Radial Evolution of Well-Observed Slow CMEs intheDistance Range 2-30 R ()
We performed a detailed analysis of 27 slow coronal mass ejections (CMEs) whose heights were measured in at least 30 coronagraphic images and were characterized by a high quality index (.4). Our primary aim was to study the radial evolution of these CMEs and their properties in the range 2-30 solar...
Gespeichert in:
Veröffentlicht in: | Solar physics 2009-07, Vol.257 (2), p.351-361 |
---|---|
Hauptverfasser: | , , , |
Format: | Artikel |
Sprache: | eng |
Online-Zugang: | Volltext |
Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
Schreiben Sie den ersten Kommentar!