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Tiny 'Firefly' satellite to study terrestrial gamma-ray flashes

Monday, 1 February 2010

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Gamma-ray flash

An artist's impression of a terrestrial gamma-ray flash.

Credit: NASA

HUNTSVILLE, USA: Gamma-ray flashes that occur in the Earth's atmosphere have been a mystery for more than 15 years. Now NASA scientists will launch the first dedicated survey of these flashes.

High-energy bursts of gamma rays typically occur far out in space, but there is a lesser known, more mysterious category: the powerful gamma ray flashes in the skies above.

Little is known about terrestrial gamma-ray flashes, or TGFs. They seem to have a connection with lightning, but TGFs themselves are something entirely different.

"In fact," says Doug Rowland of NASA's Goddard Space Flight Center, "before the 1990s nobody knew they even existed. And yet they're the most potent natural particle accelerators on Earth."

Individual particles in a TGF acquire a huge amount of energy, sometimes in excess of 20 mega-electron volts (MeV). In contrast, the colourful auroras that light up the skies at high latitudes are powered by particles with less than one thousandth as much energy.

Stowaway satellite

At this stage, there are more questions about TGFs than answers. What causes these high-energy flashes? Do they help trigger lightning - or does lightning trigger them? Could they be responsible for some of the high-energy particles in the Van Allen radiation belts, which can damage satellites?

To investigate, Rowland and his colleagues at GSFC, Siena College, Universities Space Research Association and the Hawk Institute for Space Sciences are planning to launch a tiny, football-sized satellite called Firefly. Because of its small size, Firefly will cost less than $1 million and can be launched as a 'stowaway' — aboard a rocket carrying a larger satellite into space, rather than requiring a dedicated rocket launch.

If successful, Firefly will return the first simultaneous measurements of TGFs and lightning. Most of what's known about TGFs to date has been learned from missions meant to observe gamma rays coming from deep space, such as NASA's Compton Gamma Ray Observatory, which discovered TGFs in 1994.

Surprise discovery of powerful flashes

As it stared out into space, Compton caught fleeting glimpses of gamma rays out of the corner of its 'eye', so to speak. It surprised scientists to discover that the powerful flashes were coming from Earth's atmosphere.

Subsequent data from Compton and other space telescopes have provided a tantalizingly incomplete picture of how TGFs occur: in the skies above a thunderstorm, powerful electric fields generated by the storm stretch upward for many miles into the upper atmosphere.

These electric fields accelerate free electrons, whisking them to speeds approaching the speed of light. When these ultra-high speed electrons collide with molecules in the air, the collisions release high-energy gamma rays as well as more electrons, setting up a cascade of collisions and perhaps more TGFs.