Modal and Nonmodal Growths of Symmetric Perturbations in Unbounded Domain

Qin Xu NOAA/National Severe Storms Laboratory, Norman, Oklahoma

Search for other papers by Qin Xu in
Current site
Google Scholar
PubMed
Close
Restricted access

Abstract

Modal and nonmodal growths of nonhydrostatic symmetric perturbations in an unbounded domain are examined in comparison with their hydrostatic counterparts. It is shown that the modal growth rate is a function of a single internal parameter s, the slope of the cross-band wave pattern. The maximum nonmodal growth of total perturbation energy norm is produced, also as a function of s, by an optimal combination of one geostrophic neutral mode and two paired nongeostrophic growing and decaying (or propagating) modes in the unstable (or stable) region. The hydrostatic approximation inflates the maximum modal growth rate significantly (or boundlessly) as the basic-state Richardson number Ri is small (or → 0) and inflates the maximum nonmodal growth rate significantly (or boundlessly) as |s| is large (or → ∞).

Inside the unstable region, the maximum nonmodal growth scaled by the modal growth is a bounded increasing function of growth time τ but reduces to 1 at (Ri, s) = (¼, −2) where the three modes become orthogonal to each other. Outside the unstable region, the maximum nonmodal growth is a periodic function of τ and the maximum growth time τm is bounded between ¼ and ½ of the period of the paired propagating modes. The scaled maximum nonmodal growth reaches the global maximum at s = −Ri−1 ± Ri−1(1 − Ri)1/2 (the marginal-stability boundary) for any τ if Ri ≤ 1, or at s = −1 ± (1 − Ri−1)1/2 for τ = τm if Ri > 1. When the neutral mode is filtered, the nonmodal growth becomes nongeostrophic and smaller than its counterpart growth constructed by the three modes but still significantly larger than the modal growth in general. The scaled maximum nongeostrophic nonmodal growth reaches the global maximum at s = −Ri−1 ± Ri−1(1 − Ri)1/2 for any τ if Ri ≤ 1, or at s = −Ri−1/2 for τ = τm if Ri > 1. Normalized inner products between the modes are introduced to measure their nonorthogonality and interpret their constructed nonmodal growths physically.

Corresponding author address: Qin Xu, National Severe Storms Laboratory, 120 David L. Boren Blvd., Norman, OK 73072. Email: qin.xu@noaa.gov

Abstract

Modal and nonmodal growths of nonhydrostatic symmetric perturbations in an unbounded domain are examined in comparison with their hydrostatic counterparts. It is shown that the modal growth rate is a function of a single internal parameter s, the slope of the cross-band wave pattern. The maximum nonmodal growth of total perturbation energy norm is produced, also as a function of s, by an optimal combination of one geostrophic neutral mode and two paired nongeostrophic growing and decaying (or propagating) modes in the unstable (or stable) region. The hydrostatic approximation inflates the maximum modal growth rate significantly (or boundlessly) as the basic-state Richardson number Ri is small (or → 0) and inflates the maximum nonmodal growth rate significantly (or boundlessly) as |s| is large (or → ∞).

Inside the unstable region, the maximum nonmodal growth scaled by the modal growth is a bounded increasing function of growth time τ but reduces to 1 at (Ri, s) = (¼, −2) where the three modes become orthogonal to each other. Outside the unstable region, the maximum nonmodal growth is a periodic function of τ and the maximum growth time τm is bounded between ¼ and ½ of the period of the paired propagating modes. The scaled maximum nonmodal growth reaches the global maximum at s = −Ri−1 ± Ri−1(1 − Ri)1/2 (the marginal-stability boundary) for any τ if Ri ≤ 1, or at s = −1 ± (1 − Ri−1)1/2 for τ = τm if Ri > 1. When the neutral mode is filtered, the nonmodal growth becomes nongeostrophic and smaller than its counterpart growth constructed by the three modes but still significantly larger than the modal growth in general. The scaled maximum nongeostrophic nonmodal growth reaches the global maximum at s = −Ri−1 ± Ri−1(1 − Ri)1/2 for any τ if Ri ≤ 1, or at s = −Ri−1/2 for τ = τm if Ri > 1. Normalized inner products between the modes are introduced to measure their nonorthogonality and interpret their constructed nonmodal growths physically.

Corresponding author address: Qin Xu, National Severe Storms Laboratory, 120 David L. Boren Blvd., Norman, OK 73072. Email: qin.xu@noaa.gov

Save
  • Bennetts, D. A., and B. J. Hoskins, 1979: Conditional symmetric instability—A possible explanation for frontal rainbands. Quart. J. Roy. Meteor. Soc., 105 , 945962.

