Speaker
Marco Stangalini
(ASI Agenzia Spaziale Italiana)
Description
Over the past few years, multi-line spectropolarimetry has revolutionized diagnostic capabilities, enabling the accurate identification of MHD modes in diverse structures and assessing their contributions to the energy budget of the solar atmosphere. In this presentation, I will illustrate the potential of these diagnostic techniques through the analysis of several illustrative cases. Furthermore, I will explore the synergistic application of these techniques with simplified models. In conclusion, I will outline several potential enhancements that can be driven by next-generation solar instrumentation.
| Sessions | Novel diagnostic techniques and forward modelling |
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Author
Marco Stangalini
(ASI Agenzia Spaziale Italiana)
