ERC Consolidator Grant · 2016
Unravelling The Structure and Evolution of Solar Magnetic Flux Ropes and Their Magnetosheaths
Coronal Mass Ejections (CMEs) are spectacular stellar eruptions that carry huge amounts of plasma and magnetic flux into the space. The interests in their origin, structure, and dynamics reach from fundamental plasma physics to paramount impact on their parent stars and the surrounding planets. One of the most outstanding problems in the studies of CMEs is the lack of reliable information on their magnetic field properties until observed directly. This severely limits our understanding of many aspects in the lifespan of CMEs and their far-reaching consequences. SolMAG will deliver realistic and detailed information of the magnetic fields in CMEs. We will further use this knowledge to obtain…
From the public funding record at EU CORDIS. Describes the funded project, not the reviews below.