Speaker
Sarah Gibson
(NCAR/HAO)
Description
The PUNCH mission provides new and unprecedented observations of the outer corona and inner heliosphere. However, much of the early evolution that ultimately defines the quiescent solar wind and global transients such as coronal mass ejections (CMEs) takes place in the inner corona where Metis observes, below PUNCH's field of view of approximately 6-180 solar radii. In this talk, I will first overview PUNCH current status and recent results, and than discuss synergies with Metis observations and paths for future collaboration.
Author
Sarah Gibson
(NCAR/HAO)
Co-author
Craig DeForest
