Showing posts with label Tropospheric temperatures. Show all posts

A. Luque & U. Ebert, Nature Geosci., Emergence of sprite streamers from screening-ionization waves in the lower ionosphere

Nature Geoscience, 2 (2009) 757-760; published online 25 October 2009; doi: 10.1038/ngeo662

Emergence of sprite streamers from screening-ionization waves in the lower ionosphere

Alejandro Luque1 and Ute Ebert1,2

Abstract

Sprite discharges above thunderclouds at altitudes of 40–90 km (refs 1, 2, 3, 4, 5) are usually created by a strong positive cloud-to-ground lightning flash6. Sometimes these sprite discharges emerge from a visible halo5, 7, 8, 9, and during the first stage they always propagate downwards and branch on their way5, 7, 9, 10, 11. Modelling efforts have been restricted to conditions of non-ionized air of constant density and show double-headed sprites12 or sprites starting from metal electrodes, but they do not explain why observations exclusively record sprites that propagate downwards. Here we present simulations with a numerical discharge model on a non-uniform, dynamically adapted computational grid13 to capture the wide range of emerging spatial scales, and we use realistic air and electron densities that vary with altitude. Our model shows a downward-propagating screening-ionization wave in the lower ionosphere that sharpens and collapses into a sprite streamer as it propagates farther down. Streamer velocity, diameter and length until branching agree with observations9 within measuring accuracy. We speculate that sprites generically emerge through the collapse of a wide screening-ionization wave into a sprite streamer, although this wave is only sometimes visible as a luminous halo.

¹Centrum voor Wiskunde en Informatica (CWI), PO Box 94079, 1090 GB Amsterdam, The Netherlands
²Department of Applied Physics, Eindhoven University of Technology, The Netherlands

Correspondence to: Alejandro Luque1 e-mail: luque@cwi.nl
Correspondence to: Ute Ebert1,2 e-mail: ebert@cwi.nl

Lightning storms at mid-latitudes and in the subtropics produce more nitrogen oxides (NOx) than previously thought

Nature Reports Climate Change, published online 12 November 2009; doi: 10.1038/climate.2009.117

Unlucky strike

by Stephanie Baudains

Unlucky strike
ISTOCKPHOTO / C. SPENCER
Lightning storms at mid-latitudes and in the subtropics produce more nitrogen oxides (NOx) than previously thought, finds a new study. What's more, most of the NOx pollution — a precursor to the greenhouse gas ozone — ends up in the upper troposphere, where it has a strong influence on climate.

A team led by Lesley Ott of NASA's Goddard Earth Sciences and Technology Center in Greenbelt, Maryland, used data collected during lightning storms in Germany and the United States between 1985 and 2002, along with a cloud simulation model, to estimate the amount of NOx produced by an average flash of lightning. They found that a single lightning strike produces about 7 kilograms of chemically reactive NOx. Worldwide, this amounts to an annual production of 8.6 million metric tonnes. As none of the data were collected in the tropics — where lightning may yield less NOx per flash — the global estimate may be on the high end, say the researchers.

They speculate, however, that if lightning storms become more frequent in the future, as predicted by some theoretical models, increased NOx in the upper atmosphere could affect global climate change.

See also:

Ott, L., K. Pickering, G. Stenchikov, D. Allen, A. DeCaria, B. Ridley, R.-F. Lin, S. Lang, and W.-K. Tao (2009), Production of lightning NOx and its vertical distribution calculated from 3-D cloud-scale chemical transport model simulations, J. Geophys. Res., doi: 10.1029/2009JD011880, in press.
[PDF] (accepted 15 October 2009)


Joseph Romm: NOAA -- Second hottest September on record and virtual tie for hottest in lower troposphere from satellite data

NOAA: Second hottest September on record and virtual tie for hottest in lower troposphere from satellite data

by Joseph Romm, Climate Progress blog, October 16, 2009

NOAA’s National Climatic Data Center has issued its latest monthly, “State of the Climate: Global Analysis,” which found:
The combined global land and ocean surface temperature for September 2009 was 0.62 °C (1.12 °F) above the 20th century average of 15.0 °C (59.0 °F). This was the second warmest September on record, behind 2005, and the 33rd consecutive September with a global temperature above the 20th Century average. The last below-average September occurred in 1976.
Significantly, September was only 0.04 °C (0.07 °F) off the 2005 record.

This near-record September comes fast on the heels of the second warmest August on record and warmest June-July-August for the oceans.  I previously noted that NASA reported hottest June to September on record.

