Author
Listed:
- Nicole A. Kelley
(Space Sciences Laboratory, University of California, Berkeley, 7 Gauss Way)
- David M. Smith
(University of California)
- Joseph R. Dwyer
(University of New Hampshire)
- Michael Splitt
(Florida Institute of Technology)
- Steven Lazarus
(Florida Institute of Technology)
- Forest Martinez-McKinney
(University of California)
- Bryna Hazelton
(University of Washington)
- Brian Grefenstette
(Space Radiation Laboratory, California Institute of Technology)
- Alexander Lowell
(Space Sciences Laboratory, University of California, Berkeley, 7 Gauss Way)
- Hamid K. Rassoul
(Florida Institute of Technology)
Abstract
Gamma-ray ‘glows’ are long duration (seconds to tens of minutes) X-ray and gamma-ray emission coming from thunderclouds. Measurements suggest the presence of relativistic runaway electron avalanches (RREA), the same process underlying terrestrial gamma-ray flashes. Here we demonstrate that glows are relatively a common phenomena near the tops of thunderstorms, when compared with events such as terrestrial gamma-ray flashes. Examining the strongest glow measured by the airborne detector for energetic emissions, we show that this glow is measured near the end of a downward RREA, consistent with occurring between the upper positive charge layer and the negative screening layer above it. The glow discharges the upper positive layer by ≥9.6 mA, strong enough to be an important charging mechanism of the storm. For this glow, the gamma-ray flux observed is close to the value at which relativistic feedback processes become important, with an avalanche multiplication factor of 4,500.
Suggested Citation
Nicole A. Kelley & David M. Smith & Joseph R. Dwyer & Michael Splitt & Steven Lazarus & Forest Martinez-McKinney & Bryna Hazelton & Brian Grefenstette & Alexander Lowell & Hamid K. Rassoul, 2015.
"Relativistic electron avalanches as a thunderstorm discharge competing with lightning,"
Nature Communications, Nature, vol. 6(1), pages 1-7, November.
Handle:
RePEc:nat:natcom:v:6:y:2015:i:1:d:10.1038_ncomms8845
DOI: 10.1038/ncomms8845
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