Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2942
Title: Possible Evidence of Long-Term Oscillations in the Solar Atmosphere
Authors: Raju, K. P
Singh, J
Srikanth, R
Chou, Dean-Yi
CA, TON team
Keywords: Oscillation Network;Solar and Heliospheric Observatory (SOHO);Supergranulation;Periodogram
Issue Date: Mar-2001
Publisher: Springer
Citation: Solar Physics, Vol. 199, No. 1, pp. 1 – 11
Abstract: We have obtained the temporal correlation function, Q(t), from time sequences of Caii K filtergrams and Dopplergrams from Antarctica, Taiwan Oscillation Network (TON) and Solar and Heliospheric Observatory (SOHO). Q(t) gives the time evolution of the pattern under examination, supergranulation in this case. It has been found that Q(t) shows oscillatory signals of both 5-min and long-term periods. The 5-min oscillations are suppressed by averaging the images over 10 min. An exponential decay curve which represents the lifetime trend of supergranules, is fitted to Q(t) and subtracted out. The Q(t) residuals thus obtained contain the oscillatory component and are then subjected to a periodogram analysis. Significant periodicities in the range of 1.4-10 hours have been noted. The causes of these oscillations are not fully known at present, but the instrumental and atmospheric factors can be ruled out, pointing to solar origin. Various possibilities are discussed. Some of the observed periodicities may be considered as probable candidates for long-term oscillations in the Sun, such as the elusive gravity modes.
Description: Restricted Access
URI: http://hdl.handle.net/2248/2942
ISSN: 0038-0938
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Appears in Collections:IIAP Publications

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