Sensitivity of model estimates of CME propagation and arrival time to inner boundary conditions

This release contains the scripts used to compute the result of the journal manuscript Sensitivity of model estimates of CME propagation and arrival time to inner boundary conditions by James et al. (2023). We make use of Python and Jupiter Notebook. The HUXt model (Owens et al., 2020) has been adapted to include tracking the CME nose elongation and lowering the inner boundary of the model. Using an ensemble technique, four experiments are computed to simulate the coronal mass ejection event from December 12th 2008. The ghost front theory (Scott et al., 2019) is used to assess the similarity between the time-elongation profiles of the model and observations through the STEREO/SECCHI HI1 field of view