electrical and Electronic EngineeringWuhan Polytechnic UniversityWuhan 430023China
出 版 物:《Astronomical Techniques and Instruments》 (天文技术与仪器(英文))
年 卷 期:2024年第1卷第3期
页 面:187-196页
学科分类:07[理学] 070401[理学-天体物理] 0704[理学-天文学]
基 金:supported by the National Key R&D Program of China (2022YFF0503800) the Chinese Meridian Project,the National Natural Science Foundation of China (11427901) the Strategic Priority Research Program of the Chinese Academy of Sciences (XDA15320102) the Youth Innovation Promotion Association (2022057)
主 题:Astronomical instrumentation Telescopes Solar optical telescopes Automated telescopes
摘 要:With the growing significance of space weather forecasting,multi-layer magnetic and helioseismic telescopes are emerging as a key area of ***,owing to the diverse operational processes and sophisticated hardware configurations of these devices,there is an urgent need for efficient autonomous observation *** autonomous Master Control System(MCS)can ensure efficient performance,data consistency,and stability,and the prototype presented here adopts a microservices architecture,breaking down the hardware into multiple subsystems and converting their functions into individual services.A central decision-making system leads the operations,supported by three auxiliary systems and three device control *** inter-subsystem service calls,it achieves rapid imaging and spectroscopic *** verify system stability and observation efficiency,the system was tested on the Solar Full-disk Multi-layer *** results verify this system can operate automatically for 4 consecutive months,acquire photospheric vector magnetic and Doppler velocity fields within a 15-minute interval,and measure chromospheric longitudinal magnetic and Doppler velocity fields in under 180 *** ensures consistent and stable solar monitoring and serves as a practical methodological benchmark for the development of similar devices.