NASA Spacecraft Show Three Dimensional Anatomy of a Solar Storm

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April 14, 2009


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

Rani Gran/Laura Layton 
Goddard Space Flight Center, Greenbelt, Md. 
301-286-2483/8170 
rani.c.gran@xxxxxxxx 
laura.a.layton@xxxxxxxx 

RELEASE: 09-083

NASA SPACECRAFT SHOW THREE DIMENSIONAL ANATOMY OF A SOLAR STORM

WASHINGTON -- Twin NASA spacecraft have provided scientists with their 
first view of the speed, trajectory, and three-dimensional shape of 
powerful explosions from the sun known as coronal mass ejections, or 
CMEs. This new capability will dramatically enhance scientists' 
ability to predict if and how these solar tsunamis could affect 
Earth. 

When directed toward our planet, these ejections can be breathtakingly 
beautiful and yet potentially cause damaging effects worldwide. The 
brightly colored phenomena known as auroras -- more commonly called 
Northern or Southern Lights -- are examples of Earth's upper 
atmosphere harmlessly being disturbed by a CME. However, ejections 
can produce a form of solar cosmic rays that can be hazardous to 
spacecraft, astronauts and technology on Earth. 

Space weather produces disturbances in electromagnetic fields on Earth 
that can induce extreme currents in wires, disrupting power lines and 
causing wide-spread blackouts. These sun storms can interfere with 
communications between ground controllers and satellites and with 
airplane pilots flying near Earth's poles. Radio noise from the storm 
also can disrupt cell phone service. Space weather has been 
recognized as causing problems with new technology since the 
invention of the telegraph in the 19th century. 

NASA's twin Solar Terrestrial Relations Observatory, or STEREO, 
spacecraft are providing the unique scientific tool to study these 
ejections as never before. Launched in October 2006, STEREO's nearly 
identical observatories can make simultaneous observations of these 
ejections of plasma and magnetic energy that originate from the sun's 
outer atmosphere, or corona. The spacecraft are stationed at 
different vantage points. One leads Earth in its orbit around the 
sun, while the other trails the planet. 

Using three-dimensional observations, solar physicists can examine a 
CME's structure, velocity, mass, and direction in the corona while 
tracking it through interplanetary space. These measurements can help 
determine when a CME will reach Earth and predict how much energy it 
will deliver to our magnetosphere, which is Earth's protective 
magnetic shield. 

"Before this unique mission, measurements and the subsequent data of a 
CME observed near the sun had to wait until the ejections arrived at 
Earth three to seven days later," said Angelos Vourlidas, a solar 
physicist at the Naval Research Laboratory in Washington. Vourlidas 
is a project scientist for the Sun Earth Connection Coronal and 
Heliospheric Investigation, STEREO's key science instrument suite. 
"Now we can see a CME from the time it leaves the solar surface until 
it reaches Earth, and we can reconstruct the event in 3D directly 
from the images." 

These ejections carry billions of tons of plasma into space at 
thousands of miles per hour. This plasma, which carries with it some 
of the magnetic field from the corona, can create a large, moving 
disturbance in space that produces a shock wave. The wave can 
accelerate some of the surrounding particles to high energies that 
can produce a form of solar cosmic rays. This process also can create 
disruptive space weather during and following the CME's interaction 
with Earth's magnetosphere and upper atmosphere. 

"The new vantage point of these spacecraft has revolutionized the 
study of solar physics," said Madhulika Guhathakurta, STEREO program 
scientist at NASA Headquarters in Washington. "We can better 
determine the impact of CME effects on Earth because of our new 
ability to observe in 3D." 

STEREO is part of NASA's Solar Terrestrial Probes Program in NASA's 
Science Mission Directorate in Washington. The program seeks to 
understand the fundamental physical processes of the space 
environment from the sun to Earth and other planets. 

The Solar Terrestrial Probes Program also seeks to understand how 
society, technological systems and the habitability of planets are 
affected by solar processes. This information may lead to a better 
ability to predict extreme and dynamic conditions in space, and the 
development of new technologies to increase safety and productivity 
of human and robotic space exploration. 

For more information about NASA's STEREO mission, visit: 










http://www.nasa.gov/stereo 

	
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