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dc.contributor.authorDwyer, Joseph R.
dc.contributor.authorLiu, Ningyu
dc.contributor.authorRassoul, Hamid K.
dc.date.accessioned2017-03-15T19:07:07Z
dc.date.available2017-03-15T19:07:07Z
dc.date.issued2013-08-08
dc.identifier.citationDwyer, J. R., Liu, N., & Rassoul, H. K. (2013). Properties of the thundercloud discharges responsible for terrestrial gamma-ray flashes. Geophysical Research Letters, 40(15), 4067-4073. doi:10.1002/grl.50742en_US
dc.identifier.urihttp://hdl.handle.net/11141/1227
dc.description.abstractThe source of terrestrial gamma-ray flashes (TGFs) has been an active area of research since their discovery by Compton Gamma-Ray Observatory/Burst and Transient Source Experiment in 1994. These intense bursts of gamma rays originate within thunderclouds via the rapid production of relativistic runaway electrons, accelerated by thundercloud/lightning electric fields to multi-MeV energies. Recent studies have shown that electrical discharges within thunderclouds caused by these runaway electrons can generate currents that rival those of lightning and so could serve as an alternative discharge path for thunderclouds. In particular, the discharges responsible for TGFs produce some of the largest amplitude VLF-LF radio pulses from thunderstorms and, indeed, were previously misidentified as lightning. In this article, we shall provide a brief review of TGFs and present calculations of their electrical properties inside thunderclouds and their gamma-ray and optical emissions. We shall show that the lightning-like events responsible for TGFs emit relatively little visible light and, thus, are inherently dark.en_US
dc.language.isoen_USen_US
dc.rightsThis published article is made available in accordance with the publisher’s policy. It may be subject to U.S. copyright law.en_US
dc.rights.urihttp://publications.agu.org/author-resource-center/usage-permissions/en_US
dc.titleProperties of the thundercloud discharges responsible for terrestrial gamma-ray flashesen_US
dc.typeArticleen_US
dc.identifier.doi10.1002/grl.50742


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