Speaker
Ulrich von Kusserow
(AG, DPG)
Description
According to current findings, the self-organized creation and development of our solar system took place under the diverse influence of magnetic (e. g. dynamo, reconnection, accretion, acceleration) processes. In the context of magnetohydrodynamics, these will be discussed initially at a glance and exemplarily for protostellar systems (protostars, protostellar/protoplanetary disks and winds as well as protoplanets), then specially for the young solar system itself.
Primary author
Ulrich von Kusserow
(AG, DPG)
