Antarctic ozone hole similar to last year

The Antarctic ozone hole, which forms annually in the August to October period, reached its peak size on September 11, stretching to 9.3 million square miles (24.1 million square kilometers), roughly the same size as last year’s peak of 9.3 million square miles (24 million square kilometers) on September 16, 2013. This is an area similar in size to North America.

Ozone hole
This image, using NOAA satellite data, shows the ozone hole (areas below 220 Dobson units) in shades of red. (Credit: NOAA Visualization Lab; http://www.nnvl.noaa.gov/MediaDetail2.php?MediaID=1636&MediaTypeID=1)

In comparison, the largest ozone hole area recorded to date on a single day was on September 9, 2000, at 11.5 million square miles (29.9 million square kilometers). The ozone layer helps shield life on Earth from potentially harmful ultraviolet (UV) radiation that can cause skin cancer, damage plants and phytoplankton—the top of the oceanic food chain.

“The good news is that our measurements show less thinning of the ozone over the South Pole during the past three years,” said Bryan Johnson, a researcher with NOAA’s Earth System Research Laboratory in Boulder, Colorado. “However, the rate at which ozone thins during the month of September has remained about the same for the past two decades. A decrease in this rate will be an important sign of recovery.”

South Pole balloon-borne ozonesonde observations measured a minimum amount of 120 Dobson Units of ozone this year on September 29. Ozonesonde measurements of 250 Dobson Units in August are common just before the rapid destruction of ozone in September.  NOAA releases about 50-60 ozonesonde balloons per year since 1986 to measure the ozone layer at the South Pole.  Over the last 50 years satellite and ground-based records over Antarctica show ozone column amounts ranging from 100 to 400 Dobson units, which translates to about 1 millimeter (1/25 inch) to 4 millimeters (1/6 inch) of ozone in a layer if all of the ozone were brought down to the surface.

The Antarctic ozone hole began making a yearly appearance in the early 1980s, grew in size through the 1980s and has been consistently large since 1990, with annual variability attributed to stratospheric meteorological conditions over Antarctica. The hole is caused by chlorine released by manmade chemicals called chlorofluorocarbons or CFCs that were extensively used as aerosol sprays and in refrigerators.

Ozonesonde release
NOAA Corps LTJG Joseph Phillips releases an ozonesonde that's attached to a helium balloon. The instrument will rise 18 miles into the atmosphere to measure the thickness of ozone. (Credit: Chet Waggoner, NOAA)

These chlorine compounds lead to ozone depletion in certain upper atmospheric conditions. These conditions are at their peak over Antarctica as the dark cold winter gives way to the Antarctic spring in September. Just before the sun rises over Antarctica, extremely cold temperatures in the stratosphere allow for polar stratospheric clouds to form, a rare event in the earth’s atmosphere, but a regular occurrence in the winter over Antarctica. Chemical reactions on the cloud particles convert stable chlorine compounds into unstable or reactive forms. The sun light triggers reactive chlorine and ozone chemistry that depletes ozone in a large volume over Antarctica.

Scientists first made the connection that CFCs were depleting the earth’s protective layer in 1974. In 1987, 46 nations, including the U.S., signed the Montreal Protocol, a landmark agreement to phase out production of ozone-depleting chemicals. The slow recovery of this ozone layer is one of the great international efforts to restore the planet from manmade damage.

The 2014 level of ozone depleting substances over Antarctica has declined about 9 percent below the 2000 recorded maximum. But CFCs can remain in the atmosphere for more than 50 years. The ozone layer above Antarctica likely will not return to its 1980 state until about 2070, said Paul Newman, chief scientist for atmospheres at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. Climate change may also affect the rate of ozone recovery by cooling the stratosphere, which can slow Antarctic ozone recovery.

“Year-to-year weather variability significantly impacts Antarctica ozone because warmer stratospheric temperatures can reduce ozone depletion,” said Paul A. Newman, chief scientist for atmospheres at NASA's Goddard Space Flight Center in Greenbelt, Maryland. “The ozone hole area is smaller than what we saw in the late-1990s and early 2000s, and we know that chorine levels are decreasing. However, we are still uncertain about whether a long-term Antarctic stratospheric temperature warming might be reducing this ozone depletion.”

Under the mandate of the Clean Air Act, NOAA and NASA scientists keep a close eye on the ozone layer’s health with satellite data, ground-based measurements and instruments sent up through the ozone layer via balloons. Together, these instruments provide a big picture of the thickness and area extent of the ozone hole. NOAA measures the thickness of the ozone using ground-based instruments and by sending balloons with measurement devices up 18 miles into the atmosphere from NOAA’s Antarctic station.

