A new report indicates that the vast majority of the rapid temperature increase recently observed in Europe is likely due to an unexpected greenhouse gas: water vapor. Elevated surface temperatures due to other greenhouse gases have enhanced water evaporation and contributed to a cycle that stimulates further surface temperature increases, according to a report in Geophysical Research Letters. The research could help to answer a long-debated Earth science question about whether the water cycle could strongly enhance greenhouse warming.
Swiss researchers examined surface radiation measurements from 1995 to 2002 over the Alps in Central Europe and show strongly increasing total surface absorbed radiation, concurrent with rapidly increasing temperature. The authors, led by Rolf Philipona of the World Radiation Center in Davos, show experimentally that 70 percent of the rapid temperature increase is very likely caused by water vapor feedback. They indicate that remaining 30 percent is likely due to increasing manmade greenhouse gases.
The researchers analyzed temperature and humidity changes over Europe, which jumped nearly three times above the levels predicted by general circulation models in the past two decades. They provide observational evidence that large-scale weather patterns in Europe influence annual average temperatures uniformly, but weakly. They suggest that their combined observations indicate that the region is experiencing an increasing greenhouse effect and that the dominant part of the rising heat emitted from the Earth’s atmosphere (longwave radiation) is due to water vapor increase.
Harvey Leifert | EurekAlert!
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The nearby, giant radio galaxy M87 hosts a supermassive black hole (BH) and is well-known for its bright jet dominating the spectrum over ten orders of magnitude in frequency. Due to its proximity, jet prominence, and the large black hole mass, M87 is the best laboratory for investigating the formation, acceleration, and collimation of relativistic jets. A research team led by Silke Britzen from the Max Planck Institute for Radio Astronomy in Bonn, Germany, has found strong indication for turbulent processes connecting the accretion disk and the jet of that galaxy providing insights into the longstanding problem of the origin of astrophysical jets.
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