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首页> 外文期刊>Journal of Geophysical Research. Biogeosciences >Mars Color Imager (MARCI) on the Mars Climate Orbiter
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Mars Color Imager (MARCI) on the Mars Climate Orbiter

机译:火星气候轨道仪上的火星彩色成像仪(MARCI)

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The Mars Color Imager, or MARCI, experiment on the Mars Climate Orbiter (MCO) consists of two cameras with unique optics and identical focal plane assemblies (FPAs), Data Acquisition System (DAS) electronics, and power supplies. Each camera is characterized by small physical size and mass (similar to6 X 6 X 12 cm, including baffle; < 500 g), low power requirements (< 2.5 W, including power supply losses), and high science performance (1000 X 1000 pixel, low noise). The Wide Angle (WA) camera will have the capability to map Mars in five visible and two ultraviolet spectral bands at a resolution of better than 8 km/pixel under the worst case downlink data rate. Under better downlink conditions the WA will provide kilometer-scale global maps of atmospheric phenomena such as clouds, hazes, dust storms, and the polar hood. Limb observations will provide additional detail on atmospheric structure at 1/3 scale-height resolution. The Medium Angle (MA) camera is designed to study selected areas of Mars at regional scale. From 400 km altitude its 6 degrees FOV, which covers similar to 40 km at 40 m/pixel, will permit all locations on the planet except the poles to be accessible for image acquisitions every two mapping cycles (roughly 52 sols). Eight spectral channels between 425 and 1000 nm provide the ability to discriminate both atmospheric and surface features on the basis of composition. The primary science objectives of MARCI are to (1) observe Martian atmospheric processes at synoptic scales and mesoscales, (2) study details of the interaction of the atmosphere with the surface at a variety of scales in both space and time, and (3) examine surface features characteristic of the evolution of the Martian climate over time. MARCI will directly address two of the three high-level goals of the Mars Surveyor Program: Climate and Resources. Life, the third goal, will be addressed indirectly through the environmental factors associated with the other two goals. [References: 81]
机译:火星气候成像仪(MCO)上的火星彩色成像仪(MARCI)由两个具有独特光学特性和相同焦平面组件(FPA)的相机,数据采集系统(DAS)电子设备和电源组成。每台相机的特点是体积小,重量轻(大约6 X 6 X 12厘米,包括挡板; <500克),低功耗要求(<2.5 W,包括电源损耗)和高科学性能(1000 X 1000像素) , 低噪声)。在最坏情况下的下行链路数据速率下,广角(WA)摄像机将能够在五个可见光谱带和两个紫外光谱带中绘制火星图,分辨率优于8 km /像素。在更好的下行链路条件下,西澳州将提供千米级别的大气现象的全球地图,例如云,霾,沙尘暴和极地罩。肢体观测将以1/3比例高度的分辨率提供有关大气结构的更多细节。中角(MA)相机旨在研究区域规模的火星选定区域。从400 km的高度开始,其6度FOV(以40 m /像素的速度覆盖约40 km)将允许地球上除极点之外的所有位置每两个映射周期(大约52溶胶)可用于图像采集。 425至1000 nm之间的八个光谱通道可根据成分区分大气特征和表面特征。 MARCI的主要科学目标是(1)在天气尺度和中尺度观测火星大气过程,(2)在各种时空尺度上研究大气与地面相互作用的细节,以及(3)研究火星气候随时间演变的地表特征。 MARCI将直接解决火星测量师计划的三个高级目标中的两个:气候和资源。生活是第三个目标,将通过与其他两个目标相关的环境因素来间接解决。 [参考:81]

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