 This tutorial finally concludes our journey to simulate Rayleigh Scattering for a planet’s atmosphere. The next (and final) part will show how to change the shader to also include an additional type of scattering, known as Mie Scattering.

You can find all the post in this series here:

You can refer to the Atmospheric Scattering Cheatsheet for a complete reference of all the equations used.

You can download the Unity package for this tutorial at the bottom of the page.

# Intersecting The Atmosphere  You can find all the post in this series here:

You can refer to the Atmospheric Scattering Cheatsheet for a complete reference of all the equations used.

You can download the Unity package for this tutorial at the bottom of the page.

# A Shader for the Atmospheric Sphere  You can find all the post in this series here:

You can refer to the Atmospheric Scattering Cheatsheet for a complete reference of all the equations used.

You can download the Unity package for this tutorial at the bottom of the page.

# A Journey Through the Atmosphere This post describes how to model the density of the atmosphere at different altitude. This is a critical step, since the atmospheric density is one of the parameters necessary to correctly calculate the Rayleigh scattering. You can find all the post in this series here:

You can refer to the Atmospheric Scattering Cheatsheet for a complete reference of all the equations used.

You can download the Unity package for this tutorial at the bottom of the page.

# The Mathematics of Rayleigh Scattering This post introduces the Mathematics of Rayleigh Scattering, which is the optical phenomenon that causes the sky to appear blue. The equations derived in this tutorial will be translated into shader code in the next tutorial. You can find all the post in this series here:

You can refer to the Atmospheric Scattering Cheatsheet for a complete reference of all the equations used.

You can download the Unity package for this tutorial at the bottom of the page.

# The Theory Behind Atmospheric Scattering This is the second part of the tutorial on volumetric atmospheric scattering. In this post we will start deriving the equations that govern this complex, yet beautiful optical phenomenon. You can find all the post in this series here:

You can refer to the Atmospheric Scattering Cheatsheet for a complete reference of all the equations used.

You can download the Unity package for this tutorial at the bottom of the page.

# Volumetric Atmospheric Scattering If you have lived long enough on planet Earth, you might have wondered why the sky is usually blue, yet red at sunset. The optical phenomenon which is (mostly) responsible for that is called Rayleigh scattering. This tutorial will explain how to model atmospheric scattering to reproduce many of the visual effects that planets exhibit. And if you want to render physically accurate visuals for alien planets, this is definitely the tutorial you’ve been looking for. You can find all the post in this series here:

You can refer to the Atmospheric Scattering Cheatsheet for a complete reference of all the equations used.

You can download the Unity package for this tutorial at the bottom of the page.