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Optical MEMS in space instruments for Earth observation and astronomy

机译:地球观测和天文学空间仪器中的光学模型

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Optical MEMS could be major candidates for designing future generation of space instruments. In addition to their compactness, scalability, and specific task customization, they could generate new functions not available with current technologies. We have listed new functions associated with several types of MEMS. Instrumental applications are derived and we propose two promising concepts using object selection and spectral tailoring techniques. In Earth Observation instruments, observation of scenes including bright sources leads to an important degradation of the recorded signal. We propose a new concept to remove dynamically the bright sources and obtain a field of view (FOV) with an optically enhanced SNR. Our concept consists in replacing the plain slit in classical designs by an active row of MOEMS. Experimental demonstration of this concept has been conducted on a dedicated bench: a scene with a contiguous bright area has been focused on a micromirror array and imaged on a CCD detector. After the programmable slit, the straylight issued from the bright zone is polluting the scene; the micromirrors located on the bright area are switched off, removing almost completely the straylight in the instrument. In Astronomy and Earth Observation, we propose an innovative reconfigurable instrument: a programmable wide-field spectrograph where both the FOV and the spectrum could be tailored thanks to a 2D micromirror array. The FOV is linear and each point spectrum could be modified dynamically along the second direction. A demonstrator has been designed and its realization is under way for testing the unique performances of this instrument.
机译:光学模型可能是设计未来产生空间乐器的主要候选者。除了紧凑,可伸缩性和特定的任务定制外,它们还可以生成当前技术无法提供的新功能。我们列出了与多种类型的MEMS关联的新功能。推导出乐器应用程序,我们使用对象选择和光谱定制技术提出了两个有希望的概念。在地球观测仪器中,观察包括明亮源的场景导致记录信号的重要降解。我们提出了一个新概念,以动态地删除明亮的源,并使用光学增强的SNR获取视野(FOV)。我们的概念由一行的MoEm替换古典设计中的普通狭缝。该概念的实验演示已经在专用的替补席上进行:具有连续明亮区域的场景,已经专注于微镜阵列并在CCD检测器上成像。在可编程狭缝之后,从亮区发出的跨线灯具污染了场景;位于明亮区域上的微镜被关闭,几乎完全拆下仪器中的梯形灯。在天文和地球观测中,我们提出了一种创新的可重构仪器:可编程宽场光谱仪,其中FOV和光谱都可以根据2D微镜阵列定制。 FOV是线性的,并且可以沿第二方向动态地修改每个点频谱。设计了一个示威者,并正在进行测试该仪器的独特性能。

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