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DESIGN OF A GRAZING INCIDENCE EUV IMAGING SPECTROMETER FOR THE SOLAR ORBITER ESA MISSION

机译:太阳斜面ESA掠射入射EUV成像仪的设计

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The paper describes the optical design and performance of an extreme-ultraviolet (EUV) spectrometer for imaging spectroscopy to be part of the scientific payload of the Solar Orbiter (SOLO) mission. The main scientific objectives are to study the solar polar region and observe in detail the evolution of corona structures from a favourable point of view at only 45 solar radii from the Sun (0.2 AU). The instrument concept is based on a grazing incidence telescope, (1200 m focal length, 18 arcmin x 18 arcmin FoV), in Wolter configuration couple to a normalincidence VLS grating spectrometer, which preserve the stigmaticity in an extended spectral region and in the whole field-of-view. The spectral range covered by the instrument is the 116-126 nm region at the first order and the 57-63 nm region at the second order. The spectral resolving element is 65 m? (I order), corresponding to a velocity resolution of 16 km/s.
机译:本文介绍了用于成像光谱的极紫外(EUV)光谱仪的光学设计和性能,该光谱仪是太阳轨道飞行器(SOLO)任务的科学有效载荷的一部分。主要的科学目标是研究太阳极区,并从有利的观点出发,仅在太阳的45个太阳半径(0.2 AU)下详细观察日冕结构的演变。该仪器的概念基于掠入射望远镜(焦距为1200 m,FoV为18 arcmin x 18 arcmin FoV),在Wolter配置下与法向入射VLS光栅光谱仪结合使用,可在扩展的光谱区域和整个视野中保持图像散度-观点。仪器覆盖的光谱范围在第一阶为116-126 nm区域,在第二阶为57-63 nm区域。光谱解析元素为65 m? (I阶),对应于16 km / s的速度分辨率。

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