First high-resolution coordinated observations of an active region with Solar Orbiter and DKIST | Krzysztof Barczynski
Physical Meteorological Observatory in Davos / World Radiation Centre (PMOD/WRC), Switzerland
Natural Sciences (Astrophysics and Astrononmy)
Active regions are the most dynamic structures in the solar disk. They contain numerous substructures with wide orders of sizes and lifetimes. The evolution of an active region with different time scales, the role of the small-scale structures in the active region, the mechanism triggering the transient phenomena, and the mechanism responsible for the plasma upflow at the active region border are still open issues. The main aim of the project is to focus on these open issues using high-resolution observation of the solar atmosphere obtained from different vantage points. The active region was observed during coordinated observations with Solar Orbiter and Daniel K. Inouye Solar Telescope (DKIST) on 18-21 October and 24 October 2022. Read more at https://espos.stream/2023/11/16/Barczynski/.
Link to the European Solar Physics Online Seminars (ESPOS) webpage:
If the video contains inappropriate content, please report
the video. You will be redirected to the landing page.