    • Search Google Scholar
    • Export Citation
  • Eliassen, A., 1952: Slow thermally and frictionally controlled meridional circulation in a circular vortex. Astrophys. Norvegica, 5 , 1960.

    • Search Google Scholar
    • Export Citation
  • Emanuel, K. A., 1979: Inertial instability and mesoscale convective systems. Part I: Linear theory of inertial instability in rotating viscous fluids. J. Atmos. Sci., 36 , 24252449.

    • Search Google Scholar
    • Export Citation
  • Emanuel, K. A., 1983: The Lagrangian parcel dynamics of moist symmetric instability. J. Atmos. Sci., 40 , 23682376.

  • Farrell, B. F., 1984: Modal and non-modal baroclinic waves. J. Atmos. Sci., 41 , 668673.

  • Farrell, B. F., and P. J. Ioannou, 1996: Generalized stability theory. Part I: Autonomous operators. J. Atmos. Sci., 53 , 20252040.

  • Fjortoft, R., 1944: On the frontogenesis and cyclogenesis in the atmosphere. Part I. On the stability of the stationary circular vortex. Geofys. Publ., 16 (5) 128.

    • Search Google Scholar
    • Export Citation
  • Golub, G. H., and C. F. Van Loan, 1983: Matrix Computations. Johns Hopkins University Press, 476 pp.

  • Gu, W., Q. Xu, and R. Wu, 1998: Three-dimensional instability of nonlinear viscous symmetric circulations. J. Atmos. Sci., 55 , 31483158.

    • Search Google Scholar
    • Export Citation
  • Heifetz, E., and B. F. Farrell, 2008: Non-normal growth in symmetric shear flow. Quart. J. Roy. Meteor. Soc., 134 , 16271633.

  • Kanehisa, H., 2008: Degenerate modes of symmetric instability. J. Meteor. Soc. Japan, 86 , 557562.

  • Kuo, H. L., 1954: Symmetrical disturbances in a thin layer of fluid subject to horizontal temperature gradient and rotation. J. Meteor., 11 , 399411.

    • Search Google Scholar
    • Export Citation
  • Lighthill, M. J., 1958: Introduction to Fourier Analysis and Generalised Functions. Cambridge University Press, 79 pp.

  • Miller, T. L., 1984: The structures and energetics of fully nonlinear symmetric baroclinic waves. J. Fluid Mech., 142 , 343362.

  • Ooyama, K., 1966: On the stability of the baroclinic circular vortex: A sufficient criterion for instability. J. Atmos. Sci., 23 , 4353.

    • Search Google Scholar
    • Export Citation
  • Stone, P. H., 1966: On non-geostrophic baroclinic stability. J. Atmos. Sci., 23 , 390400.

  • Stone, P. H., 1972: On non-geostrophic baroclinic stability: Part III. The momentum and heat transports. J. Atmos. Sci., 29 , 419426.

  • Xu, Q., 1986: Conditional symmetric instability and mesoscale rainbands. Quart. J. Roy. Meteor. Soc., 112 , 315334.

  • Xu, Q., 2003: Nearly symmetric and nearly baroclinic instabilities in the presence of diffusivity. Part I: Growth rate patterns. J. Fluid Mech., 492 , 181205.

    • Search Google Scholar
    • Export Citation
  • Xu, Q., 2007: Modal and nonmodal symmetric perturbations. Part I: Completeness of normal modes and constructions of nonmodal solutions. J. Atmos. Sci., 64 , 17451763.

    • Search Google Scholar
    • Export Citation
  • Xu, Q., and X. P. Zhou, 1982: Baroclinic and inertial instability in a nonhydrostatic atmosphere. Sci. Atmos. Sinica, 6 , 355367.

  • Xu, Q., and J. H. E. Clark, 1985: The nature of symmetric instability and its similarity to convective and inertial instability. J. Atmos. Sci., 42 , 28802883.

    • Search Google Scholar
    • Export Citation
  • Xu, Q., T. Lei, and S. Gao, 2007: Modal and nonmodal symmetric perturbations. Part II: Nonmodal growths measured by total perturbation energy. J. Atmos. Sci., 64 , 17641781.

    • Search Google Scholar
    • Export Citation
All Time Past Year Past 30 Days
Abstract Views 0 0 0
Full Text Views 86 35 7
PDF Downloads 30 18 2