What is most interesting about this report from the National Oceanic and Atmospheric Administration is the temperature report from the lower troposphere (“the lowest 8 km (5 miles) of the atmosphere”) — the satellite data that began in 1979 analyzed by the University of Alabama in Huntsville (UAH) and Remote Sensing Systems (RSS).

UAH and RSS say September was also the second warmest in their records — a mere 0.01 °C off the 1998 record.  NOAA reports that the lower troposphere warming trend for September is
  • +0.13 °C/decade (UAH)
  • +0.18 °C/decade (UAH
So yes, the satellite data also shows that the lower atmosphere is warming, contrary to what you may have heard.

In fact, the mid-troposphere (about 2-6 miles above the Earth, which includes a portion of the lower stratosphere) is also warming, according to both UAH and RSS.  It’s not warming quite as fast because as the lower troposphere in part “because the stratosphere has cooled due to increasing greenhouse gases in the troposphere and losses of ozone in the stratosphere.”

The global temperature anomaly for the month looked like this:
http://www.ncdc.noaa.gov/sotc/get-file.php?report=global&file=map-blended-mntp&year=2009&month=9&ext=gif
Although the United States as a whole was “1.0 °F above the 20th century average,” with record-tying temperatures in California, as usual the deniers had a few seemingly cool places in the country on which to feast.

We are still seeing staggering warming in some of the worst places from the perspective of the planet as a whole, the land of the the permafrost permamelt, which currently contains contains more carbon than the atmosphere (see here).

Again, what makes these record temps especially impressive is that we’re only in a weak El Niño, and we’re at “the deepest solar minimum in nearly a century,” according to NASA.

Stay tuned.  The heat is on — or, rather, it’s never been off.

Link:  http://climateprogress.org/2009/10/16/noaa-second-hottest-september-on-record-and-virtual-tie-for-hottest-in-lower-troposphere-from-satellite-data/

Steiner, Kirchengas, Lackner, Pirscher, Borsche, Foelsche, GRL 2009, Atmospheric temperature change detection with GPS radio occultation 1995-2008

Geophysical Research Letters, 36 (2009)  L18702; doi: 10.1029/2009GL039777.

Atmospheric temperature change detection with GPS radio occultation 1995 to 2008

A. K. Steiner, G. Kirchengas, B. C. Lackner, B. Pirscher, M. Borsche, and U. Foelsche (Wegener Center for Climate and Global Change and Institute for Geophysics, Astrophysics, and Meteorology, University of Graz, Graz, Austria)

Received 26 June 2009; accepted 26 August 2009; published 22 September 2009

Abstract

Existing upper air records of radiosonde and operational satellite data recently showed a reconciliation of temperature trends but structural uncertainties remain. GPS radio occultation (RO) provides a new high-quality record, profiling the upper troposphere and lower stratosphere with stability and homogeneity. Here we show that climate trends are since recently detected by RO data, consistent with earliest detection times estimated by simulations. Based on a temperature change detection study using the RO record within 1995–2008 we found a significant cooling trend in the tropical lower stratosphere in February while in the upper troposphere an emerging warming trend is obscured by El Niño variability. The observed trends and warming/cooling contrast across the tropopause agree well with radiosonde data and basically with climate model simulations, the latter tentatively showing less contrast. The performance of the short RO record to date underpins its capability to become a climate benchmark record in the future.

Steiner, A. K., G. Kirchengast, B. C. Lackner, B. Pirscher, M. Borsche & U. Foelsche (2009), Atmospheric temperature change detection with GPS radio occultation 1995 to 2008, Geophys. Res. Lett., 36, L18702; doi: 10.1029/2009GL039777.

Steven A. Cummer et al., Nature Geoscience, 2009, Quantification of the troposphere-to-ionosphere charge transfer in a gigantic jet

Nature Geoscience, published online 23 August 2009; doi: 10.1038/ngeo607

Quantification of the troposphere-to-ionosphere charge transfer in a gigantic jet

Steven A. Cummer1, Jingbo Li1, Feng Han1, Gaopeng Lu1, Nicolas Jaugey1, Walter A. Lyons2 and Thomas E. Nelson2

