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  • 1
    Online Resource
    Online Resource
    American Meteorological Society ; 2013
    In:  Journal of the Atmospheric Sciences Vol. 70, No. 8 ( 2013-08-01), p. 2614-2628
    In: Journal of the Atmospheric Sciences, American Meteorological Society, Vol. 70, No. 8 ( 2013-08-01), p. 2614-2628
    Abstract: The feedback between planetary-scale eddies and analogs of the midlatitude eddy-driven jet and the subtropical jet is investigated in a barotropic β-plane model. In the model the subtropical jet is generated by a relaxation process and the eddy-driven jet by an imposed wavemaker. A minimum zonal phase speed bound is proposed in addition to the established upper bound, where the zonal phase speed of waves must be less than that of the zonal mean zonal flow. Cospectral analysis of eddy momentum flux convergence shows that eddy activity is generally restricted by these phase speed bounds. The wavenumber-dependent minimum phase speed represents a turning line for meridionally propagating waves. By varying the separation distance between the relaxation and stirring regions, it is found that a sustained, double-jet state is achieved when either a critical or turning latitude forms in the interjet region. The interjet turning latitude filters eddies by zonal wavenumber such that shorter waves tend to be reflected off of the relaxed jet and are confined to the eddy-driven jet. The interjet region is transparent to long waves that act to blend the jets and may be associated with barotropic instability. The eddy-driven and relaxed jets tend to merge owing to the propagation of these long waves through the relaxed jet waveguide.
    Type of Medium: Online Resource
    ISSN: 0022-4928 , 1520-0469
    RVK:
    Language: English
    Publisher: American Meteorological Society
    Publication Date: 2013
    detail.hit.zdb_id: 218351-1
    detail.hit.zdb_id: 2025890-2
    SSG: 16,13
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  • 2
    Online Resource
    Online Resource
    American Meteorological Society ; 2016
    In:  Journal of the Atmospheric Sciences Vol. 73, No. 5 ( 2016-05-01), p. 2179-2201
    In: Journal of the Atmospheric Sciences, American Meteorological Society, Vol. 73, No. 5 ( 2016-05-01), p. 2179-2201
    Abstract: The eddy-driven and subtropical jets are two dynamically distinct features of the midlatitude upper-troposphere circulation that are often merged into a single zonal wind maximum. Nonetheless, the potential for a distinct double-jet state in the atmosphere exists, particularly in the winter hemisphere, and presents a unique zonal-mean flow with two waveguides and an interjet region with a weakened potential vorticity gradient upon which Rossby waves may be generated, propagate, reflect, and break. The authors investigate the interaction of two groups of atmospheric waves—those with wavelengths longer and shorter than the deformation radius—within a double-jet mean flow in an idealized atmospheric model. Patterns of eddy momentum flux convergence for long and short waves differ greatly. Short waves behave following classic baroclinic instability theory such that their eddy momentum flux convergence is centered at the eddy-driven jet core. Long waves, on the other hand, reveal strong eddy momentum flux convergence along the poleward flank of the eddy-driven jet and within the interjet region. This pattern is enhanced when two jets are present in the zonal-mean zonal wind.
