NASA NTRS · 20060041730
A Statistical Study of CME Plasma Flows
Abstract
Many studies of the interplanetary manifestations of coronal mass ejections (CMEs) have focused on the shock driver gas or on the regions that display a flux-rope magnetic topology. Somewhat less attention has been paid to investigating how the solar wind returns to its ambient, pre-CME condition.
Explore related subjects
Keep this discovery
Explore connections, maps & timelines
Goldstein, R., Neugebauer, M., Clay, D.. 1997-11-01. A Statistical Study of CME Plasma Flows. https://ntrs.nasa.gov/citations/20060041730
Cite the original work for its findings. Save a collection to share your selection of sources.