Abstract

Gigantic jets are the clearest manifestation of direct electrical coupling between tropospheric thunderstorms and the ionosphere. They are leaders1, 2, 3 that emerge from electrical breakdown near the top of thunderstorms4 and extend all the way to the lower edge of the ionosphere near 90-km altitude5. By contrast, blue jets6 and other related events7, 8 terminate at much lower altitudes. Gigantic jets have been observed from the ground5, 9, 10 and from orbit11. Some seem to be consistent with an upward-propagating negative discharge of 1,000-2,000 C km total charge moment change 9, but others have not been connected to distinguishable electromagnetic signatures10. Here we report simultaneous low-light video images and low-frequency magnetic field measurements of a gigantic jet that demonstrate the presence and dynamics of a substantial electric charge transfer between the troposphere and the ionosphere. The signatures presented here confirm the negative polarity of gigantic jets4 and constrain the lightning processes associated with them. The observed total charge transfer from the thunderstorm to the ionosphere is 144 C for the assumed channel length of 75 km, which is comparable to the charge transfer in strong cloud-to-ground lightning strokes.

¹Electrical and Computer Engineering Department, Duke University, Durham, NC 27708, U.S.A.

²FMA Research, Inc., Yucca Ridge Field Station, Fort Collins, CO 80524, U.S.A.

*Correspondence: Steven A. Cummer1 e-mail: cummer@ee.duke.edu

Link to abstract: http://www.nature.com/ngeo/journal/vaop/ncurrent/abs/ngeo607.html

Steven Cummer et al.: Gigantic jets blast electricity into upper atmosphere

Gigantic jets blast electricity into upper atmosphere

The gigantic jet observed by Steven Cummer and his team. The thunderstorm that produced this jet was over 300 kilometres away, below the visible horizon (Image: Steven Cummer)

The gigantic jet observed by Steven Cummer and his team. The thunderstorm that produced this jet was over 300 kilometres away, below the visible horizon (Image: Steven Cummer)

See YouTube video: Gigantic jets

by Michael Marshall, New Scientist, August 23, 2009

The ancient Greeks might have thought Zeus was furious with heaven itself. The power of lightning strikes that shoot upwards from storm clouds has been measured for the first time – and they turn out to be every bit as powerful as normal lightning.

First caught on camera in 2003, "gigantic jets" shoot upwards from thunderclouds and can reach altitudes above 80 kilometres. But it wasn't until 21 July last year that Steven Cummer at Duke University in Durham, North Carolina, and his colleagues managed to measure the electrical discharge from a single gigantic jet, released from tropical storm Cristobal.

"No one had been very close to one with the right radio instrumentation before," Cummer says. "So we didn't know whether they just petered out without doing anything much, or whether they actually took some charge and dumped it somewhere."

Electric jet

The jet came out of a high storm cloud, beginning at an altitude of about 14 kilometres, and shot upwards for a further 75 kilometres.

At those heights, the atmosphere is a much better electrical conductor than at ground level because of ionising radiation from space. As a result, the jet was able to discharge 144 coulombs of charge into the upper atmosphere in about 1 second.

This is comparable to the charge transferred by a large cloud-to-ground lightning strike.

"It's fantastic that they see such a high charge transfer between the thundercloud and the ionosphere," says Victor Pasko of Pennsylvania State University in University Park.

Changing weather

Gigantic jets could be important for our ability to predict lightning strikes.

"There is this newly identified path for discharging the thunderstorm, and a lot of charge can be moved," says Cummer. "In storms that can produce gigantic jets, it might influence what other lightning is happening in the storm."

This time, however, the team found no difference in the rate of ordinary lightning strikes around the time of the gigantic jet. "I'm surprised they saw no drop in lightning rates before or after the jet – but that might be because of the sheer size of the storm," says Pasko.

Gigantic jets are one of a host of new atmospheric phenomena discovered in recent years. Other examples are spritesMovie Camera and blue jets.

Journal reference: Nature Geoscience, DOI: 10.1038/ngeo607 (in press)

Link: http://www.newscientist.com/article/dn17664-gigantic-jets-blast-electricity-into-upper-atmosphere.html

D. M. Romps & Z. Kuang: Cyclones spurt water into stratosphere, feeding global warming

Cyclones spurt water into stratosphere, feeding global warming

ScienceDaily (April 21, 2009) — Scientists at Harvard University have found that tropical cyclones readily inject ice far into the stratosphere, possibly feeding global warming.

The finding, published in Geophysical Research Letters, provides more evidence of the intertwining of severe weather and global warming by demonstrating a mechanism by which storms could drive climate change. Many scientists now believe that global warming, in turn, is likely to increase the severity of tropical cyclones.

