'Dynamic Sun' is a conference series, which provides a highly visible platform to the observers, theoreticians,
numerical modellers and instrumentation experts in the fields of solar and stellar physics and space science to
discuss cutting edge scientific challenges. The first and
second Dynamic Sun meetings focused on solar magnetism and
MHD wave phenomena in the solar atmosphere and took place in 2016 in Varanasi, India and 2018 in Angkor Wat, Cambodia.|
The Dynamic Sun III meeting will follow up on the success of the first two. The focus of the Dynamic Sun III meeting will be to discuss in detail the recent achievements and future research related to the multi-wavelength solar and stellar observations. Special attention will be paid to the solar-stellar connection and the key results and goals of the current and proposed space and ground-based instruments.
This meeting will also be useful for future scientific data interpretation from a new generation instruments, e.g., the Daniel K. Inouye Solar Telescope (DKIST), Solar Orbiter, European Solar Telescope (EST), Atacama Large Millimeter/Submillimeter Array (ALMA), Solar Parker Probe, VLT, SKA. In particular, a session will be devoted to Solar and Stellar ALMA results.
We warmly welcome participation of internationally recognised experts in the fields of solar and stellar physics, early career researchers and PhD students. Dynamic Sun III will help to establish long-term relationships between research groups.
The conference will cover the following scientific themes: