Propagation and Breakdown of Internal Inertio-Gravity Waves
near Critical Levels in the Middle Atmosphere
Manabu D. Yamanaka
Institute of Space and Astronautical Science,
Meguro, Tokyo 153, Japan
and Hiroshi Tanaka
Water Research Institute, Nagoya University,
Chikusa, Nagoya 464, Japan
Journal of the Meteorological Society of Japan ,
vol.62, no.1, pp.1-17.
A part of M.Sc Thesis by M. D. Yamanaka
submitted to Graduate School of Science, Nagoya University
in February 1982,
accepted in March 1982.
First manuscript received: December 28, 1982;
Final manuscript accepted: December 6, 1983
Published: February, 1984
ABSTRACT ,
CONTENTS ,
CORRECTIONS ,
FIGURES ,
REFERENCES ,
CITATIONS
Abstract
Behaviors of internal inertio-gravity waves (IIGW)
near Jones' critical levels are studied theoretically
in view of a possible origin of turbulence layers in the middle atmosphere.
The inertial effect associated with the earth's rotation cannot be neglected
when time constant of the wave is large.
Assuming that the vertical shear and Coriolis factor are constant,
exact solution of IIGW are obtained from inviscid and linear equations.
The asymptotic expressions are derived by means of
the Liouville-Green method developed by Olver (1974)
which leads to an exact dispersion relation near the critical levels.
Two important features about critical level problem of IIGW are found
from the dispersion relation:
valve effect across the Jones' critical levels
in somewhat different sense from Grimshaw (1975, 1980),
and presense of a pair of turning levels
between both Jones' critical levels.
Coupling these features,
we predict that IIGW is absorbed or reflected by the Jones' critical levels
depending on the directions of wave-front.
The absorption rate and the thickness of turbulence layer produced by
critical level breakdown increase as the wave-fronts tend to direct to
the zonal direction,
on the other hand IIGW is substantially reflected
when they direct to the meridional direction.
With increase of basic Richardson number the turning levels approach
asymptotically the critical levels,
so that turbulence layers inside the critical levels become thinner
than those outside them.
These features vanish in the course of non-inertial gravity waves.
The relation between IIGW and turbulence layers is calculated
to compare with the turbulence layers observed in the stratosphere
and to have information on IIGW's propagating upwards to the mesosphere
and thermosphere.
In general,
thickness of the turbulence layers associated with IIGW's is thinner
than that associated with non-inertial gravity waves
for common mesoscale wavelength domain.
Contents
- 1. Introduction
- 2. Equations and Solutions
- 2.1. Governing Equations
- 2.2. Exact Solutions
- 2.3. Asymptotic Solutions
- 3. Vertical Propagation of IIGW in a Shear Flow
- 3.1. Local Dispersion Relation
- 3.2. Propagation of IIGW far from the Critical Levels
- 3.3. Propagation in the Vicinity of Jones' Critical Levels
- 4. Wave Behaviors near Jones' Critical Levels
- 4.1. Valve Effect
- 4.2. Turning Levels
- 4.3. Wave Absorption Associated with Jones' Critical Levels
- 5. Formation of Turbulence Layers
- 5.1. Local Convective Instability
- 5.2. Turbulence Layers Generated by IIGW Breakdown
- 6. Conclusion
- Appendix A: Notations
- Appendix B: Treatment for f = 0
- Appendix C: Treatment for l = 0
- Appendix D: Liouville-Green Method
Developed by Olver (LGO Method)
- Appendix E: Examples of LGO Method
- Appendix F: Group Velocity
near Jones' Critical Level
Corrections and Additional Remarks
- Subsection 2.1 (p.3 left), Eq.(9):
Denominator of the second term must be read as
$\omega^{2} (\omega^{2} - f^{2})$
- Subsection 2.2 (p.3 right), Eq.(19):
- Caption of Fig.1 (p.5 left):
`The' must be printed as `the'.
- Subsection 2.3 (p.5 right):
The third case printed as (a) must be read as (c).
- Caption of Fig.2 (p.8):
`$u_{z}$' must be printed as `$\overline{u}_{z}$'.
- Caption of Fig.4 (p.10):
`with' must be inserted between `the basic flow'
and `the Jones' critical level'.
List of Figures
(No Tabales)
- Fig. 1.
Locations of turning levels for the basic Richardson number
$J (= N^{2} / \overline{u}_{z}^{2})$ parameterizing $\nu (= l / k)$.
- Fig. 2.
Local dispersion relation ($\omega$-$m$ diagram) for $\overline{u}_{z} < 0$
obtained by the LGO method.
- Fig. 3.
Vertical profile of $\Re [ \tilde{w} ]$ of IIGW for $\overline{u}_{z} < 0$
calculated from the asymptotic solution based on the LGO method.
- Fig. 4.
Schematic illustrations of the rays relative to the basic flow
with the Jones' critical level.
References
(Updated after publication)
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List of Original Papers
by M. D. Yamanaka
Bibliography
by any authors
M. D. YAMANAKA homepage (English)
E-mail : yamanaka@kurasc.kyoto-u.ac.jp