"Since water vapor is an important greenhouse gas, an increase of water vapor in the stratosphere would warm the Earth's surface," says David M. Romps, a research associate in Harvard's Department of Earth and Planetary Science. "Our finding that tropical cyclones are responsible for many of the clouds in the stratosphere opens up the possibility that these storms could affect global climate, in addition to the oft-mentioned possibility of climate change affecting the frequency and intensity of tropical cyclones."

Romps and co-author Zhiming Kuang, assistant professor of climate science in Harvard's Faculty of Arts and Sciences, were intrigued by earlier data suggesting that the amount of water vapor in the stratosphere has grown by roughly 50 percent over the past 50 years. Scientists are currently unsure why this increase has occurred; the Harvard researchers sought to examine the possibility that tropical cyclones might have contributed by sending a large fraction of their clouds into the stratosphere.

Using infrared satellite data gathered from 1983 to 2006, Romps and Kuang analyzed towering cloud tops associated with thousands of tropical cyclones, many of them near the Philippines, Mexico, and Central America. Their analysis demonstrated that in a cyclone, narrow plumes of miles-tall storm clouds can rise so explosively through the atmosphere that they often push into the stratosphere.

Romps and Kuang found that tropical cyclones are twice as likely as other storms to punch into the normally cloud-free stratosphere, and four times as likely to inject ice deep into the stratosphere.

"It is ... widely believed that global warming will lead to changes in the frequency and intensity of tropical cyclones," Romps and Kuang write in Geophysical Research Letters. "Therefore, the results presented here establish the possibility for a feedback between tropical cyclones and global climate."

Typically, very little water is allowed passage through the stratosphere's lower boundary, known as the tropopause. Located some 6 to 11 miles above the Earth's surface, the tropopause is the coldest part of the Earth's atmosphere, making it a barrier to the lifting of water vapor into the stratosphere: As air passes slowly through the tropopause, it gets so cold that most of its water vapor freezes out and falls away.

But if very deep clouds, such as those in a tropical cyclone that can rise through the atmosphere at speeds of up to 40 miles per hour, can punch through the tropopause too quickly for this to happen, they can deposit their ice in the warmer overlying stratosphere, where it then evaporates.

"This suggests that tropical cyclones could play an important role in setting the humidity of the stratosphere," Romps and Kuang write.

Romps and Kuang's research was funded by the Eppley Foundation and NASA.

Lu, Deser & Reichler: Cause of the widening of the tropical belt since 1958

Geophysical Research Letters, 36, L03803; doi:10.1029/2008GL036076.

Cause of the widening of the tropical belt since 1958

Jian Lu (Advanced Study Program, National Center for Atmospheric Research, Boulder, CO, USA; and Center for Ocean-Land-Atmosphere Studies, Calverton, MD, USA), Clara Deser (National Center for Atmospheric Research, Boulder, CO, USA), and Thomas Reichler (Department of Meteorology, University of Utah, Salt Lake City, UT, USA)

Abstract

Previous studies have shown that the width of the tropical belt has been increasing since at least the late 1970s based on a variety of metrics. One such metric, the frequency of occurrence of a high-altitude tropopause characteristic of the tropics, is used here to show that the observed widening of the tropics can be accurately replicated by an atmospheric general circulation model forced by the observed evolution of global SST and sea ice distributions as well as the direct radiative effects from both natural and anthropogenic sources. Contrasting this simulation with one forced by the observed SST and sea ice distributions alone reveals that the widening trend can be attributed entirely to direct radiative forcing, in particular those related to greenhouse gases and stratospheric ozone depletion. SST forcing causes no significant change in the width of the tropics, and even a contraction in some seasons.

(Received 22 September 2008, accepted 30 December 2008, published 5 February 2009.)

Lu, J., C. Deser, and T. Reichler (2009), Cause of the widening of the tropical belt since 1958, Geophys. Res. Lett., 36, L03803; doi:10.1029/2008GL036076.

Link to abstract: http://www.agu.org/pubs/crossref/2009/2008GL036076.shtml

D. Rind et al., Exploring the stratospheric/tropospheric response to solar forcing

Journal of Geophysical Research -- Atmospheres, 113, D24103; doi:10.1029/2008JD010114.

