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dc.contributor.authorSunjerga, A.
dc.contributor.authorRubinstein, M.
dc.contributor.authorPineda, Nicolau
dc.contributor.authorMostajabi, A.
dc.contributor.authorAzadifar, M.
dc.contributor.authorRomero Durán, David
dc.contributor.authorVan der Velde, Oscar Arnoud
dc.contributor.authorMontañá Puig, Juan
dc.contributor.authorFigueras i Ventura, Jordi
dc.contributor.authorBesic, Nikola
dc.contributor.authorGrazioli, Jacopo
dc.contributor.authorHering, Alessandro
dc.contributor.authorGermann, Urs
dc.contributor.authorDiendorfer, Gerhard
dc.contributor.authorRachidi-Haeri, Farhad
dc.contributor.otherUniversitat Politècnica de Catalunya. Doctorat en Enginyeria Elèctrica
dc.contributor.otherUniversitat Politècnica de Catalunya. Departament d'Enginyeria Elèctrica
dc.date.accessioned2020-01-28T15:56:23Z
dc.date.available2022-04-01T00:29:58Z
dc.date.issued2020-04
dc.identifier.citationSunjerga, A. [et al.]. LMA observations of upward lightning flashes at the Säntis Tower initiated by nearby lightning activity. "Electric power systems research", Abril 2020, vol. 181, p. 1-12.
dc.identifier.issn0378-7796
dc.identifier.urihttp://hdl.handle.net/2117/175966
dc.description.abstractWe present in this paper lightning current measurements, LMA (Lightning Mapping Array) data and fast antenna electric fields associated with upward flashes observed at the Säntis Tower during summer of 2017. The LMA network consists of six stations that were installed in the vicinity of the tower at distances ranging from 100¿m to 11¿km from it. Out of 20 LMA recorded flashes here we analyze in detail three so-called ‘other-triggered flashes’, triggered by preceding activity. Based on the lightning activity derived from the European Lightning Detection Network (EUCLID) in an area within 30¿km from the tower and within a 1-s time window before the start of the upward tower flashes, only one out of 20 flashes was classified as ‘other-triggered’(OT). However, the investigations based on the LMA data reveal that 3 more flashes of the 20 analyzed were preceded by nearby activity and should therefore be classified as OT flashes. We analyze conditions conducive to the OT flashes, such as the charge structure of the clouds, polarity of preceding leaders and level of activity of the storm. The LMA source active time period was on average seven times higher for the OT flashes than that for self-initiated flashes.
dc.format.extent12 p.
dc.language.isoeng
dc.subjectÀrees temàtiques de la UPC::Enginyeria elèctrica
dc.subject.lcshLightning
dc.subject.lcshElectric fields
dc.subject.otherLightning
dc.subject.otherLightning mapping array
dc.subject.otherOther-triggered lightning
dc.subject.otherCurrent
dc.subject.otherCharge structure
dc.subject.otherLeader polarity
dc.subject.otherRadar
dc.subject.otherElectric field
dc.titleLMA observations of upward lightning flashes at the Säntis Tower initiated by nearby lightning activity
dc.typeArticle
dc.subject.lemacLlamps
dc.subject.lemacCamps elèctrics
dc.subject.lemacRadar
dc.contributor.groupUniversitat Politècnica de Catalunya. LRG - Lightning Research Group
dc.identifier.doi10.1016/j.epsr.2019.106067
dc.description.peerreviewedPeer Reviewed
dc.relation.publisherversionhttps://www.sciencedirect.com/science/article/abs/pii/S0378779619303864
dc.rights.accessOpen Access
local.identifier.drac26537999
dc.description.versionPostprint (author's final draft)
local.citation.authorSunjerga, A.; Rubinstein, M.; Pineda, N.; Mostajabi, A.; Azadifar, M.; Romero, D.; Van Der Velde, O.; Montanya, J.; Figueras, J.; Besic, N.; Grazioli, J.; Hering, A.; Germann, U.; Diendorfer, G.; Rachidi-Haeri , F.
local.citation.publicationNameElectric power systems research
local.citation.volume181
local.citation.startingPage1
local.citation.endingPage12


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