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

机译:天文学级科学,具有低成本的EUV天文使命

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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 ~170-260? 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:对资金机构的各种需求使得难以维持提供资金天文学任务的支出所需的支出水平,即研究社区希望能够提供。多亿多亿/美元观察者这样的混乱,XMM-牛顿和HST都是非常成功的,但JWST已经淘汰了,并为同等的大型X射线任务计划似乎是持有的。此外,中等大小ESA Andnasa任务在未来十年内仅提供少数机会。默认情况下,默认情况下,非常令人兴奋和科属生物。如果卫星使命成本可能会显着减少,因此5-10倍,我们会打开任何机构目前不提供的新参数空间。仪器技术的重要内容加上了光学系统的简化和高效的发展,高性能小卫星平台和地面系统导致了一些低成本的展望的前景。在本文中,我们概述了一种基于成功的探测火箭般的火箭般的起重机。这包括高通量正常入射极端紫外光光谱仪,该设计适用于SSTL 300平台上的住宿。我们利用分段衍射光栅从〜170-260提供总波长覆盖率?通过将各个元素的多层调谐到不同的重叠范围。我们概述了使命的能力和科学目标,以及它们如何影响卫星平台的设计和操作。我们结束了讨论这种类型的特派团如何运行作为星座和散发稀疏孔径,可以为未来的单一的“伟大的观测所”提供科学上可行的替代品。©(2012)照片光学仪表工程师的版权协会(SPIE)。仅供个人使用的摘要下载。

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