Temporal evolution of tritium-³He age in the North Atlantic : implications for thermocline ventilation
Temporal evolution of tritium-³He age in the North Atlantic : implications for thermocline ventilation
Date
1997-09
Authors
Robbins, Paul E.
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Date Created
Location
Eastern North Atlantic
DOI
10.1575/1912/5712
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Keywords
Thermoclines
Tritium dating
Oceanus (Ship : 1975-) Cruise OC52
Oceanus (Ship : 1975-) Cruise OC79
Oceanus (Ship : 1975-) Cruise OC202
Atlantis II (Ship : 1963-) Cruise AII107
Atlantis II (Ship : 1963-) Cruise AII109
Meteor (Ship) Cruise M56
Meteor (Ship) Cruise M64
Meteor (Ship) Cruise M69
Endeavor (Ship: 1976-) Cruise EN143
Tritium dating
Oceanus (Ship : 1975-) Cruise OC52
Oceanus (Ship : 1975-) Cruise OC79
Oceanus (Ship : 1975-) Cruise OC202
Atlantis II (Ship : 1963-) Cruise AII107
Atlantis II (Ship : 1963-) Cruise AII109
Meteor (Ship) Cruise M56
Meteor (Ship) Cruise M64
Meteor (Ship) Cruise M69
Endeavor (Ship: 1976-) Cruise EN143
Abstract
This thesis is a study of the physical mechanisms that ventilate the subtropical
thermocline of the eastern North Atlantic. The starting point is an analysis of the
existent historical database of natural and anthropogenic tracers, with special emphasis
on 3He and tritium, that can be used to infer rates of ventilation. If the flow is
predominantly advective, the temporal evolution of coupled transient tracers can be
used to define a tracer age which measures the elapsed time since a water parcel was
resident in the surface mixed layer. A principle finding is that the observed tracer
age shows a large and systematic change over time. Tritium-3He age in the eastern
Atlantic thermocline is seen to increase over time; the magnitude of the change is
greatest for the deeper, more slowly ventilated layers of the thermocline.
The first hypothesis examined is that the observed shift in the tracer age field
is the manifestation of a slackening of the physical ventilation. A time series of the
meridional geostrophic velocity shear in the eastern Atlantic shows no indication of a
change in the strength of the large-scale circulation. Uncertainty of the geostrophic
calculation due to data sparsity and mesoscale eddy contamination prevents conclusive
rejection of the hypothesis of a changing circulation. There are other tracers which
offer useful clues: comparison of the tritium-3He age field with dissolved oxygen
reveals a temporal trend in the property-property correlation. The spatial structure of
the oxygen field, however, shows no long-term evolution over time. From this line of
evidence it is concluded that the physical ventilation of the thermocline has not altered
over time and, therefore, the temporal change in the tritium-3He age field must be the
signal of the tritium invasion itself. A second hypothesis, which analysis shows is more consistent with the observations,
is that the changing tracer age is a consequence of mixing effects in the
ventilation of 3He and tritium. Numerical simulations of the thermocline ventilation of
3H and 3He are performed to examine the steadiness of the tracer age field under different
advective-diffusive regimes. A one-dimensional model is constructed based on the assumption that the totality of the fluid in the thermocline derives from subduction
out of the surface mixed layer. The temporal behavior of the tracer age field is found
to be dependent on the radiotracer Peclet number, which measures the ratio of the
diffusive and advective time scales. In a model with steady circulation, the observed
temporal behavior of the tracer age field can be reproduced only when the effects of
lateral mixing play a significant role in the process of ventilation. The vertical structure
and magnitude of the implied lateral diffusivity are, however, inconsistent with
other observations. The numerical simulations are next extended to two-dimensions
to allow for the presence of a pool of unventilated, re-circulated water within the
anti-cyclonic, subtropical gyre. Comparison of the model with the observed transient
tracer field in the lower thermocline shows consistency with conventional estimates of
lateral mixing rates only when the diffusively ventilated "pool" region extends across
the entire zonal domain of the gyre. In contrast, the transient tracer fields in the upper
portion of the thermocline are best reproduced when the isopycnal surfaces are ventilated
by advection directly from the surface mixed layer. The results obtained here
are consistent with numerical simulations which reveal a prominent role for mesoscale
eddies in the ventilation of the thermocline.
Description
Submitted in partial fulfillment of the requirements for the degree of Doctor of Philosophy at the Massachusetts Institute of Technology and the Woods Hole Oceanographic Institution September 1997
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Citation
Robbins, P. E. (1997). Temporal evolution of tritium-³He age in the North Atlantic : implications for thermocline ventilation [Doctoral thesis, Massachusetts Institute of Technology and Woods Hole Oceanographic Institution]. Woods Hole Open Access Server. https://doi.org/10.1575/1912/5712