Instability and energetics in a baroclinic ocean
Citable URI
https://hdl.handle.net/1912/2468Location
28°N, 69°40'W32° 10'N, 64°30'W
DOI
10.1575/1912/2468Keyword
Rossby waves; Ocean waves; Wavemotion; Ocean currentsAbstract
This thesis is made of two separate, but interrelated parts.
In Part I the instability of a baroclinic Rossby wave
in a twolayer ocean of inviscid fluid without topography,
is investigated and its results are applied in the ocean.
The velocity field of the basic state (the wave) is characterized
by significant horizontal and vertical shears, nonzonal
currents, and unsteadiness due to its westward propagation.
This configuration is more relevant to the ocean
than are the steady, zonal 'meteorological' flows, which
dominate the literature of baroclinic instability. Truncated
Fourier series are used in perturbation analyses.
The wave is found to be unstable for a wide range of
the wavelength; growing perturbations draw their energy from
kinetic or potential energy of the wave depending upon
whether the wavelength, 2πL, is much smaller or larger than
2πLρ, respectively, where Lρ is the internal radius of deformation. When the shears are comparable dynamically,
L~Lρ , the balance between the two energy transfer processes is very sensitive to the ratios L/Lρ and U/C as well,
where U is a typical current speed, and C a typical phase
speed of the wave. For L = Lρ they are augmenting if
U < C, yet they detract from each other if U > C.
The betaeffect tends to stabilize the flow, but perturbations
dominated by a zonal velocity can grow irrespective
of the betaeffect.
It is necessary that growing perturbations are comprised
of both barotropic and baroclinic modes vertically.
The scale of the fastest growing perturbation is significantly
larger than L for barotropically controlled flows
(L < Lρ ), reduces to the wave scale L for a mixed kind
(L ~ Lρ ) and is fixed slightly larger than Lρ for baroclinically controlled flows (L > Lρ ).
Increasing supply of potential energy causes the normalized
growth rate, αL/U, to increase monotonically as
L → Lρ from below. As L increases beyond Lρ,
the growth rate αLρ /U shows a slight increase, but soon
approaches an asymptotic value.
In a geophysical eddy field like the ocean this model
shows possible pumping of energy into the radius of deformation
(~ 40 km rational scale, or 250 km wavelength) from
both smaller and larger scales through nonlinear interactions,
which occur without interference from the betaeffect.
The efolding time scale is about 24 days if
U = 5 cm/sec and L = 90 km. Also it is strongly suggested
that, given the observed distribution of energy versus
length scale, eddyeddy interactions are more vigorous than
eddymean interaction, away from intènse currents like the
Gulf Stream. The flux of energy toward the deformation
scale, and the interaction of barotropic and baroclinic
modes, occur also in fully turbulent 'computer' oceans, and
these calculations provide a theoretical basis for source of
these experimental cascades.
In Part II an available potential energy (APE) is defined
in terms appropriate to a limited area synoptic density
map (e.g., the 'MODEI' data) and then in terms appropriate
to timeseries of hydrographic station at a single geographic location (e. g., the 'Panulirus' data).
Instantaneously the APE shows highly variable spatial
structure, horizontally as well as vertically, but the vertical
profile of the average APE from 19 stations resembles
the profile of vertical gradient of the reference stratification.
The eddy APE takes values very similar to those of
the average kinetic energy density at 500 m, 1500 m and
3000 m depth in the MODE area.
In and above the thermocline the APE has roughly the
same level in the MODE area (centered at 28°N, 69° 40'W) as
at the Panulirus station (32° 10'N, 64° 30'W), yet in the
deep water there is significantly more APE at the Panulirus
station. This may in part indicate an island effect near
Bermuda.
Description
Submitted in partial fulfillment of the requirements for the degree of Doctor of Philosophy at the Massachusetts Institute and the Woods Hole Oceanographic Institution August 1975
Collections
Suggested Citation
Thesis: Kim, Kuh, "Instability and energetics in a baroclinic ocean", 197508, DOI:10.1575/1912/2468, https://hdl.handle.net/1912/2468Related items
Showing items related by title, author, creator and subject.

Understanding the ocean carbon and sulfur cycles in the context of a variable ocean : a study of anthropogenic carbon storage and dimethylsulfide production in the Atlantic Ocean
Levine, Naomi M. (Massachusetts Institute of Technology and Woods Hole Oceanographic Institution, 201002)Anthropogenic activity is rapidly changing the global climate through the emission of carbon dioxide. Ocean carbon and sulfur cycles have the potential to impact global climate directly and through feedback loops. Numerical ... 
Oceanic lithosphere magnetization : marine magnetic investigations of crustal accretion and tectonic processes in midocean ridge environments
Williams, Clare M. (Massachusetts Institute of Technology and Woods Hole Oceanographic Institution, 200709)The origin of symmetric alternating magnetic polarity stripes on the seafloor is investigated in two marine environments; along the ridge axis of the fast spreading East Pacific Rise (EPR) (9º 25’9º 55’N) and at Kane ... 
A study of ocean wave statistical properties using nonlinear, directional, phaseresolved ocean wavefield simulations
Henry, Legena Albertha (Massachusetts Institute of Technology and Woods Hole Oceanographic Institution, 201002)In the present work, we study the statistics of wavefields obtained from nonlinear phaseresolved simulations. The numerical model used to generate the waves models wavewave interactions based on the fully nonlinear ...