GREAT太赫兹外差光谱仪对地球中间层和热层原子氧的观测

H. Richter, C. Buchbender, R. Güsten, R. Higgins, B. Klein, J. Stutzki, H. Wiesemeyer, H. Hübers
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引用次数: 1

摘要

原子氧控制着地球中间层和低层热层的光化学和能量平衡。它的浓度极难用遥感技术测量,因为它只有很少的光学活性跃迁。目前的间接测量涉及光化学模型,结果并不总是一致的,特别是当用不同的仪器获得时。此外,这些方法不包括100公里以上的高度。我们报告了在4.7448太赫兹处原子氧的4.7太赫兹精细结构跃迁的直接测量,使用了平流层红外天文观测台上的德国太赫兹天文接收机。我们的测量结果与大气模式和100公里以下的卫星观测结果吻合得很好。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Observation of Atomic Oxygen in the Mesosphere and Thermosphere of Earth with the THz Heterodyne Spectrometer GREAT
Atomic oxygen governs photochemistry and energy balance of the mesosphere and lower thermosphere of the Earth. Its concentration is extremely difficult to measure with remote sensing techniques since it has only few optically active transitions. Current indirect measurements involve photochemical models and the results are not always in agreement, particularly when obtained with different instruments. In addition, altitudes above 100 km are not covered by these methods. We report on direct measurements of the 4.7-THz fine-structure transition of atomic oxygen at 4.7448 THz using the German Receiver for Astronomy at Terahertz Frequencies on board the Stratospheric Observatory for Infrared Astronomy. Our measurements agree well with atmospheric models and satellite observations below 100 km.
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