Localization of the source of terrestrial neutron bursts detected in thunderstorm atmosphere
To localize an altitude of the neutron source responsible for the neutron flux enhancements observed on the ground, numerical simulations of photonuclear production and transport to on‐ground detector locations were carried out. The neutron fluence calculated for the volumetric source located at the...
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Published in | Journal of Geophysical Research: Space Physics Vol. 115; no. A5 |
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Main Authors | , , , |
Format | Journal Article |
Language | English |
Published |
Washington
Blackwell Publishing Ltd
01.05.2010
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Subjects | |
Online Access | Get full text |
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Summary: | To localize an altitude of the neutron source responsible for the neutron flux enhancements observed on the ground, numerical simulations of photonuclear production and transport to on‐ground detector locations were carried out. The neutron fluence calculated for the volumetric source located at the altitudes 8–12 km is consistent with that estimated from neutron numbers measured on the ground. This altitude range is consistent with the idea that the burst of hard γ rays detected recently by Tsuchiya et al. (2007, 2009) originate from a volumetric intracloud γ ray source. Most likely, the photonuclear reactions caused by bremsstruhlung of descending relativistic runaway electron avalanches account for the neutron flux increases observed in the thunderstorm atmosphere. |
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Bibliography: | istex:4C30E27A582870DF2DD4E978BDA0E895538F725F ark:/67375/WNG-HTXQZBNN-B Tab-delimited Table 1. ArticleID:2009JA014750 ObjectType-Article-1 SourceType-Scholarly Journals-1 ObjectType-Feature-2 content type line 23 |
ISSN: | 0148-0227 2169-9380 2156-2202 2169-9402 |
DOI: | 10.1029/2009JA014750 |