Coronal Mass Ejections (CMEs), sporadic eruptions of magnetized plasma from the Sun, present a significant concern for society’s reliance on space-based infrastructure. Our study uniquely delves into the evolution of thermodynamic properties of CMEs, a facet often less understood due to both remote and in-situ observational limitations. This seminar will briefly discuss the used analytical model (FRIS: Flux Rope Internal State) and the model-derived distance-dependent evolution of various internal parameters at coronal heights where thermodynamic measurements have been challenging. Read more at https://espos.stream/2024/02/22/Khuntia/.
Further information
Further reading
Link to the European Solar Physics Online Seminars (ESPOS) webpage:
https://espos.stream/2024/02/22/Khuntia/
