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Collision-Induced Absorption of H_2 Pairs in the High Frequency Wing of the Rototranslational Spectrum

机译:旋转转换谱的高频翼碰撞诱导的H_2对吸收

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摘要

The spectra of hydrogen in the 5 μm window of Jupiter have been recorded at temperatures of 297.5 and 77.5 K for gas densities ranging from 51 to 610 amagats. The binary absorption coefficient has been determined by extrapolation to zero density of the measured profiles. These extrapolated measurements are compared with calculations from the extended Birnbaum-Cohen model which represents the existing quantum profiles with full accuracy. Within the experimental errors, which are rather larger at low temperature, the agreement is satisfactory at room as well as low temperature.
机译:Jupiter的5μm窗口中氢气的光谱已经在297.5和77.5k的温度下记录,用于从51到610安​​格塔格的气体密度。二元吸收系数已经通过外推至测量型材的零密度来确定。将这些外推测量与来自延伸的Birnbaum-Cohen模型的计算进行了比较,该模型表示具有完全精度的现有量子谱。在低温下相当较大的实验误差中,该协议在房间以及低温下令人满意。

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