NASA Spacecraft Aids in Forecast of Solar Radiation Storms

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May 25, 2007

Dwayne Brown
Headquarters, Washington
202-358-1726
RELEASE: 07-123

NASA SPACECRAFT AIDS IN FORECAST OF SOLAR RADIATION STORMS

WASHINGTON - NASA's Solar and Heliospheric Observatory (SOHO) now 
enables scientists to forecast solar radiation storms, giving future 
astronauts, traveling to the moon and Mars, time to seek shelter and 
ground controllers time to safeguard satellites. The new method for 
the first time offers as much as one hour advance notice when a storm 
is approaching. 

"Solar radiation storms are notoriously difficult to predict. They 
often take us by surprise, but now we've found a way to anticipate 
these events," says Arik Posner, a physicist in NASA's Science 
Mission Directorate, Washington. Posner is on temporary assignment to 
NASA from Southwest Research Institute, San Antonio. Posner developed 
the technique. His study appears in a recent issue of the journal 
Space Weather.

Solar radiation storms are swarms of electrons, protons and heavy ions 
accelerated to high speed by explosions on the sun. On Earth, humans 
are protected from these particles by Earth's atmosphere and magnetic 
field. Astronauts in Earth orbit also are protected since Earth's 
magnetic field extends far enough to shield them. Solar radiation 
storms are a potential risk factor for astronauts working on the 
surface of the moon or Mars since neither has a substantial magnetic 
field.

"A one hour warning would reduce the odds of being caught in a solar 
storm outside of a lunar habitat, where astronauts are most 
vulnerable," says Francis Cucinotta, chief scientist for the NASA 
Space Radiation Program at NASA's Johnson Space Center, Houston. 

Spacecraft and satellites would also benefit. Subatomic particles 
striking computer processors and other electronics can cause onboard 
computers to suddenly reboot or issue nonsense commands. If a 
satellite operator knows that a storm is coming, the craft can be 
placed in a protective "safe mode" until the storm passes. 

The type of particle most feared by safety experts is the ion, an atom 
that has lost one or more of its charge-balancing electrons. 
Energetic ions can damage tissue and break strands of DNA, an effect 
not fully understood in terms of human disease.

The goal of researchers is to forecast when the ions will arrive. "The 
key is electrons. They are always detected ahead of the more 
dangerous ions," says Posner. While this has been known for years, 
only recently has this research turned the "electrons first" aspect 
of radiation storms into a tool for forecasting. 

Every radiation storm is a mix of electrons, protons and heavier ions. 
The electrons, being lighter and faster than the others, race out 
ahead. By measuring the "rise time and intensity of the initial 
electron surge" Posner could predict how many ions were following and 
when they would arrive. 

The key to the breakthrough was the Comprehensive Suprathermal and 
Energetic Particle Analyzer (COSTEP) instrument on board the 
observatory. COSTEP counts particles coming from the sun and measures 
their energies. Posner looked at hundreds of radiation storms 
recorded by COSTEP between 1996 and 2002, and was able to construct 
an empirical, predictive matrix that involved plugging an electron 
data into the matrix, and an ion forecast emerging.

After testing the results, the matrix was used on COSTEP data gathered 
in 2003, a year not yet analyzed and which formed no part of the 
matrix itself. The matrix was applied to the electron data and as a 
result, it successfully predicted all four major ion storms of 2003 
with advance warnings ranging from 7 to 74 minutes.

"While the method is not yet perfect, I'd like to improve that," 
Posner says. Improvements will come as Posner works his way through 
even more of COSTEP's dataset.

"Launched with SOHO in 1995, COSTEP has been operating through an 
entire solar cycle including the recent solar maximum in 2001, and it 
is still going strong," says Prof. Bernd Heber, COSTEP's principle 
investigator at the University of Kiel, Germany.

The method is being considered by planners at the Johnson Space Center 
in their design of future lunar missions. "Posner's technique reduces 
the odds of exposure by more than 20 percent compared to current 
methods, allowing astronauts to venture farther from their outpost. 
That's good for both science and exploration," says Cucinotta.

"NASA's Vision for Space Exploration will lead humans away from 
Earth's protective magnetic cocoon and into the unprotected seas of 
outer space," says Posner. "New scientific knowledge concerning basic 
processes of space will ensure safe, effective achievement of NASA's 
future space exploration activities."

SOHO is a project of international cooperation between the European 
Space Agency and NASA. For more information on NASA's study of the 
solar system, visit: 

http://www.nasa.gov/mission_pages/soho/index.html

	
-end-



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