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Observatory-class science with a low-cost EUV astronomy mission

机译:具有低成本EUV天文学任务的天文台科学

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The various demands on funding agencies make it difficult to sustain the level of expenditure required to provide thebroad range of space astronomy missions that the research community would like to have available. Multi-billionpound/dollar observatories such Chandra, XMM-Newton and HST have been enormously successful, but JWST has beendelayed and plans for an equivalent large X-ray mission seem to be on-hold. Furthermore, the medium size ESA andNASA missions provide only a small number of opportunities over the next decade. Much exciting and importantscience, by default, will not be done. If satellite mission costs could be reduced significantly, by a factor of 5-10, wewould open up a new parameter space of opportunity that is not currently offered by any agency. Significantimprovement in instrument technology coupled with simplification of optical systems and the development of efficient,high performance small satellite platforms and ground systems has led to the prospect of the development of some low-costopportunities. In this paper, we outline one such possible mission, based on a successful sounding rocket-bornepayload. This comprises a high throughput normal incidence extreme ultraviolet spectrometer, with the design adaptedfor accommodation on the SSTL 300 platform. We make use of a segmented diffraction grating to provide an overallwavelength coverage from ~170-260Å by tuning the multi-layers of the individual elements to different, overlappingranges. We outline the capability and science goals of the mission, and how they influence the design and operation ofthe satellite platform. We conclude with a discussion of how missions of this type operating both as constellations andas formation flying sparse apertures, could offer a scientifically viable alternative to monolothic 'great observatory'missions in the future.© (2012) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
机译:对资助机构的各种要求使其难以维持研究界希望提供的范围广泛的空间天文学任务所需的支出水平。钱德拉(Chandra),XMM-牛顿(Newton)和HST等数十亿磅/美元的天文台已经取得了巨大的成功,但是JWST已被推迟,并且类似的大型X射线任务计划也被搁置了。此外,在未来十年中,中等规模的ESA和NASA任务仅提供少量机会。默认情况下,许多激动人心且重要的科学将无法完成。如果卫星任务成本可以大幅度降低5到10倍,我们将开辟一个新的参数机会空间,而这是任何机构目前都无法提供的。仪器技术的显着进步,加上光学系统的简化以及高效,高性能的小型卫星平台和地面系统的发展,带来了一些低等机会的发展前景。在本文中,我们以成功探测火箭运载的有效载荷为基础,概述了一种可能的任务。这包括一个高通量法向入射极紫外光谱仪,其设计适用于SSTL 300平台。我们使用分段衍射光栅,通过将各个元素的多层调整为不同的重叠范围,以提供约170-260Å的总波长覆盖范围。我们概述了任务的能力和科学目标,以及它们如何影响卫星平台的设计和运行。最后,我们讨论了这种类型的任务,无论是作为星座还是作为飞行稀疏孔径的编队,都可以在将来提供科学上可行的替代单峰“大天文台”任务的方法。©(2012)COPYRIGHT光电仪器工程师协会(SPIE)。摘要的下载仅允许个人使用。

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