Coronal Mass Ejections
Abstract
Nature and Structure of Coronal Mass Ejections Specific Examples Pre-Ejection "Swelling" of the Coronal Helmet Streamer Formation and Outward Propagation of the Mass Ejection Post-Ejection Depletion of the Helmet Streamer Region Pre-Eruption Evolution of the Prominence and Corona The Mass Ejection and Prominence Eruption The Post-Ejection Corona Summary Some Measured Properties Shape or Geometry Angular Size Locations The Propagation of Mass Ejections Through the Corona The Origin of Coronal Mass Ejections Some Essential Facts Large Spatial Scales Occurrence in (and Disruption of) Closed Magnetic Structures, - Including Those not Related to Active Regions The Huge Variability in the Phenomenon Mass Ejections and Prominence Eruptions Mass Ejections and "Optical" Solar Flares Mass Ejections and Soft X-Ray Flares Formation (and Acceleration) of a Mass Ejection Within the - SMM Field of View Formation (and Initial Acceleration) of a Mass Ejection in - the Low Corona Association with an X-Ray Flare That Rises from a Very Low - Background Level in the GOES Data A Major Coronal Mass Ejection with no Detectable X-Ray Flare What, Then, is the Origin of Coronal Mass Ejection? Summary
- Publication:
-
The many faces of the sun: a summary of the results from NASA's Solar Maximum Mission.
- Pub Date:
- 1999
- Bibcode:
- 1999mfs..conf..143H