Response of the solar atmosphere to the photospheric plasma motion

Authors
Dr.
Jörg Büchner
Date and time
10 Nov 2009 - 23:00 Europe/London
Address

Aula

Talk language
English
Slides language
English
Serie number
0
Description
The dynamics of the solar atmosphere is largely controlled by its magnetic coupling to the photosphere of the Sun. Since the solar magnetic field is complex, numerical simulation must be utilized to investigate the coupling processes. Results will be shown of treating this way the two unresolved issues - the heating of the corona and the acceleration of the solar wind.