diff --git a/MANIFEST.in b/MANIFEST.in index a6d94b3..83fe26d 100644 --- a/MANIFEST.in +++ b/MANIFEST.in @@ -1,8 +1,3 @@ include README.md include LICENCE -include requirements.txt -include docs/vevoda_2022_infrared_sky_teaser.png -include docs/docs/prague_sky.png -include docs/analytical_sky.png -include docs/uniform_sky.png -include docs/gui-1.png \ No newline at end of file +include requirements.txt \ No newline at end of file diff --git a/README.md b/README.md index e2c9ae1..33a136d 100644 --- a/README.md +++ b/README.md @@ -1,6 +1,6 @@ # The skylight project ![GitHub top language](https://img.shields.io/github/languages/top/evgkanias/sky) [![GitHub license](https://img.shields.io/github/license/evgkanias/sky)](https://github.com/evgkanias/sky/blob/main/LICENSE) ![GitHub last-commit](https://img.shields.io/github/last-commit/evgkanias/sky) ![Build Status](https://app.travis-ci.com/evgkanias/sky.svg?branch=main) -![vevoda_2022_teaser](docs/vevoda_2022_infrared_sky_teaser.png) +![vevoda-2022-teaser](https://raw.githubusercontent.com/evgkanias/sky/a3eb1e695daeca79d8e4c82b281208745a8f24ad/docs/vevoda_2022_infrared_sky_teaser.png) This Python package implements three models that provide skylight information. @@ -9,7 +9,7 @@ This Python package implements three models that provide skylight information. This model (proposed by [VĂ©voda P. et al., 2022](https://cgg.mff.cuni.cz/publications/infrared-skymodel-2022/); original C++ code [here](https://cgg.mff.cuni.cz/wp-content/uploads/2022/09/vevoda_2022_infrared_sky_implementation.zip)) interpolates the skylight properties by using stored data for a range of parameters, and it does not include data for the angle of polarisation (this is calculated by using the analytical solution). -![prague-sky-model](docs/prague_sky.png) +![prague-sky-model](https://raw.githubusercontent.com/evgkanias/sky/a3eb1e695daeca79d8e4c82b281208745a8f24ad/docs/prague_sky.png) There are three available datasets that work with the Prague Sky Model, which can be downloaded form here: * [Google Drive with the near-infrared (SWIR) dataset](https://drive.google.com/file/d/1ZOizQCN6tH39JEwyX8KvAj7WEdX-EqJl/view?usp=sharing) @@ -25,14 +25,14 @@ This model (proposed by [Wilkie A. et al., 2004](http://dx.doi.org/10.2312/EGWR/ [Preetham A. J. et al., 1999](https://dl.acm.org/doi/pdf/10.1145/311535.311545)) includes radiance and polarisation information. -![analytic-sky-model](docs/analytical_sky.png) +![analytic-sky-model](https://raw.githubusercontent.com/evgkanias/sky/a3eb1e695daeca79d8e4c82b281208745a8f24ad/docs/analytical_sky.png) ### 3. Uniform model This model provides the same information for any sky conditions and viewing directions, and it could be used as a baseline model. -![uniform-sky-model](docs/uniform_sky.png) +![uniform-sky-model](https://raw.githubusercontent.com/evgkanias/sky/a3eb1e695daeca79d8e4c82b281208745a8f24ad/docs/uniform_sky.png) ## Installation @@ -80,7 +80,7 @@ If you prefer to use a graphical user interface for this package, there is a sep use. This is named the [sky-gui](https://github.com/evgkanias/sky-gui) and it allows for interactive exploration of the skylight properties for the different models. However, in this version, only the Prague Sky Model is supported. -![gui-teaser](docs/gui-1.png) +![gui-teaser](https://raw.githubusercontent.com/evgkanias/sky/a3eb1e695daeca79d8e4c82b281208745a8f24ad/docs/gui-1.png) ## Report an issue