Solar Origins of Interplanetary Shocks
L.K. Harra
Solar-B will provide unprecedented detail of the changes in the solar
atmosphere leading up to the eruption
of coronal mass ejections. The SOT will provide measurements of flows
and shear in the photospheric magnetic field,
XRT will provide high resolution full Sun images to track global
responses, and EIS will provide measurements of
flows and dynamics in the solar atmosphere. I will discuss the recent
observations made with the array of space and ground-based
observations currently available on the sources of coronal mass
ejections, and will discuss how Solar-B will be able to push
forward our understanding of these dramatic events.
Correspondence
Louise Harra (lkh@mssl.ucl.ac.uk), UCL-MSSL
presentation
invited