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Forget Star Wars -- BlueGene Brightens Galaxy


In a new experiment (LOPES), astrophysicists at the Netherlands Foundation for Research in Astronomy (ASTRON) have recorded the brightest and fastest radio blasts ever seen in the sky. Using a protype of a new high-tech radio telescope (LOFAR), along with IBM's BlueGene supercomputer, the researchers showed that the radio flashes are produced in the Earth's atmosphere by the impact of the most energetic particles produced in the cosmos. These particles are called ultra-high energy cosmic rays and their origin is an ongoing puzzle. The astrophysicists now hope that their finding will shed new light on the mystery of these particles.

The scientists used an array of radio antennas located within a field of particle detectors of the KASCADE Grande experiment at the Forschungszentrum Karlsruhe. They showed that whenever a very energetic cosmic particle hit the Earth atmosphere a corresponding radio pulse was recorded in the direction of the incoming particle. Using imaging techniques from radio astronomy, the group even produced digital film sequences of these events, yielding the fastest movies ever produced in radio astronomy. The particle detectors provided them with basic information about the incoming cosmic rays.

What does all of this really mean?

"By building ever larger telescopes we can detect and sense ever fainter radio signals, ever fainter means ever more distant, and because these signals travel the Universe at the speed of light, ever more distant means ever further back in time," said Dr. Eugene J. de Geus, ASTRON general affairs.

"LOFAR will be so sensitive, that we expect to detect signals from the period in the evolution of the universe when, after the big bang, the first stars or galaxies formed (this period is called the epoch of reionization). This will provide us with a very basic understanding of the physics of the early universe," he continued.

The use of the LOFAR system, he says, is not limited to just astrophysics. By linking sensors to complex models running on BlueGene, researchers will find more information on the geology of the subsurface, crop-growth, and meteorology, for example.

The radio telescope LOPES (LOFAR Prototype Station) uses prototype antennas of LOFAR to be built after 2006 in the Netherlands and parts of Germany. LOFAR has a radical new design, combining a multitude of cheap low-frequency antennas which collect the radio signals from the entire sky at once. Connected by high-speed internet, the BlueGene supercomputer then has the ability to detect unusual signals and make images of interesting regions on the sky without moving any mechanical structure.

Before teaming with IBM, the LOPES project team knew they needed an industry partner that could help them obtain very large processing power capabilities (27.5 Tflops) and accomodations for large sustained data input streams of 400 Gb/s.

"Futhermore, internally to the supercomputer, the amount of data being passed around explodes to 46 Tb/sec (i.e. 46 trillion complex calculations per second). The internal architecture of BlueGene is eminently suited to this purpose," said Eugène de Geus, ASTRON general affairs.

The researchers were able to show that the strength of the emitted radio signal was a direct measure of the cosmic ray energy. "It is amazing that with simple FM radio antennas we can measure the energy of some of the smallest particles coming from the cosmos" says ASTRON's Prof. Heino Falcke, who initiated and supervised the experiment. "If we would have sensitive radio eyes, we would see the sky sparkle with radio flashes", he adds.

The detection has been confirmed in part by a French group using the large radio telescope of the Paris observatory at Nançay. Historically, work on radio emission from cosmic rays was first done in the late 1960ies with the first claims of detections. However, no useful information could be extracted with the technology of these days, work ceased quickly, and the historic results came into question. The main shortcomings were the lack of imaging capabilities, the low time resolution, and the lack of a well-calibrated particle detector array. All of this has been overcome with the LOPES experiment.

de Gues feels that the project will open up a new field of HPC centered on "data-intensive" supercomputing or "streaming supercomputing." He believes that such coupled systems could become very wide-spread because they allow scientists to obtain a better undestanding of the environment.

As a next step, the astrophysicists want to use the upcoming LOFAR array in the Netherlands and Germany for cosmic ray research and install LOFAR-like radio antennas at the giant cosmic ray experiment "AUGER" in Argentina. The group hopes to use the new technique for detecting and understanding the nature of the highest energy cosmic rays and also detect the elusive ultra- high energy neutrinos.


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