A model of the seasonal circulation in the Arabian Sea forced by observed winds

https://doi.org/10.1016/0079-6611(85)90017-5Get rights and content

Abstract

Results of a numerical model of the wind driven seasonal circulation in the Arabian Sea are presented, with particular emphasis on the ocean's response to the monsoon winds. The model equations are the fully nonlinear reduced gravity transport equations in spherical coordinates. The model resolution is 1/8° in the east-west direction and 1/4° in the north-south direction. The model basin geometry corresponds as closely as possible to that of the north-west Indian Ocean from 40°E to 73°E and from 10°S to 25°N, and includes the gulfs of Aden and Oman, and the islands of Socotra and the Seychelles. The southern boundary and a portion of the eastern boundary, from the equator to 6°S, representing the opening between the Maldives and the Chagos Archipelago, are open boundaries. At other boundaries, the no-slip condition is applied. The wind stress data used to force the model comes from the NOAA National Climate Center's TD-9757 Global Marine Sums data, which consists of monthly mean winds compiled on 1° squares from over 60 years of ship observations. These data are interpolated in time using the mean and first five Fourier harmonics at each point, and then interpolated linearly to the model grid. The model equations are integrated in time using centered finite differences in time and space (a leap-frog scheme), with lateral friction treated by a Dufort-Frankel scheme.

After a one year spin up, the model settles into a regular periodic seasonal cycle, even though the solution to the model equations is locally highly nonlinear, with large nonlinear eddies developing in the same location at the same time of year from one year to the next. The development of the model Somali Current system with the onset of the (northern hemisphere) summer monsoon is consistent with the available observations in the region. The model reproduces many of the observed features in this region, such as the two-gyre circulation pattern, and the timing and movement of these features corresponds well with their real world counterparts. The model also shows an eastward jet forming in late June to early July at 13°N, just to the east of Socotra. This jet is fed by flow coming out of the great whirl. The break down of the two-gyre pattern occurs in mid to late August, when the southern gyre breaks up into several smaller eddies, the northern-most of which coalesces with the great whirl. Numerous small cyclonic eddies develop along the Arabian coast, from the Gulf of Oman into the Gulf of Aden, in early to mid August, and persist well into the winter monsoon. The model shows that it is possible to simulate very complicated flows, if one has sufficient wind data, using fairly simple models with a realistic basin geometry.

References (26)

  • A.J. Busalacchi et al.

    The seasonal variability in a model of the tropical Pacific

    Journal of Physical Oceanography

    (1980)
  • B.J. Cagle et al.

    Arabian Sea project of 1980 - Composites of infrared images

  • M.A. Cane

    The response of an equatorial ocean to simple wind stress patterns: I. Model formulation and analytical results

    Journal of Marine Research

    (1979)
  • Cited by (88)

    • 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 Oceanography
      Citation 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.

    • Intrinsic Versus Wind-Forced Great Whirl Non-Seasonal Variability

      2024, Journal of Geophysical Research: Oceans
    View all citing articles on Scopus
    View full text