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Parametric subharmonic instability and the β-effect Chan, Ian
Abstract
Parametric subharmonic instability (PSI) is a nonlinear interaction between a resonant triad of waves, in which energy is transferred from low wavenumber, high frequency modes to high wavenumber, low frequency modes. In the ocean, PSI is thought to be one of the mechanisms responsible for transferring energy from M₂ internal tides (internal gravity waves with diurnal tidal frequency) to near-inertial waves (internal gravity waves with frequency equal to the local Coriolis frequency) near the latitude of 28.9 degrees. Due to their small vertical scale, near-inertial waves generate large vertical shear and are much more efficient than M₂ internal tides at generating shear instability needed for vertical mixing, which is required to maintain ocean stratification. The earlier estimate of the time-scale for the instability is an order of magnitude larger than the time-scale observed in a recent numerical simulation (MacKinnon and Winters) (MW). An analytical model was developed by (Young et al. 2008) (YTB), and their findings agreed with the MW estimation; however as YTB assumed a constant Coriolis force, the model cannot explain the intensificaiton of PSI near 28.9 degrees as observed in the model of MW; in addition, the near-ineartial waves can propagate a significant distance away from the latitude of 28.9 degrees. This thesis extends the YTB model by allowing for a linearly varying Coriolis parameter (β-effect) as well as eddy diffusion. A linear stability analysis shows that the near-inertial wave field is unstable to perturbations. We show that the β-effect results in a shortening in wave length as the near-inertial waves propagate south; horizontal eddy diffusion is therefore enhanced to the south, and limits the meridional extent of PSI. The horizontal diffusion also affects the growth rate of the instability. A surprising result is that as the horizontal diffusion vanishes, the system becomes stable; this can be demonstrated both analytically and numerically. Mathematically, the β-effect renders the spatial differential operator nonnormal, which is characterized with the aid of pseudo-spectra. Our results suggest the possibility of large amplitude transient growth in near-inertial waves in regimes that are asymptotically stable to perturbations.
Item Metadata
Title |
Parametric subharmonic instability and the β-effect
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Creator | |
Publisher |
University of British Columbia
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Date Issued |
2010
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Description |
Parametric subharmonic instability (PSI) is a nonlinear interaction between a resonant
triad of waves, in which energy is transferred from low wavenumber, high
frequency modes to high wavenumber, low frequency modes. In the ocean, PSI is
thought to be one of the mechanisms responsible for transferring energy from M₂
internal tides (internal gravity waves with diurnal tidal frequency) to near-inertial
waves (internal gravity waves with frequency equal to the local Coriolis frequency)
near the latitude of 28.9 degrees. Due to their small vertical scale, near-inertial waves
generate large vertical shear and are much more efficient than M₂ internal tides at
generating shear instability needed for vertical mixing, which is required to maintain
ocean stratification.
The earlier estimate of the time-scale for the instability is an order of magnitude
larger than the time-scale observed in a recent numerical simulation (MacKinnon and Winters) (MW). An analytical model was developed by (Young et al. 2008) (YTB), and their findings agreed with the MW estimation; however as YTB assumed a constant Coriolis force, the model cannot explain the intensificaiton of PSI near 28.9 degrees as observed in the model of MW; in addition, the
near-ineartial waves can propagate a significant distance away from the latitude of
28.9 degrees.
This thesis extends the YTB model by allowing for a linearly
varying Coriolis parameter (β-effect) as well as eddy diffusion. A linear stability analysis shows that the near-inertial wave field is
unstable to perturbations. We show that the β-effect results in a shortening in
wave length as the near-inertial waves propagate south; horizontal eddy diffusion
is therefore enhanced to the south, and limits the meridional extent of PSI. The
horizontal diffusion also affects the growth rate of the instability. A surprising
result is that as the horizontal diffusion vanishes, the system becomes stable; this
can be demonstrated both analytically and numerically.
Mathematically, the β-effect renders the spatial differential operator nonnormal, which is characterized with the aid of pseudo-spectra. Our results suggest the possibility of large amplitude transient growth in near-inertial
waves in regimes that are asymptotically stable to perturbations.
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Genre | |
Type | |
Language |
eng
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Date Available |
2010-09-03
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Provider |
Vancouver : University of British Columbia Library
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Rights |
Attribution-NonCommercial-NoDerivs 3.0 Unported
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DOI |
10.14288/1.0071275
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URI | |
Degree | |
Program | |
Affiliation | |
Degree Grantor |
University of British Columbia
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Graduation Date |
2010-11
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Campus | |
Scholarly Level |
Graduate
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Rights URI | |
Aggregated Source Repository |
DSpace
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Rights
Attribution-NonCommercial-NoDerivs 3.0 Unported