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Fermi Improves Its Vision For Thunderstorm Gamma-ray Flashes

Thanks to improved data analysis techniques and a new operating mode, the Gamma-ray Burst Monitor (GBM) aboard NASA's Fermi Gamma-ray Space Telescope is now 10 times better at catching the brief outbursts of high-energy light mysteriously produced above thunderstorms.

The outbursts, known as terrestrial gamma-ray flashes (TGFs), last only a few thousandths of a second, but their gamma rays rank among the highest-energy light that naturally occurs on Earth. The enhanced GBM discovery rate helped scientists show most TGFs also generate a strong burst of radio waves, a finding that will change how scientists study this poorly understood phenomenon.

Lightning emits a broad range of very low frequency (VLF) radio waves, often heard as pop-and-crackle static when listening to AM radio. The World Wide Lightning Location Network (WWLLN), a research collaboration operated by the University of Washington in Seattle, routinely detects these radio signals and uses them to pinpoint the location of lightning discharges anywhere on the globe to within about 12 miles (20 km).

Scientists have known for a long time TGFs were linked to strong VLF bursts, but they interpreted these signals as originating from lightning strokes somehow associated with the gamma-ray emission.

"Instead, we've found when a strong radio burst occurs almost simultaneously with a TGF, the radio emission is coming from the TGF itself," said co-author Michael Briggs, a member of the GBM team.

The researchers identified much weaker radio bursts that occur up to several thousandths of a second before or after a TGF. They interpret these signals as intracloud lightning strokes related to, but not created by, the gamma-ray flash.

Scientists suspect TGFs arise from the strong electric fields near the tops of thunderstorms. Under certain conditions, the field becomes strong enough that it drives a high-speed upward avalanche of electrons, which give off gamma rays when they are deflected by air molecules.

"What's new here is that the same electron avalanche likely responsible for the gamma-ray emission also produces the VLF radio bursts, and this gives us a new window into understanding this phenomenon," said Joseph Dwyer, a physics professor at the Florida Institute of Technology in Melbourne, Fla., and a member of the study team.

Because the WWLLN radio positions are far more precise than those based on Fermi's orbit, scientists will develop a much clearer picture of where TGFs occur and perhaps which types of thunderstorms tend to produce them.

Watch this video on YouTube.

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Another multimedia item related to this story:
     Terrestrial Gamma-ray Flashes Create Antimatter (id 10706)
More information on this topic available at:
http://www.nasa.gov/mission_pages/GLAST/news/vision-improve.html

Lightning in the clouds is directly linked to events that produce some of the highest-energy light naturally made on Earth: terrestrial gamma-ray flashes (TGFs). An instrument aboard NASA's Fermi Gamma-ray Space Telescope was recently fine-tuned to better catch TGFs, and this allowed scientists to discover that TGFs emit radio waves, too.    Lightning in the clouds is directly linked to events that produce some of the highest-energy light naturally made on Earth: terrestrial gamma-ray flashes (TGFs). An instrument aboard NASA's Fermi Gamma-ray Space Telescope was recently fine-tuned to better catch TGFs, and this allowed scientists to discover that TGFs emit radio waves, too.

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This image, taken in May 2008 as the Fermi Gamma-ray Space Telescope was being readied for launch, highlights the detectors of the spacecraft's Gamma-ray Burst Monitor (GBM). The GBM is an array of 14 crystal detectors designed for transient lower-energy gamma-ray outbursts, such as TGFs.  Labeled. Credit: NASA/Jim Grossmann    This image, taken in May 2008 as the Fermi Gamma-ray Space Telescope was being readied for launch, highlights the detectors of the spacecraft's Gamma-ray Burst Monitor (GBM). The GBM is an array of 14 crystal detectors designed for transient lower-energy gamma-ray outbursts, such as TGFs. Labeled.

Credit: NASA/Jim Grossmann

Available formats:
  2500 x 1820     JPEG       4 MB


This image, taken in May 2008 as the Fermi Gamma-ray Space Telescope was being readied for launch, highlights the detectors of the spacecraft's Gamma-ray Burst Monitor (GBM). The GBM is an array of 14 crystal detectors designed for transient lower-energy gamma-ray outbursts, such as TGFs. Unlabeled. Credit: NASA/Jim Grossmann    This image, taken in May 2008 as the Fermi Gamma-ray Space Telescope was being readied for launch, highlights the detectors of the spacecraft's Gamma-ray Burst Monitor (GBM). The GBM is an array of 14 crystal detectors designed for transient lower-energy gamma-ray outbursts, such as TGFs. Unlabeled.

Credit: NASA/Jim Grossmann

Available formats:
  2500 x 1820     JPEG       4 MB


This image, taken in May 2008 as the Fermi Gamma-ray Space Telescope was being readied for launch, highlights the detectors of the spacecraft's Gamma-ray Burst Monitor (GBM). The GBM is an array of 14 crystal detectors designed for transient lower-energy gamma-ray outbursts, such as TGFs. Uncropped. Credit: NASA/Jim Grossmann    This image, taken in May 2008 as the Fermi Gamma-ray Space Telescope was being readied for launch, highlights the detectors of the spacecraft's Gamma-ray Burst Monitor (GBM). The GBM is an array of 14 crystal detectors designed for transient lower-energy gamma-ray outbursts, such as TGFs. Uncropped.

Credit: NASA/Jim Grossmann

Available formats:
  5000 x 7470     JPEG     18 MB

Short URL to This Page:http://svs.gsfc.nasa.gov/goto?11131
Animation Number:11131
Completed:2012-11-02
Animators:Walt Feimer (HTSI)
 Scott Wiessinger (USRA)
 Hal Pierce (SSAI)
 Joseph Dwyer (FIT)
Video Editor:Scott Wiessinger (USRA)
Narrator:Scott Wiessinger (USRA)
Producer:Scott Wiessinger (USRA)
Scientists:Valerie Connaughton (NASA MSFC/University of Alabama)
 Michael Briggs (NASA/MSFC)
Writers:Francis Reddy (Syneren Technologies)
 Scott Wiessinger (USRA)
Platforms/Sensors/Data Sets:Fermi/Gamma Ray Burst Monitor/Terrestrial Gamma Flashes
 Fermi
Series:Narrated Movies
 Astrophysics Features
Goddard TV Tape:G2012-115 -- Fermi TGF Radio
Please give credit for this item to:
NASA/Goddard Space Flight Center. However, individual images should be credited as indicated above.
 
Keywords:
SVS >> Gamma Ray
SVS >> HDTV
SVS >> Lightning
SVS >> Music
SVS >> Storm
GCMD >> Earth Science >> Spectral/Engineering >> Radio Wave
SVS >> Astrophysics
SVS >> Edited Feature
SVS >> Fermi
 
 


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Many of our multimedia items use the GCMD keywords. These keywords can be found on the Internet with the following citation:
Olsen, L.M., G. Major, K. Shein, J. Scialdone, S. Ritz, T. Stevens, M. Morahan, A. Aleman, R. Vogel, S. Leicester, H. Weir, M. Meaux, S. Grebas, C.Solomon, M. Holland, T. Northcutt, R. A. Restrepo, R. Bilodeau, 2013. NASA/Global Change Master Directory (GCMD) Earth Science Keywords. Version 8.0.0.0.0

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