Age | Commit message (Collapse) | Author | |
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2020-01-09 | Calculate Rayleigh coefficients using Nishita and Hillaire | Adrian Kummerlaender | |
i.e. plugging the values for n and N given in [1, Sec. 3.3] into eqs. (1) resp. (3) given by [2]. [1]: Hillaire. “Physically Based Sky, Atmosphere and Cloud Rendering in Frostbite” [2]: Nishita et. al. “Display of the Earth Taking into Account Atmospheric Scattering” | |||
2020-01-09 | Fix exposure value in bluedot example | Adrian Kummerlaender | |
2020-01-03 | Improve structure, play around with phase functions | Adrian Kummerlaender | |
2019-12-19 | Basic sky rendering using the model by Nishita et al. | Adrian Kummerlaender | |
See "Display of the earth taking into account atmospheric scattering" (Nishita et al., 1993) `bluedot.py` renders the full earth disk while rotating the sun around it. `sunrise.py` renders the rise of the sun. Physical model constants may be changed in `planets.py`. |