Tidal oscillations in the Caspian Sea


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Abstract

Long-term hourly data from 12 tide gauge stations were used to examine the character of tidal oscillations in the Caspian Sea. Diurnal and semidiurnal tidal peaks are well-defined in sea level spectra in the Middle and South Caspian basins. High-resolution spectral analysis revealed that the diurnal sea level oscillations in the Middle Caspian Basin have a gravitational origin, while those in the South Caspian Basin are mainly caused by radiational effects: the amplitude of diurnal radiational harmonic S1 is much higher than those of gravitational harmonics О1, P1, and K1. In the North Caspian Basin, there are no gravitational tides and only weak radiational tides are observed. A semidiurnal type of tide is predominant in the Middle and South Caspian basins. Harmonic analysis of the tides for individual annual series with subsequent vector averaging over the entire observational period was applied to estimate the mean amplitudes and phases of major tidal constituents. The amplitude of the M2 harmonic reaches 5.4 cm in the South Caspian Basin (at Aladga). A maximum tidal range of 21 cm was found at the Aladga station in the southeastern part of the Caspian Sea, whereas the tidal range in the western part of the South Caspian Basin varies from 5 to 10 cm.

About the authors

I. P. Medvedev

Shirshov Institute of Oceanology; Fedorov Institute of Applied Geophysics

Author for correspondence.
Email: patamates@gmail.com
Russian Federation, Moscow; Moscow

E. A. Kulikov

Shirshov Institute of Oceanology

Email: patamates@gmail.com
Russian Federation, Moscow

A. B. Rabinovich

Shirshov Institute of Oceanology; Institute of Ocean Sciences

Email: patamates@gmail.com
Russian Federation, Moscow; Sidney, British Columbia

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