Abstract

AbstractThis paper describes global characteristics of the westward‐propagating planetary wave with a period of ∼4 days and zonal wavenumber 2, here referred to as quasi‐4‐day wave (Q4DW), which is considered to be a manifestation of the (2,1) Rossby normal mode. A climatology of the Q4DW is derived from geopotential height measurements by the Aura Microwave Limb Sounder during August 2004–December 2020. In the mesosphere and lower thermosphere (MLT), amplitude maxima occur at mid latitudes in May and August in the Northern Hemisphere, and in February and November in the Southern Hemisphere. With the amplitude exceeding 300 m, the Q4DW sometimes becomes the dominant mode of traveling planetary waves in the MLT. The seasonal variation is largely determined by the zonal mean state. As predicted by previous modeling work, the amplitude grows rapidly with height on the equatorward side of the critical layer, where the zonal mean flow is weakly eastward relative to the wave. The wave growth can be particularly large when there is a region of unstable mean flow across the boundary of the critical layer. This condition is met not only during the seasonal amplification of the Q4DW but also during some Arctic sudden stratospheric warming events, leading to an unseasonal enhancement.

Highlights

  • Classical wave theory utilizes the linearized equations governing atmospheric flow to describe properties of wave motions in the atmosphere (e.g. Lindzen & Chapman, 1969; Forbes, 1995)

  • We present the seasonal climatology of the quasi-4-day wave (Q4DW) derived from the long-term record of Aura/Microwave Limb Sounder (MLS) geopotential height during August 2004–December 2020

  • The results suggest that the Q4DW is the predominant W2 component in the mid-latitude mesosphere and lower thermosphere (MLT)

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Summary

Introduction

Classical wave theory utilizes the linearized equations governing atmospheric flow to describe properties of wave motions in the atmosphere (e.g. Lindzen & Chapman, 1969; Forbes, 1995). Classical wave theory utilizes the linearized equations governing atmospheric flow to describe properties of wave motions in the atmosphere Under the assumption of a simplified atmosphere without dissipation and zonal mean winds, the linearized equations are separable in latitude and height. The latitude equation is known as Laplace’s tidal equation. The solutions to Laplace’s tidal equation are expressed in form of Hough functions, which give the latitudinal structure of waves. The height equation specifies the vertical structure of each Hough mode for given atmospheric forcing. In the absence of forcing, the assumption of an isothermal atmosphere with a rigid lower boundary (zero vertical velocity at the surface) leads to a single solution to Laplace’s tidal equation. The corresponding Hough functions represent free (unforced) oscillations or normal modes of the atmosphere

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