The solar corona - a hot topic

The corona is a halo of hot plasma that forms the sun's outer atmosphere. The temperature of the corona is several hundred times higher than the surface of the sun. How this is possible is one of the most hotly debated questions in astrophysics.

Like in a cooking pot, plasma rises from the interior of the sun, cools down and sinks back down again. In the process, the plasma streams intertwine and twist the solar magnetic field, which also penetrates the solar atmosphere and thus supplies energy to the corona. However, this process is not fully understood. In my talk, I will
discuss how we study coronal heating using astronomical observations and supercomputers.

Speaker: Dr. Cosima Breu, School of Mathematics and Statistics, University of St. Andrews

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Advance sales for this event have ended. Tickets are now available at the box office. The box office opens one hour before the start of the event.

Where does the event happen? Planetarium „Stellarium Erkrath“
Bürgerhaus Erkrath - Eingang West
Sedentaler Straße 105
40699, Erkrath

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