Models and data combined to progress towards a better understanding of the magnetism of solar-type stars
681 views
03.09.2015
Affiliation
IRAP Toulouse / France
Main category
Natural Sciences (Astrophysics and Astrononmy)
Abstract
We will review recent progress made in modeling solar-type stars in 2D and 3D in the recent years. In particular, we will focus on advances in our understanding of the dynamo processes in such astrophysical objects and the necessary ingredients to reproduce what is found in the observations. We will also present recent attempts to introduce such observational data into multi-D MHD models. The idea is to implement data assimilation techniques to solar physics in order to have some tools to give tentative predictions of future solar activity.
Further information
Further reading
Language
DOI
Conference
Do you have problems viewing the pdf-file? Download presentation here
If the presentation contains inappropriate content, please report the presentation. You will be redirected to the landing page.