Author:
Scholten O.,Hare B. M.,Dwyer J.,Liu N.,Sterpka C.,Kolmašová I.,Santolík O.,Lán R.,Uhlíř L.,Buitink S.,Corstanje A.,Falcke H.,Huege T.,Hörandel J. R.,Krampah G. K.,Mitra P.,Mulrey K.,Nelles A.,Pandya H.,Rachen J. P.,Trinh T. N. G.,ter Veen S.,Thoudam S.,Winchen T.
Abstract
AbstractThe common phenomenon of lightning still harbors many secrets such as what are the conditions for lightning initiation and what is driving the discharge to propagate over several tens of kilometers through the atmosphere forming conducting ionized channels called leaders. Since lightning is an electric discharge phenomenon, there are positively and negatively charged leaders. In this work we report on measurements made with the LOFAR radio telescope, an instrument primarily build for radio-astronomy observations. It is observed that a negative leader rather suddenly changes, for a few milliseconds, into a mode where it radiates 100 times more VHF power than typical negative leaders after which it spawns a large number of more typical negative leaders. This mode occurs during the initial stage, soon after initiation, of all lightning flashes we have mapped (about 25). For some flashes this mode occurs also well after initiation and we show one case where it is triggered twice, some 100 ms apart. We postulate that this is indicative of a small (order of 5 km$$^2$$
2
) high charge pocket. Lightning thus appears to be initiated exclusively in the vicinity of such a small but dense charge pocket.
Funder
Stichting voor Fundamenteel Onderzoek der Materie
Nederlandse Organisatie voor Wetenschappelijk Onderzoek
Grantová Agentura České Republiky
Agentura Pro Zdravotnický Výzkum České Republiky
European Research Council
Fonds Wetenschappelijk Onderzoek
Deutsche Forschungsgemeinschaft
National Foundation for Science and Technology Development
Khalifa University of Science, Technology and Research
Publisher
Springer Science and Business Media LLC
Cited by
9 articles.
订阅此论文施引文献
订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献