Updated the tutorials

nichollsh · Sep 16, 2024 · f082a1d · f082a1d
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diff --git a/docs/paper/paper.md b/docs/paper/paper.md
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 It is important that we are able to accurately model the atmospheres of (exo)planets. This is because their atmospheres play a crucial role in setting the environment and conditions on the planet, including how the planet evolves over astronomical timescales. Additionally, it is primarily by observation of their atmospheres that we are able to characterise exoplanets. There is demand for accurate atmosphere models in the context of lava worlds: planets with permanent or fleeting magma oceans.
 
-AGNI[^1] is a Julia program designed to solve for the temperature and radiation environment within the atmospheres of rocky (exo)planets. It leverages a well established FORTRAN code to calculate radiative fluxes from a given atmospheric temperature structure and composition, which -- alongside representations of convection and other processes -- enables an energy-conserving numerical solution for the atmospheric conditions. In contrast to most other numerical atmosphere codes, AGNI uses an Newton-Raphson optimisation method to obtain this solution which enables improved performance and scalability. AGNI was specifically developed for use alongside planetary interior models within a coupled framework, although it can also be easily applied to scientific problems as a standalone code. It can be interacted with as a library, or as an executable which reads configuration files.
+AGNI[^1] is a Julia program designed to solve for the temperature and radiation environment within the atmospheres of rocky (exo)planets. It leverages a well established FORTRAN code to calculate radiative fluxes from a given atmospheric temperature structure and composition, which -- alongside representations of convection and other processes -- enables an energy-conserving numerical solution for the atmospheric conditions. In contrast to most other numerical atmosphere codes, AGNI uses an Newton-Raphson optimisation method to obtain this solution which enables improved performance and scalability. AGNI was specifically developed for use alongside planetary interior models within a coupled framework, although it can also be easily applied to scientific problems as a standalone code. It can be interacted with as a library, or as an executable which reads configuration files. There are notebook tutorials in the repository, and the documentation can be read online [here](https://nichollsh.github.io/AGNI/).
 
 [^1]: AGNI can be found on GitHub [here](https://github.com/nichollsh/AGNI).
 

diff --git a/tutorials/01_canonical-runaway.ipynb b/tutorials/01_canonical-runaway.ipynb
diff --git a/tutorials/02_convergence.ipynb b/tutorials/02_convergence.ipynb