NASA's TSIS-1 keeps an eye on sun's power over ozone

November 22, 2017 by Rani Gran, NASA
Light can be split into many wavelengths and a rainbow illustrates this in visible light. Each color is a different wavelength of light. NASA’s TSIS- 1 will see more than 1,000 wavelength bands of sunlight reaching the top of the atmosphere, including light we cannot sense with our eyes. Credit: Matthew Almon Roth (via Creative Commons)

High in the atmosphere, above weather systems, is a layer of ozone gas. Ozone is Earth's natural sunscreen, absorbing the sun's most harmful ultraviolet radiation and protecting living things below. But ozone is vulnerable to certain gases made by humans that reach the upper atmosphere. Once there, they react in the presence of sunlight to destroy ozone molecules.

Currently, several NASA and National Oceanic and Atmospheric Administration (NOAA) satellites track the amount of ozone in the and the solar energy that drives the photochemistry that creates and destroys ozone. NASA is now ready to launch a new instrument to the International Space Station that will provide the most accurate measurements ever made of sunlight as seen from above Earth's atmosphere—an important component for evaluating the long-term effects of ozone-destroying chemistry. The Total and Spectral solar Irradiance Sensor (TSIS-1) will measure the total amount of sunlight that reaches the top of Earth's atmosphere and how that light is distributed between different wavelengths, including ultraviolet wavelengths that we cannot sense with our eyes, but are felt by our skin and harmful to our DNA.

This is not the first time NASA has measured the total light energy from the sun. TSIS-1 succeeds previous and current NASA missions to monitor incoming sunlight with technological upgrades that should improve stability, provide three times better accuracy and lower interference from other sources of light, according to Candace Carlisle, TSIS-1 project manager at NASA's Goddard Space Flight Center in Greenbelt, Maryland.

"We need to measure the full spectrum of sunlight and the individual wavelengths to evaluate how the sun affects Earth's atmosphere," said Dong Wu, TSIS-1 project scientist at Goddard.

Antarctic ozone hole, Oct. 10, 2017: Purple and blue represent areas of low ozone concentrations in the atmosphere; yellow and red are areas of higher concentrations. Carbon tetrachloride (CCl4), which was once used in applications such as dry cleaning and as a fire-extinguishing agent, was regulated in 1987 under the Montreal Protocol along with other chlorofluorocarbons that destroy ozone and contribute to the ozone hole over Antarctica. Credit: NASA's Goddard Space Flight Center

TSIS-will see more than 1,000 wavelength bands from 200 to 2400 nanometers. The visible part of the spectrum our eyes see goes from about 390 nanometers (blue) to 700 nanometers (red). A nanometer is one billionth of a meter.

"Each color or wavelength of light affects Earth's atmosphere differently," Wu said.

TSIS-1 will see different types of ultraviolet (UV) light, including UV-B and UV-C. Each plays a different role in the . UV-C rays are essential in creating ozone. UV-B rays and some naturally occurring chemicals regulate the abundance of ozone in the upper atmosphere. The amount of ozone is a balance between these natural production and loss processes. In the course of these processes, UV-C and UV-B rays are absorbed, preventing them from reaching Earth's surface and harming living organisms. Thinning of the ozone layer has allowed some UV-B rays to reach the ground.

In the 1970s, scientists theorized that certain human-made chemicals found in spray cans, air conditioners and refrigerators could throw off the natural balance of ozone creation and depletion and cause an unnatural depletion of the protective ozone. In the 1980s, scientists observed consistent with the concentrations of these chemicals and confirmed this theory.

The picture on the left shows a calm sun from October 2010. The right side, from October 2012, shows a much more active and varied solar atmosphere as the sun moves closer to peak solar activity, or solar maximum. NASA's Solar Dynamics Observatory (SDO) captured both images. Credit: NASA's Goddard Space Flight Center/SDO

Ozone loss was far more severe than expected over the South Pole during the Antarctic spring (fall in the United States), a phenomenon that was named "the Antarctic ." The discovery that human-made chemicals could have such a large effect on Earth's atmosphere brought world leaders together. They created an international commitment to phase out ozone-depleting chemicals called the Montreal Protocol, which was universally ratified in 1987 by all countries that participate in the United Nations, and has been updated to tighten constraints and account for additional ozone depleting chemicals.

A decade after the ratification of the Montreal Protocol, the amount of human-made ozone-destroying chemicals in the atmosphere peaked and began a slow decline. However, it takes decades for these chemicals to completely cycle out of the upper atmosphere, and the concentrations of these industrially produced molecules are not all decreasing as expected, while additional, new compounds are being created and released.

More than three decades after ratification, NASA satellites have verified that ozone losses have stabilized and, in some specific locations, have even begun to recover due to reductions in the ozone-destroying chemicals regulated under the Montreal Protocol.

As part of their work in monitoring the recovery of the ozone hole, scientists use computer models of the atmosphere that simulate the physical, and weather processes in the atmosphere. These atmospheric models can then take input from ground and satellite observations of various atmospheric gases, both natural and human-produced, to help predict ozone layer recovery. They test the models by simulating past changes and then compare the results with satellite measurements to see if the simulations match past outcomes. To run the best possible simulation, the models also need accurate measurements of sunlight across the spectrum.

TSIS-1 will be affixed to the International Space Station in December 2017 TSIS-1 operates like a sun flower: it follows the Sun, from the ISS sunrise to its sunset, which happens every 90 minutes. At sunset, it rewinds, recalibrates and waits for the next sunset. Credit: NASA/LASP

"Atmospheric models need of sunlight across the to model the ozone layer correctly," said Peter Pilewskie, TSIS-1 lead scientist at the Laboratory for Atmospheric and Space Physics in Boulder, Colorado. Scientists have learned that variations in UV radiance produce significant changes in the results of the computer simulations.

Overall, solar energy output varies by approximately 0.1 percent—or about 1 watt per square meter between the most and least active part of an 11-year solar cycle. The solar cycle is marked by the alternating high and low activity periods of sunspots, dark regions of complex magnetic activity on the sun's surface. While UV light represents a tiny fraction of the total sunlight that reaches the top of Earth's atmosphere, it fluctuates much more, anywhere from 3 to 10 percent, a change that in turn causes small changes in the chemical composition and thermal structure of the upper .

That's where TSIS-1 comes in. "[TSIS] measurements of the solar spectrum are three times more accurate than previous instruments," said Pilewskie. Its high quality measurements will allow scientists to fine tune their computer models and produce better simulations of the layer's behavior—as well as other atmospheric processes influenced by sunlight, such as the movement of winds and weather that are.

TSIS-1 joins a fleet of NASA's Earth-observing missions that monitor nearly every aspect of the Earth system, watching for any changes in our environment that could harm life.

Explore further: NASA instrument key to understanding solar powered planet arrives at Kennedy Space Center

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