Here is a surprising paradox: while the Earth's surface is warming, the upper atmosphere has been cooling for decades. This phenomenon, one of the clearest signs of climate change, was known but poorly understood until now. Today, researchers at Columbia University have identified the main mechanism behind this stratospheric cooling.
Unlike what happens near the ground, where carbon dioxide (CO2) acts like a blanket trapping heat, in the stratosphere (between 7 and 31 miles, or 11β50 km, of altitude), it behaves like a cooling system. CO2 molecules absorb infrared energy rising from the Earth and re-emit much of it into space. With increasing CO2, the stratosphere becomes more efficient at radiating heat away, causing its temperature to drop.
View of Earth from the International Space Station during Expedition 66. Credit: NASA
This discovery, published in Nature Geoscience, is based on refined mathematical models. The researchers identified a specific range of infrared wavelengths, which they call the "Goldilocks zone," where interaction with CO2 is most efficient at cooling the atmosphere. As CO2 levels rise, this zone expands, strengthening the cooling. The effects of ozone and water vapor are negligible in comparison.
The study also shows that cooling intensifies with altitude: it is weak in the lower stratosphere but reaches about 8 degrees Celsius of cooling at the stratopause (the upper boundary) for each doubling of CO2 concentration. This cooling has an unexpected feedback effect: by allowing the stratosphere to radiate more heat, it also aggravates surface warming. Since the 1980s, the stratosphere has cooled by about 2 degrees Celsius, more than ten times what would occur without human emissions.
According to the authors, this work is not intended to prove global warming, which is already well established. Rather, it offers a detailed understanding of a major atmospheric process. The equations developed could also be used to study the stratospheres of other planets or exoplanets.