What is FlareLab Project
A contribution of the basic understanding of magnetic activity of the sun surface is one of the main itentions of this project. Especially the phenomenon of the coronal mass ejection (CME) is under examination. An important role for this are playing magnetic flux ropes, which can storage magnetic energie, because they are twisted. This energy can be released eruptive, which could be oberved from the SOHO satellite.
At the FlareLab project we are creating and analysing magnetic flux tubes, in the experiment and in the simulation. This project is based on the work of J.F. Hansen and P.M. Bellan (2001). The solar models of T. Toeroek and B. Kliem (2003) and as well of V.S. Titov and P. Demoulin (1999) are used for interpretation.