Sep 6 – 10, 2021
Europe/Rome timezone


Poster Session 1.1

Sep 6, 2021, 10:45 AM



Poster Session 1.1

  • Etienne Pariat (LESIA, Observatoire de Paris)

Presentation materials

Dr Bernadett Belucz (1) Solar Physics and Space Plasma Research Centre, School of Mathematics and Statistics, University of Sheffield, Hicks Building, Hounsfield Road Sheffield, S3 7RH, UK, 2)Department of Astronomy, Eötvös Loránd University, 1/A Pázmány Péter sétány, H-1117, Budapest, Hungary, 3)Gyula Bay Zoltań Solar Observatory (GSO), Hungarian Solar Physics Foundation (HSPF), Petőfi tér 3., Gyula, H-5700, Hungary)
9/6/21, 11:37 AM
Session 1 - Solar Interior, Dynamo, Large-Scale Flows and the Solar Cycle

In various classes of dynamo models, spot-producing magnetic fields are generated as axisymmetric toroidal flux-ropes. While mean-field models produce axisymmetric broad toroidal fields, full 3D convective models produce axisymmetric toroidal wreaths. All these models can reproduce various longitude-averaged features, such as solar-like butterfly diagrams. In recent simulations, we show that...

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