Exploring the stratospheric/tropospheric response to solar forcing

D. Rind (NASA Goddard Institute for Space Studies, Columbia University, New York, NY, USA), J. Lean (Naval Research Laboratory, Washington, DC, USA), and J. Lerner, P. Lonergan and A. Leboissitier (Center for Climate Systems Research, Columbia University, New York, NY, USA)

Abstract

We use the new Goddard Institute for Space Studies Global Climate Middle Atmosphere Model 3 with four different resolutions to investigate various aspects of solar cycle influence on the troposphere/stratosphere system. Three different configurations of sea surface temperatures are used to help determine whether the tropospheric response is due to forcing from above (UV variations impacting the stratosphere) or below (total solar irradiance changes acting through the surface temperature field). The results show that the stratospheric response is highly repeatable and significant. With the more active sun, the annual residual circulation change features relative increased upwelling in the Southern Hemisphere and downwelling in the Northern Hemisphere. Stratospheric west wind increases extend down into the troposphere, especially during Southern Hemisphere winter, and in some runs the jet stream weakens and moves poleward. The predominant tropospheric response consists of warming in the troposphere, with precipitation decreases south of the equator and in the Northern Hemisphere subtropics and midlatitudes, with increases north of the equator especially over southern Asia. The tropospheric response is often not significant, but is fairly robust among the different simulations. These features, which have been reported in observations and other model studies, appear to be driven both from the stratosphere and the surface; nevertheless, they account for only a small percentage of the total variance. More accurate simulations of the solar cycle stratospheric ozone response, the quasi-biennial oscillation, and coupled atmosphere-ocean dynamics are necessary before any conclusions can be deemed definitive.

(Received 12 March 2008, accepted 20 August 2008, published 16 December 2008.)

Citation: Rind, D., J. Lean, J. Lerner, P. Lonergan, & A. Leboissitier (2008), Exploring the stratospheric/tropospheric response to solar forcing, J. Geophys. Res., 113, D24103, doi:10.1029/2008JD010114.

Link to abstract: http://www.agu.org/pubs/crossref/2008/2008JD010114.shtml

D. H. Bromwich et. al., Surface and Mid-tropospheric Climate Change in Antarctica

AGU 2008 Fall Meeting

Abstract: C41A-0497

Surface and Mid-tropospheric Climate Change in Antarctica

D. H. Bromwich* (e-mail: bromwich.1@osu.edu; Byrd Polar Research Center, Ohio State University, 1090 Carmack Road, Columbus, OH 43210, U.S.A.),
A. J. Monaghan (e-mail: monaghan@ucar.edu; Research Applications Laboratory, National Center for Atmospheric Research, P.O. Box 3000, Boulder, CO 80307, U.S.A.), and S. R. Colwell (e-mail: src@bas.ac.uk; British Antarctic Survey, High Cross, Madingley Road, Cambridge, CB3 0ET, U.K.)

Near-surface air temperatures and 500-hPa temperatures over Antarctica for 1960-2007 have been reconstructed over the entire continent using manned station observations and radiosonde records, respectively, from the READER database maintained by British Antarctic Survey. The 50-year trends found in our near-surface temperature reconstruction agree with recent work by others using a variety of spatial extrapolation techniques. It is found that the statistically significant Antarctic Peninsula near-surface warming on an annual basis has spread into West Antarctica reaching as far as east as the Pine Island Bay-Thwaites Glacier region. The warming is most marked in recent years with 2007 being the warmest year in the 1960-2007 interval. In contrast to the western (eastern) Antarctic Peninsula warming which is maximized in winter (summer), the warming over West Antarctica is maximized in the spring (SON) and in that season statistically significant warming stretches across all of West Antarctica and into northern Victoria Land. Weak near-surface warming is found over East Antarctica and the continent as a whole on an annual basis although continental warming in the spring is statistically significant and driven largely by the strong and widespread changes in West Antarctica. The 1960-2007 500-hPa temperature reconstruction is compared to the changes described by Turner et al. (2005), who found strong winter warming in radiosonde records over Antarctica for 1971-2003 but noted greater uncertainty over West Antarctica where there are few observational constraints.

Cite:
Bromwich, D. H. et al. (2008), Surface and mid-tropospheric climate change in Antarctica, Eos Trans. AGU, 89(53), Fall Meet. Suppl., Abstract C41A-0497.

NASA's SABER Reveals the Upper Atmosphere’s “Breathing” Pattern, In Rhythm With the Sun

SABER Reveals the Upper Atmosphere’s “Breathing” Pattern, In Rhythm With the Sun

December 15, 2008
A coronal hole, the dark spot beginning just below the sun's center and extending to the right, is shown opening up in this image by NASA satellite STEREO. A coronal hole, the dark spot beginning just below the sun's center and extending to the right, is shown opening up in this image by NASA satellite STEREO. The NASA satellite SABER has detected a periodic "breathing" response in the Earth's upper atmosphere in response to never-before-observed, regular coronal hole openings on the sun's surface. The coronal holes release high-powered solar winds that disturb the upper atmosphere of Earth and force it to emit energy to maintain the earth's radiation budget. (Image credit: NASA/STEREO.)

