Each day, thunderstorms around the world produce about a thousand 
quick bursts of gamma rays, some of the highest-energy light naturally 
found on Earth. By merging records of events seen by NASA's Fermi 
Gamma-ray Space Telescope with data from ground-based radar and 
lightning detectors, scientists have completed the most detailed 
analysis to date of the types of thunderstorms involved. 
"Remarkably, we have found that any thunderstorm can produce gamma
 rays, even those that appear to be so weak a meteorologist wouldn't 
look twice at them," said Themis Chronis, who led the research at the 
University of Alabama in Huntsville (UAH).
New research merging Fermi data with information from ground-based radar
 and lightning networks shows that terrestrial gamma-ray flashes arise 
from an unexpected diversity of storms and may be more common than 
currently thought. Play video
The outbursts, called terrestrial gamma-ray flashes (TGFs), were 
discovered in 1992 by NASA's Compton Gamma-Ray Observatory, which 
operated until 2000. TGFs occur unpredictably and fleetingly, with 
durations less than a thousandth of a second, and remain poorly 
understood.
In late 2012, Fermi scientists employed new techniques that 
effectively upgraded the satellite's Gamma-ray Burst Monitor (GBM), 
making it 10 times more sensitive to TGFs and allowing it to record weak
 events that were overlooked before.
"As a result of our enhanced discovery rate, we were able to show 
that most TGFs also generate strong bursts of radio waves like those 
produced by lightning," said Michael Briggs, assistant director of the 
Center for Space Plasma and Aeronomic Research at UAH and a member of 
the GBM team. 
Previously, TGF positions could be roughly estimated based on 
Fermi's location at the time of the event. The GBM can detect flashes 
within about 500 miles (800 kilometers), but this is too imprecise to 
definitively associate a TGF with a specific storm.
Ground-based lightning networks use radio data to pin down strike 
locations. The discovery of similar signals from TGFs meant that 
scientists could use the networks to determine which storms produce 
gamma-ray flashes, opening the door to a deeper understanding of the 
meteorology powering these extreme events.
Chronis, Briggs and their colleagues sifted through 2,279 TGFs 
detected by Fermi's GBM to derive a sample of nearly 900 events 
accurately located by the Total Lightning Network operated by Earth 
Networks in Germantown, Maryland, and the World Wide Lightning Location 
Network, a research collaboration run by the University of Washington in
 Seattle. These systems can pinpoint the location of lightning 
discharges -- and the corresponding signals from TGFs -- to within 6 
miles (10 km) anywhere on the globe.
From this group, the team identified 24 TGFs that occurred within 
areas covered by Next Generation Weather Radar (NEXRAD) sites in 
Florida, Louisiana, Texas, Puerto Rico and Guam. For eight of these 
storms, the researchers obtained additional information about 
atmospheric conditions through sensor data collected by the Department 
of Atmospheric Science at the University of Wyoming in Laramie.
"All told, this study is our best look yet at TGF-producing 
storms, and it shows convincingly that storm intensity is not the key," 
said Chronis, who will present the findings Wed., Dec. 17, in an invited
 talk at the American Geophysical Union meeting in San Francisco. A 
paper describing the research has been submitted to the Bulletin of the 
American Meteorological Society.
Scientists suspect that TGFs arise from strong electric fields 
near the tops of thunderstorms. Updrafts and downdrafts within the 
storms force rain, snow and ice to collide and acquire electrical 
charge. Usually, positive charge accumulates in the upper part of the 
storm and negative charge accumulates below. When the storm's electrical
 field becomes so strong it breaks down the insulating properties of 
air, a lightning discharge occurs.
Under the right conditions, the upper part of an intracloud 
lightning bolt disrupts the storm's electric field in such a way that an
 avalanche of electrons surges upward at high speed. When these 
fast-moving electrons are deflected by air molecules, they emit gamma 
rays and create a TGF.
About 75 percent of lightning stays within the storm, and about 
2,000 of these intracloud discharges occur for each TGF Fermi detects.
The new study confirms previous findings indicating that TGFs tend
 to occur near the highest parts of a thunderstorm, between about 7 and 9
 miles (11 to 14 kilometers) high. "We suspect this isn't the full 
story," explained Briggs. "Lightning often occurs at lower altitudes and
 TGFs probably do too, but traveling the greater depth of air weakens 
the gamma rays so much the GBM can't detect them."
Based on current Fermi statistics, scientists estimate that some 
1,100 TGFs occur each day, but the number may be much higher if 
low-altitude flashes are being missed.
While it is too early to draw conclusions, Chronis notes, there 
are a few hints that gamma-ray flashes may prefer storm areas where 
updrafts have weakened and the aging storm has become less organized. 
"Part of our ongoing research is to track these storms with NEXRAD radar
 to determine if we can relate TGFs to the thunderstorm life cycle," he 
said.
Production editor: Dr. Tony Phillips | Credit: Science@NASA
More information:
Download video in HD formats from NASA Goddard's Scientific Visualization Studio
Fermi Improves its Vision for Thunderstorm Gamma-Ray Flashes (12.06.2012)
NASA's Fermi Catches Thunderstorms Hurling Antimatter into Space (01.10.2011)
Credits:
More information:
Download video in HD formats from NASA Goddard's Scientific Visualization Studio
Fermi Improves its Vision for Thunderstorm Gamma-Ray Flashes (12.06.2012)
NASA's Fermi Catches Thunderstorms Hurling Antimatter into Space (01.10.2011)