NASA Satellites Discover What Powers Northern Lights

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July 24, 2008

Dwayne Brown
Headquarters, Washington
202-358-1726
dwayne.c.brown@xxxxxxxx

Laura Layton
Goddard Space Flight Center, Md.
301-286-8170
laura.a.layton@xxxxxxxx

RELEASE: 08-185

NASA SATELLITES DISCOVER WHAT POWERS NORTHERN LIGHTS

GREENBELT, Md. -- Researchers using a fleet of five NASA satellites 
have discovered that explosions of magnetic energy a third of the way 
to the moon power substorms that cause sudden brightenings and rapid 
movements of the aurora borealis, called the Northern Lights.

The culprit turns out to be magnetic reconnection, a common process 
that occurs throughout the universe when stressed magnetic field 
lines suddenly snap to a new shape, like a rubber band that's been 
stretched too far. 

"We discovered what makes the Northern Lights dance," said Dr. 
Vassilis Angelopoulos of the University of California, Los Angeles. 
Angelopoulos is the principal investigator for the Time History of 
Events and Macroscale Interactions during Substorms mission, or 
THEMIS.

Substorms produce dynamic changes in the auroral displays seen near 
Earth's northern and southern magnetic poles, causing a burst of 
light and movement in the Northern and Southern Lights.

Substorms often accompany intense space storms that can disrupt radio 
communications and global positioning system signals and cause power 
outages. Solving the mystery of where, when, and how substorms occur 
will allow scientists to construct more realistic substorm models and 
better predict a magnetic storm's intensity and effects.

"As they capture and store energy from the solar wind, the Earth's 
magnetic field lines stretch far out into space. Magnetic 
reconnection releases the energy stored within these stretched 
magnetic field lines, flinging charged particles back toward the 
Earth's atmosphere," said David Sibeck, THEMIS project scientist at 
NASA's Goddard Space Flight Center in Greenbelt, Md. "They create 
halos of shimmering aurora circling the northern and southern poles."

Scientists directly observe the beginning of substorms using five 
THEMIS satellites and a network of 20 ground observatories located 
throughout Canada and Alaska. Launched in February 2007, the five 
identical satellites line up once every four days along the equator 
and take observations synchronized with the ground observatories. 
Each ground station uses a magnetometer and a camera pointed upward 
to determine where and when an auroral substorm will begin. 
Instruments measure the auroral light from particles flowing along 
Earth's magnetic field and the electrical currents these particles 
generate. 

During each alignment, the satellites capture data that allow 
scientists to precisely pinpoint where, when, and how substorms 
measured on the ground develop in space. On Feb. 26, 2008, during one 
such THEMIS lineup, the satellites observed an isolated substorm 
begin in space, while the ground-based observatories recorded the 
intense auroral brightening and space currents over North America.

These observations confirm for the first time that magnetic 
reconnection triggers the onset of substorms. The discovery supports 
the reconnection model of substorms, which asserts a substorm 
starting to occur follows a particular pattern. This pattern consists 
of a period of reconnection, followed by rapid auroral brightening 
and rapid expansion of the aurora toward the poles. This culminates 
in a redistribution of the electrical currents flowing in space 
around Earth. 

THEMIS is the fifth medium-class mission under NASA's Explorer 
Program. The program, managed by the Explorers Program Office at 
Goddard provides frequent flight opportunities for world-class space 
investigations in heliophysics and astrophysics. The University of 
California, Berkeley's Space Sciences Laboratory in Berkeley, Calif., 
managed the project development and is currently operating the THEMIS 
mission. ATK Space (formerly Swales Aerospace) of Beltsville, Md., 
built the THEMIS satellites. 

The THEMIS team's findings will appear online July 24 in Science 
Express and Aug. 14 in the journal science. For more information 
about the THEMIS mission, visit:

http://www.nasa.gov/themis

	
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