Dynamic Sun II: Solar magnetism from interior to the corona
Abstract
The “Dynamics Sun II” conference will address the role of the solar magnetism for the variety of dynamical plasma processes which are responsible for the energy transport from the interior of the Sun to the outer layers of the solar atmosphere. Also, an additional session devoted to the Sun-driven magnetospheric dynamics will be included. The main focus of the Dynamic Sun II meeting will be to discuss in detail the recent achievements in understanding photospheric, chromospheric and coronal dynamics, energy transport between the lower and upper layers of solar interior and the solar atmosphere, dynamical processes in the confined solar transients. Special attention will be paid to the key results and goals of the current and proposed space and ground-based instruments. These topics are also aligned with the long-term goals of current and proposed space/solar missions. This meeting will be also useful for future scientific data interpretation from forthcoming new generation ground-based instruments, e.g., the Daniel K. Inouye Solar Telescope (DKIST, USA), European Solar Telescope (EST, Europe), new Indian facilities (MAST, upcoming 2m-NLST, Aditya-I) and more recently CHROMIS (located alongside CRISP at the Swedish 1-m Solar Telescope), which will be able to significantly advance scientific understanding of our solar-terrestrial environment.
Document Details
- Document Type
- DoD Grant Award
- Publication Date
- Apr 09, 2018
- Source ID
- FA23861811009
Entities
People
- Viktor Fedun
Organizations
- Air Force Office of Scientific Research
- United States Air Force
- University of Sheffield Department of Psychology