Physics
Scientific paper
Oct 2004
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004esasp.559..353b&link_type=abstract
"Proceedings of the SOHO 14 / GONG 2004 Workshop (ESA SP-559). "Helio- and Asteroseismology: Towards a Golden Future". 12-16 Jul
Physics
1
Helioseismology, Time Distance, Solar P-Modes Lifetime
Scientific paper
We use the method of time-distance analysis to measure lifetimes of solar p-modes in the range l=100-600 with data taken with the Taiwan Oscillation Network (TON). The lifetimes of p-modes are determined by the changes in the amplitude and width of the cross-correlation function of a wave packet with number of skips. The amplitude of cross-correlation function decreases pontentially with the number of skips as in the previous study Chou et al.(2001). This decrease has been interpreted as the effect of the finite p-mode lifetime. In this study, we find that the width of cross-correlation function increases with the number of skips. We interpret this phenomenon as the effect of the dispersion of the wave packet. We include this effect in the determination of lifetime of the wave packet. We also study the change in lifetime between solar minimum and maximum.
Burtseva Olga
Chou Dean-Yi
Kholikov Sh. S.
Serebryanskiy Alexander
TON Team
No associations
LandOfFree
On Lifetimes of High-L Solar P-Modes Ton Data does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with On Lifetimes of High-L Solar P-Modes Ton Data, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and On Lifetimes of High-L Solar P-Modes Ton Data will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-841982