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High-Resolution Camera on AXAF

机译:关于演讲的高分辨率

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The high resolution camera (HRC) will be one of the two focal plane instruments on the Advanced X-ray Astrophysics Facility, (AXAF). AXAF is a major NASA space observatory and is scheduled for launch in 1998. AXAF will perform high resolution spectrometry and imaging in the x-ray band of 0.1 to 10 keV. The HRC instrument consists of two detectors, the HRC-I for imaging and the HRC-S for spectroscopy. Each HRC detector consists of chevron pairs of microchannel plates (MCPs) and a crossed grid charge readout. Spatial resolutions of the HRC detectors are less than 25 micrometer (less than 0.5'). The HRC-I is a 100 by 100 mm detector primarily for imaging, the HRC-S is an approximately 30 by 300 mm detector which is optimized to function as the readout for the low energy transmission grating spectrometer (LETGS). The development of the HRC is a collaborative effort between the Smithsonian Astrophysical Observatory, University of Leicester UK and the Osservatorio Astronomico, G.S. Vaiana, Palermo Italy. In this paper we present the most recent design, development and testing of the HRC instrument.
机译:高分辨率相机(HRC)将是先进X射线天体物理学设施(AXAF)的两个焦平面仪器之一。 Axaf是一个主要的美国航空航天局空间天文台,并于1998年计划推出.AxAF将在0.1至10keV的X射线带中进行高分辨率光谱和成像。 HRC仪器由两个检测器组成,用于成像的HRC-I和用于光谱的HRC-S。每个HRC探测器由Chevron对的微通道板(MCP)和交叉网格电荷读数组成。 HRC探测器的空间分辨率小于25微米(小于0.5')。 HRC-I主要是100 mm的探测器,主要用于成像,HRC-S是大约30乘300mm检测器,该检测器被优化,以用作低能量传输光栅光谱仪(左闲)的读出。 HRC的发展是史密森天体物理天文台,莱斯特大学英国和奥斯特·奥里诺天文学,G.S.Vaiana,巴勒莫意大利的努力努力。在本文中,我们提供了HRC仪器的最新设计,开发和测试。

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