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dc.contributor.authorVan der Velde, Oscar Arnoud
dc.contributor.authorLyons, Walter A.
dc.contributor.authorNelson, Thomas E.
dc.contributor.authorCummer, Steven A.
dc.contributor.authorLi, Jingbo
dc.contributor.authorBunnell, James
dc.contributor.otherUniversitat Politècnica de Catalunya. Departament d'Enginyeria Elèctrica
dc.date.accessioned2017-03-13T11:08:39Z
dc.date.available2017-03-13T11:08:39Z
dc.date.issued2007-10-17
dc.identifier.citationVan Der Velde, O., Lyons, W. A., Nelson, T. E., Cummer, S., Li, J., Bunnell, J. Analysis of the first gigantic jet recorded over continental North America. "Journal of geophysical research: atmospheres", 17 Octubre 2007, vol. 112, núm. D20104.
dc.identifier.issn2169-8996
dc.identifier.urihttp://hdl.handle.net/2117/102375
dc.description.abstract[1] Two low-light cameras near Marfa, Texas, recorded a gigantic jet over northern Mexico on 13 May 2005 at approximately 0423:50 UTC. Assuming that the farthest of two candidate storm systems was its source, the bright lower channel ended in a fork at around 50–59 km height with the very dim upper branches extended to 69–80 km altitude. During the time window containing the jet, extremely low frequency magnetic field recordings show that there was no fast charge moment change larger than 50 coulomb times kilometers (C km) but there was a larger and slower charge moment change of 520 C km over 70 ms. The likely parent thunderstorm was a high-precipitation supercell cluster containing a persistent mesocyclone, with radar echo tops of at least 17 km. However, photogrammetric analysis suggests that the gigantic jet occurred over the forward flank downdraft region with echo tops of 14 km. This part of the supercell may have had an inverted-polarity charge configuration as evidenced by positive cloud-to-ground lightning flashes (+CG) dominating over negative flashes (-CG), while -CGs occurred under the downwind anvil. Four minutes before the gigantic jet, -CG activity practically ceased in this area, while +CG rates increased, culminating during the 20 s leading up to the gigantic jet with four National Lightning Detection Network–detected +CGs. A relative lull in lightning activity of both polarities was observed for up to 1.5 min after the gigantic jet. The maturing storm subsequently produced 30 sprites between 0454 and 0820 UTC, some associated with extremely large impulse charge moment change values.
dc.language.isoeng
dc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/3.0/es/
dc.subjectÀrees temàtiques de la UPC::Física
dc.subjectÀrees temàtiques de la UPC::Energies::Energia elèctrica
dc.subject.lcshAtmospheric physics
dc.subject.othergigantic jet supercell lightning
dc.titleAnalysis of the first gigantic jet recorded over continental North America
dc.typeArticle
dc.subject.lemacFísica atmosfèrica
dc.contributor.groupUniversitat Politècnica de Catalunya. LRG - Lightning Research Group
dc.identifier.doi10.1029/2007JD008575
dc.description.peerreviewedPeer Reviewed
dc.rights.accessOpen Access
local.identifier.drac19633786
dc.description.versionPostprint (published version)
local.citation.authorVan Der Velde, O.; Lyons, W. A.; Nelson, T. E.; Cummer, S.; Li, J.; Bunnell, J.
local.citation.publicationNameJournal of geophysical research: atmospheres
local.citation.volume112
local.citation.numberD20104


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