San Francisco – A NASA satellite has observed for the first time a “breathing” – an expansion and contraction – of the Earth’s upper atmosphere in response to periodic, high-speed solar winds.

Jeff Thayer, of the University of Colorado, Geoff Crowley, of Atmospheric and Space Technology Research Associates, and Marty Mlynczak, of NASA Langley Research Center, will present their findings on Monday, Dec. 15, at 2 p.m., at the American Geophysical Union conference in San Francisco. The instrument, SABER, which stands for Sounding of the Atmosphere using Broadband Emission Radiometry, was developed at NASA Langley.

SABER has revealed solar flare-ups – and a rapid Earth cooling response – on a nearly regular, 9-day schedule. The cause appears to be coronal holes, which project strong solar winds, positioned 120 degrees apart on the sun’s surface. As the sun rotates every 27 days, these solar winds typically hit Earth every 9 days. The high-speed winds sometimes appear with a 7-day periodicity, indicating that a fourth hole opens up.

Sunspots unleash solar flares that create a ripple effect well beyond Earth. But when that energy flow does reach Earth, the atmosphere reciprocates by ejecting radiation as a cooling effect to maintain the planet’s energy balance. That cooling response creates the expansion and contraction of the upper atmosphere.

“No one’s ever seen this type of data because it’s never been measured,” said Mlynczak, SABER’s associate principal investigator.

The findings open the possibility of improving predictions of satellite drag (which are important for tracking low-earth-orbit spacecraft) and of the ionospheric electron concentration, which affects radio communications and GPS signals. The periodic nature of the solar disturbances may also influence the climate and climate change of the upper atmosphere.

“It seems these periodicities have appeared in this last solar cycle, not necessarily in the previous two cycles,” said Janet Kozyra, George Carignan research professor at the University of Michigan, who has worked with SABER data. “This was never reported in past solar cycles.”

Kozyra said learning about a regular feature of a climate system advances knowledge.

“When you have a periodic behavior in a chaotic system, it helps you to predict,” she said. “We learn a lot about how the whole system functions.”

Through the end of September 2008, the sun was “spotless” on 200 days of the year. Not a single sunspot flared up on those days. The Earth’s reaction to this period has been dramatic and directly observed for the first time. In addition to observing the nearly clockwork response to coronal holes opening up on the sun’s surface, SABER has also observed the Earth’s upper atmosphere’s muted response to the sun’s lull – one of its quietest periods in half a century.

SABER, operating since 2002, has been approved for four more years of operation, which should allow for a critical 11-year data set. That would cover the radiative activity of Earth’s upper atmosphere for the entirety of an 11-year solar cycle.

In addition to the “breathing,” the atmosphere’s response to the sun’s sometimes furious, sometimes quiet activity has surprised Mlynczak in a number of ways.

In the quiet solar year of 2008, for instance, the upper atmosphere’s ultraviolet radiation emissions dipped to levels 10 times lower than when SABER’s observations began in 2002. At the same time, SABER detected far more short-term changes in solar activity than previously thought.

“It looks noisy,” Mlynczak said. “But it’s not statistical noise, it’s not instrument noise. It’s geophysical noise.”

SABER also spots massive spikes in energy flow that rise and then dissipate quickly. The atmosphere, it turns out, can dump radiation into space extremely efficiently in response to a burst of solar activity and maintain Earth’s radiation budget.

Kozyra has been fascinated by the role the sun continues to play in Earth’s upper atmosphere even during one of the quietest solar periods in centuries. She expected that this solar minimum would allow for study of how the troposphere influences the rest of the upper atmosphere without solar interference.

“What we actually found was that it didn’t happen. We were seeing the atmosphere was being very strongly driven by the sun,” Kozyra said. “That’s very surprising. We’re learning more about what space weather looks like, and it wasn’t what we thought.”

Questions follow these discoveries. Do the short-term fluctuations need to be programmed into climate-prediction models? Mlynczak isn’t sure yet. Getting it right will be important to the continued refinement of climate prediction.

“What’s the response of the upper atmosphere to global change?” Mlynczak said. Climate change is causing a cooling effect in the upper atmosphere, compared to the warming trend with surface temperature. “We need to make sure we’ve got the predictions of global cooling of the upper atmosphere correct.”

