AbstractIt is common to use imaging instruments such as EUV and X-ray imagers and coronagraphs to study large-scale phenomena such as coronal mass ejections and coronal waves. Although high resolution spectroscopy is generally limited to a small field of view, its importance in understanding global phenomena should not be under-estimated. I will review current spectroscopic observations of large-scale dynamic phenomena such as global coronal waves and coronal mass ejections. The aim is to determine plasma parameters such as flows, temperatures and densities to obtain a physical understanding of these phenomena.
Spectroscopic observations of coronal waves and coronal mass ejections
Advances in Space Research ; 41 , 1 ; 138-143
2007-06-03
6 pages
Aufsatz (Zeitschrift)
Elektronische Ressource
Englisch
Spectroscopic observations of coronal waves and coronal mass ejections
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