S. de Wet
Articles written in Journal of Astrophysics and Astronomy
Volume 29 Issue 1-2 March 2008 pp 207-210
We apply the ring diagram technique to source regions of halo coronal mass ejections (CMEs) to study changes in acoustic mode parameters before, during, and after the onset of CMEs.We find that CME regions associated with a low value of magnetic flux have line widths smaller than the quiet regions, implying a longer life-time for the oscillation modes. We suggest that this criterion may be used to forecast the active regions which may trigger CMEs.
Volume 40 | Issue 6
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