The effect of data-driving and relaxation models on magnetic flux rope evolution and stability
Context. Understanding the flux rope eruptivity and effects of data driving in modelling solar
eruptions is crucial for correctly applying different models and interpreting their results. Aims …
eruptions is crucial for correctly applying different models and interpreting their results. Aims …
Sunspots Identification Through Mathematical Morphology: The Method
The implementation of automated methods for sunspot detection is essential to obtain better
objectivity, efficiency, and accuracy in identifying sunspots and analysing their …
objectivity, efficiency, and accuracy in identifying sunspots and analysing their …
Solar magnetic flux rope identification with GUITAR: GUI for Tracking and Analysing flux Ropes
Modelling the early evolution of magnetic flux ropes (MFRs) in the solar atmosphere is
crucial for understanding their destabilization and eruption mechanism. Identifying the …
crucial for understanding their destabilization and eruption mechanism. Identifying the …