R. Johnson , P. Bernath , B. Billinghurst , J. Zhao
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引用次数: 0
摘要
需要氮和甲烷的碰撞诱导吸收(CIA)光谱来模拟土星卫星土卫六等天体大气中的辐射传递。我们展示了氮和甲烷在 40-600 cm-1 范围内的罕见、极低温傅立叶变换红外光谱旋转诱导吸收(CIA)。我们发现甲烷在 123.8 K 时的峰值 CIA 为 2.05×10-5 cm-1/amagat2 ,而氮气在 102.5 K 的平均温度下的峰值为 1.65×10-5 cm-1/amagat2 。
Collision induced absorption spectra of N2 and CH4
Collision-induced absorption (CIA) spectra of nitrogen and methane are needed to model radiative transfer in atmospheres of objects such as Saturn's moon, Titan. We present rare, extremely low temperature Fourier transform infrared spectra of nitrogen and methane rototranslation CIA in the range of 40–600 cm−1. The peak CIA of methane was found to be 2.05×10−5 cm−1/amagat2 at 123.8 K while nitrogen had a peak value of 1.65×10−5 cm−1/amagat2 at an average temperature of 102.5 K. These measurements were made possible by the unique instrumentation available at the Far-IR beamline at the Canadian Light Source.
期刊介绍:
Papers with the following subject areas are suitable for publication in the Journal of Quantitative Spectroscopy and Radiative Transfer:
- Theoretical and experimental aspects of the spectra of atoms, molecules, ions, and plasmas.
- Spectral lineshape studies including models and computational algorithms.
- Atmospheric spectroscopy.
- Theoretical and experimental aspects of light scattering.
- Application of light scattering in particle characterization and remote sensing.
- Application of light scattering in biological sciences and medicine.
- Radiative transfer in absorbing, emitting, and scattering media.
- Radiative transfer in stochastic media.