Wednesday,
August 20, 2014

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UT Dallas Researchers to Work on NASA's Space Weather Mission Launching in 2017

Researchers at The University of Texas at Dallas are pushing the boundaries of science as they investigate how everyday thunderstorms influence “space weather” occurring where Earth’s atmosphere meets the void.

Dr. Rod Heelis, director of UT Dallas’ William B. Hanson Center for Space Sciences, and his colleagues recently were chosen to design and build an experiment that will fly onboard a new NASA satellite mission called the Ionospheric Connection Explorer (ICON).

Scintillation

Click to enlarge: When high-frequency radio waves, such as those used for the Global Positioning System (GPS), travel through a disturbed layer of Earth's electrically charged atmosphere (the ionosphere), they can be disrupted. Source: U.S. Air Force Research Laboratory.

The ICON satellite, slated for launch in 2017, will orbit about 350 miles above Earth, in a region of the upper atmosphere called the ionosphere. The satellite will carry a suite of instruments built by various institutions, including UT Dallas.

As the name suggests, the ionosphere consists of charged particles called ions, which are created when high-energy sunlight strips away electrons from atmospheric gases, such as nitrogen and oxygen. Just as the movement of air in Earth’s lower atmosphere drives surface weather, a mixture of neutral gasses, ions and free electrons in the ionosphere move around and create “space weather.”

There’s a practical reason why scientists – including those at UT Dallas – have been studying the ionosphere for decades, said Heelis, an expert on space weather who has been on the faculty since 1973.

“Disturbances and turbulence in this region interfere with radio signals, as well as GPS signals used in navigation. So predicting when and where interference will occur is a high priority,” said Heelis, who holds the Distinguished Chair in Natural Sciences and Mathematics.  “A better understanding of the dynamics of the ionosphere and the factors that affect it will help us develop models to more accurately forecast space weather.”

Ion Velocity Meter

An ion velocity meter built by UT Dallas space scientists, similar to the one pictured above, will fly onboard a satellite as part of a new NASA satellite mission to study space weather.

Until recently, scientists thought that the sun was the sole driver of space weather. Evidence is mounting, however, that the Earth’s surface weather, such as run-of-the-mill thunderstorms, also can affect the ionosphere.

It’s this interaction between surface weather and space weather that is the focus of the ICON mission. The UT Dallas instrument is called the Ion Velocity Meter. It will gather data at the site of the spacecraft, such as the velocity, temperature and density of ions, while other instruments will remotely measure the state of the neutral atmosphere below the satellite, Heelis said. 

“This is an exciting opportunity to discover the reasons for the connections between surface weather and space weather that have only come to light in the last 10 years,” he said.

NASA is funding the ICON mission through the space agency’s Explorer program. Scientists at the Space Sciences Laboratory at the University of California, Berkeley will oversee the mission, while UT Dallas, the U.S. Naval Research Laboratory and the University of Illinois at Urbana-Champaign will provide experiments. In addition, scientists from the National Center for Atmospheric Research and Atmospheric & Space Technology Research Associates will participate in the data interpretation.  

Media Contact: Amanda Siegfried, UT Dallas, (972) 883-4335, amanda.siegfried@utdallas.edu
or the Office of Media Relations, UT Dallas, (972) 883-2155, newscenter@utdallas.edu


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