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1. Identificação
Tipo de ReferênciaArtigo em Evento (Conference Proceedings)
Siteplutao.sid.inpe.br
Código do Detentorisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identificador8JMKD3MGP3W/3GDQK7U
Repositóriosid.inpe.br/plutao/2014/06.03.21.43.38
Última Atualização2014:09.18.16.57.04 (UTC) administrator
Repositório de Metadadossid.inpe.br/plutao/2014/06.03.21.43.39
Última Atualização dos Metadados2018:06.04.23.39.31 (UTC) administrator
Rótulolattes: 4161737266837399 2 SaraivaCWZAPHBBMB:2014:OpEvIn
Chave de CitaçãoSaraivaCWZAPHBBMB:2014:OpEvIn
TítuloOptical evidences of the inception mechanisms of natural bipolar cloud-to-ground lightning
FormatoDVD
ProjetoFAPESP (under grant numbers 08/56711-4, 2010/01742-2 and partially by 2009/15235-8).
Ano2014
Data de Acesso23 maio 2024
Tipo SecundárioPRE CI
Número de Arquivos1
Tamanho1838 KiB
2. Contextualização
Autor 1 Saraiva, Antônio Carlos V.
 2 Campos, Leandro Zanella de Souza
 3 Williams, Earle R.
 4 Zepka, Gisele dos Santos
 5 Alves, Jéferson
 6 Pinto Jr., Osmar
 7 Heckman, Stan
 8 Buzato, Tiago Santos
 9 Bailey, Jeffrey C.
10 Morales, Carlos A.
11 Blakeslee, Richard J.
Grupo 1
 2 DGE-CEA-INPE-MCTI-GOV-BR
 3
 4 DGE-CEA-INPE-MCTI-GOV-BR
 5 GES-CEA-SPG-INPE-MCTI-GOV-BR
 6 CST-CST-INPE-MCTI-GOV-BR
 7
 8 YYY-CST-INPE-MCTI-GOV-BR
Afiliação 1 Instituto Nacional de Pesquisas Espaciais (INPE)
 2 Instituto Nacional de Pesquisas Espaciais (INPE)
 3 Massachusetts Institute of Technology
 4 Instituto Nacional de Pesquisas Espaciais (INPE)
 5 Instituto Nacional de Pesquisas Espaciais (INPE)
 6 Instituto Nacional de Pesquisas Espaciais (INPE)
 7 Earth Networks Germantown, MD, USA
 8 Instituto Nacional de Pesquisas Espaciais (INPE)
 9 University of Alabama in Huntsville
10 Universidade de São Paulo (USP)
11 NASA Marshall Space Flight Center
Endereço de e-Mail do Autor 1 acvsaraiva@gmail.com
 2 leandro.zanella@gmail.com
 3
 4 gisele.zepka@inpe.br
 5
 6 osmar@dge.inpe.br
Endereço de e-Mailmarcelo.pazos@inpe.br
Nome do EventoInternational Lightning Detection Conference, 23 (ILDC); and International Lightning Meteorology Conference, 5 (ILMC).
Localização do EventoTucson
Datamar. 18-19, 2014 / mar. 20-21, 2014
Editora (Publisher)Vaisala
Volume1
Título do LivroProceedings
Tipo TerciárioPaper
Histórico (UTC)2014-06-03 21:43:39 :: lattes -> administrator ::
2018-06-04 23:39:31 :: administrator -> marcelo.pazos@inpe.br :: 2014
3. Conteúdo e estrutura
É a matriz ou uma cópia?é a matriz
Estágio do Conteúdoconcluido
Transferível1
Tipo do ConteúdoExternal Contribution
Tipo de Versãopublisher
Palavras-Chavebipolar lightning
atmospheric electricity
recoil leaders
bidirectional leader model
dart leaders
positive lightning
ResumoHigh-speed video records of two bipolar cloud-to-ground flashes were analyzed in detail. They were both initiated by single positive return strokes and were followed by more than one subsequent negative stroke. Due to the elevated cloud-base height of its parent thunderstorm, the initiation processes of each subsequent stroke could be registered optically below cloud base. In the first event (Case 1) it was possible to observe that all four subsequent negative strokes were initiated by recoil leaders that retraced one horizontal channel segment previously ionized by the positive leader that preceded the first stroke. Those recoil leaders connected to the original vertical channel segment and propagated towards ground, producing four subsequent strokes that had the same ground contact point of the original positive discharge. The second event (Case 2), on the other hand, presented fifteen subsequent strokes that were initiated by recoil leaders that did not reach the original channel of the positive stroke. They diverged vertically towards ground, making contact approximately 11 kilometers away from the original positive strike point. These are the first optical evidences that both single- and multiple-channel bipolar flashes occur as a consequence of recoil leader activity in the branches of the initial positive return stroke. For both events their total channel length increased progressively with time at a growth rate equivalent to a propagation speed of the order of 104 m/s, comparable to those reported for typical positive leaders.
