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Submillimeter Limb-emission Sounder JEM/SMILES aboard the Space Station

机译:太空站上的亚毫米肢体发声仪JEM / SMILES

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A submillimeter limb-emission sounder, that is to be aboard the Japanese Experiment Module (JEM, dubbed as "KIBO") at the International Space Station, has been designed. This payload, Superconducting Submillimeter-wave Limb-emission Sounder (SMILES), is aimed at global mappings of stratospheric trace gases by means of the most sensitive submillimeter receiver ever operated in space. Such sensitivity is ascribed to a Superconductor-Insulator-Superconductor (SIS) mixer, which is operated at 4.5K in a dedicated cryostat combined with a mechanical cooler. SMITES will observe ozone-depletion-related molecules such as ClO, HCl, HO_2, HNO_3, BrO and O_3 in the frequency bands at 624.32-626.32GHz and 649.12-650.32GHz. A scanning antenna will cover tangent altitudes from 10 to 60km in every 53 seconds, while tracing the latitudes from 38S to 65N along its orbit. This global coverage makes SMILES a useful tool of observing the low- and mid-latitudinal areas as well as the Arctic peripheral region. The molecular emissions will be detected by two units of acousto-optic spectrometers (AOS), each of which has coverage of 1.2GHz with a resolution of 1.8MHz. This high-resolution spectroscopy will allow us to detect weak emission lines attributing to less-abundant species.
机译:在国际空间站的日本实验模块(JEM,被称为“ KIBO”)上,设计了一种亚毫米级的肢体发射测深仪。这种有效载荷,即超导亚毫米波肢体探测仪(SMILES),旨在通过有史以来在太空中运行的最敏感的亚毫米波接收机,对平流层痕量气体进行全球测绘。这种敏感性归因于超导体-绝缘体-超导体(SIS)混合器,该混合器在与机械冷却器结合的专用低温恒温器中以4.5K运行。 SMITES将在624.32-626.32GHz和649.12-650.32GHz频段观察与臭氧消耗有关的分子,例如ClO,HCl,HO_2,HNO_3,BrO和O_3。扫描天线每53秒将覆盖10至60 km的切线高度,同时沿其轨道追踪38S至65N的纬度。 SMILES的全球覆盖范围使它成为观察低纬度和中纬度地区以及北极外围地区的有用工具。分子发射将由两个单位的声光光谱仪(AOS)检测,每个光谱仪的覆盖范围为1.2GHz,分辨率为1.8MHz。这种高分辨率的光谱学将使我们能够检测出归因于数量较少的物种的弱发射线。

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