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On the low-frequency variability in the Indian Ocean

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Dynamic Planet

Part of the book series: International Association of Geodesy Symposia ((IAG SYMPOSIA,volume 130))

Abstract

This paper presents the results of an investigation of low-frequency variability in the Indian Ocean (IO) primarily using satellite altimeter sea surface height (SSH) observations and expendable bathy-thermograph (XBT) data. We found that in most regions of the IO the low-frequency part of the SSH spectra (corresponding to signals with periods of a few months or longer) is concentrated in four frequency bands separated by substantial spectral gaps. These bands correspond to periods of approximately 6 months, 12 months, 18–20 months and more than 30 months (hereafter referred to as the 30-month band). For both 18–20-month and 30-month bands the spectral density shows a dipole-like pattern with some degree of similarity; however, analysis of the spatial-temporal evolution of these signals suggests that the 18–20-month signal is an internal mode of the IO, while that of the 30-month component propagates from the Pacific Ocean, in particular with a much stronger signal during the period from 1998 to 2003.

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Sakova, I.V., Meyers, G., Coleman, R. (2007). On the low-frequency variability in the Indian Ocean. In: Tregoning, P., Rizos, C. (eds) Dynamic Planet. International Association of Geodesy Symposia, vol 130. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-540-49350-1_7

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