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Multiple Instrument Distributed Aperture Sensor (MIDAS) Science Payload Concept

机译:多仪器分布式孔径传感器(MIDAS)科学有效载荷概念

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We describe the Multiple Instrument Distributed Aperture Sensor (MIDAS) concept, an innovative approach to future planetary science mission remote sensing that enables order of magnitude increased science return. MIDAS provides a large-aperture, wide-field, diffraction-limited telescope at a fraction of the cost, mass and volume of conventional space telescopes, by integrating advanced optical interferometry technologies. All telescope optical assemblies are integrated into MIDAS as the primary remote sensing science payload, thereby reducing the cost, resources, complexity. I&T and risks of a set of back-end science instruments (SI's) tailored to a specific mission. MIDAS interfaces to multiple science instruments, enabling sequential and concurrent functional modes, thereby expanding the potential planetary science return many fold. Passive imaging modes with MIDAS enable remote sensing at diffraction-limited resolution sequentially by each science instrument, or at lower resolution by multiple science instruments acting concurrently on the image, such as in different wavebands. Our MIDAS concept inherently provides nanometer-resolution hyperspectral passive imaging without the need for any moving parts in the science instruments. For planetary science missions, the MIDAS optical design provides high-resolution imaging for long dwell times at high altitudes, thereby enabling real-time, wide-area remote sensing of dynamic surface characteristics. In its active remote sensing modes, using an integrated solid-state laser source, MIDAS enables LIDAR, vibrometry, surface illumination, and various active or ablative spectroscopies. Our concept is scalable to apertures well over 10m, achieved by autonomous deployments or manned assembly in space. MIDAS is a proven candidate for future planetary science missions, enabled by our continued investments in focused MIDAS technology development areas. In this paper we present the opto-mechanical design for a 1.5m MIDAS point design, including its accommodation of back-end science instruments.
机译:我们描述了多仪器分布式孔径传感器(MIDAS)的概念,这是对未来行星科学任务遥感的一种创新方法,可以使数量级的科学回报得以提高。 MIDAS通过集成先进的光学干涉技术,提供了一种大口径,宽视场,衍射受限的望远镜,而成本,质量和体积却只有传统太空望远镜的一小部分。所有望远镜光学组件都作为主要的遥感科学有效负载集成到MIDAS中,从而降低了成本,资源和复杂性。 I&T和针对特定任务量身定制的一组后端科学仪器(SI)的风险。 MIDAS与多种科学仪器接口,支持顺序和并发的功能模式,从而将潜在的行星科学收益扩大了许多倍。使用MIDAS的无源成像模式可以通过每个科学仪器顺序以衍射极限分辨率进行遥感,或者通过同时作用在图像上(例如在不同的波段中)的多个科学仪器以较低的分辨率进行遥感。我们的MIDAS概念固有地提供了纳米分辨率的高光谱无源成像,而无需科学仪器中的任何移动部件。对于行星科学任务,MIDAS光学设计可在高海拔地区长时间停留时提供高分辨率成像,从而能够实时,大范围遥感动态表面特征。在其主动遥感模式下,MIDAS使用集成的固态激光源,可以进行激光雷达,振动测量,表面照明以及各种主动或烧蚀光谱学。通过自主部署或在太空中有人值守的装配,我们的概念可扩展到10m以上的光圈。由于我们在重点MIDAS技术开发领域的持续投资,MIDAS被证明是未来行星科学任务的可靠候选者。在本文中,我们介绍了1.5m MIDAS点设计的光机械设计,包括其后端科学仪器的容纳情况。

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