NOAA and NASA also use data taken by the Ozone Mapping Profiler Suite (OMPS) instrument on board the Suomi-National Polar-Orbiting Partnership satellite to monitor the earth’s ozone layer. This instrument replaced the NOAA Solar Backscatter UltraViolet/2 ozone profiler and NASA Total Ozone Mapping Spectrometer.  NOAA’s Climate Prediction Center has been monitoring the Earth’s ozone layer for over 30 years, analyzing ozone concentration at various altitudes in the ozone layer as well as the total column amount of ozone. These measurements provide a three dimensional perspective of the ozone layer. This provides the means to monitor the ozone layer’s health and to make sure it is on the road to recovery.

Source: NOAA

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NOAA joins with Princeton and other institutions in six-year study to help public better understand Southern Ocean

NOAA is one of 10 institutions working together on the Southern Ocean Carbon and Climate Observations and Modeling program, or SOCCOM, a six-year, $21 million initiative to improve our understanding of the importance and health of the Southern Ocean encircling Antarctica. (Image by Oscar Schofield, Rutgers University)

The Southern Ocean that encircles Antarctica lends a considerable hand in keeping Earth's temperature hospitable by soaking up half of the human-made carbon in the atmosphere and a majority of the planet's excess heat. Yet, the inner workings — and global importance — of this ocean that accounts for 30 percent of the world's ocean area remains relatively unknown to scientists, as observations remain hindered by dangerous seas.

NOAA is one of 10 institutions working together on the Southern Ocean Carbon and Climate Observations and Modeling program, or SOCCOM, a six-year, $21 million initiative to improve our understanding of the importance and health of the Southern Ocean encircling Antarctica. (Image by Oscar Schofield, Rutgers University)

Princeton University, NOAA and eight other partner institutions now seek to make the Southern Ocean better known scientifically and publicly through a $21 million program that will create a biogeochemical and physical portrait of the ocean using hundreds of robotic floats deployed around Antarctica and an expanded computational capacity. The Southern Ocean Carbon and Climate Observations and Modeling program, or SOCCOM, is a six-year initiative headquartered at Princeton and funded by the National Science Foundation’s Division of Polar Programs, with additional support from the NOAA and NASA. The U.S. Argo program, led by CPO's Steven Piotrowicz, will play a major role in the project. 

"The scarcity of observations in the Southern Ocean and inadequacy of earlier models, combined with its importance to the Earth's carbon and climate systems, means there is tremendous potential for groundbreaking research in this region," Sarmiento said.
Central to the program are roughly 200 floats outfitted with biogeochemical sensors that will provide almost continuous information related to the ocean's carbon, nutrient (nitrate, in particular) and oxygen content, both at and deep beneath the surface. The floats are augmented biogeochemical versions of the nearly 4,000 Argo floats deployed worldwide to measure ocean salinity and temperature. SOCCOM marks the first large-scale deployment of these biogeochemical floats.

"These floats are revolutionary and this major new observational initiative will give us unprecedented year-round coverage of biogeochemistry in the Southern Ocean," Sarmiento said.

The Southern Ocean research will involve using Argo type floats equipped with new sensors that measure pH, nitrates in addition to temperature and salinity. (NOAA)

The floats will increase the monthly data currently coming out of the Southern Ocean by 10 to 30 times, Sarmiento said. That data will be used to improve recently developed high-resolution earth-system models, which will allow for a better understanding of the Southern Ocean and for better projections of Earth’s climate and biogeochemical trajectory. In keeping with SOCCOM's knowledge sharing, or "broader impacts," component, all the information collected will be freely available to the public, researchers and industry.

SOCCOM will provide direct observations to further understand the importance of the Southern Ocean as suggested by models and ocean studies. Aside from carbon and heat uptake, models have indicated that the Southern Ocean delivers nutrients to lower-latitude surface waters that are critical to ocean ecosystems around the world. In addition, the impacts of ocean acidification as levels of carbon dioxide in atmosphere increase are projected to be most severe in the Southern Ocean.

Other than administering the project, Sarmiento and other Princeton researchers will co-lead the modeling and broader impacts components, as well as coordinated data management. Researchers from NOAA's Geophysical Fluid Dynamics Laboratory housed on Princeton's Forrestal Campus will carry out high-resolution earth-system simulations in support of the modeling effort, which is led by the University of Arizona and includes collaborators from the University of Miami.

The floats will be constructed at the University of Washington with sensors from the Monterey Bay Aquarium Research Institute; NOAA’s Climate Program Office will provide half of the basic Argo floats. Float deployment, observation analysis and data assimilation will be led by the Scripps Institution of Oceanography at the University of California-San Diego. Climate Central, a non-profit science and journalism organization based in Princeton, will oversee the broader-impacts component. Researchers from Oregon State University and NOAA will develop the floats’ carbon algorithms.

