Buraco na camada de ozônio supera o tamanho registrado em 2007
outubro 8, 2008 1 Comentário
Buraco na camada de ozonio no dia 07/10/2008
Relatório da ESA, European Space Agency, afirma buraco na camada de ozônio superou o registrado em 2007, embora tenha sido menor do que recorde de 2006. A camada de ozônio é uma camada protetora atmosférica encontrada cerca de 25 quilômetros de altitude, atuando como um filtro solar, “blindando” a vida na Terra dos nocivos raios ultravioletas, que podem aumentar o risco de câncer de pele e catarata, além de prejudicar a vida marinha. Por Henrique Cortez*, do EcoDebate, com informações da ESA.
Em 2007a área da camada de ozônio, ao longo do Pólo Sul, alcançou 27 milhões de quilômetros quadrados, 2 milhões de quilômetros quadrados a mais do que os 25 milhões de quilômetros quadrados registrados em 2007. O recorde anterior ocorreu em 2006, quando o buraco atingiu a extensão de 29 milhões de quilômetros quadrados , tamanho equivalente ao continente norte-americano.
ESA 7 October 2008: The 2008 ozone hole – a thinning in the ozone layer over Antarctica – is larger both in size and ozone loss than 2007 but is not as large as 2006.
Ozone is a protective atmospheric layer found in about 25 kilometres altitude that acts as a sunlight filter shielding life on Earth from harmful ultraviolet rays, which can increase the risk of skin cancer and cataracts and harm marine life.
This year the area of the thinned ozone layer over the South Pole reached about 27 million square kilometres, compared to 25 million square kilometres in 2007 and a record ozone hole extension of 29 million square kilometres in 2006, which is about the size of the North American continent.
The depletion of ozone is caused by extreme cold temperatures at high altitude and the presence of ozone-destructing gases in the atmosphere such as chlorine and bromine, originating from man-made products like chlorofluorocarbons (CFCs), which were phased out under the 1987 Montreal Protocol but continue to linger in the atmosphere.
Ozone hole extension during the last 10 years
Depending on the weather conditions, the size the Antarctic ozone hole varies every year. During the southern hemisphere winter, the atmosphere above the Antarctic continent is kept cut off from exchanges with mid-latitude air by prevailing winds known as the polar vortex – the area in which the main chemical ozone destruction occurs. The polar vortex is characterized by very low temperatures leading to the presence of so-called stratospheric clouds (PSCs).
As the polar spring arrives in September or October, the combination of returning sunlight and the presence of PSCs leads to a release of highly ozone-reactive chlorine radicals that break ozone down into individual oxygen molecules. A single molecule of chlorine has the potential to break down thousands of molecules of ozone.
Julian Meyer-Arnek of the German Aerospace Centre (DLR), which monitors the hole annually, explained the impact of regional meteorological conditions on the time and range of the ozone hole by comparing 2007 with 2008.
“In 2007 a weaker meridional heat transport was responsible for colder temperatures in the stratosphere over the Antarctic, leading to an intensified formation of PSCs in the stratosphere,” Meyer-Arnek said. “Therefore, we saw a fast ozone hole formation in the beginning of September 2007.”
“In 2008 a stronger-than-usual meridional heat transport caused warmer temperatures in the Antarctic stratosphere than usual, reducing the formation of PSCs. Consequently, the conversion of chemically inactive halogens into ozone-destroying substances was reduced. As a result in the beginning of September 2008, the ozone hole area was slightly smaller than average,” he continued.
Chlorine activation and ozone hole extension
Chlorine activation early September 2008
“Since the polar vortex remained undisturbed for a long period, the 2008 ozone hole became one of the largest ever observed.”
Minimum values of the ozone layer of about 120 Dobson Units are observed this year compared to around 100 Dobson Units in 2006. A Dobson Unit is a unit of measurement that describes the thickness of the ozone layer in a column directly above the location of measurement.
DLR’s analysis is based upon the Scanning Imaging Absorption Spectrometer for Atmospheric Cartography (SCIAMACHY) atmospheric sensor onboard ESA’s Envisat, the Global Ozone Monitoring Experiment (GOME) aboard ESA’s ERS-2 and its follow-on instrument GOME-2 aboard EUMETSAT’s MetOp.
Scientists say that since the size and precise time of the ozone hole is dependent on the year-to-year variability in temperature and atmospheric dynamics, the detection of signs of ozone recovery is difficult.
“In order to detect these signs of recovery, a continuous monitoring of the global ozone layer and in particular of the Antarctic ozone hole is crucial,” Meyer-Arnek said.
Monthly averages of total ozone values
Average of total ozone values for September 2008
In order to train the next generation of atmospheric scientists to continue the monitoring, students at ESA’s Advanced Atmospheric Training Course, held 15–20 September at University of Oxford, UK, were given the task of analysing this year’s ozone hole with Envisat sensors.
Studying the Envisat data, the students’ findings were in line with atmospheric scientists that the south polar vortex was more concentric in 2008 than in 2007, leading to a relatively late onset of ozone depletion, and that the size of this year’s hole is similar to previous years.
“This exercise led us to realise that although many questions have been answered and much has been learned about the stratospheric chemistry and atmospheric dynamics driving ozone hole behaviour, many new questions must be raised especially concerning ozone hole recovery,” said Deborah C Stein Zweers, a post-doc satellite researcher from the Royal Netherlands Meteorological Institute (KNMI) who attended the course.
“We want to know when the ozone hole will recover, how its recovery will be complicated by an environment with increasing greenhouse gases and how atmospheric dynamics will shape future ozone holes. These and many other questions will attract the attention of our generation of scientists for the next several decades.”
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