    Type of Medium: Online Resource
    ISSN: 0022-4928 , 1520-0469
    RVK:
    Language: English
    Publisher: American Meteorological Society
    Publication Date: 2016
    detail.hit.zdb_id: 218351-1
    detail.hit.zdb_id: 2025890-2
    SSG: 16,13
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  • 3
    Online Resource
    Online Resource
    American Meteorological Society ; 2001
    In:  Journal of Physical Oceanography Vol. 31, No. 2 ( 2001-02), p. 554-571
    In: Journal of Physical Oceanography, American Meteorological Society, Vol. 31, No. 2 ( 2001-02), p. 554-571
    Type of Medium: Online Resource
    ISSN: 0022-3670 , 1520-0485
    Language: English
    Publisher: American Meteorological Society
    Publication Date: 2001
    detail.hit.zdb_id: 2042184-9
    detail.hit.zdb_id: 184162-2
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  • 4
    Online Resource
    Online Resource
    American Meteorological Society ; 2002
    In:  Journal of Physical Oceanography Vol. 32, No. 6 ( 2002-06), p. 1699-1720
    In: Journal of Physical Oceanography, American Meteorological Society, Vol. 32, No. 6 ( 2002-06), p. 1699-1720
    Type of Medium: Online Resource
    ISSN: 0022-3670 , 1520-0485
    Language: English
    Publisher: American Meteorological Society
    Publication Date: 2002
    detail.hit.zdb_id: 2042184-9
    detail.hit.zdb_id: 184162-2
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  • 5
    Online Resource
    Online Resource
    American Meteorological Society ; 2011
    In:  Journal of Physical Oceanography Vol. 41, No. 9 ( 2011-09-01), p. 1605-1623
    In: Journal of Physical Oceanography, American Meteorological Society, Vol. 41, No. 9 ( 2011-09-01), p. 1605-1623
    Abstract: This paper examines the factors determining the distribution, length scale, magnitude, and structure of mesoscale oceanic eddies in an eddy-resolving primitive equation simulation of the Southern Ocean [Modeling Eddies in the Southern Ocean (MESO)]. In particular, the authors investigate the hypothesis that the primary source of mesoscale eddies is baroclinic instability acting locally on the mean state. Using local mean vertical profiles of shear and stratification from an eddying primitive equation simulation, the forced–dissipated quasigeostrophic equations are integrated in a doubly periodic domain at various locations. The scales, energy levels, and structure of the eddies found in the MESO simulation are compared to those predicted by linear stability analysis, as well as to the eddying structure of the quasigeostrophic simulations. This allows the authors to quantitatively estimate the role of local nonlinear effects and cascade phenomena in the generation of the eddy field. There is a modest transfer of energy (an “inverse cascade”) to larger scales in the horizontal, with the length scale of the resulting eddies typically comparable to or somewhat larger than the wavelength of the most unstable mode. The eddies are, however, manifestly nonlinear, and in many locations the turbulence is fairly well developed. Coherent structures also ubiquitously emerge during the nonlinear evolution of the eddy field. There is a near-universal tendency toward the production of grave vertical scales, with the barotropic and first baroclinic modes dominating almost everywhere, but there is a degree of surface intensification that is not captured by these modes. Although the results from the local quasigeostrophic model compare well with those of the primitive equation model in many locations, some profiles do not equilibrate in the quasigeostrophic model. In many cases, bottom friction plays an important quantitative role in determining the final scale and magnitude of eddies in the quasigeostrophic simulations.
    Type of Medium: Online Resource
    ISSN: 0022-3670 , 1520-0485
    Language: English
    Publisher: American Meteorological Society
    Publication Date: 2011
    detail.hit.zdb_id: 2042184-9
    detail.hit.zdb_id: 184162-2
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  • 6
    Online Resource
    Online Resource
    American Meteorological Society ; 1999
    In:  Journal of the Atmospheric Sciences Vol. 56, No. 11 ( 1999-06), p. 1579-1593
    In: Journal of the Atmospheric Sciences, American Meteorological Society, Vol. 56, No. 11 ( 1999-06), p. 1579-1593
    Type of Medium: Online Resource
    ISSN: 0022-4928 , 1520-0469
    RVK:
    Language: English
    Publisher: American Meteorological Society
    Publication Date: 1999
    detail.hit.zdb_id: 218351-1
    detail.hit.zdb_id: 2025890-2
    SSG: 16,13
    Location Call Number Limitation Availability
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  • 7
    Online Resource
    Online Resource
    Journal of Marine Research/Yale ; 1997
    In:  Journal of Marine Research Vol. 55, No. 2 ( 1997-03-01), p. 223-275
    In: Journal of Marine Research, Journal of Marine Research/Yale, Vol. 55, No. 2 ( 1997-03-01), p. 223-275
    Type of Medium: Online Resource
    ISSN: 0022-2402 , 1543-9542