Patrick Lynch, NASA's Langley Research Center

Link to article: http://www.nasa.gov/topics/earth/features/AGU-SABER.html

Andrew Dessler et al.: Water Vapor Confirmed As Major Player In Climate Change Using Data from AIRS on NASA's Aqua Satellite

Water Vapor Confirmed As Major Player In Climate Change

ScienceDaily, Nov. 18, 2008 — Water vapor is known to be Earth's most abundant greenhouse gas, but the extent of its contribution to global warming has been debated. Using recent NASA satellite data, researchers have estimated more precisely than ever the heat-trapping effect of water in the air, validating the role of the gas as a critical component of climate change.

Andrew Dessler and colleagues from Texas A&M University in College Station confirmed that the heat-amplifying effect of water vapor is potent enough to double the climate warming caused by increased levels of carbon dioxide in the atmosphere.

With new observations, the scientists confirmed experimentally what existing climate models had anticipated theoretically. The research team used novel data from the Atmospheric Infrared Sounder (AIRS) on NASA's Aqua satellite to measure precisely the humidity throughout the lowest 10 miles of the atmosphere. That information was combined with global observations of shifts in temperature, allowing researchers to build a comprehensive picture of the interplay between water vapor, carbon dioxide, and other atmosphere-warming gases. The NASA-funded research was published recently in the American Geophysical Union's Geophysical Research Letters.

"Everyone agrees that if you add carbon dioxide to the atmosphere, then warming will result," Dessler said. "So the real question is, how much warming?"

The answer can be found by estimating the magnitude of water vapor feedback. Increasing water vapor leads to warmer temperatures, which causes more water vapor to be absorbed into the air. Warming and water absorption increase in a spiraling cycle.

Water vapor feedback can also amplify the warming effect of other greenhouse gases, such that the warming brought about by increased carbon dioxide allows more water vapor to enter the atmosphere.

"The difference in an atmosphere with a strong water vapor feedback and one with a weak feedback is enormous," Dessler said.

Climate models have estimated the strength of water vapor feedback, but until now the record of water vapor data was not sophisticated enough to provide a comprehensive view of at how water vapor responds to changes in Earth's surface temperature. That's because instruments on the ground and previous space-based could not measure water vapor at all altitudes in Earth's troposphere -- the layer of the atmosphere that extends from Earth's surface to about 10 miles in altitude.

AIRS is the first instrument to distinguish differences in the amount of water vapor at all altitudes within the troposphere. Using data from AIRS, the team observed how atmospheric water vapor reacted to shifts in surface temperatures between 2003 and 2008. By determining how humidity changed with surface temperature, the team could compute the average global strength of the water vapor feedback.

"This new data set shows that as surface temperature increases, so does atmospheric humidity," Dessler said. "Dumping greenhouse gases into the atmosphere makes the atmosphere more humid. And since water vapor is itself a greenhouse gas, the increase in humidity amplifies the warming from carbon dioxide."

Specifically, the team found that if Earth warms 1.8 degrees Fahrenheit, the associated increase in water vapor will trap an extra 2 Watts of energy per square meter (about 11 sq. ft.).

"That number may not sound like much, but add up all of that energy over the entire Earth surface and you find that water vapor is trapping a lot of energy," Dessler said. "We now think the water vapor feedback is extraordinarily strong, capable of doubling the warming due to carbon dioxide alone."

Because the new precise observations agree with existing assessments of water vapor's impact, researchers are more confident than ever in model predictions that Earth's leading greenhouse gas will contribute to a temperature rise of a few degrees by the end of the century.

"This study confirms that what was predicted by the models is really happening in the atmosphere," said Eric Fetzer, an atmospheric scientist who works with AIRS data at NASA's Jet Propulsion Laboratory in Pasadena, Calif. "Water vapor is the big player in the atmosphere as far as climate is concerned."


Adapted from materials provided by NASA/Goddard Space Flight Center.

NASA/Goddard Space Flight Center (2008, November 18). Water Vapor Confirmed As Major Player In Climate Change. ScienceDaily. Retrieved November 18, 2008, from http://www.sciencedaily.com­ /releases/2008/11/081117193013.htm

Link to article and animated graphs of water vapor around the planet:
http://www.nasa.gov/topics/earth/features/vapor_warming.html

Highly recommended further reading:
http://earthobservatory.nasa.gov/Features/WaterVapor/water_vapor.php

Benjamin Santer et al.: Observed warming in tropical troposphere now shown to have no fundamental disagreement with climate model simulations

Claim That Simulated Temperature Trends For Tropics Inconsistent With Observations Is Flawed, Experts Argue

CLICK TO ENLARGE (Credit: Image courtesy of DOE/Lawrence Livermore National Laboratory)

ScienceDaily (Oct. 10, 2008) — A team led by Livermore scientists has helped reconcile the differences between simulated and observed temperature trends in the tropics.

