LCDR David M. Ruth
Winter 2001
Naval Postgraduate School
Code 35
Monterey, CA 93943-5114
dmruth@nps.navy.mil
Operational Oceanography
OC3570
Potential Vorticity
Distribution along CALCOFI Line 67
1.
Introduction
Potential vorticity has been
shown to be useful in studies of large-scale ocean circulation. In an ideal fluid, potential vorticity is a
conserved quantity, and the fundamental equation governing the evolution of large-scale
ocean circulation is the potential vorticity equation. Keffer (1985) maps potential vorticity
within four different density layers for the North and South Atlantic, North
and South Pacific, and Indian Oceans, and uses these maps to evaluate the
character of the thermocline of the world’s oceans. Talley and McCartney (1982) infer the circulation of Labrador Sea
Water at mid-depths in the North Atlantic using potential vorticity as a water
mass tracer. Talley (1988) presents
vertical sections and maps of potential vorticity to give a three-dimensional
picture of circulation in the North Pacific Ocean.
In this study, a smaller
horizontal scale (O(100km)) is considered.
Potential vorticity is computed and contoured along CALCOFI Line 67, and
the structure of the water column along this transect is observed.
2.
Methods
a.
Collection
b.
Analysis
MATLAB 5.3 was used for all
data extraction, computation, and plotting.
For each station, raw CTD data values were scanned and plots were
inspected for “bad” data points (none were identified). A Hanning forward-and-backward filter was
applied to smooth the data. Several
filter widths were considered; the final width used for analysis (a 50-point
filter for each 500-point data set) was chosen as the best compromise of
feature resolution and noise suppression.
Potential vorticity, (f/ρ)dρ/dz,
was directly computed for each station using the “Buoyancy (Brunt-Väisälä)
Frequency” routine in MATLAB’s SEAWATER library. Plots and contours of temperature, salinity, density anomaly, and
potential vorticity were produced to evaluate the vertical structure along the
sampled section as discussed below. The
“truncation” of all the plots at the easternmost station is due to the partial
data set (121 vice 500 data points) at that location.
ADCP data, already averaged
in the available data set, were smoothed using MATLAB’s “pcolor” and “interp”
features, and alongshore current was plotted and evaluated in conjunction with
the potential vorticity analysis.
AVHRR satellite imagery for
the location and time of this experiment was also studied to identify any
surface features with distinct sea surface temperature signatures. Cloud cover was very limiting during this
time period, making only a few images useful for comparison with the other
data.
3.
Observations
a. Temperature
and salinity
For small changes in latitude, the influential variable in the calculation of potential vorticity is the fractional change in density with depth, ρ-1dρ/dz. Profiles (Figures 2 and 3) and contours (Figures 4 and 5) of temperature and salinity provide a glimpse of the overall density structure along the sample line. In general, the lowest surface temperatures and highest surface salinities are found closest to shore, with temperature increasing and salinity decreasing seaward (two anomalies in the surface salinity trend are discussed below). A strong thermocline is evident between 50 and 100 dbar; the halocline extends from about 50 to 150 dbar. At the station nearest to shore, the thermocline and halocline are weakest. Profiles of temperature and salinity statistics (Figure 6) show that horizontal variability of both parameters is greatest in the mixed layer. Contours of density anomaly (Figure 7) confirm the presence of a strong density gradient between 50 and 150 dbar west of 122˚W, as well as a weaker vertical density gradient closest to shore. From these observations, one would expect potential vorticity maxima at depths coinciding with the thermocline and halocline. Horizontal variability of potential vorticity, if any, should occur shallower than 150 dbar. Where the vertical density gradient is weakest (the easternmost stations), potential vorticity should be low.
