论文标题
Tor Vergata Symartic太阳能望远镜（TSST）的光学设计
Optical design of the Tor vergata Synoptic Solar Telescope (TSST)
论文作者
论文摘要
天气全盘太阳能望远镜是目前和未来太阳能物理和太空天气的基本工具。它们通常用于研究和监测太阳能通过在不同波长下使用高的时间节奏观测值。 TSST（Tor Vergata Synoptic太阳能望远镜）是一种新的Synoptic望远镜，由两个光谱通道组成：A h $α$α$（656.3 nm）望远镜和一个基于Potassium（KI D1）吸收光谱线的基于Magneto Optical Filter（MOF）基于望远镜的望远镜。 H $α$观测对于识别燃烧区域至关重要。基于MOF的望远镜将产生太阳光球的视线图和多普勒格拉姆，它们分别用于研究活性区域中磁场的几何形状和太阳气氛的动力学。在这项工作中，我们介绍了基于MOF的望远镜的TSST以及光学设计和特性，其光学方案是带有无像差成像透镜的双杀伤力80mm折射器。
Synoptic full-disk solar telescope are fundamental instruments for present and future Solar Physics and Space Weather. They are typically used to study and monitor the solar activity by using high temporal cadence observations at different wavelength. The TSST (Tor vergata Synoptic Solar Telescope) is a new synoptic telescope composed of two spectral channels: an H$α$ (656.3 nm) telescope and a Magneto Optical Filter (MOF)-based telescope in the Potassium (KI D1) absorption spectral line at 769.9 nm. H$α$ observations are fundamental for the identification of flaring regions. The MOF-based telescope will produce line of sight magnetograms and dopplergrams of the solar photosphere, which are respectively used to study the magnetic field's geometry in active regions and dynamics of the solar atmosphere. In this work, we present an overview on the TSST and the optical design and characteristics of the MOF-based telescope, whose optical scheme is a double-Keplerian 80mm refractor with an aberration-free imaging lens.
