The vector equation of radiative transfer is solved both for conservative and non-conservative planetary atmospheres using the method of discrete ordinates. The atmosphere, bounded by a Lambert bottom, is considered plane-parallel: and homogeneous. The scattering in the atmosphere obeys the Rayleigh
โฆ LIBER โฆ
Polarization Models for Rayleigh Scattering Planetary Atmospheres
โ Scribed by Esther Buenzli; Hans M. Schmid; Franco Joos
- Book ID
- 106472313
- Publisher
- Springer Netherlands
- Year
- 2009
- Tongue
- English
- Weight
- 273 KB
- Volume
- 105
- Category
- Article
- ISSN
- 1573-0794
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