| 1. Identificação | ||||
| Tipo de Referência | Artigo em Evento (Conference Proceedings) | |||
| Site | mtc-m21d.sid.inpe.br | |||
| Código do Detentor | isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S | |||
| Identificador | 8JMKD3MGP3W34T/4878DDP | |||
| Repositório | sid.inpe.br/mtc-m21d/2022/12.13.17.41 | |||
| Repositório de Metadados | sid.inpe.br/mtc-m21d/2022/12.13.17.41.34 | |||
| Última Atualização dos Metadados | 2023:01.03.16.46.27 (UTC) administrator | |||
| Chave Secundária | INPE--PRE/ | |||
| Chave de Citação | AbbasiBSKRKRRSMLSOBHP:2022:OpCoTe | |||
| Título | The Optical Counterpart of Terrestrial Gamma-ray Flashes Observations at the Telescope Array Detector  | |||
| Ano | 2022 | |||
| Data de Acesso | 18 maio 2024 | |||
| Tipo Secundário | PRE CI | |||
| 2. Contextualização | ||||
| Autor | 1 Abbasi, Racha 2 Belz, John 3 Saba, Marcelo Magalhães Fares 4 Krehbiel, Paul R. 5 Remington, Jackson 6 Kieu, Ny 7 da, Silva Diego Rhamon Reis 8 Rison, William 9 Rodeheffer, Dan 10 Stanley, Mark A. 11 Mazich, Joeseph 12 LeVon, Ryan 13 Smout, Kieran 14 O'Brien, Kaleigh 15 Bratrud, Gradce 16 Husseini, Nour 17 Petrizze, Alex | |||
| Identificador de Curriculo | 1 2 3 8JMKD3MGP5W/3C9JHP6 | |||
| Grupo | 1 2 3 DISSM-CGCT-INPE-MCTI-GOV-BR 4 5 6 7 MET-MET-DIPGR-INPE-MCTI-GOV-BR | |||
| Afiliação | 1 Loyola University Chicago 2 University of Utah 3 Instituto Nacional de Pesquisas Espaciais (INPE) 4 New Mexico Tech 5 University of Utah 6 Loyola University Chicago 7 Instituto Nacional de Pesquisas Espaciais (INPE) 8 New Mexico Tech 9 New Mexico Tech 10 New Mexico Institute of Mining and Technology 11 Loyola University Chicago 12 University of Utah 13 University of Utah 14 Loyola University Chicago 15 Loyola University Chicago 16 IMSA 17 University of Utah | |||
| Endereço de e-Mail do Autor | 1 2 3 marcelosaba@gmail.com 4 5 6 7 dieggo522@hotmail.com | |||
| Nome do Evento | AGU Fall Meeting | |||
| Localização do Evento | Chicago, IL | |||
| Data | 12-16 Dec. 2022 | |||
| Editora (Publisher) | AGU | |||
| Histórico (UTC) | 2022-12-13 17:41:34 :: simone -> administrator :: 2023-01-03 16:46:27 :: administrator -> simone :: 2022 | |||
| 3. Conteúdo e estrutura | ||||
| É a matriz ou uma cópia? | é a matriz | |||
| Estágio do Conteúdo | concluido | |||
| Transferível | 1 | |||
| Tipo do Conteúdo | External Contribution | |||
| Resumo | This work presents the observations of the optical counterpart of a downward-directed terrestrial gamma ray flashes at the Telescope Array (TA) detector. The Telescope Array detector is located in the southwestern desert of the State of Utah. The combination of size and elevation makes it a unique tool that allows us to study thunderstorms. Currently it is the largest ultra-high energy cosmic ray experiment in the Northern Hemisphere. The surface detector array part of the TA experiment, used in these observations, is composed of 507 scintillator detectors on a 1.2 km square grid covering a 700-kilometer square in area, 1400 m above sea level. Previous downward-directed Terrestrial Gamma-ray Flashes (TGFs) observations, using the 700 km2 Telescope Array Surface Detector (TASD), established that observed lightning-correlated energetic particles are downward-directed gamma-ray showers. Moreover, these downward-directed gamma-ray showers were found to be correlated with the early leader and the initial burst pulse stage of cloud-to-ground lightning. In this work, we use the TASD detector, together with a high-speed video camera, in conjunction with the suite of lightning instruments at the TASD site, to report on the optical emission of downward-directed terrestrial gamma ray flashes. The suite of gamma and lightning instruments, timing resolution, and source proximity offers us an unprecedented look at the TGF phenomena. The optical emission observations, together with in-progress efforts, should allow us to better understand which runaway electron production model is responsible for gamma-ray production in the atmosphere. Results from this study allow us to further the understanding of the initiation and propagation mechanism of terrestrial gamma ray flashes. In addition will allow us to further our ability to compare the most recent satellite optical emissions counterpart of upward-directed TGFs to that of downward-directed TGFs. | |||
| Área | MET | |||
| Arranjo | The Optical Counterpart... | |||
| Conteúdo da Pasta doc | não têm arquivos | |||
| Conteúdo da Pasta source | não têm arquivos | |||
| Conteúdo da Pasta agreement |
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| 4. Condições de acesso e uso | ||||
| Grupo de Usuários | simone | |||
| Visibilidade | shown | |||
| Permissão de Atualização | não transferida | |||
| 5. Fontes relacionadas | ||||
| Unidades Imediatamente Superiores | 8JMKD3MGPCW/3F35TRS 8JMKD3MGPCW/46KUATE | |||
| Acervo Hospedeiro | urlib.net/www/2021/06.04.03.40 | |||
| 6. Notas | ||||
| Campos Vazios | archivingpolicy archivist booktitle callnumber copyholder copyright creatorhistory descriptionlevel dissemination doi e-mailaddress edition editor format isbn issn keywords label language lineage mark mirrorrepository nextedition notes numberoffiles numberofvolumes orcid organization pages parameterlist parentrepositories previousedition previouslowerunit progress project publisheraddress readergroup readpermission rightsholder schedulinginformation secondarydate secondarymark serieseditor session shorttitle size sponsor subject targetfile tertiarymark tertiarytype type url versiontype volume | |||
| 7. Controle da descrição | ||||
| e-Mail (login) | simone | |||
| atualizar | ||||