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April 14, 2009

Media Contacts:

Kristi Marren, Johns Hopkins University Applied Physics Laboratory
240-228-6268 or 443-778-6268

Rani Gran, NASA Goddard Space Flight Center
(301) 286-2483

Capturing a Solar Storm in 3-D
APL Spacecraft Experts Enhance Systems to Reconstruct 3-D STEREO Imagery

The APL—built and —operated twin STEREO observatories have made the first 3-D measurements of solar explosions, known as coronal mass ejections, enabling scientists to see their size and shape, and image them as they travel approximately 93 million miles from the sun to Earth. Scientists will be able to use this information to help determine how these strong solar storms will impact Earth's atmosphere.

The Solar TErrestrial RElations Observatory's science data is enhanced, in part, due to the STEREO guidance and control team at The Johns Hopkins University Applied Physics Laboratory (APL), in Laurel, Md. They're helping mission scientists more easily reconstruct 3-D imagery by very accurately pointing the spacecraft and reducing its jitter or movement. "By tuning each spacecraft's control software, much like a race car's control system is tuned for optimal performance on the track, spacecraft system performance is now approximately five times better than at launch and seven times better than specifications require," says Andy Driesman, STEREO's system engineer at APL.

Since launch in 2006, the APL team has been proactively tuning spacecraft and ground systems, maximizing data return and optimizing contact with satellites used to downlink data. The APL-based STEREO mission operations center downloads 6-9 gigabytes of data each day — approximately 20-80 percent more data than the science team expected.

Coronal mass ejections are powerful solar explosions that can have damaging effects when hitting Earth's upper atmosphere at speeds of nearly one million miles-per-hour. These giant clouds of electrically charged gas called plasma can disrupt satellite communications, GPS and/or cell phone signals, or induce large currents in power grids, which can cause power disruptions or black outs.

"Using STEREO observations, we can extract a CME's properties and are able to determine when it will reach Earth, at what speed, and with how much energy it will impact Earth's magnetosphere," says Angelos Vourlidas, of the Naval Research Laboratory, and project scientist for STEREO's SECCHI (Sun Earth Connection Coronal and Heliospheric Investigation) imaging suite. Disruptions to the magnetic envelope surrounding Earth can often trigger auroras. These bright bands of light, often visible at night in northern and southern regions, can interfere with communications between air-traffic controllers and pilots flying near Earth's polar regions.

STEREO is sponsored by NASA Headquarters' Science Mission Directorate, Washington, D.C. NASA Goddard Space Flight Center's (GSFC) Solar Terrestrial Probes Program Office, in Greenbelt, Md., manages the mission, instruments and science center. APL designed and built the spacecraft and is operating the twin observatories for NASA during the mission.

For more information, visit http://stereo.jhuapl.edu/ and http://stereo.gsfc.nasa.gov/.

 

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image for a larger version.
 

Print-resolution image from telescopes onboard STEREO spacecraft showing a coronal mass ejection event on December 12-13, 2008. Data from both spacecraft are shown simultaneously.

Print-resolution image depicting STEREO-A viewing a coronal mass ejection leaving the sun between December 12-13, 2008.

At the Edge of Titan's Dunes
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At the Edge of Titan's Dunes
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The Applied Physics Laboratory, a division of The Johns Hopkins University, meets critical national challenges through the innovative application of science and technology. For more information, visit www.jhuapl.edu.