Solar physics  

LEARNING OUTCOMES You will learn about the history of formation of the Sun and its future evolution. You will understand the processes of energy production and transfer in the Sun; the structure of the solar atmosphere, corona and solar wind; the generation and evolution of solar magnetic fields; and the physics behind the solar cycle, solar seismology, and solar storms. You will learn about current and past solar space missions as well as ground observatories and will apply your knowledge to study various aspects of the Sun using real data. CONTENT Formation of the Sun and the solar system, future evolution of the Sun. Standard solar model. Solar atmosphere. Solar oscillations and helioseismology. Convection. Solar rotation. Solar dynamo and solar cycle. Chromosphere and solar corona. Solar wind. Solar storms and eruptions.
Presential
English
Solar physics
English

Funded by the European Union. Views and opinions expressed are however those of the author(s) only and do not necessarily reflect those of the European Union or HaDEA. Neither the European Union nor the granting authority can be held responsible for them. The statements made herein do not necessarily have the consent or agreement of the ASTRAIOS Consortium. These represent the opinion and findings of the author(s).