The Meteorological Research Flight
(MRF) former aircraft (C-130) was one of six research aircraft that
participated in the second Aerosol Characterisation Experiment (ACE-2)
between June-July 1997 over the sub-tropical North Atlantic Ocean
between the Canary Islands and the Portuguese coast. ACE-2 was a follow-up
to ACE-1 that was conducted in unpolluted conditions near Tasmania.
ACE-2 was funded primarily by the European Union, but also by individual
national agencies, ultimately to assess the aerosol radiative forcing
over the North Atlantic region. The aircraft from the UK, France (Merlin
and Fokker 27), Germany (Dornier), Netherlands (Citation) and the
USA (Pelican) were based at Tenerife during the experiment and worked
together with ground-based sites and a Ukrainian research ship to:
- document the physical and chemical aerosol species and their
characteristics affecting the region;
- determine the physical and chemical processes controlling these
characteristics, the life cycles of the aerosol types and implications
for radiative transfer;
- assess the regional direct and indirect aerosol radiative forcing
in the region.
The major contribution of the MRF C-130 was to carry out three
Lagrangian experiments. These involved tagging a parcel of
air within the marine boundary layer (MBL) near the Portuguese coast
from the ACE-2 ship with a perfluorocarbon inert tracer gas and
constant-level smart balloons (fitted with GPS transponders). This
tagged air parcel was then followed over three back-to-back flights
that covered between 26-30 hours of evolution. This method is the
only effective way of determining the processes influencing aerosol
evolution, i.e. a Eulerian method of spot measurements in space
and time cannot reveal the processes at work. The first Lagrangian
was carried out in a very clean maritime air mass that had spent
more than five days over the North Atlantic. The other two were
within continental air masses originating over Europe.
As an example of the data collected with the C-130, Fig. 1 below
shows a series of three aerosol number-size distributions, one from
each of the Lagrangians, covering the particle diameter (D) range
50 nm 5.0 mm. The green curve shows a representative spectrum
from the first Lagrangian. It can be seen immediately that concentrations
are much lower than the other two polluted Lagrangians, except for
particles smaller than 0.04 mm which may be a result of new nucleation
in either the MBL or lower free troposphere (FT). The curve is bimodal
with the Aitken mode and accumulation mode lying at 0.03 and 0.2
mm, respectively. The lower end of the coarse mode (consisting of
sea-salt particles) can be seen above 1 mm. It is thought that this
bimodality is the result of cloud processing with particles above
this dip providing the cloud condensation nuclei (CCN) in stratocumulus
and weak cumulus clouds.
Figure 1. Aerosol number-size distributions
The red curve shows a representative aerosol size distribution
from the second Lagrangian. Concentrations are higher than the first
Lagrangian at sizes above 0.03 mm. This is because of the source
of particles over the European continent. The spectrum is bimodal
with the Aitken and accumulation modes at 0.06 and 0.03 mm, respectively.
These modes, together with the Hoppel dip in between, lie at a greater
size than during the first Lagrangian. This is probably because
the maximum supersaturation at cloud base is lower in a polluted
cloud than a clean one as a result of more activating cloud droplets
depleting the available water vapour and so limiting the attainable
supersaturation. Therefore, the critical cut-off size for CCN tends
to increase in a polluted cloud. In the first and second Lagrangians,
the aerosol spectrum in number terms is dominated by the Aitken
mode.
The blue curve shows a representative aerosol size distribution
from the third Lagrangian. One broad mode can be seen peaking at
0.1 mm, although there is a hint of a bulge at larger sizes that
constitutes the accumulation mode as particles grew slowly by coagulation
and other mainly non-cloudy processes over a number of days. The
accumulation mode does not protrude to sizes as large as the second
Lagrangian, probably due to the lack of cloud processing.
We have been able to put together a generalised description of
a European continental outbreak of pollution over the sub-tropical
North Atlantic from all the ACE-2 activities. Figure 2 shows a schematic
diagram of the main features of such an event:
Figure 2. Main features of a continental outbreak
of pollution over the sub-tropical North Atlantic
Over the continent, the surface heating in the summer months produces
a deep (2 to 5 km) convectively-driven continental boundary layer
(CBL). The anthropogenic pollution produced over the continent is
relatively well mixed throughout the CBL. When this is advected
over the relatively cold sea, the surface fluxes cause a new MBL
to form which rapidly grows as the air moves away from the coast.
Having lost the strong surface forcing, the CBL collapses under
the influence of the subsidence in the FT. The MBL grows within
the pollution layer and as the top of the MBL is generally very
stable a part of the pollution is trapped in a layer close to the
surface. The pollution associated with the residual CBL above the
top of the developing MBL will be differentially advected away as
there is generally a vertical wind shear associated with the temperature
inversion capping the MBL.
Eventually, the subsidence in the FT limits the growth of the MBL
(1 to 2 km) and clean tropospheric air can be entrained into the
MBL. It is this process which has the greatest effect on diluting
the pollution in the MBL and assisting in the evolution of the continental
air mass into a clean maritime air mass. Washout of the pollution
by drizzle produced by clouds in the MBL is thought to be minimal
as the high levels of pollution and soluble aerosol limit the size
of the cloud droplets below the size where coalescence can be effective.
The evolution of the MBL also has a modifying effect on the evolution
of the aerosol characteristics. As the air moves over progressively
warmer seas the MBL deepens and moisture builds up and stratocumulus
clouds form at the top of the MBL. If the MBL gets deep enough,
the generation of turbulent kinetic energy, either by wind shear
or cloud top cooling, may not be enough to maintain a well-mixed
MBL. The cloud layer then becomes decoupled from the moisture source
at the surface. The MBL can become layered with a well-mixed surface
layer and a layer containing the cloud. Moisture builds up in the
surface mixed layer (SML), it becomes conditionally unstable and
cumulus clouds will grow from the top, which will help maintain
the stratocumulus layer by locally supplying it with moisture.
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