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A high stability multi-CCD focal plane for ESA imaging missions

机译:用于ESA成像任务的高稳定性多CCD焦平面

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摘要

Results are described from a high-stability multi-CCD demonstration focal plane assembly developed by MSSL under ESA contract, using new large-format CCD42-C0s from e2v technologies. Space-based planetary-transit hunting and asteroseismology missions such as ESA's Eddington and NASA's Kepler require large multi-CCD focal planes with a stringent requirement on stability, both thermal and electronic. Other significant requirements are wide dynamic range and a moderately high readout rate of ~1.2 Mpix s~(-1) per output (in this case using a 16 bit CCD signal processor ASIC from CCLRC RAL). The high digital data rate (Eddington has in total ~3 focal planes each with 12 output chains) is achieved using SpaceWire links. The demo-FPA is flight-representative in terms of performance, mass, power and component selection. This work provides real-world data for future ESA studies. It is also compatible with the Gaia radial velocity spectrometer (RVS) focal plane, which has many similar requirements.
机译:由MSSL根据ESA合同开发的高稳定性多CCD演示焦平面组件(使用e2v技术的新型大幅面CCD42-C0s)描述了结果。诸如ESA的Eddington和NASA的Kepler之类的天基行星运输狩猎和星震学任务需要大型的多CCD焦平面,对热和电子的稳定性都有严格的要求。其他重要要求还包括宽动态范围和每个输出约1.2 Mpix s(-1)的较高读出率(在这种情况下,使用CCLRC RAL的16位CCD信号处理器ASIC)。使用SpaceWire链接可以实现较高的数字数据速率(爱丁顿总共有约3个焦平面,每个焦平面都有12条输出链)。演示FPA在性能,质量,功率和组件选择方面具有飞行代表性。这项工作为将来的ESA研究提供了真实的数据。它也与Gaia径向速度谱仪(RVS)焦平面兼容,后者具有许多相似的要求。

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