Helioseismic Ring Analysis of CME Source Regions

Details Helioseismic Ring Analysis of CME Source Regions Helioseismic Ring Analysis of CME Source Regions

2007-12-12

arxiv.org/abs/0712.1995v1

J. Astrophys. Astr., 2008, 29,207

Astronomy and Astrophysics

Astrophysics

Accepted for publication in J. Astrophys. Astr. Also available at http://www2.nso.edu/staff/sushant/paper.html

Scientific paper

10.1007/s12036-008-0026-x

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.

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