外观
论文arXiv 2607.135619 天前
AIMS 微服务架构主控系统的设计与实现
原文链接：Design and Implementation of a Microservice-Architecture Master Control System for AIMS（arXiv 2607.13561 · 发布日期：2026-10-19）
Design and Implementation of a Microservice-Architecture Master Control System for AIMS
面向 AIMS 高自主观测需求，论文设计微服务主控系统，并在三台望远镜不同自动化等级上验证稳定性。
核心要点
- 问题源于 AIMS 高海拔远程站址、异构多机构部件和复杂观测模式。
- 方法提出 L0–L5 自动化分类、三层系统框架和微服务软件架构。
- 关键技术包括自动指向跟踪、自动对焦，以及环境自适应观测。
- 系统已在 AIMS、WenQuan 和 SFMM 三台望远镜上验证可行性与稳定性。
验证范围与局限：验证范围为三台地基太阳望远镜，自动化等级分别覆盖 L1、L2 和 L3。
英文摘要 (Abstract)
Abstract The mid-infrared solar magnetic field telescope AIMS (An Infrared System for the Accurate Measurement of Solar Magnetic Field) is the first ground-based telescope designed to directly measure solar magnetic fields via Zeeman splitting in the 8–14 μm band, overcoming the century-long bottleneck of model-dependent indirect measurements. Its remote high-altitude site, heterogeneous multi-institute components, and complex observation modes comprising Fourier Transform Infrared (FTIR) spectropolarimetry and broadband imaging demand a highly autonomous Master Control System (MCS). We present the design and implementation of the AIMS MCS, featuring three key contributions: (1) a novel L0–L5 telescope automation classification inspired by the SAE J3016 autonomous driving standard, providing clear boundaries and a progressive evolution roadmap; (2) a three-layer system framework—device control, autonomy support, and central decision—implemented with a microservice software architecture that achieves loose coupling, high cohesion, and continuous integration of heterogeneous components; and (3) a suite of key enabling technologies including automatic pointing/tracking, autofocus via lucky-frame selection combined with power spectral ratio analysis, and environment-adaptive observation integrating auto-exposure, cloud detection, and power/thermal monitoring. The MCS has been validated across three telescopes at progressive automation levels: AIMS itself (L1, stable operation >2 years since April 2024), the WenQuan Solar Magnetic Field Telescope (L2, stable operation >3 years since February 2023), and the Solar Full-disk Multi-layer Magnetograph SFMM (L3, continuous autonomous operation >2.5 years since October 2023). Collectively, these deployments underscore the feasibility and stability of the proposed architecture, establishing a robust and scalable foundation for the next generation of embodied intelligent telescopes.
作者：Li-Yue Tong, Jia-Ben Lin, Jun-Feng Hou
来源
本页事实对应的公开页面，以原文为准。