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1. Identificação
Tipo de ReferênciaArtigo em Revista Científica (Journal Article)
Siteplutao.sid.inpe.br
Código do Detentorisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
IdentificadorJ8LNKAN8RW/3C63NS8
Repositóriodpi.inpe.br/plutao/2012/06.21.19.04
Última Atualização2012:10.17.18.59.56 (UTC) marciana
Repositório de Metadadosdpi.inpe.br/plutao/2012/06.21.19.04.39
Última Atualização dos Metadados2020:09.09.10.51.06 (UTC) marciana
DOI10.1029/2011RS004794
ISSN0048-6604
Rótulolattes: 0505123426174183 12 WilliamsKBSNABCDHLSTS:2012:RoHa
Chave de CitaçãoWilliamsKBSNABCDHLSTS:2012:RoHa
TítuloResolution of the sprite polarity paradox: The role of halos
ProjetoHungarian Scientific Research Fund (OTKA:K72474); NSF (AGS-1010657); National Science Foundation (ATM-0842751); Office of Naval Research (N00014090443)
Ano2012
Data de Acesso18 maio 2024
Tipo SecundárioPRE PI
Número de Arquivos1
Tamanho1313 KiB
2. Contextualização
Autor 1 Williams, E.
 2 Kuo, C. -L.
 3 Bór, J.
 4 Sátori, G.
 5 Newsome, Robert
 6 Adachi, Toru
 7 Boldi, Robert
 8 Chen, A.
 9 Downes, Eric
10 Hsu, R. R.
11 Lyons, W.
12 Saba, Marcelo Magalhães Fares
13 Taylor, M.
14 Su, H T
Identificador de Curriculo 1
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12 8JMKD3MGP5W/3C9JHP6
Grupo 1
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12 CST-CST-INPE-MCTI-GOV-BR
Afiliação 1 Parsons Laboratory, Massachusetts Institute of Technology, Cambridge, MA 02139, United States
 2 Department of Physics, National Chen Kung University, Tainan 70101, Taiwan
 3 Research Centre for Astronomy and Earth Sciences, GGI, Hungarian Academy of Sciences, Csatkai u. 6-8, Sopron, Hungary
 4 Research Centre for Astronomy and Earth Sciences, GGI, Hungarian Academy of Sciences, Csatkai u. 6-8, Sopron, Hungary
 5 STAR Laboratory, Department of Electrical Engineering, Stanford University, Stanford, CA 94305, United States
 6 STAR Laboratory, Department of Electrical Engineering, Stanford University, Stanford, CA 94305, United States
 7 Faculty of Engineering, Design, and Information Technology, University of Bahrain Polytechnic, PO Box 33349, Isa Town, Bahrain
 8 Department of Physics, National Chen Kung University, Tainan 70101, Taiwan
 9 Parsons Laboratory, Massachusetts Institute of Technology, Cambridge, MA 02139, United States
10 Department of Physics, National Chen Kung University, Tainan 70101, Taiwan
11 FMA Research, Inc., 46050 Weld County Rd. 13, Ft. Collins, CO 80524, United States
12 Instituto Nacional de Pesquisas Espaciais (INPE)
13 Center for Atmospheric and Space Sciences, Utah State University, Ogden, UT 84322-4405, United States
14 Department of Physics, National Chen Kung University, Tainan 70101, Taiwan
Endereço de e-Mail do Autor 1
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12 marcelo.saba@inpe.br
Endereço de e-Mailmarcelo.saba@inpe.br
RevistaRadio Science
Volume47
Número2
Páginas1-12
Nota SecundáriaB1_GEOCIÊNCIAS
Histórico (UTC)2012-06-22 00:11:00 :: lattes -> secretaria.cpa@dir.inpe.br :: 2012
2012-10-17 18:59:56 :: secretaria.cpa@dir.inpe.br -> administrator :: 2012
2018-06-05 00:01:45 :: administrator -> marciana :: 2012
2020-09-09 10:51:06 :: marciana -> simone :: 2012
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-Chaveelectrical engineering
radio
halo
ResumoThis study revisits the sprite polarity paradox, first manifest by observations that exceptional cloud-to-ground flashes with negative polarity generally did not produce detectable sprites. The paradox is here resolved by the Transient Luminous Event (TLE) known as the halo, which on account of its inferior brightness (0.3 MR versus 1.5 MR) and substantially shorter duration (1 ms versus 10-100 ms) in comparison with the sprite, is not readily detectable in ground-based video cameras with standard field duration (16.7-20 ms). Observations with improved temporal resolution (ISUAL (Imager of Sprites and Upper Atmospheric Lightnings) from space and PIPER (Photometric Imager of Precipitated Electron Radiation) observations from the ground) provide evidence that flashes with negative polarity dominate the global halo population, and that the halo numbers are more than sufficient to account for the previously missing TLEs. The evidence for lightning polarity-dependent TLEs (sprites, positive and halos, negative) is attributable to the well established but incompletely understood contrast in the behavior of negative and positive lightning flashes to ground. Copyright 2012 by the American Geophysical Union.
ÁreaCEA
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4. Condições de acesso e uso
URL dos dadoshttp://urlib.net/ibi/J8LNKAN8RW/3C63NS8
URL dos dados zipadoshttp://urlib.net/zip/J8LNKAN8RW/3C63NS8
Idiomapt
Arquivo AlvoWilliams 2012 sprite polarity paradox.pdf
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5. Fontes relacionadas
Unidades Imediatamente Superiores8JMKD3MGPCW/3F3T29H
Lista de Itens Citandosid.inpe.br/mtc-m21/2012/07.13.14.54.40 1
DivulgaçãoWEBSCI; AGU; MGA; COMPENDEX.
Acervo Hospedeirodpi.inpe.br/plutao@80/2008/08.19.15.01
6. Notas
Campos Vaziosalternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel format isbn lineage mark mirrorrepository month nextedition notes orcid parameterlist parentrepositories previousedition previouslowerunit progress readergroup rightsholder schedulinginformation secondarydate secondarykey session shorttitle sponsor subject tertiarymark tertiarytype typeofwork url
7. Controle da descrição
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