Universe  ID: 10706

Terrestrial Gamma-ray Flashes Create Antimatter

Released on January 10, 2011
NASA's Fermi Gamma-ray Space Telescope has detected beams of antimatter launched by thunderstorms. Acting like enormous particle accelerators, the storms can emit gamma-ray flashes, called TGFs, and high-energy electrons and positrons. Scientists now think that most TGFs produce particle beams and antimatter.

For additional animations showing bremsstrahlung and pair production gamma ray reactions, go here.

For more visualizations showing Fermi's TGF detections, go to#3747, #3748, and #3756.

For animations of the Fermi spacecraft and matter/antimatter, go to#10707 and #10651.

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TGFs produce high-energy electrons and positrons. Moving near the speed of light, these particles travel into space along Earth's magnetic field.

Watch this video on the NASAexplorer YouTube channel.

For complete transcript, click here.

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Interactions with matter can produce gamma rays and vice versa. So-called "bremsstrahlung" gamma rays result when high-energy electrons traveling close to the speed of light become deflected by passing near an atom or molecule. In pair production, a gamma ray passing through the electron shell of an atom transforms into two particles: an electron and its antimatter opposite, a positron.
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Animated diagram showing the behavior and composition of TGF emissions.

Credit: NASA/Goddard Space Flight Center/J. Dwyer/Florida Inst. of Technology

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A TGF produces gamma rays (magenta) as well as high-energy electrons (yellow) and positrons (green). This simulation tracks a TGF and its particle beams from their origin altitude of 9.3 miles (15 km) to 373 miles (600 km), beyond Fermi's orbit.

Credit: Joe Dwyer/Florida Inst. of Technology

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Sidebar: How thunderstorms launch particle beams into space
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On Dec. 14, 2009, while NASA's Fermi flew over Egypt, the spacecraft intercepted a particle beam from a terrestrial gamma-ray flash (TGF) that occurred over its horizon. Fermi's Gamma-ray Burst Monitor detected the signal of positrons annihilating on the spacecraft — not once, but twice. After passing Fermi, some of the particles reflected off of a magnetic "mirror" point and returned.
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On Dec. 14, 2009, while NASA's Fermi flew over Egypt, the spacecraft intercepted a particle beam from a terrestrial gamma-ray flash (TGF) that occurred over its horizon. Fermi's Gamma-ray Burst Monitor detected the signal of positrons annihilating on the spacecraft — not once, but twice. After passing Fermi, some of the particles reflected off of a magnetic "mirror" point and returned. No Labels.
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Fermi's position relative to the TGF it detected.
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Artist interpretation of the cloud of electrons and positrons passing through the Fermi satellite and causing it to emit gamma rays.
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Artist interpretation of electrons accelerating upwards from a thunderhead.
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Map of all terrestrial gamma-ray flashes detected by Fermi's Gamma-ray Burst Monitor through the end of 2010.

For animated version, go here,

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This image from the Meteosat 9 weather satellite was taken on Dec. 14, 2009, about 7 minutes after Fermi detected positrons from a TGF. No storms are present over Egypt, where Fermi was located at the time of the event, but thunderstorms are plentiful over Zambia.

Credit: SSEC/Univ. of Wisconsin, Madison

 

Related

NASA's Fermi Catches Gamma-ray Flashes from Tropical Storms
NASA's Fermi Helps Scientists Study Gamma-ray Thunderstorms
Fermi Improves Its Vision For Thunderstorm Gamma-ray Flashes

For More Information

http://www.nasa.gov/mission_pages/GLAST/news/fermi-thunderstorms.html

Credits

Walt Feimer (HTSI): Lead Animator
Scott Wiessinger (UMBC): Animator
Joseph Dwyer (FIT): Animator
Chris Meaney (HTSI): Animator
Scott Wiessinger (UMBC): Video Editor
Karen Fox (ADNET Systems, Inc.): Narrator
Scott Wiessinger (UMBC): Producer
Francis Reddy (University of Maryland College Park): Lead Science Writer
Scott Wiessinger (UMBC): Writer
Francis Reddy (University of Maryland College Park): Graphics
Francis Reddy (University of Maryland College Park): Visualizer
Tom Bridgman (Global Science and Technology, Inc.): Visualizer
Please give credit for this item to:
NASA/Goddard Space Flight Center. However, each image should be credited as indicated above.

Science Paper:
http://www.agu.org/journals/pip/gl/2010GL046259-pip.pdf

Short URL to share this page:
https://svs.gsfc.nasa.gov/10706

Missions:
Fermi Gamma-ray Space Telescope
GLAST

Data Used:
Fermi
view all stories where this data set is used
Note: While we identify the data sets used in these visualizations, we do not store any further details nor the data sets themselves on our site.

This item is part of these series:
Narrated Movies
Fermi
Goddard Shorts
Astrophysics Animations
Astrophysics Simulations
Astrophysics Stills
Astrophysics Features

Goddard TV Tape:
G2010-083 -- Fermi TGF Antimatter

Keywords:
SVS >> Antimatter
SVS >> Electron
SVS >> HDTV
SVS >> Lightning
SVS >> Satellite
GCMD >> Earth Science >> Spectral/Engineering >> Gamma Ray
SVS >> Astrophysics
SVS >> GLAST
SVS >> Edited Feature
SVS >> Gamma Ray Observatory
SVS >> Fermi
DLESE >> Narrated
NASA Science >> Universe

GCMD 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