11–22 Jan 2010
Nordita seminar room
Europe/Stockholm timezone

Video recordings can be found on the individual pages for each talk. Just scroll down on the list of Nordita events.

The objective of the School is to provide training for PhD students working in magnetohydrodynamics in general, and in astrophysical dynamos, the geodynamo, and laboratory dynamos in particular. A proper understanding of dynamos has become mandatory in many fields of research. Solar activity with its 11 year cycle is just one example where we are still lacking a theoretically consistent model in spite of the urgent need to predict the intensity of the next cycle. The latter is particularly critical is estimating the life time of artificial satellites in Earth orbit and hence the need for costly service missions. In the last 10 years major theoretical advances have led to a much deeper understanding of dynamos at large magnetic Reynolds numbers. In addition, three different laboratory experiments have now been successful in displaying dynamo action, broadening the range of phenomena that need to be understood theoretically.

Prerequisites

The students are expected to have basic training in theoretical physics including electrodynamics and vector calculus.

Confirmed teachers

Starts
Ends
Europe/Stockholm
Nordita seminar room
Roslagstullsbacken 23