b. Potential
vorticity
Contours of potential
vorticity (Figure 8, plotted down to 300 dbar) depict several features worthy
of discussion. Most prominent is the
potential vorticity “ridge” at about 60 dbar, with two well-defined local
maxima in the vicinity of longitudes 123˚40’W and 125˚00’W. This ridge coincides with the steep vertical
density gradient seen on the temperature, salinity, and density anomaly
plots. The potential vorticity graphic,
however, makes it much easier to identify precisely where the density gradient
is steepest (see overlay of potential vorticity and density anomaly contours,
Figure 9). An interesting question is
whether the two potential vorticity peaks are associated with any particular
flow feature(s). The horizontal extent
of the smaller peak is O(30km), while that of the larger is O(100km). Both peaks are larger than the internal
Rossby radius of deformation (Ri ≈ 10km), and thus it is reasonable that these anomalies
might identify a specific large-scale flow feature. Although no resolvable feature was evident in the study of
several satellite images covering the location and time of this experiment,
salinity contours and ADCP data both substantiate a flow anomaly associated
with these peaks. Specifically,
significant salinity minima (<33 psu, Figure 5) exist at shallow depths
exactly above the locations of the potential vorticity maxima. These salinity minima might be expected as a
result of advection of fresher surface water from the north. The ADCP data (Figure 10) confirm the presence
of two anomalous cores of southward flow (>30 cm/s) in the upper 50 dbar
above the potential vorticity maxima.
Little horizontal variation
in potential vorticity exists shallower than 30 dbar and deeper than 200 dbar,
as expected. Closest to shore (around
122˚W), potential vorticity is nearly constant with depth, in stark contrast
to the strong ridge evident to the west along the rest of the section. Near-shore upwelling significantly reduces
the vertical density gradient in the water column, and thus the vertical
“flatness” of potential vorticity in the east serves as an indicator of both
the strength and extent of this upwelling phenomenon.
4.
Discussion
a. Data
processing
An important objective of this study was to familiarize the student with the details and procedures of data collection and processing. The at-sea portion of this project gave me an immensely greater appreciation for the amount of work involved in obtaining a useful data set for study. Even more instructive was the task of meaningfully processing the data sets of interest. Some tasks were easier than expected: for example, the computation of potential vorticity was simplified by searching out and finding an existing MATLAB routine that performed the calculation directly. This prevented having to code a potential vorticity routine “from scratch.” More difficult than expected was the manipulation of data in its raw form to a matrix form that could be used for computation. Another challenge was finding the appropriate filter width and contour interval to best smooth the temperature and salinity data and display the potential vorticity results. Many filter width and contour interval combinations were run to find which suppressed as much noise as possible without sacrificing the resolution of important features. The selection of an “optimal” combination was fairly subjective. In the end, this exercise provided or built upon several skills which will be vital for any future scientific research in which I am involved.
b. Results
While potential vorticity is perhaps not the most intuitive
variable from which to infer ocean structure, the observations in this
experiment highlight some utility of this parameter. Contours of potential vorticity quantitatively identify the
distribution of density gradients in the water column. In this study, local maxima in the potential
vorticity field were correlated with flow features verified by salinity and
current data. Vertical potential
vorticity isopleths are expected where the water column is “well-ventilated,”
and in this study the column of nearly homogeneous potential vorticity
corresponds precisely to an upwelling region.
A possible area for further study would be to map potential vorticity
with depth over some horizontal area of interest (for example, the area bound
by 35N-38N and 122W-125W) and observe what three-dimensional structure is
represented. Overall, this brief study
suggests that potential vorticity analysis can be a useful approach to the
study of ocean circulation, even at scales as small as O(100km).
REFERENCES
Keffer, T., 1985: The Ventilation of the World’s Oceans: Maps of the Potential Vorticity
Field. J. Phys. Oceanogr., 15, 509-523.
Talley, L.D., 1988: Potential Vorticity Distribution
in the North Pacific. J. Phys.
Oceanogr., 18, 89-106.
Talley, L.D., and McCartney, M.S., 1982:
Distribution and Circulation of Labrador Sea
Water. J. Phys. Oceanogr., 12,
1189-1205.
FIGURES