    Language: English
    Publisher: Journal of Marine Research/Yale
    Publication Date: 1997
    detail.hit.zdb_id: 410655-6
    detail.hit.zdb_id: 2066603-2
    SSG: 12
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  • 8
    Online Resource
    Online Resource
    Cambridge University Press (CUP) ; 2019
    In:  Journal of Fluid Mechanics Vol. 862 ( 2019-03-10), p. 162-199
    In: Journal of Fluid Mechanics, Cambridge University Press (CUP), Vol. 862 ( 2019-03-10), p. 162-199
    Abstract: Rayleigh–Bénard convection is one of the most well-studied models in fluid mechanics. Atmospheric convection, one of the most important components of the climate system, is by comparison complicated and poorly understood. A key attribute of atmospheric convection is the buoyancy source provided by the condensation of water vapour, but the presence of radiation, compressibility, liquid water and ice further complicate the system and our understanding of it. In this paper we present an idealized model of moist convection by taking the Boussinesq limit of the ideal-gas equations and adding a condensate that obeys a simplified Clausius–Clapeyron relation. The system allows moist convection to be explored at a fundamental level and reduces to the classical Rayleigh–Bénard model if the latent heat of condensation is taken to be zero. The model has an exact, Rayleigh-number-independent ‘drizzle’ solution in which the diffusion of water vapour from a saturated lower surface is balanced by condensation, with the temperature field (and so the saturation value of the moisture) determined self-consistently by the heat released in the condensation. This state is the moist analogue of the conductive solution in the classical problem. We numerically determine the linear stability properties of this solution as a function of Rayleigh number and a non-dimensional latent-heat parameter. We also present some two-dimensional, time-dependent, nonlinear solutions at various values of Rayleigh number and the non-dimensional condensational parameters. At sufficiently low Rayleigh number the system converges to the drizzle solution, and we find no evidence that two-dimensional self-sustained convection can occur when that solution is stable. The flow transitions from steady to turbulent as the Rayleigh number or the effects of condensation are increased, with plumes triggered by gravity waves emanating from other plumes. The interior dries as the level of turbulence increases, because the plumes entrain more dry air and because the saturated boundary layer at the top becomes thinner. The flow develops a broad relative humidity minimum in the domain interior, only weakly dependent on Rayleigh number when that is high.
    Type of Medium: Online Resource
    ISSN: 0022-1120 , 1469-7645
    Language: English
    Publisher: Cambridge University Press (CUP)
    Publication Date: 2019
    detail.hit.zdb_id: 1472346-3
    detail.hit.zdb_id: 218334-1
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  • 9
    Online Resource
    Online Resource
    Wiley ; 2022
    In:  Quarterly Journal of the Royal Meteorological Society Vol. 148, No. 744 ( 2022-04), p. 1127-1130
    In: Quarterly Journal of the Royal Meteorological Society, Wiley, Vol. 148, No. 744 ( 2022-04), p. 1127-1130
    Abstract: In their comment, Davison and Haynes remark on an apparent time‐step sensitivity in the model presented by Vallis and Penn, such that in their own simulations the excitability is lost when using a smaller time step. However, this reply shows that if the condensational time‐scale is suitably small then excitable behaviour can be achieved over a range of time steps, including very small ones, with very similar energy levels and large‐scale behaviour at both large and small time steps. In particular, an eastward‐propagating disturbance resembling the Madden–Julian Oscillation can still be reproduced, independent of time step. Certainly there are numerical, mathematical, and physical difficulties in understanding a system in which condensation occurs on short time‐scales, and this reply discusses further the applicability of the results to the real atmosphere.
    Type of Medium: Online Resource
    ISSN: 0035-9009 , 1477-870X
    URL: Issue
    RVK:
    RVK:
    Language: English
    Publisher: Wiley
    Publication Date: 2022
    detail.hit.zdb_id: 3142-2
    detail.hit.zdb_id: 2089168-4
    SSG: 14
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  • 10
    Online Resource
    Online Resource
    Wiley ; 1996
    In:  Quarterly Journal of the Royal Meteorological Society Vol. 122, No. 529 ( 1996-01), p. 291-322
    In: Quarterly Journal of the Royal Meteorological Society, Wiley, Vol. 122, No. 529 ( 1996-01), p. 291-322
    Type of Medium: Online Resource
    ISSN: 0035-9009 , 1477-870X
    URL: Issue
    RVK:
    RVK:
    Language: English
    Publisher: Wiley
    Publication Date: 1996
    detail.hit.zdb_id: 3142-2
    detail.hit.zdb_id: 2089168-4
    SSG: 14
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