ÁreaCEA
Arranjo 1urlib.net > Fonds > Produção anterior à 2021 > DIDGE > Optical evidences of...
Arranjo 2urlib.net > BDMCI > Fonds > Produção pgr ATUAIS > GES > Optical evidences of...
Arranjo 3urlib.net > BDMCI > Fonds > Produção anterior à 2021 > COCST > Optical evidences of...
Conteúdo da Pasta docacessar
Conteúdo da Pasta sourcenão têm arquivos
Conteúdo da Pasta agreementnão têm arquivos
4. Condições de acesso e uso
URL dos dadoshttp://plutao.sid.inpe.br/ibi/8JMKD3MGP3W/3GDQK7U
URL dos dados zipadoshttp://plutao.sid.inpe.br/zip/8JMKD3MGP3W/3GDQK7U
Idiomaen
Arquivo AlvoSaraiva et al-Optical evidences of the inception mechanisms of natural bipolar CGL-2014-ILDC-ILMC.pdf
Grupo de Usuárioslattes
marcelo.pazos@inpe.br
Grupo de Leitoresadministrator
marcelo.pazos@inpe.br
Visibilidadeshown
Permissão de Leituraallow from all
Permissão de Atualizaçãonão transferida
5. Fontes relacionadas
VinculaçãoTrabalho não Vinculado à Tese/Dissertação
Repositório Espelhoiconet.com.br/banon/2006/11.26.21.31
Unidades Imediatamente Superiores8JMKD3MGPCW/3EU29DP
8JMKD3MGPCW/3F2PBEE
8JMKD3MGPCW/3F3T29H
Lista de Itens Citandosid.inpe.br/bibdigital/2013/10.01.22.11 4
sid.inpe.br/bibdigital/2013/10.19.20.40 2
sid.inpe.br/bibdigital/2013/10.12.21.02 1
Acervo Hospedeirodpi.inpe.br/plutao@80/2008/08.19.15.01
6. Notas
NotasInformações Adicionais: High-speed video records of two bipolar cloud-to-ground flashes were analyzed in detail. They were both initiated by single positive return strokes and were followed by more than one subsequent negative stroke. Due to the elevated cloud-base height of its parent thunderstorm, the initiation processes of each subsequent stroke could be registered optically below cloud base. In the first event (Case 1) it was possible to observe that all four subsequent negative strokes were initiated by recoil leaders that retraced one horizontal channel segment previously ionized by the positive leader that preceded the first stroke. Those recoil leaders connected to the original vertical channel segment and propagated towards ground, producing four subsequent strokes that had the same ground contact point of the original positive discharge. The second event (Case 2), on the other hand, presented fifteen subsequent strokes that were initiated by recoil leaders that did not reach the original channel of the positive stroke. They diverged vertically towards ground, making contact approximately 11 kilometers away from the original positive strike point. These are the first optical evidences that both single- and multiple-channel bipolar flashes occur as a consequence of recoil leader activity in the branches of the initial positive return stroke. For both events their total channel length increased progressively with time at a growth rate equivalent to a propagation speed of the order of 104 m/s, comparable to those reported for typical positive leaders..
Campos Vaziosarchivingpolicy archivist callnumber copyholder copyright creatorhistory descriptionlevel dissemination doi edition editor isbn issn lineage mark nextedition numberofvolumes orcid organization pages parameterlist parentrepositories previousedition previouslowerunit progress publisheraddress resumeid rightsholder schedulinginformation secondarydate secondarykey secondarymark serieseditor session shorttitle sponsor subject type url
7. Controle da descrição
e-Mail (login)marcelo.pazos@inpe.br
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