Using state-of-the-art observational datasets and results from computer model simulations archived at Lawrence Livermore National Laboratory, LLNL researchers and colleagues from 11 other scientific institutions have refuted a recent claim that simulated temperature trends in the tropics are fundamentally inconsistent with observations. This claim was based on the application of a flawed statistical test and the use of older observational datasets.

Climate model experiments invariably predict that human-caused greenhouse gas increases should lead to more warming in the tropical troposphere (the lowest layer of the atmosphere) than at the tropical land and ocean surface. This predicted “amplification” behavior is in accord with basic theoretical expectations.

Until several years ago, however, most satellite and weather balloon records suggested that the tropical troposphere had warmed substantially less than the surface.

For nearly a decade, this apparent discrepancy between simulations and reality was a major conundrum for climate scientists. The discrepancy was at odds with the overwhelming body of other scientific evidence pointing toward a “discernible human influence” on global climate.

A paper published online last year in the International Journal of Climatology claimed to show definitively that “models and observations disagree to a statistically significant extent” in terms of their tropical temperature trends. This claim formed the starting point for an investigation by a large team of climate modelers and observational data specialists, which was led by LLNL’s Benjamin Santer.

In marked contrast to the earlier claim, Santer’s international team found that there is no fundamental discrepancy between modeled and observed trends in tropical temperatures.

“We’ve gone a long way toward reconciling modeled and observed temperature trends in the problem area of the tropics,” said Santer, the lead author of a paper now appearing online in the International Journal of Climatology.

There are two reasons for this reconciliation.

First, the analysis that reported disagreement between models and observations had applied an inappropriate statistical test, which did not account for the statistical uncertainty in observed warming trends. This uncertainty arises because the human-caused component of recent temperature changes is not perfectly known in any individual observed time series – it must be estimated from data that are influenced by both human effects and the “noise” of natural climate variability. Examples of such “noise” include large El Niño and La Niña events, which have pronounced effects on the year-to-year variability of tropical temperatures.

The Livermore-led consortium applied this inappropriate test to randomly generated data. The test revealed a strong bias in the method toward “detecting” differences that were not real.

The consortium modified the test to correctly account for uncertainty in estimating temperature trends from noisy observational data. With this modified test, there were no longer pervasive, statistically significant differences between simulated and observed tropical temperature trends.

The second reason for the reconciliation of models and observations was the availability of new and improved observational datasets, both for surface and tropospheric temperatures. The developers of these datasets used different procedures to identify and adjust for biases (such as those caused by changes over time in the instruments and platforms used to measure temperature).

Access to multiple, independently produced datasets provided the LLNL-led consortium with a valuable perspective on the inherent uncertainty in observations. Many of the recently developed observational datasets showed larger warming aloft than at the surface, and were more consistent with climate model results.

Even with improved datasets, there are still important uncertainties in observational estimates of recent tropospheric temperature trends that may never be fully resolved, and are partly a consequence of historical observing strategies, which were geared toward weather forecasting rather than climate monitoring.

“We should apply what we learned in this study toward improving existing climate monitoring systems, so that future model evaluation studies are less sensitive to observational ambiguity,” Santer said.

Other researchers in this international consortium were Karl Taylor, Peter Gleckler and Stephen Klein (all at Livermore); Peter Thorne at the United Kingdom Meteorological Office Hadley Centre; Leo Haimberger at the University of Vienna; Tom Wigley and Doug Nychka at the National Center for Atmospheric Research; John Lanzante at the National Oceanic and Atmospheric Administration (NOAA)/Geophysical Fluid Dynamics Laboratory; Susan Solomon at the NOAA/Earth System Research Laboratory; Melissa Free at the NOAA/Air Resources Laboratory; Phil Jones at the University of East Anglia; Tom Karl at the NOAA/National Climatic Data Center; Carl Mears and Frank Wentz at Remote Sensing Systems; Gavin Schmidt at the NASA/Goddard Institute for Space Studies; and Steve Sherwood at Yale University.

LLNL researchers were supported by the Office of Biological and Environmental Research in the U.S. Department of Energy's Office of Science.