Coupled atmosphere-ocean general circulation models are the simplest models which
are capable of simulating both the variability which occurs within each component
of the climate system, and the variability which arises from the interactions between
them. Only recently has it become computationally feasible to use coupled general
circulation models to study climate variability and change on timescales of O(104)
years and longer. Flux adjustments are often employed to maintain a control climate
that is both stable and realistic; however, the magnitude of the adjustments
represents a source of concern.
This study employs the CSIRO Mk3L climate system model, a low-resolution
coupled atmosphere-sea ice-ocean general circulation model. The atmospheric and
oceanic components are spun up independently; the resulting atmospheric simulation
is realistic, while the deep ocean is too cold, too fresh and too buoyant. The
spin-up runs provide the initial conditions for the coupled model, which is used to
conduct a 1400-year control simulation for pre-industrial conditions. After some
initial adjustment, the simulated climate experiences minimal drift. The dominant
mode of internal variability is found to exhibit the same spatial structure and correlations
as the observed El Ni˜no-Southern Oscillation phenomenon.
The ability of Mk3L to simulate the climate of the mid-Holocene is evaluated. It
correctly simulates increased summer temperatures at northern mid-latitudes, and
cooling in the tropics. However, it is unable to capture some of the regional-scale
features of the mid-Holocene climate, with the precipitation over northern Africa
being deficient. The model simulates a 13% reduction in the strength of El Ni˜no,
a much smaller decrease than that implied by the palaeoclimate record.
A 1400-year transient simulation is then conducted, in which the atmospheric
CO2 concentration is stabilised at three times the pre-industrial value. The transient
simulation exhibits a reduction in the rate of North Atlantic Deep Water formation,
followed by its gradual recovery, and a cessation of Antarctic Bottom Water formation.
The global-mean surface air temperature warms 2.7◦C upon a trebling of
CO2, and 5.3◦C by the end of the simulation.
A number of modifications to the spin-up procedure for the ocean model are
evaluated. A phase shift in the prescribed sea surface temperatures and salinities is
found to reduce the phase lag between the model and observations, and to lead to
a reduction in the magnitude of the diagnosed flux adjustments. When this spin-up
run is used to initialise the coupled model, the reduced flux adjustments are found
to have negligible impact upon the nature of the internal variability. While the flux
adjustments are not found to have any direct influence upon the response of the
model to external forcing, they are found to have an indirect influence via their
effect upon the rate of drift within the control simulation.
An iterative spin-up technique is also developed, whereby the response of the
ocean model is used to derive a set of effective surface tracers. These result in a
much more realistic vertical density profile within the ocean. The coupled model
exhibits slightly increased internal variability, with reduced convection within the
ocean. There is a slightly greater surface warming in response to an increase in
the atmospheric CO2 concentration, with the reduced convection resulting in slower
penetration of the surface warming to depth.
| Identifer | oai:union.ndltd.org:ADTP/246223 |
| Creators | Phipps, SJ |
| Source Sets | Australiasian Digital Theses Program |
| Detected Language | English |
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