Solar Flare Prediction
The importance of Space Weather forecasting is rapidly increasing because of the impact solar eruptions may have on the entire (near-)terrestrial environment and the rising sensitivity of our technosphere. Our aim is to develope a flare intensity and onset time prediction tool that is substantially more precise than those currently available. Most flare and CME forecast methods are applied on the solar surface, however they occur in the solar atmosphere. Therefore, in our project, we apply and critically assess a new measure for predicting eruptive non-potentiality in solar active regions by utilising 3D magnetic mapping across the solar atmosphere. To achieve a leap forward, here, we generalise our forecasting methods by applying them through the solar atmosphere in order to determine an optimum height range in the lower solar atmosphere for predicting flares and CMEs.