53,760 research outputs found
Seismic investigation of the solar structure using GONG frequencies
Using the recently obtained GONG frequencies, we investigate the properties
of the solar interior by constructing solar models with various input physics
like opacities, equation of state, nuclear reaction rates etc. The differential
asymptotic inversion technique is then used to infer the relative difference in
sound speed between the Sun and solar models. Here we apply these results to
test equation of state and different formulation for calculating the convective
flux.Comment: Latex, 2 pages, 3 figures, To appear in the IAU Symp. # 181:
"Sounding solar and stellar interiors", eds. F.X. Schmider & J. Provos
Helioseismic Ring Analysis of CME Source Regions
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.Comment: Accepted for publication in J. Astrophys. Astr. Also available at
http://www2.nso.edu/staff/sushant/paper.htm
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