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Cosmic rays hit Space-Age high

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September 30, 2009

An artist's concept of the heliosphere, a magnetic bubble that partially protects the sola...

An artist's concept of the heliosphere, a magnetic bubble that partially protects the solar system from cosmic rays - represented by the long, white arrows (Image: Richard Mewaldt/Caltech)

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NASA has a warning for everyone planning a trip to Mars in the near future – it might be a good idea to wrap yourself in tinfoil when you travel (maybe dress like Jack Black’s character in the movie Be Kind Rewind). Seriously, according to sensors on NASA's ACE (Advanced Composition Explorer) spacecraft, galactic cosmic rays have just hit a Space Age high.

"In 2009, cosmic ray intensities have increased 19 percent beyond anything we've seen in the past 50 years," says Richard Mewaldt of the California Institute of Technology. "The increase is significant, and it could mean we need to re-think how much radiation shielding astronauts take with them on deep-space missions."

The universe balances itself …

Caltech says the cause of the surge is solar minimum, a deep lull in solar activity that began around 2007 and continues today. But when solar activity is low, cosmic rays go up, and right now solar activity is as weak as it has been in modern times, setting the stage for what Mewaldt calls "a perfect storm of cosmic rays."

"We're experiencing the deepest solar minimum in nearly a century," says Dean Pesnell of the Goddard Space Flight Center, "so it is no surprise that cosmic rays are at record levels for the Space Age."

Galactic cosmic rays generate from outside our solar system. They are subatomic particles - mainly protons but also some heavy nuclei - accelerated to almost light speed by distant supernova explosions. A single cosmic ray can disable a satellite if it hits an integrate circuit. Rays give off "air showers" of secondary particles when they hit Earth's atmosphere, hence they pose a health hazard to astronauts.

Thankfully for us, the sun's magnetic field is our first line of defense against these highly-charged, energetic particles. From Mercury to Pluto and beyond, the solar system is surrounded by a bubble of solar magnetism called the heliosphere. It initiates from the sun's inner magnetic dynamo and is inflated to enormous proportions by the solar wind. When a cosmic ray tries to enter the solar system, it has to battle through the heliosphere's outer layers; and if it makes it inside, there is a secondary force of magnetic fields waiting to scatter and deflect the intruder.

"At times of low solar activity, this natural shielding is weakened, and more cosmic rays are able to reach the inner solar system," explains Pesnell.

Mewaldt says three aspects of the current solar minimum are combining to create the perfect storm. Firstly, the sun's magnetic field is weak. "There has been a sharp decline in the sun's interplanetary magnetic field (IMF) down to only 4 nanoTesla (nT) from typical values of 6-8nT," he says. "This record-low IMF undoubtedly contributes to the record-high cosmic ray fluxes."

Secondly, the solar wind is flagging. "Measurements by the Ulysses spacecraft show that solar wind pressure is at a 50-year low," he says, "so the magnetic bubble that protects the solar system is not being inflated as much as usual." A smaller bubble gives cosmic rays a shorter-shot into the solar system. Once a cosmic ray enters the solar system, it must ‘swim upstream’ against the solar wind. Solar wind speeds have dropped to very low levels in 2008 and 2009, making it easier than usual for a cosmic ray to proceed.

Finally, the current sheet is flattening. Mewaldt says imagine the sun wearing a ballerina's skirt as wide as the entire solar system with an electrical current flowing along the wavy folds. That is the "heliospheric current sheet," a vast transition zone where the polarity of the sun's magnetic field changes from plus (north) to minus (south). The current sheet is important because cosmic rays tend to be guided by its folds. Lately, Mewaldt says the current sheet has been flattening itself out, allowing cosmic rays more direct access to the inner solar system.

"If the flattening continues as it has in previous solar minima, we could see cosmic ray fluxes jump all the way to 30 percent above previous Space Age highs," Mewaldt warns.

But fear not! Earth is in no great peril from the extra cosmic rays. The planet's atmosphere and magnetic field combine to form a formidable shield against space radiation, protecting humans on the surface. History says we've weathered storms much worse than this. Seemingly, hundreds of years ago, cosmic ray fluxes were at least 200 percent higher than they are now. Researchers know this because when cosmic rays hit the atmosphere, they produce an isotope of beryllium, 10Be, which is preserved in polar ice. By examining ice cores, it is possible to estimate cosmic ray fluxes more than 1,000 years into the past. Even with the recent surge, cosmic rays today are much weaker than they have been at times in the past millennium.

"The space era has so far experienced a time of relatively low cosmic ray activity," says Mewaldt. "We may now be returning to levels typical of past centuries."

NASA spacecraft will continue to monitor the situation as solar minimum unfolds. But just in case, I’m transferring all my old video tapes to DVD.

1 Comment

What they don't tell you is what happens at the next solar maximum... estimated at around 2012!

Jesse Kuch
30th September, 2009 @ 09:15 pm PDT
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