A model of the seasonal circulation in the Arabian Sea forced by observed winds
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Dynamics of intraseasonal oscillations in the Bay of Bengal during summer monsoons captured by mooring observations
2020, Deep-Sea Research Part II: Topical Studies in OceanographyCitation Excerpt :The oceanic circulation in the Indian Ocean (IO) is unique, signified by seasonal flow reversals, significant freshwater input, basin exchanges, variability of local forcing and remote forcing via planetary waves. Although previous work (e.g. Lighthill, 1969; Cox, 1970; Luther and O’ Brien, 1985) shows that the semiannual reversal of currents in the Bay of Bengal (BoB) is closely related to monsoon winds, the details are complicated in that numerical experiments demonstrate the influence of remote forcing from the interior of the equatorial IO, which is also related to monsoon winds (Yu et al., 1991; Clarke and Liu, 1993). Equatorial Kelvin waves, commonly interpreted as Wyrtki (1973) jets, propagate eastward along the equator during April/May and September/October.
Interannual variability of Kelvin wave propagation in the wave guides of the equatorial Indian Ocean, the coastal Bay of Bengal and the southeastern Arabian Sea during 1993-2006
2010, Deep-Sea Research Part I: Oceanographic Research PapersThe Red Sea outflow regulated by the Indian monsoon
2006, Continental Shelf ResearchIntrinsic Versus Wind-Forced Great Whirl Non-Seasonal Variability
2024, Journal of Geophysical Research: OceansVariability of Arabian Sea surface circulation and chlorophyll distribution: a remote sensing estimation
2022, Terrestrial, Atmospheric and Oceanic Sciences