Spectroscopic observation of planetary and Moon exospheres in the ultraviolet

M. Pelizzo, M. Padovani, A. Corso, G. Santi, M. Uslenghi, D. Faccini, M. Fiorini, S. Incorvaia, G. Toso, E. Fabbrica, M. Carminati, C. Fiorini, G. Favaro, M. Bazzan, G. Maggioni, G. Naletto, V. Andretta, A. Milillo
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引用次数: 1

Abstract

The planetary extreme ultraviolet spectrometer (PLUS) is a project funded by the Italian Space Agency focused on the development of an extreme (EUV) and far-ultraviolet (FUV) high-performance spectrograph, which adopts a dual channel optical scheme. Thanks to an optimized layout based on the use of variable line space (VLS) gratings in an off-Rowland configuration, high spectral and spatial resolution are achieved. The efficiency improvement is obtained by the optimization of the coatings on the optical components. Improved detection limit, shorter observations integration time and unprecedented performance in terms of dynamic range will be achieved by the use of high resolution/dynamic range solar blind photon counting detectors. The photon counting detectors will be based on a micro-channel plate (MCP) coupled with an application specific integrated circuit (ASIC) read out system.
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行星和月球外逸层的紫外光谱观测
行星极紫外光谱仪(PLUS)是由意大利航天局资助的一个项目,重点开发极(EUV)和远紫外(FUV)高性能光谱仪,采用双通道光学方案。由于基于在off-Rowland配置中使用可变线空间(VLS)光栅的优化布局,实现了高光谱和空间分辨率。通过对光学元件表面涂层的优化,实现了效率的提高。高分辨率/动态范围太阳盲光子计数探测器将提高探测极限,缩短观测积分时间,并在动态范围方面实现前所未有的性能。光子计数探测器将基于微通道板(MCP)和专用集成电路(ASIC)读出系统。
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