WASHINGTON -- A new analysis has revealed that advanced satellite-based instrument capabilities are needed for global monitoring of microscopic particles, or aerosols, in the stratospheric layer of the atmosphere. Aerosols in the stratosphere -- located above approximately 12 kilometers -- increase drastically after a volcanic eruption, leading to changes in the Earth's climate and providing a critical opportunity to test scientific models designed to predict short- and long-term climate variations.
Researchers from NASA Goddard Institute for Space Studies in New York and the National Academy of Sciences in Kyiv, Ukraine, report the new findings in The Optical Society (OSA) journal Optics Express.
When a volcano erupts, large amounts of ash and sulfuric-acid particles can blanket the entire planet, blocking much of the sunlight and temporarily causing global cooling. Scientists are now exploring whether this blanketing effect could be used to counteract global warming by injecting man-made aerosols in the stratosphere. Such geoengineering projects would also require a way to monitor the amount and size of artificial particulates in the stratosphere and the resulting climate effect.
"The global nature of natural and man-made stratospheric aerosols means that a specialized Earth-orbiting instrument is necessary to obtain comprehensive information on their properties and distribution," said Janna Dlugach, a member of the research team from the Ukraine's National Academy of Sciences. "This information is critical for testing climate models and for monitoring climate effects from potential geoengineering projects and major volcanic eruptions, which can affect the livelihood of the entire population."
Monitoring aerosols from space
Over the next decade NASA plans to carry out a specialized mission to monitor aerosols and clouds on Earth. This mission would include an instrument that measures not only the brightness of sunlight reflected by the atmosphere and Earth's surface but also the light's polarization, which carries rich information about the size, composition and amount of aerosol particles.
"The technical characteristics of this future polarimeter are currently the subject of active debate among the scientific community," said Michael Mishchenko, a member of the research team from NASA. "Our paper brings into this discussion the necessity of monitoring not just aerosols in the lower atmosphere, but also stratospheric aerosols that could become a major part of the climate system in the case of a major volcanic eruption or the implementation of a massive geoengineering program."
Measurements of reflected sunlight by orbital instruments are usually dominated by bright water clouds, the land surface and aerosols found in the troposphere -- the atmospheric layer closest to the ground. "This is not problematic when stratospheric aerosols are minimal and thus unimportant relative to tropospheric aerosols," explained Dlugach. "However, it becomes essential to separate out the light coming from stratospheric aerosols in the case of volcanic eruptions or geoengineering activities."
Separating stratospheric aerosols
In the new study, the researchers argue that any future aerosol-monitoring orbital instrument should provide measurements within a narrow spectral channel centered at 1.378 micrometers. "At this wavelength the water vapor in the troposphere can almost completely absorb the sunlight scattered by clouds, terrestrial surfaces and tropospheric aerosols," said Mishchenko. "This enables us to infer the properties of stratospheric aerosols separately from those of tropospheric aerosols."
The researchers used simulated measurements to determine the best way to measure stratospheric aerosols. They began by using a realistic model of stratospheric aerosols to calculate the theoretical brightness and polarization of sunlight that these aerosols would reflect into space. They then added measurement errors that mimic those found in actual satellite data. With the resulting information, they simulated several types of realistic measurements to determine which provides enough information to determine the amount, size and composition of stratospheric aerosols.
"We found that measuring the brightness of light alone does not allow the inference of stratospheric aerosols," said Dlugach. "Our analysis suggests that future aerosol-monitoring space mission should include an instrument that can obtain precise polarization measurements of a terrestrial scene from multiple angles at the 1.378-micrometer wavelength."
The strong water-vapor absorption channel is necessary to cancel out light coming from the lower atmosphere and surface while precise polarization measurements from multiple angles yield detailed information about stratospheric aerosols.
Next, the researchers plan to analyze more challenging observation conditions that would put additional requirements on the instrument design. They also want to determine whether combining polarimetric and lidar observations from the same orbital platform would be beneficial for certain conditions.
Paper: M. I. Mishchenko, J. M. Dlugach, A. A. Lacis, L. D. Travis, B. Cairns, "Retrieval of volcanic and man-made stratospheric aerosols from orbital polarimetric measurements," Opt. Express, 27, 4, A158-A170 (2019).
About Optics Express
Optics Express reports on new developments in all fields of optical science and technology every two weeks. The journal provides rapid publication of original, peer-reviewed papers. It is published by The Optical Society and edited by James Leger from the University of Minnesota. Optics Express is an open-access journal and is available at no cost to readers online at: OSA Publishing.
About The Optical Society
Founded in 1916, The Optical Society (OSA) is the leading professional organization for scientists, engineers, students and business leaders who fuel discoveries, shape real-life applications and accelerate achievements in the science of light. Through world-renowned publications, meetings and membership initiatives, OSA provides quality research, inspired interactions and dedicated resources for its extensive global network of optics and photonics experts. For more information, visit osa.org.
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