Performance of compact multilayer coated telescopes at soft x-ray/EUV and far ultraviolet wavelengths
Performance of compact multilayer coated telescopes at soft x-ray/EUV and far ultraviolet wavelengths
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DOI：
10.1117/12.55728
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发表时间：
1990-10
影响因子：
1.3
通讯作者：
R. Hoover;T. Barbee;P. Baker;J. Lindblom;M. J. Allen;C. Forrest;C. Kankelborg;R. H. O'Neal;Elizabeth S. Paris;A. Walker
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文献类型：
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作者：
R. Hoover;T. Barbee;P. Baker;J. Lindblom;M. J. Allen;C. Forrest;C. Kankelborg;R. H. O'Neal;Elizabeth S. Paris;A. Walker
我们已经开发了紧凑的软X射线/EUV（XUV）和远紫外（FUV）多层镀膜望远镜的研究太阳色球日冕，日冕/太阳风界面。因为它们工作在短波长（~40 <？< 1550 A），40至127 mm的适度孔径允许以非常高的角分辨率（0.1至0.7 arcsec）进行观测。除了允许传统的垂直入射光学配置，如卡塞格伦，里奇-克雷蒂安，赫歇尔在XUV波长使用，多层膜还允许窄波长带（？~30至100），以选择用于成像。由此产生的望远镜为研究色球/日冕界面的精细结构和日冕及日冕/太阳风界面的大尺度结构提供了一种非常强大和灵活的诊断仪器。在以前的论文中，我们描述了一种新的太阳火箭有效载荷，多光谱太阳望远镜阵列（MSSTA），由17个紧凑型望远镜组成。在本文中，我们报告的七个MSSTA里奇-克雷蒂安望远镜的性能。
We have developed compact soft x-ray/EUV (XUV) and farultraviolet (FUV) multilayer coated telescopes for the study of the solar chromosphere corona, and corona/solar wind interface. Because they operate at short wavelengths (~40 < ? < 1550 A), the modest apertures of 40 to 127 mm allow observations at very high angular resolution (0.1 to 0.7 arcsec). In addition to permitting traditional normal incidence optical configurations such as Cassegrain, Ritchey-Chretien, and Herschelian to be used at XUV wavelengths, multilayer coatings also allow a narrow wavelength band (?/?? ~30 to 100) to be selected for imaging. The resuIting telescopes provide a very powerful and flexible diagnostic instrument for the study of both the fine scale structure of the chromosphere/ corona interface and the large scale structure of the corona and corona/ solar wind interface. In previous papers we described a new solar rocket payload, the Multi-Spectral Solar Telescope Array (MSSTA), composed of 17 of these compact telescopes. In this paper we report on the performance of the seven MSSTA Ritchey-Chretien telescopes.