Resonant Continuum Modes in the Eady Model with Rigid Lid

Johannes Jenkner Institute for Meteorology and Geophysics, University of Innsbruck, Innsbruck, Austria

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Martin Ehrendorfer Institute for Meteorology and Geophysics, University of Innsbruck, Innsbruck, Austria

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Abstract

The Eady model with rigid upper lid is considered. The resonant, linearly amplifying solution that exists in the situation of neutral normal modes when an infinitely thin potential vorticity (PV) perturbation is located precisely at the steering level of a zero-PV neutral mode is explicitly derived. This resonant solution is discussed by partitioning the solution into nonzero-PV and zero-PV contributions. It possesses key observed properties of a growing baroclinic structure. The partitioning of the resonant solution clearly demonstrates the existence of modal growth in a short-wave Eady setting. In contrast to the semi-infinite model, a nonamplifying zero-PV contribution is necessary, in addition to the resonant part, to ensure vanishing vertical velocity at both the upper and the lower lid.

* Current affiliation: Institute for Atmospheric and Climate Science, ETH Zürich, Zürich, Switzerland

Corresponding author address: Martin Ehrendorfer, Institute for Meteorology and Geophysics, University of Innsbruck, Innrain 52, A-6020 Innsbruck, Austria. Email: martin.ehrendorfer@uibk.ac.at

Abstract

The Eady model with rigid upper lid is considered. The resonant, linearly amplifying solution that exists in the situation of neutral normal modes when an infinitely thin potential vorticity (PV) perturbation is located precisely at the steering level of a zero-PV neutral mode is explicitly derived. This resonant solution is discussed by partitioning the solution into nonzero-PV and zero-PV contributions. It possesses key observed properties of a growing baroclinic structure. The partitioning of the resonant solution clearly demonstrates the existence of modal growth in a short-wave Eady setting. In contrast to the semi-infinite model, a nonamplifying zero-PV contribution is necessary, in addition to the resonant part, to ensure vanishing vertical velocity at both the upper and the lower lid.

* Current affiliation: Institute for Atmospheric and Climate Science, ETH Zürich, Zürich, Switzerland

Corresponding author address: Martin Ehrendorfer, Institute for Meteorology and Geophysics, University of Innsbruck, Innrain 52, A-6020 Innsbruck, Austria. Email: martin.ehrendorfer@uibk.ac.at

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