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Blue building with silver towers and hose in foreground.
Photo Credit: Peter Rejcek
The IceCube laboratory at the South Pole Station, with hoses for the hotwater drill system in the foreground. The cables attached to the detector strings feed into the silver towers on either side of the building. The data from the neutrino telescope is processed here before being transmitted to the University of Wisconsin-Madison. 
 

Unexpected Results

In fact, even though major construction was just completed, and the final seven strings that were installed this season won’t be fully online until May 2011, the neutrino telescope has been taking data for several years now.

Recently, IceCube scientists detected an unusual pattern in cosmic ray intensity toward the Earth’s Southern Hemisphere, with an excess of cosmic rays detected in one part of the sky and a deficit in another. A similar lopsidedness, called “anisotropy,” has been seen from the Northern Hemisphere by other cosmic ray experiments. [See related story: Background noise.]

One possible explanation for the irregular pattern is the remains of an exploded supernova in the Milky Way Galaxy.

Additionally, IceCube is recording more than 10,000 neutrinos per year coming from the interaction of the cosmic ray-charged particles within the Earth's atmosphere. But very few of these neutrinos, especially those discovered coming through the Earth from the Northern Hemisphere, are the high-energy particles that the telescope was designed to detect.

Orange flags fly in front of buildings.
Photo Credit: Peter Rejcek
Orange flags mark the location of IceTop tanks and IceCube detector strings across a cubic kilometer of ice at the South Pole.
Hoses run between modular buildings.
Photo Credit: Peter Rejcek
A web of hoses run between buildings at the hotwater drill camp.
Two red buildings with winch in background.
Photo Credit: Peter Rejcek
The IceCube drill towers, with the South Pole Station in the distance.

Jens Dreyer, one of two IceCube personnel who will spend the winter at the South Pole to operate the experiment during the dark, cold months in 2011, said he’s been fortunate to see one such event.

In the previous winter, his predecessors only detected three during the eight months of winter isolation.

“The more energetic an event, the more rare it is,” Dreyer said.

Proof of concept

That such an experiment could even be attempted is an equally rare event. And it all started more than 20 years ago.

In 1987, Francis Halzen External Non-U.S. government site, the principal investigator on IceCube at UW-Madison, wrote the first paper on the idea of using Antarctic ice as a medium to ensnare neutrinos. Other physicists had been trying to use DOM-like instruments in water, but Halzen believed ice would work better than the ocean.

It then took about 10 years to make the now-famous AMANDA experiment work. Construction of the Antarctic Muon and Neutrino Detector Array was a sort of proof of concept for IceCube. The first detector string for AMANDA went down into South Pole ice in 1993. Four years later, AMANDA recorded the first-ever precision map of a high-energy neutrino event.

That’s about the time when Karle got involved.

“The most important thing was that it proved this was possible: To use ice as a medium and — what seemed to be a crazy idea — to put sensors 2.5 kilometers underneath the ice,” he said.

Still, even with the success of AMANDA, the proposal to build IceCube seemed daunting to many.

Remember that the South Pole Station is at the bottom of the world, requiring most materials and fuel to be flown across the continent aboard LC-130 aircraft operated by the New York Air National Guard External U.S. government site. The field season is short — scarcely more than three months — with time available for drilling even shorter based on the effort required to unpack and repack the drill camp every year.

“It’s amazing we were able to do it. Back in the AMANDA days, we wouldn’t have thought it would have been possible to put in 86 strings in that sort of time,” said Gary Hill, a physicist and lead DOM deployer from Australia.

“There’s a big sense of satisfaction that we were able to pull it off in the end,” he added. “Now we look forward to seeing the data that comes from it. It’s a mixture of emotions, but positive. It’s time to move on with it.” Back   1 2 3   Next

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Curator: Peter Rejcek, Antarctic Support Contract | NSF Official: Winifred Reuning, Division of Polar Programs