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|    BAMA    |    Science Research Echo    |    1,586 messages    |
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|    Message 53 of 1,586    |
|    Roger Nelson to All    |
|    Thunderstorms Make Antimatter    |
|    12 Jan 11 08:09:40    |
      Thunderstorms Make Antimatter               Jan. 11, 2011: Scientists using NASA's Fermi Gamma-ray Space Telescope have       detected beams of antimatter produced above thunderstorms on Earth, a       phenomenon never seen before.               Scientists think the antimatter particles were formed inside thunderstorms in       a terrestrial gamma-ray flash (TGF) associated with lightning. It is estimated       that about 500 TGFs occur daily worldwide, but most go undetected.               "These signals are the first direct evidence that thunderstorms make       antimatter particle beams," said Michael Briggs, a member of Fermi's Gamma-ray       Burst Monitor (GBM) team at the University of Alabama in Huntsville (UAH). He       presented the findings Monday, during a news briefing at the American       Astronomical Society meeting in Seattle.       [...]       An artist's concept of antimatter spraying above a thunderhead. [video]       Fermi is designed to monitor gamma rays, the highest energy form of light.        When antimatter striking Fermi collides with a particle of normal matter, both       particles immediately are annihilated and transformed into gamma rays. The GBM       has detected gamma rays with energies of 511,000 electron volts, a signal       indicating an electron has met its antimatter counterpart, a positron. [...]       Although Fermi's GBM is designed to observe high-energy events in the       universe, it's also providing valuable insights into this strange phenomenon.       The GBM constantly monitors the entire celestial sky above and the Earth       below. The GBM team has identified 130 TGFs since Fermi's launch in 2008.               "In orbit for less than three years, the Fermi mission has proven to be an       amazing tool to probe the universe. Now we learn that it can discover       mysteries much, much closer to home," said Ilana Harrus, Fermi program       scientist at NASA Headquarters in Washington.       [...]       Fermi was above Egypt on Dec. 14, 2009, when a burst of positrons emerged from       an African thunderstorm. [larger image]               The spacecraft was located immediately above a thunderstorm for most of the       observed TGFs, but in four cases, storms were far from Fermi. In addition,       lightning-generated radio signals detected by a global monitoring network       indicated the only lightning at the time was hundreds or more miles away.       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 to the south. The distant       storm was below Fermi's horizon, so any gamma rays it produced could not have       been detected.               "Even though Fermi couldn't see the storm, the spacecraft nevertheless was       magnetically connected to it," said Joseph Dwyer at the Florida Institute of       Technology in Melbourne, Fla. "The TGF produced high-speed electrons and       positrons, which then rode up Earth's magnetic field to strike the spacecraft."               The beam continued past Fermi, reached a location, known as a mirror point,       where its motion was reversed, and then hit the spacecraft a second time just       23 milliseconds later. Each time, positrons in the beam collided with       electrons in the spacecraft. The particles annihilated each other, emitting       gamma rays detected by Fermi's GBM.               Scientists long have suspected TGFs arise from the strong electric fields near       the tops of thunderstorms. Under the right conditions, they say, the field       becomes strong enough that it drives an upward avalanche of electrons.       Reaching speeds nearly as fast as light, the high-energy electrons give off       gamma rays when they're deflected by air molecules. Normally, these gamma rays       are detected as a TGF.               [...]       Click to view the three steps thunderstorms must take to produce bursts of       anti-matter. [more]               But the cascading electrons produce so many gamma rays that they blast       electrons and positrons clear out of the atmosphere. This happens when the       gamma-ray energy transforms into a pair of particles: an electron and a       positron. It's these particles that reach Fermi's orbit.               The detection of positrons shows many high-energy particles are being ejected       from the atmosphere. In fact, scientists now think that all TGFs emit       electron/positron beams. A paper on the findings has been accepted for       publication in Geophysical Research Letters.               "The Fermi results put us a step closer to understanding how TGFs work," said       Steven Cummer at Duke University. "We still have to figure out what is special       about these storms and the precise role lightning plays in the process."                        Editor: Dr. Tony Phillips | Credit: Science@NASA               More Information       Fermi Home Page -- from NASA               Are TGFs Hazardous to Air Travelers? --- Science@NASA               Firefly Mission to Study Terrestrial Gamma-ray Flashes -- (Science@NASA)               What Comes Out of the Top of a Thunderstorm? -- (Science@NASA)               NASA's Fermi Gamma-ray Space Telescope is an astrophysics and particle physics       partnership. It is managed by NASA's Goddard Space Flight Center in Greenbelt,       Md. It was developed in collaboration with the U.S. Department of Energy, with       important contributions from academic institutions and partners in France,       Germany, Italy, Japan, Sweden and the United States.               The GBM Instrument Operations Center is located at the National Space Science       Technology Center in Huntsville, Ala. The team includes a collaboration of       scientists from UAH, NASA's Marshall Space Flight Center in Huntsville, the       Max Planck Institute for Extraterrestrial Physics in Germany and other       institutions.                       Regards,               Roger              --- D'Bridge 3.59        * Origin: NCS BBS (1:3828/7)    |
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