Measuring Climate Change
Astrobiology Magazine’s climate blog, The Hot Zone, recently spoke with Dr. Marty Mlynczak of NASA’s Langley Research Center about the limitations of the technology we have on hand to measure climate change. Some of aspects of Earth’s climate are difficult to measure, yet could be important in understanding how the Earth’s climate affects habitability. Developing new technologies and techniques to help us understand our climate could prove useful in elucidating the links between climate and our planet’s biosphere.
"The Electromagnetic Spectrum" — Radio waves, microwaves, x-rays, gamma rays, and the spectrum of visible colors are all really the same thing – electromagnetic energy. The differences are their wavelengths. Radio waves are long, measuring as much as hundreds of meters between peaks. Gamma ray wavelengths are extremely short, as little as trillionths of a meter. A photon of shorter-wavelength light packs more energy than a photon of longer-wavelength light.
Image credit: Herschel Space Observatory
When we think of climate change we tend to think only of near-earth phenomenon: changes in average temperature, diminishing polar ice, changes in weather patterns, variations in El Niño effects, and measurements of atmospheric C02. Most of these data are collected either at the Earth’s surface or else they are viewed from afar, by satellites.
After I spoke with Dr. Marty Mlynczak, a senior research scientist based at NASA’s Langley, Virginia research centre, I realized that often there were limitations to what technology on hand could measure. And some of what isn’t – or wasn’t – being measured is very important indeed for our understanding of climate change.
Radiative emissions of water vapour at the far infrared part of the electromagnetic spectrum, for instance – that is, wavelengths between 15 and 100 micrometers – could not be measured directly until very recently. The lack of accurate measurement of radiation at this wave length, it turns out, really matters: based on the results yielded by climate models, scientists studying the atmosphere hypothesized that half of all of the cooling emissions into the outer parts of the atmosphere were in the far infra-red part of the spectrum.
FIRST researchers from NASA Langley as the FIRST container is loaded to travel to Colorado on its first stage of its journey to Chile. From left to right: David Johnson, Martin Mlynczak, Richard Cageao, Glenn Farnsworth and Joseph (Joe) Lee.
Credit: NASA/Sean Smith
Dr. Mlynczak is very interested in the far-infrared part of the electromagnetic spectrum. “All infrared energy relevant to the Earth’s climate occurs at the shorter wavelenths,” he wrote in a 2006 paper.* He believes being able to measure radiative emissions in the upper troposphere at far-infrared wavelengths is crucial to our understanding of how the Earth’s atmosphere cools. The trouble was, said Dr. Mlynczak, “There wasn’t an instrument available that could measure this part of the spectrum.”
So he and his colleagues built one.
Dr. Mlynczak’s team launched a prototype of the the Far-Infrared Spectroscopy of the Troposphere (FIRST) instrument during a high-altitude balloon flight from Fort Sumner, New Mexico in June of 2005. It was a success.
“FIRST opens a new window on the spectrum that can be used for studying atmospheric radiation and climate, cirrus clouds, and water vapor in the upper troposphere,” wrote Dr. Mlynczak.*
In October of this year, Dr. Mlynczak and his colleagues traveled to a location high up in the Andes mountains of Chile, the Atacama desert, an altitude of 17,600. Because it’s one of the driest regions on Earth, the Atacama desert offers an ideal environment for measuring water vapor.
At this altitude, said Dr. Mlynczak, there’s nothing getting in the way of accurate measurement. “We’re above everything. We’re above the pollution. It’s the ideal location for atmospheric observation.”
*Source: Martin Mlynczak et al, “First light from the Far-Infrared Spectroscopy of the Troposphere (FIRST) instrument,” Geophysical Research Letters, Vol. 33, 4 April, 2006