NASA Probes Suggest Magnetic Bubbles Reside At Solar System Edge

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June 09, 2011

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

Jia-Rui Cook 
Jet Propulsion Laboratory, Pasadena, Calif. 
818-354-0850 
jccook@xxxxxxxxxxxx   


RELEASE: 11-174

NASA PROBES SUGGEST MAGNETIC BUBBLES RESIDE AT SOLAR SYSTEM EDGE

WASHINGTON -- Observations from NASA's Voyager spacecraft, humanity's 
farthest deep space sentinels, suggest the edge of our solar system 
may not be smooth, but filled with a turbulent sea of magnetic 
bubbles. 

While using a new computer model to analyze Voyager data, scientists 
found the sun's distant magnetic field is made up of bubbles 
approximately 100 million miles wide. The bubbles are created when 
magnetic field lines reorganize. The new model suggests the field 
lines are broken up into self-contained structures disconnected from 
the solar magnetic field. The findings are described in the June 9 
edition of the Astrophysical Journal. 

Like Earth, our sun has a magnetic field with a north pole and a south 
pole. The field lines are stretched outward by the solar wind or a 
stream of charged particles emanating from the star that interacts 
with material expelled from others in our corner of the Milky Way 
galaxy. 

The Voyager spacecraft, nearly 10 billion miles away from Earth, are 
traveling in a boundary region. In that area, the solar wind and 
magnetic field are affected by material expelled from other stars in 
our corner of the Milky Way galaxy. 

"The sun's magnetic field extends all the way to the edge of the solar 
system," said astronomer Merav Opher of Boston University. "Because 
the sun spins, its magnetic field becomes twisted and wrinkled, a bit 
like a ballerina's skirt. Far, far away from the sun, where the 
Voyagers are, the folds of the skirt bunch up." 

Understanding the structure of the sun's magnetic field will allow 
scientists to explain how galactic cosmic rays enter our solar system 
and help define how the star interacts with the rest of the galaxy. 

So far, much of the evidence for the existence of the bubbles 
originates from an instrument aboard the spacecraft that measures 
energetic particles. Investigators are studying more information and 
hoping to find signatures of the bubbles in the Voyager magnetic 
field data. 

"We are still trying to wrap our minds around the implications of the 
findings," said University of Maryland physicist Jim Drake, one of 
Opher's colleagues. 

Launched in 1977, the Voyager twin spacecraft have been on a 33-year 
journey. They are en route to reach the edge of interstellar space. 
NASA's Jet Propulsion Laboratory in Pasadena, Calif., built the 
spacecraft and continues to operate them. The Voyager missions are a 
part of the Heliophysics System Observatory, sponsored by the 
Heliophysics Division of NASA's Science Mission Directorate in 
Washington. 

To view supporting images about the research, visit: 


http://www.nasa.gov/sunearth   

	
-end-



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