“The SOCCOM effort is the first systematic expansion of the US Argo program into biogeochemistry. The unique subsurface ocean observations from SOCCOM will contribute towards our efforts to observe the global oceans,” said David Legler, director of NOAA’s Climate Observations Division.

In addition, NASA will support a complementary project involving researchers at the University of Maine and Rutgers University that will equip the floats with bio-optical sensors intended to gather data about biological processes in the water column.

This web story was written by Morgan Kelly, science writer for Princeton University, and includes an additional quote from NOAA's David Legler

Source: NOAA

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March of the penguin genomes

Adélie penguins.
Credit: David Lambert

Two penguin genomes have been sequenced and analyzed for the first time in the open access, open data journal GigaScience. Timely for the holiday season, the study reveals insights into how these birds have been able to adapt to the cold and hostile Antarctic environment.

Antarctic penguins are subject to extremely low temperatures, high winds, and profound changes in daylight. They have developed complicated biological systems to regulate temperature and store energy for long-term fasting. Most studies have focused on the physiological and behavioral aspects of their biology, but an international team of researchers has now analyzed the DNA of two Antarctic penguins (Adélie and emperor) relative to other bird species, revealing the genetic basis of their adaptations and their evolutionary history in response to climate change.

Using the historical genetic record within the DNA across bird species, the researchers estimate that penguins first appeared around 60 million years ago. The study shows that the Adélie penguin population increased rapidly about 150,000 years ago when the climate became warmer, but later declined by 40% about 60,000 years ago during a cold and dry glacial period. In contrast, the emperor penguin population remained stable, suggesting that they were better adapted to glacial conditions, for example, by being able to protect their eggs from freezing temperatures and incubate them on their feet.

Cai Li, Team Lead at BGI-Shenzhen, China, said: "These different patterns in historical population change also suggest that future climate change may have impacts on the two penguin species. For example, the fact that emperor penguins didn't experience the same population boom as Adélie penguins in warm climates means that they could suffer more from global warming, and this needs to be considered in conservation efforts in Antarctica."
Both penguins were found to have expanded genes related to beta-keratins -- the proteins which make up 90% of feathers. They also had at least 13 genes responsible for a single type of beta-keratin, which is the highest number compared to all other known bird genomes. This would explain their importance in ensuring that penguin feathers are short, stiff and densely packed to minimize heat loss, remain waterproof and aid underwater flight. Likely to be responsible for penguins' thick skin, the team also identified a gene called DSG1, which is known to be involved in a human dermatological disease characterized by thick skin on the palms and soles.

Fat storage is critical for penguins to withstand the cold and survive long fasting periods -- up to four months in emperor penguins. The two penguins were found to have exploited different adaptations for lipid metabolism in the course of their evolution, which may also provide insight into their contrasting abilities for coping with climate change. The researchers found eight genes involved in lipid metabolism in the Adélie penguin, and three in the emperor penguin.

During their evolutionary history, the wings (or forelimbs) of penguins changed profoundly for wing-propelled diving in the water. The team identified 17 forelimb-related genes in the penguin genomes that had unique changes. One of the genes in particular, EVC2, showed a larger number of genetic changes compared to other birds. Mutations of EVC2 in humans cause Ellis-van Creveld syndrome, characterized by short-limb dwarfism and short ribs.
Guojie Zhang, Assistant Professor at the University of Copenhagen and Associate Director at China National GeneBank, BGI-Shenzhen, China, said: "Penguins show distinct evolution relative to other bird species. They can't fly, have specialized skin and feathers, degenerated wings, and live in a cold environment in which most other birds could not survive. 

Comparative genomics is a powerful tool for providing answers on the molecular basis of these evolutionary changes and how organisms deal with the conditions they are exposed to. Our study has revealed several of these secrets for the two penguins."

David Lambert, Professor of Evolutionary Biology at Griffith University, Australia, said: "Although Adélie and Emperor penguins both breed on the Antarctic continent, they do so in very different ways. By sequencing the genomes of two penguin species we have been able to compare many of the genes that are responsible for these different abilities to do the same thing -- namely to survive and breed in Antarctica. This study is particularly important because it now provides us with the opportunity to conduct large scale evolutionary studies of both species."

These papers are part of a series of reports from the Avian Phylogenomics Project that are being published in concert in multiple journals. The authors of several Science papers will unveil new genomic results related to the avian tree of life, and a number of papers are also published in BMC Genomics, BMC Evolutionary Biology and Genome Biology.

Avian Genome Collection on BioMed Central: http://www.biomedcentral.com/series/avian

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