Azimuthal C/O Variations in a Planet-Forming Disk

<p><strong>DALI physical-chemical disk models presented in &#39;Azimuthal C/O Variations in a Planet-Forming Disk&#39; (Keyte et al. 2023).</strong></p> <p>There are two individual models included here. The &#39;baseline&#39; model is used to produce outputs for the region of the disk where C/O=0.5. The &#39;elevated&#39; model is used to produce outputs for the regions of the disk where C/O=1.5.</p> <p>The baseline model can be run in the normal way, but the outputs themselves are already included in the folder.</p> <p>The &#39;elevated&#39; model will not run in the regular way. The source code has been edited so that it can take in the abundances from a previous run as the starting point for the chemistry (in the form of an <em>out.dat</em> style table). The outputs are already included, but should you want to rerun the model yourself, follow the steps in the readme file within the folder.</p> <p>The final &#39;composite&#39; model presented in the paper is created by splicing together the outputs (as described in Keyte et al. 2023). This is achieved using a custom Python script, please contact me if you would like to use this.</p>