|COOKIES: By using this website you agree that we can place Google Analytics Cookies on your device for performance monitoring.|
Quiescent prominence fine structure modelling
If you have a question about this talk, please contact Dr. Jaroslav Dudik.
Unprecedented amount of detailed, high-resolution observations of prominence fine structures provided by present space-borne and ground-based observatories represents a significant challenge for prominence modelling. Today’s models have to cope with the increasingly finer dimensions and ever better resolved dynamics of the observed fine structures. However, the increasing complexity of the prominence fine structure models opens new opportunities for deepening our understanding of these spectacular solar features.
Currently, prominence fine structure modelling stands on three main pillars: simulations of prominence magnetic field configurations, modelling of radiative transfer in the prominence plasma, and modelling of prominence fine structure dynamics. We will review the state-of-the-art and achievements of the present models and show the capabilities of the new generation of prominence fine structure models, combining the prominence magnetic field simulations with realistic representation of the prominence plasma and radiative transfer computations.
This talk is part of the Informal Lunch Seminars in AFD series.
This talk is included in these lists:
Note that ex-directory lists are not shown.
Other lists2030 vision for the Cambridge sub-region Algebraic Geometry Seminar Cambridge Fly Meetings
Other talksThe physician's Stammbuch: humanist cultures of medical networking Interindividual variation of brain and cognition The waxing and waning of PIMMS: experimental but not computational support for prediction error driving episodic memory CGHR Research Group Rothschild Lecture: The Hawaiian Plume: What do Surface Observables Tell Us? Dr Pia Kvistborg: What T cells see on human cancer