1. Identificação | |
Tipo de Referência | Artigo em Revista Científica (Journal Article) |
Site | plutao.sid.inpe.br |
Código do Detentor | isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S |
Identificador | J8LNKAN8RW/3C63NS8 |
Repositório | dpi.inpe.br/plutao/2012/06.21.19.04 |
Última Atualização | 2012:10.17.18.59.56 (UTC) marciana |
Repositório de Metadados | dpi.inpe.br/plutao/2012/06.21.19.04.39 |
Última Atualização dos Metadados | 2020:09.09.10.51.06 (UTC) marciana |
DOI | 10.1029/2011RS004794 |
ISSN | 0048-6604 |
Rótulo | lattes: 0505123426174183 12 WilliamsKBSNABCDHLSTS:2012:RoHa |
Chave de Citação | WilliamsKBSNABCDHLSTS:2012:RoHa |
Título | Resolution of the sprite polarity paradox: The role of halos |
Projeto | Hungarian Scientific Research Fund (OTKA:K72474); NSF (AGS-1010657); National Science Foundation (ATM-0842751); Office of Naval Research (N00014090443) |
Ano | 2012 |
Data de Acesso | 18 maio 2024 |
Tipo Secundário | PRE PI |
Número de Arquivos | 1 |
Tamanho | 1313 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 2 3 4 5 6 7 8 9 10 11 12 8JMKD3MGP5W/3C9JHP6 |
Grupo | 1 2 3 4 5 6 7 8 9 10 11 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 2 3 4 5 6 7 8 9 10 11 12 marcelo.saba@inpe.br |
Endereço de e-Mail | marcelo.saba@inpe.br |
Revista | Radio Science |
Volume | 47 |
Número | 2 |
Páginas | 1-12 |
Nota Secundária | B1_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 Conteúdo | concluido |
Transferível | 1 |
Tipo do Conteúdo | External Contribution |
Tipo de Versão | publisher |
Palavras-Chave | electrical engineering radio halo |
Resumo | This 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. |
Área | CEA |
Arranjo | urlib.net > BDMCI > Fonds > Produção anterior à 2021 > COCST > Resolution of the... |
Conteúdo da Pasta doc | acessar |
Conteúdo da Pasta source | não têm arquivos |
Conteúdo da Pasta agreement | não têm arquivos |
|
4. Condições de acesso e uso | |
URL dos dados | http://urlib.net/ibi/J8LNKAN8RW/3C63NS8 |
URL dos dados zipados | http://urlib.net/zip/J8LNKAN8RW/3C63NS8 |
Idioma | pt |
Arquivo Alvo | Williams 2012 sprite polarity paradox.pdf |
Grupo de Usuários | administrator lattes secretaria.cpa@dir.inpe.br simone |
Visibilidade | shown |
Política de Arquivamento | denypublisher6 allowfinaldraft |
Permissão de Leitura | allow from all |
Permissão de Atualização | não transferida |
|
5. Fontes relacionadas | |
Unidades Imediatamente Superiores | 8JMKD3MGPCW/3F3T29H |
Lista de Itens Citando | sid.inpe.br/mtc-m21/2012/07.13.14.54.40 1 |
Divulgação | WEBSCI; AGU; MGA; COMPENDEX. |
Acervo Hospedeiro | dpi.inpe.br/plutao@80/2008/08.19.15.01 |
|
6. Notas | |
Campos Vazios | alternatejournal 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 | |
e-Mail (login) | simone |
atualizar | |
|