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High-resolution telescope cluster I: overview and technical status

机译:高分辨率望远镜组I:概述和技术状态

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Abstract: High spatial resolution observations of the solar photosphere, chromosphere, and corona, at soft x-ray, EUV, and VUV wavelengths, are essential to the resolution of virtually every major problem pertaining to the structure and dynamics of the solar atmosphere. The Advanced Solar Observatory (ASO) is a proposed major NASA observatory that is planned to address a wide range of problems relating to the Sun. A major component of the ASO, the high resolution telescope cluster (HRTC) will be dedicated to high resolution studies of the atmosphere at soft x-ray, XUV, EUV, and VUV wavelengths. The HRTC will contain an array of telescopes that provide high resolution spectroheliograms in lines and continuum emitted over the full range of temperatures (approximately 4,500 K to 100,000,000 K) present in the outer solar atmosphere with angular resolution as high as on the order of magnitude 0.03 arc second. We analyze a model HRTC instrument complement consisting of the following instruments: (1) a 60 - 90 cm aperture vacuum-ultraviolet telescope covering the spectral range from $lambda$lambda 1200 - 3300 angstroms, (2) a 40 - 50 cm aperture EUV telescope covering the spectral range $lambda$lambda 450 - 1200 angstroms, (3) three 40 - 50 cm aperture XUV telescopes covering the spectral range $lambda$lambda 170 - 350 angstroms, (4) a 40 cm aperture soft x-ray telescope covering the spectral range $lambda$lambda 10 - 170 angstroms, (5) a 40 cm aperture x-ray telescope covering the spectral range $lambda$lambda 1.5 - 10 angstroms, (6) flare spectrometers and polarimeters covering the spectral range $lambda$lambda 0.001 - 1150 angstroms, and (7) four coronagraph/spectrographs able to image the corona to approximately 30 solar radii. We discuss the observational requirements which the HRTC must meet, the characteristics and anticipated performance of the HRTC model instruments, the technology necessary for their development, and various options for the deployment of HRTC. !73
机译:摘要:在软X射线,EUV和VUV波长下对太阳光球,色球层和日冕的高空间分辨率观测,对于解决几乎所有与太阳大气的结构和动力学有关的主要问题都是至关重要的。先进太阳天文台(ASO)是拟议中的主要NASA天文台,旨在解决与太阳有关的各种问题。高分辨率望远镜组(HRTC)是ASO的主要组成部分,将致力于在软X射线,XUV,EUV和VUV波长下对大气进行高分辨率研究。 HRTC将包含一系列望远镜,这些望远镜将在外部太阳大气中存在的整个温度范围(约4,500 K至100,000,000 K)内,以线和连续谱的形式提供高分辨率的光谱辐射图,其角分辨率高达0.03数量级。弧秒。我们分析了由以下仪器组成的模型HRTC仪器的补充:(1)60至90 cm孔径的真空紫外望远镜,其光谱范围从$ lambda $ lambda 1200-3300埃,(2)40至50 cm孔径的EUV覆盖光谱范围$ lambda $ lambda 450-1200埃的望远镜,(3)三个光谱范围$ lambda $ lambda 170-350埃XUV望远镜,(4)一个40 cm孔径的软X射线望远镜覆盖光谱范围$ lambda $ lambda 10-170埃,(5)覆盖光谱范围$ lambda $ lambda 1.5-10埃的40厘米孔径x射线望远镜,(6)覆盖光谱范围$ lambda的火炬光谱仪和旋光仪λ0.001至1150埃,以及(7)四个日冕仪/能谱仪,能够将日冕成像到大约30个太阳半径。我们讨论了HRTC必须满足的观测要求,HRTC模型仪器的特性和预期性能,其开发所必需的技术以及HRTC部署的各种选择。 !73

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