Variation of Oscillation Mode Parameters over the Solar Cycle 23: An Analysis on Different Time Scales
Solar and Stellar Astrophysics
2009-03-13 v1
Abstract
We investigate the variation in the mode parameters obtained from time series of length 9, 36, 72 and 108 days to understand the changes occurring on different time-scales. The regression analysis between frequency shifts and activity proxies indicates that the correlation and slopes are correlated and both increase in going from time series of 9 to 108 days. We also observe that the energy of the mode is anti-correlated with solar activity while the rate at which the energy is supplied remains constant over the solar cycle.
Keywords
Cite
@article{arxiv.0903.2074,
title = {Variation of Oscillation Mode Parameters over the Solar Cycle 23: An Analysis on Different Time Scales},
author = {S. C. Tripathy and F. Hill and K. Jain and J. W. Leibacher},
journal= {arXiv preprint arXiv:0903.2074},
year = {2009}
}
Comments
4 pages, To appear in the conference proceeding of GONG 2008 / SOHO XXI