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Active Pixel Sensor Developments for Future ESA Space Science Missions

机译:未来ESA空间科学任务的活跃像素传感器开发

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Optical imaging sensors in space science payloads were, until now, exclusively based on CCDs due to their superior optical performance and existing successful heritage. However recent technological improvements within the CMOS world as well as the commercial market have led to Active Pixel Sensor (APS) designs offering an advantageous alternative to CCDs. Their high suitability as a detector for virtually every wavelength range of sensors promises a very significant gain in complexity, power and integration. They also offer the possibility of high radiation hardness and high - speed readout. These points have motivated the choice of APS technology for the imaging payloads of the ESA BepiColombo MPO (Mercury Planetary Orbiter). Other missions, such as Solar Orbiter, follow the same trend This paper gives an overview of the foreseen developments by ESA in that respect.
机译:在空间科学有效载荷中的光学成像传感器直到现在,由于其优越的光学性能和现有的成功遗产,专门基于CCD。然而,CMOS世界内的最近技术改进以及商业市场导致有源像素传感器(APS)设计,为CCD提供有利的替代品。它们作为探测器的高适度适用性,几乎每个波长范围的传感器都承担了复杂性,功率和集成的非常显着的增益。它们还提供高辐射硬度和高速读数的可能性。这些要点有动力选择APS技术,用于ESA Bepicolombo MPO(汞行星轨道)的成像有效载荷。其他特派团,如太阳能轨道,遵循相同的趋势本文概述了ESA在这方面的预见。

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