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Methods for ray-tracing thermal modelling of Saturn's main rings
The thermal emission and temperatures of the main rings of Saturn depend on the energy the ring particles absorb, reflect and scatter and/or on their Bond albedo, emissivity, thermal inertia, rotation rate and porosity. However, the energy that each particle absorbs also depends on the amount of ene...
| Autores principales: | , |
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| Formato: | Online Artículo Texto |
| Lenguaje: | English |
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Elsevier
2021
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| Acceso en línea: | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC8374635/ https://www.ncbi.nlm.nih.gov/pubmed/34430338 http://dx.doi.org/10.1016/j.mex.2021.101457 |