对xmm -牛顿光学监测器暴露在木星光线下的影响的研究

S Sullivan, M J Page, A A Breeveld, S Rosen, A Talavera
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引用次数: 0

摘要

经过近18年的成功和安全运行,2017年7月17日和18日,xmm -牛顿的光学监测器(OM)在其视觉(V)滤镜中观测到木星——一个比安全亮度限制亮10等的物体。物体从名义EPIC pn轴向负Y方向暴露40角秒,产生一个耗尽灵敏度的补丁。在V型滤镜中两次曝光,每次曝光4000秒,在70 × 40弧秒的区域内灵敏度下降;在V滤光器中,吞吐量的下降幅度从34%到UV波段的15%不等,但在平场曝光中,下降幅度达到45%。波长依赖性表明,探测器的大部分损坏是由于离子反馈造成的光电阴极的灵敏度损失,而高达15%的损坏可能是由于MCP的增益耗尽。讨论了造成探测器损坏的物理机制,以及未来OM运行可能存在的解决方案和机会。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
An investigation into the effect of exposing XMM-Newton’s Optical Monitor to the light of Jupiter
Abstract After nearly 18 years of successful and safe operations, on 2017 July 17th and 18th XMM-Newton’s Optical Monitor (OM) observed Jupiter – an object 10 magnitudes brighter than safe brightness limits – in it’s Visual (V) filter. The object was exposed 40 arc seconds from the nominal EPIC pn boresight in the negative Y direction, creating a patch of depleted sensitivity. Two exposures of 4000s each in the V filter left the sensitivity depleted in an area 70 by 40 arcsec; with the decrease in throughput varying from 34 per cent in the V filter to 15 per cent in the UV bands, but reaching a depth of 45 per cent in flat field exposures. The wavelength dependency suggests the majority of the detector damage is due to loss of sensitivity in the photocathode from damage inflicted by ion feedback, while up to 15 per cent could be due to gain depletion of the MCP. The physical mechanisms causing the damage to the detector are discussed as well as possible solutions and opportunities that exist for the future operation of the OM.
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