用部分频率重分布模拟行星大气中的H2荧光
Modeling H2 Fluorescence in Planetary Atmospheres with Partial Frequency Redistribution
摘要：
介绍了氢分子荧光发射谱线部分频率再分布（PRD）效应的模拟、一般计算近似及其在行星大气和星际介质中的应用。我们的模型适用于FUSE观测木星，土星和反射星云，允许独立确认的H2丰度和行星大气的结构。
英文摘要：
We present the modeling of partial frequency redistribution (PRD) effects for the fluorescent emission lines of molecular hydrogen, the general computational approximations, and the applications to planetary atmospheres, as well as interstellar medium. Our model is applied to FUSE observations of Jupiter, Saturn, and reflection nebulae, allowing an independent confirmation of the H2 abundance and the structure of planetary atmospheres.
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