MIRO的分子激发和辐射传递模型

2009 IEEE Aerospace conference Pub Date : 2009-03-07 DOI:10.1109/AERO.2009.4839628

P. von Allmen, Seungwon Lee, L. Kamp, S. Gulkis

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引用次数: 0

摘要

我们实现并验证了分子云辐射传输模型，并研究了67P/Churyumov-Gerasimenko彗星的水发射线。结果表明，水发射谱线的光谱分布取决于彗发的物理性质。该工具将用于解释MIRO的观测结果，并将帮助建立彗星的流体动力学模型。

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Molecular excitation and radiative transfer model for MIRO

We have implemented and validated a model for the radiative transfer in molecular clouds and studied the water emission line for Comet 67P/Churyumov-Gerasimenko. Results are reported that show that the spectral profiles for water emission lines depend on the physical properties of the coma. This tool will be used to interpret observations by MIRO and will help build hydrodynamics models of comets.

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2009 IEEE Aerospace conference

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