With the Swedish Solar Telescope on La Palma we can see amazing details (shown by Luc last week): bright points, sheets, ribbons, flowers, micro-pores. These solar features are correlated with the magnetic field. Using 3D Magnetoconvection simulations I will show how these features get their appearance and what they tell us about the Solar photosphere.
Mats Carlsson: "Modelling Solar Magnetoconvection"
Fredagskollokvium
Abstract.
Publisert 12. aug. 2009 11:40
- Sist endret 15. juni 2011 13:48