Changes in Stratospheric Winds May Not Have a Large Impact on Long-Term Changes in Tropospheric Ozone

New NASA research on natural ozone cycles suggests ozone levels in the lowest part of Earth's atmosphere probably won't be affected much by projected future strengthening of the circulating winds that transport ozone between Earth's two lowest atmospheric layers.

Astronauts aboard the International Space Station captured this photograph of Earth's atmospheric layers on July 31, 2011, revealing the troposphere (orange-red) to the stratosphere and above. Earth-observing instruments in space allow scientists to better understand the chemistry and dynamics occurring within and between these layers. Credit: NASA/JSC Gateway to Astronaut Photography of Earth

The finding is good news, since human and plant health are harmed by exposure to ozone near the ground. Significant increases in ozone in Earth's lowest atmospheric layer, the troposphere, would also lead to additional climate warming because ozone is a greenhouse gas.

The research, which studied the natural ups and downs in ozone in the troposphere and stratosphere, increases our ability to reliably predict future changes in ozone in Earth's troposphere. This information is useful for developing effective air quality and climate policies.

Jessica Neu, an atmospheric scientist at NASA's Jet Propulsion Laboratory in Pasadena, Calif., and colleagues used NASA satellite observations to show that short-term periodic strengthening and weakening of circulating winds in Earth's stratosphere -- the layer right above the troposphere -- account for about half of the observed year-to-year changes in the amount of tropospheric ozone in Earth's northern mid-latitudes. Those are the same latitudes where North America, most of Europe and Central Asia are located. In a first-of-its-kind estimate, they calculated that a 40-percent change in the strength of stratospheric winds increases tropospheric ozone levels by an average of about two percent over Earth's northern mid-latitudes at an altitude of about 16,000 feet (5,000 meters). Results are published this month in the journal Nature Geoscience.

While a two-percent change in ozone is small, it does represent a significant natural variation in tropospheric ozone, which has large seasonal changes but only varies by about four percent from year to year at these altitudes in Earth's northern mid-latitudes. As the human contribution to ozone levels evolves due to increased development and stricter air quality controls, the relative importance of natural sources of tropospheric ozone such as the stratosphere will also shift.

Global climate models project the stratospheric circulating winds of particular interest to Neu and colleagues are expected to strengthen by about 30 percent over the coming century in response to increased greenhouse gas emissions, but the impacts on tropospheric ozone had been highly uncertain.

"If the correlations between tropospheric ozone and changing stratospheric circulation found in this study hold true in the future, the small changes in tropospheric ozone we measured show it's unlikely the projected long-term changes in stratospheric winds will have a big impact on long-term changes in tropospheric ozone in the future," said Neu.

The researchers studied changes in the well-established global wind circulation of the stratosphere. Like water in a fountain, winds in the tropics rise up, move toward Earth's poles, and then descend over middle and high latitudes. In these regions, the descending air carries ozone-rich air from the stratosphere to the troposphere.

To quantify how ozone responds to changes in wind circulation, Neu and colleagues investigated two natural phenomena known to contribute to shorter-term circulation changes: the El Niño/Southern Oscillation and the stratospheric Quasi-Biennial Oscillation. The study focused on the northern mid-latitudes because that is where most stratospheric ozone enters the troposphere.

The researchers used water vapor measurements from the Microwave Limb Sounder (MLS) instrument on NASA's Aura satellite from 2005 to 2010 to infer wind circulation changes driven by these two natural phenomena. They compared the magnitude and timing of those changes with measurements of stratospheric and tropospheric ozone from Aura's MLS and Tropospheric Emission Spectrometer (TES) instruments, respectively. JPL developed and manages both instruments.

"This sort of study is exciting because it reveals connections between the stratosphere and troposphere on timescales of a few years, with implications for connections on multi-decadal -- or longer -- timescales," said Anne Douglass, Aura project scientist at NASA's Goddard Space Flight Center in Greenbelt, Md. "The connections can be quantified only because the observational record from Aura instruments is long."

While the mechanisms that change wind circulation over the course of six months, such as the El Niño/Southern Oscillation, are different from those that change it over the course of a century, the difference "likely doesn't matter in terms of the impact on tropospheric ozone," Neu said. "This study gives us confidence that the impact in the future will be on the same order of magnitude -- around two percent."

NASA monitors Earth's vital signs from land, air and space with a fleet of satellites and ambitious and ground-based observation campaigns. NASA develops new ways to observe and study Earth's interconnected natural systems with long-term data records and computer analysis tools to better see how our planet is changing. The agency shares this unique knowledge with the global community and works with institutions in the United States and around the world that contribute to understanding and protecting our home planet.

For more information about NASA's Earth science activities in 2014, visit: http://www.nasa.gov/earthrightnow

For more information about NASA programs, visit: http://www.nasa.gov

For more information about MLS and TES, visit: http://mls.jpl.nasa.gov/index-eos-mls.php and http://tes.jpl.nasa.gov/

JPL is managed for NASA by the California Institute of Technology, Pasadena.

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