WSM3 Questions

How has the corona evolved since WSM1?

How do the plasma properties in coronal streamers and holes compare between WSM1 and WSM3?
How has the coronal large scale field changed since WSM1?

How stable are coronal structures over the WSM3 rotation?

How do coronal streamers change over the WSM3 rotation?
How do active regions change over the WSM3 rotation?
How does the coronal field change over the WSM3 rotation?

How do CMEs reshape the corona?

How is the lower corona connected to the upper corona?

How is the photospheric field connected to the coronal field?
How do active regions affect coronal streamers?
Where are streamer and coronal hole boundaries in the lower corona?
Where is it hot?
Where do we see velocity?

How is the corona connected to the solar wind?

How does a more dynamic corona affect structural connections between the corona and in situ?
Can we connect magnetic clouds to their sources during WSM3?

This list of questions reads somewhat like a wish list for most of solar physics. This should not be surprising, considering that the purpose of the Whole Sun Month campaigns is to encourage observers and theoriticians to work on the problems which most interest them, but looking at the same global corona. For this reason our list of questions is by no means complete or exclusive.