1 - Instituto de Biologia da UFRJ
1 - Instituto de Biologia da UFRJ
1 - Instituto de Biologia da UFRJ
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Team Lea<strong>de</strong>r<br />
Dr. Neusa Maria Paes Leme – CRN/INPE<br />
Vice-Team Lea<strong>de</strong>r<br />
Dr. Emília Correia – INPE/CRAAM<br />
Introduction<br />
The monitoring of the Antarctic atmosphere and ocean<br />
and their influence on South America is being built on<br />
a consoli<strong>da</strong>ted basis as continuous studies have been<br />
un<strong>de</strong>rtaken by Brazilian researchers in the Antarctic region<br />
for <strong>de</strong>ca<strong>de</strong>s. The i<strong>de</strong>a is to give continuity to these studies,<br />
which require long-term series, for a better un<strong>de</strong>rstanding<br />
of global changes, and to use the <strong>da</strong>ta in numerical mo<strong>de</strong>ls<br />
of climate and weather forecasting so more trustworthy<br />
forecasts can be done. The mentioned projects, because<br />
they were not being consi<strong>de</strong>red as monitoring activities<br />
over the years, have always been un<strong>de</strong>r the threat of<br />
interruption. More than two <strong>de</strong>ca<strong>de</strong>s of continuous studies<br />
on the ozone hole and on the influence of Antarctic cold<br />
fronts on our climate, besi<strong>de</strong>s other highly relevant studies,<br />
must, therefore, have their continuity guaranteed. It is<br />
essential that such activities are associated with a long term<br />
monitoring program.<br />
Antarctica plays an essential role in the thermal<br />
equilibrium of the planet. In relation to South America<br />
this is especially relevant. The climate of the Southern<br />
hemisphere is essentially controlled by air masses originated<br />
from the frozen continent.<br />
It is well known that the energy, which comes from the<br />
Sun, is not constant and can cause variation on the earth’s<br />
climate, on global meteorology, and on the environment.<br />
Recent studies have shown that solar radiation can alter<br />
the physical-chemical properties of the atmosphere and<br />
can influence the wind regime and the amount of UV<br />
radiation, which reaches the earth’s surface, as well as the<br />
cloud coverage and precipitation.<br />
The un<strong>de</strong>rstanding of the interaction between the<br />
chemistry of the atmosphere and climate change is a new<br />
and instigating research area. The connection between<br />
atmosphere and solar radiation, especially UV, which<br />
triggers the chemical reactions and these, in their turn,<br />
<strong>de</strong>pend on the temperature, atmospheric circulation<br />
and climate, are now been studied in an integrated and<br />
systematic manner.<br />
New questions are arising with the observed changes<br />
on the atmospheric temperature profile, especially with<br />
the increase on the troposphere (near surface, as a result of<br />
green house gases) and the <strong>de</strong>crease of the low stratosphere<br />
(between 15 and 20 Km, because of the <strong>de</strong>struction of<br />
ozone hole) and of the mesosphere (between 90 and 100<br />
km, cause attributed to the increase of green house gases).<br />
The main questions are: What are the chemical changes<br />
that are occurring in the different layers of the atmosphere<br />
with increase of UV radiation and changes in temperature?<br />
What are the consequences for the dynamic, circulation and<br />
equilibrium between the atmospheric layers?<br />
Objectives<br />
Monitor and Evaluate<br />
Changes in chemistry and atmospheric dynamics and its<br />
influence on climate, involving: the interaction Sun – Earth,<br />
the temperature in the mesosphere, planetary waves, the<br />
Hole in the Ozone, trace gas associated with the chemistry<br />
of the ozone layer, greenhouse effect emissions, greenhouse<br />
gases caused by human activity in the area of the Brazilian<br />
Antarctic Station Coman<strong>da</strong>nte Ferraz (EACF, Portuguese<br />
acronym, from now on) and the impacts of UV radiation<br />
in the ecosystem.<br />
Activities Developed<br />
The activities of Thematic Area 1 are divi<strong>de</strong>d into five<br />
themes:<br />
1. Sun-Earth Relationship<br />
2. Dynamics of Upper Atmosphere (Mesosphere)<br />
3. Climatology of Ozone and UV Radiation<br />
4. Meteorology<br />
5. Greenhouse gases and aerosols<br />
Science Highlights - Thematic Area 1 |<br />
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