The topographic effect of a meridional marine ridge on the spin-down of a cyclonic eddy, which is embedded in a zonal mean flow, is examined by use of a two layer numerical model. It is shown that the cyclonic eddy initially given on the eastern flank of the marine ridge decays in a short time. This result is common to all cases with the different volume transports of the mean flow (30 ~ 70 Sv) and of the cyclonic eddy (15 ~ 35 Sv). During the decay process, the cyclonic eddy shifts mainly northward into the shallower region, which is different from the dominant westward shift of the isolated cyclonic eddy. If the mean flow across over the marine ridge at the more northern latitude, the cyclonic eddy spins down more rapidly. A mean flow shifts zonal or south-eastward over a western side of the ridge, while it deflects north-eastward over an eastern side. The deflection angle of mean flow over the ridge depends on the intensity of lower layer velocity and density stratification. It is suggested that the topographic effect of the meridional marine ridge on the cyclonic eddy with mean flow is influenced both by the global phenomena that controls the inclination of the mean flow from zonal direction and by the local phenomena that controls the intensity of the topographic effect of the marine ridge.
IntroductionIn Part I of this study (Sekine, 1989), the topographic effect of a meridional marine ridge on the spin-down of an isolated cyclonic eddy had been studied by use of a two-layer numerical model. It has been shown by Part I that a cyclonic eddy on the eastern flank of a marine ridge decays in a shorter time in comparison with those given on the western flank. The fast decay on the eastern side is attributable to the planetary β effect that carries the cyclonic eddy westward to a shallower region over the eastern flank of the ridge, in which significant spin-down is induced by shrink of a water column due to the conservation of absolute potential vorticity (e.g., Pedlosky, 1979;Gill, 1982). In contrast to this, because the westward shift by the planetary β effect carries a cyclonic eddy to a deeper region over a western flank of the ridge, a stretching of the cyclonic water column results in spin-up of the cyclonic eddy. On the basis of these results, it is inferred by Part I that a cyclonic eddy accompanied by a large meander of the Kuroshio on the eastern side of the Izu Ridge decays in a shorter time than that on the western side (Sekine et al., 1985).However, because a mean flow accompanying with the cyclonic eddy was not considered in Part I, the details of the spin-down was not fully discussed. In the present study, as a succeeding study of Part I, the effect of mean flow on the spin-down of a cyclonic eddy is examined with reference to the topographic effect of the meridional marine ridge.