Quantcast

Strange Little Sunspot May Herald the Coming Storm

August 17, 2006

On July 31st, a tiny sunspot was born. It popped up from the sun’s interior, floated around a bit, and vanished again in a few hours. On the sun this sort of thing happens all the time and, ordinarily, it wouldn’t be worth mentioning. But this sunspot was special: It was backward.

“We’ve been waiting for this,” says David Hathaway, a solar physicist at the Marshall Space Flight in Huntsville, Alabama. “A backward sunspot is a sign that the next solar cycle is beginning.”

“Backward” means magnetically backward. Hathaway explains:

Sunspots are planet-sized magnets created by the sun’s inner magnetic dynamo. Like all magnets in the Universe, sunspots have north (N) and south (S) magnetic poles. The sunspot of July 31st popped up at solar longitude 65o W, latitude 13o S. Sunspots in that area are normally oriented N-S. The newcomer, however, was S-N, opposite the norm.

A picture is worth a 1000 words. In the magnetic map of the sun, below, N is white and S is black. The backward sunspot is circled:

This tiny spot of backwardness matters because of what it might foretell: A really big solar cycle.

Solar activity rises and falls in 11-year cycles, swinging back and forth between times of quiet and storminess. Right now the sun is quiet. “We’re near the end of Solar Cycle 23, which peaked way back in 2001,” explains Hathaway. The next cycle, Solar Cycle 24, should begin “any time now,” returning the sun to a stormy state.

Satellite operators and NASA mission planners are bracing for this next solar cycle because it is expected to be exceptionally stormy, perhaps the stormiest in decades. Sunspots and solar flares will return in abundance, producing bright auroras on Earth and dangerous proton storms in space: full story.

But when will Solar Cycle 24 begin?

“Maybe it already did–on July 31st,” says Hathaway. The first spot of a new solar cycle is always backwards. Solar physicists have long known that sunspot magnetic fields reverse polarity from cycle to cycle. N-S becomes S-N and vice versa. “The backward sunspot may be the first sunspot of Cycle 24.”

It sounds exciting, but Hathaway is cautious on several fronts:

First, the sunspot lasted only three hours. Typically, sunspots last days, weeks or even months. Three hours is fleeting in the extreme. “It came and went so fast, it was not given an official sunspot number,” says Hathaway. The astronomers who number sunspots didn’t think it worthy!

Second, the latitude of the spot is suspicious. New-cycle sunspots almost always pop up at mid-latitudes, around 30o N or 30o S. The backward sunspot popped up at 13o S. “That’s strange.”

These odd-isms stop Hathaway short of declaring the onset of a new solar cycle. “But it looks promising,” he says.

Even if Cycle 24 has truly begun, “don’t expect any great storms right away.” Solar cycles last 11 years and take time to build up to fever pitch. For a while, perhaps one or two years, Cycle 23 and Cycle 24 will actually share the sun, making it a hodgepodge of backward and forward spots. Eventually, Cycle 24 will take over completely; then the fireworks will really begin.

Meanwhile, Hathaway plans to keep an eye out for more backward sunspots.

On the Net:

NASA

SOHO Mission




comments powered by Disqus