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Development of infrared imaging devices for the observation of planetary atmosphere

Development of infrared imaging devices for the observation of planetary atmosphere
开发用于观测行星大气的红外成像装置
批准号:
13440142
负责人:
NAKAMURA Masato
金额:
$9.6万
依托单位国家:
日本
项目类别:
Grant-in-Aid for Scientific Research (B)
财政年份:
2001
资助国家:
日本
项目状态:
已结题
起止时间:
2001 至 2002

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项目成果

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中文摘要
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英文摘要
The motion of the atmosphere of Venus at the altitude of less than 70km has not been studied because it is prevented by the thick cloud layer. But it became possible to observe the motion of lower clouds and surface of Venus after infrared ray turned out to pass through the thick cloud layer. We aimed at the observation of the motion of the atmosphere using Venusian clouds and surface as tracers by the infrared camera in the spacecraft orbiting around Venus. This approach will be the first one in the world.In this study, we developed the imaging device and optical system for infrared camera which can be used in the exploration of Venus and also future exploration of another planet. It is especially important to develop the imaging device and optical system in two bands, near-infrared region (1-3μm) and mid-infrared region (8-12μm). The former corresponds to the emission from the bottom of clouds (at the altitude of 50-70km), which enables us to observe the motion of the atmosphere. On the contrary, the latter corresponds to the thermal radiation from the top of clouds. As a result, it turned out to be best to use PtSi Schottky device in near infrared region and bolometer array in mid-infrared region as radioresistant imaging device. Schottky device needs to be cooled to 60K, and one stage Stirling cooler proved to be able to accomplish it.This research is relatively close to the development of infrared observation spacecraft in astronomical field. In this field, the technology which reduces a thermal noise to the minimum by cooling the infrared device has been improved for the observation of far, dark stars or young planetary system. But, if it is installed to planetary exploration spacecraft, it will be prolonged exposure to the radiation and also the much harsher heat condition than ground-based astronomical observations. In this time, the development of the infrared device suitable for the planetary orbiter was needed, and it was sufficiently achieved.
期刊论文(36)
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会议论文
M. Nakamura, and T. Imamura: "Japanese Venus atmospheric mission"Yuseijin. 10(3). (2001)
M. Nakamura 和 T. Imamura:“日本金星大气任务”Yuseijin。
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通讯作者:
T. Imamura, and G. L Hashimoto: "Microphysics of Venusian clouds in rising tropical air."J. Atmos. Sci. 58. 3597-3612 (2001)
T. Imamura 和 G. L Hashimoto:“热带空气上升中金星云的微观物理学”。
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松田佳久, 今村剛: "金星大気の謎にせまる日本の金星探査計画"科学. 71(9). 1162-1164 (2001)
Yoshihisa Matsuda,Tsuyoshi Imamura:“日本的金星探索计划接近金星大气层的奥秘”,《科学》71(9) 1162-1164 (2001)。
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通讯作者:
Y. Matsuda, and T. Imamura: "Revealing the mystery of Venusian atmosphere by Japanese Venus mission"Kagaku. 71(9). (2001)
Y. Matsuda 和 T. Imamura:“日本金星任务揭示金星大气层之谜” Kagaku。
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