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  • American Meteorological Society  (2)
  • 2010-2014  (2)
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  • American Meteorological Society  (2)
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  • 1
    Publication Date: 2014-07-29
    Description: El Niño–Southern Oscillation (ENSO) is a pronounced mode of climate variability that originates in the tropical Pacific and affects weather patterns worldwide. Growing evidence suggests that despite extensive changes in tropical climate, ENSO was active over vast geological epochs stretching millions of years from the late Cretaceous to the Holocene. In particular, ENSO persisted during the Pliocene, when a dramatic reduction occurred in the mean east–west temperature gradient in the equatorial Pacific. The mechanisms for sustained ENSO in such climates are poorly understood. Here a comprehensive climate model is used to simulate ENSO for a broad range of tropical Pacific mean climates characterized by different climatological SST gradients. It is found that the simulated ENSO remains surprisingly robust: when the east–west gradient is reduced from 6° to 1°C, the amplitude of ENSO decreases only by 30%–40%, its dominant period remains close to 3–4 yr, and the spectral peak stays above red noise. To explain these results, the magnitude of ocean–atmosphere feedbacks that control the stability of the natural mode of ENSO (the Bjerknes stability index) is evaluated. It is found that as a result of reorganization of the atmospheric Walker circulation in response to changes in the mean surface temperature gradient, the growth/decay rates of the ENSO mode stay nearly constant throughout different climates. These results explain the persistence of ENSO in the past and, in particular, reconcile the seemingly contradictory findings of ENSO occurrence and the small mean east–west temperature gradient during the Pliocene.
    Print ISSN: 0894-8755
    Electronic ISSN: 1520-0442
    Topics: Geography , Geosciences , Physics
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  • 2
    Publication Date: 2013-12-01
    Description: This study is motivated by Arctic Ocean observations of sub–mixed layer eddies found at large distances from their assumed formation region of a surface ocean front. Eddy formation is explored through high-resolution numerical simulations of surface fronts, separating two mixed layers, with a range of configurations similar to those observed in the Arctic Ocean. This study finds that frontal instabilities lead to the development of self-propagating dipoles, which have the potential to propagate far from the front if interactions with other eddies are avoided. However, most dipoles are unbalanced, consisting of a dominating surface cyclone and a weaker anticyclone below, and thus propagate on curved trajectories with eventual recirculation back to the front. Their maximum separation distance from the front depends on the ratio of self-advecting velocities ϵ; balanced dipoles that have ϵ ≈ 1, and the ability to propagate far from the front. For dipoles generated numerically, this study estimates ϵ using analytical solutions of a 2½-layer quasigeostrophic model for Gaussian vortices. The distribution of the ratio ϵ for these dipoles is found to be skewed toward higher values (i.e., cyclones are dominant in dipoles). Sensitivity experiments suggest that shallow fronts that separate mixed layers of approximately equal depths favor the development of balanced dipoles that can self-propagate over long distances.
    Print ISSN: 0022-3670
    Electronic ISSN: 1520-0485
    Topics: Geosciences , Physics
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