The flare-CME relationship – determining factors (if any!) Sarah Matthews, Lucie Green, Hilary Magee, Louise Harra & Len Culhane MSSL, University College.
What can helicity redistribution in solar eruptions tell us about reconnection in these events? by Brian Welsch, JSPS Fellow (Short-Term ), Space Sciences.
Flux Collision Models of Prominence Formation
MHD simulations on eruption triggered by flux emergence
Confined X-class Flares vs. Eruptive ones Non-CME associated X-class Flares vs.
Lecture 4 The Formation and Evolution of CMEs. Coronal Mass Ejections (CMEs) Appear as loop like features that breakup helmet streamers in the corona.
Lecture 4 The Formation and Evolution of CMEs
On Coronal Mass Ejections and Configurations of the Ambient Magnetic Field
What can helicity redistribution in solar eruptions tell us about reconnection in these events?
