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MPE Press Release January 10, 2011
 
 
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Space telescope catches antimatter from terrestrial thunderstorms

Normally astronomers look deep into space, but in the latest finding from the NASA Fermi Gamma-ray Space Telescope presented on Monday, Jan. 10, during a news briefing at the American Astronomical Society meeting, they detected an antimatter signal from Earth. Created in energetic processes above thunderstorms, when such an antimatter beam strikes the spacecraft, it actually becomes a source of the gamma-ray light it was designed to observe. Scientists at the Max Planck Institute for Extraterrestrial Physics (MPE) were responsible for the development of the detectors and the power supplies of the Fermi Gamma-ray Burst Monitor (GBM), which led to this discovery, and contributed to the calibration and data analysis for this particular result.

TGF
While Fermi flew over Egypt, the GBM intercepted a particle beam from a terrestrial gamma-ray flash (TGF) that occurred in a thunderstorm below its horizon.
Credit: NASA/Goddard Space Flight Center


When an antimatter particle strikes Fermi, it will collide with a particle of normal matter. Both particles are immediately annihilated and transformed into gamma rays of characteristic energy. The GBM detected gamma rays with energies of 511,000 electron volts, a signal indicating that an electron has met its antimatter counterpart -- a positron. For comparison, visible light has energies between 2 and 3 electron volts.

The scientists think that the antimatter particles were formed in a terrestrial gamma-ray flash (TGF), a brief burst of gamma rays produced inside thunderstorms that is somehow associated with lightning. "These gamma photons have typical energies of 20-40 million electron volts, and these are usually detected as TGF," says Andreas v. Kienlin, scientist at the MPE who led the development of the Fermi GBM.

Theorists estimate that about 500 TGFs occur worldwide each day, but most go undetected. Even though Fermi's GBM is designed to observe high-energy events in the distant universe, the GBM team has identified 130 TGFs since Fermi's launch. During one TGF, which occurred on Dec. 14, 2009, Fermi was located over Egypt. But the active storm was in Zambia, some 2,800 miles (4,500 km) to the south. Because the distant storm was below Fermi's horizon, any gamma that rays it produced could not have been detected by the GBM. High-speed electrons and positrons produced in the TGF, however, could travel along the Earth's magnetic field to strike the spacecraft and produce a pulse of gamma rays that was picked up by Fermi's GBM. "This signal is the first direct evidence that thunderstorms make antimatter particle beams," said Michael Briggs, a member of the GBM team at the University of Alabama.

The detection of positrons thus proves that copious high-energy particles are indeed being ejected from the atmosphere. In fact, scientists now think that all TGFs emit electron/positron beams. "However, we still don't know how these TGFs are produced, and we also do not quite understand how the classical lightning forms," says Jochen Greiner from the MPE, the German principal investigator of the GBM. Even though turbulence in thunderclouds can produce large voltages, they are not strong enough to ionize the air and to lead to sparks. TGFs could provide the trigger.

A paper on the findings will appear in a forthcoming issue of Geophysical Research Letters.


Press releases :
  For more information, images and animations on the Web, see the external link NASA press release

Links :
  internal linkFermi GBM at MPE

Contact :
  internal link Dr. Hannelore Hämmerle
Press Officer
Max-Planck-Institut für extraterrestrische Physik
phone: +49 89 30000-3980
email: hanneh@mpe.mpg.de
  internal link Dr. Jochen Greiner
Max-Planck-Institut für extraterrestrische Physik
phone: +49 89 30000-3847
email: jcg@mpe.mpg.de
  internal link Dr. Andreas von Kienlin
Max-Planck-Institut für extraterrestrische Physik
phone: +49 89 30000-3514
email: azk@mpe.mpg.de
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