Abstract
Any investigation of the dynamical behavior of fluid flow on the mesoscale should involve a thorough study of mesoscale instabilities. Symmetric instability is one of only a very few instabilities which are known to have distinctly mesoscale characteristics. The physical nature of the instability and the conditions under which it may occur are described in this chapter.
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References
Emanuel, K. A., 1979: Inertial instability and mesoscale con-vective systems, Part I: Linear theory of inertial instability in rotating viscous fluids, J. Atmos. Sci., 36, pp. 2425–2449.
Walton, I. C., 1975: The viscous nonlinear symmetric baro- clinic instability of a zonal shear flow, J. Fluid Mech., 68, pp. 757–768.
Kuo, H.-L., 1954: Symmetrical disturbances in a thin layer of fluid subject to a horizontal temperature gradient and rotation, J. Meteor., 11, pp. 399–411.
Stone, P. H., 1972: On non-geostrophic baroclinic stability: Part III. The momentum and heat transports, J. Atmos. Sci., 29, pp. 419–426.
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© 1983 Springer Science+Business Media Dordrecht
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Emanuel, K.A. (1983). Symmetric Instability. In: Lilly, D.K., Gal-Chen, T. (eds) Mesoscale Meteorology — Theories, Observations and Models. NATO ASI Series, vol 114. Springer, Dordrecht. https://doi.org/10.1007/978-94-017-2241-4_11
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DOI: https://doi.org/10.1007/978-94-017-2241-4_11
Publisher Name: Springer, Dordrecht
Print ISBN: 978-90-481-8390-6
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