The basic topics to be addressed at the Symposium are as follows:
- Differently scaled solar convection and magnetoconvection and models of stellar convection will be the subject of a first session.
- A second session will be devoted to the theory of solar and stellar differential rotation and meridional circulation in parallel with relevant observational data.
- Solar and stellar global dynamos will be discussed at a third session along with solar-cycle observational patterns and predictions.
- The helioseismological inversions describing the rotational-velocity distribution in the solar interior and also asteroseismology will, together with local helioseismology, be a subject of a fourth session.
- A consideration of local active processes such as observed patterns of active-region development, magnetic-flux emergence, local dynamo, small-scale motions, sunspot and starspot formation, etc., is planned to be on the agenda of a fifth session.
- Additionally, a section dedicated to Miscellaneous subjects will be held.
Here, the Final Programme of the Symposium (of 14 August 2023) can be viewed and downloaded.
Here, the Book of Abstracts can be viewed and downloaded.