摘要: The observed spectrum of Jovian atmosphere exhibits spectral features of H2, CH4, C2H6, NH3, H2O, GeH4 and CH3D. Analytical programs were developed for radiative transfer calculations and for retrieval of lower atmospheric composi... 展开
作者 | Abbas, M. M. | ||
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原报告号 | N8514779 | 总页数 | 3 |
报告类别/文献类型 | NASA / NTIS科技报告 | ||
关键词 | Atmospheric composition Jupiter atmosphere Emission spectra Infrared spectra Voyager project Computer programs Data reduction Inversions Mathematical models Michelson interferometers Radiative transfer |