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1. Identificação
Tipo de ReferênciaResumo em Evento (Conference Proceedings)
Sitemtc-m16d.sid.inpe.br
Código do Detentorisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identificador8JMKD3MGP7W/3EC2GAH
Repositóriosid.inpe.br/mtc-m19/2013/06.25.13.37
Última Atualização2013:06.25.19.11.48 (UTC) administrator
Repositório de Metadadossid.inpe.br/mtc-m19/2013/06.25.13.37.23
Última Atualização dos Metadados2021:01.03.02.14.21 (UTC) administrator
Rótuloself-archiving-INPE-MCTI-GOV-BR
Chave de CitaçãoHöllerBeMoBlBaAl:2013:GrSpLi
TítuloGround-based and space-borne lightning observations during CHUVA
Ano2013
Data de Acesso03 maio 2024
Tipo SecundárioPRE CI
Número de Arquivos2
Tamanho1992 KiB
2. Contextualização
Autor1 Höller, H.
2 Betz, H. -D.
3 Morales, C.
4 Blakeslee, R.
5 Bailey, J.
6 Albrecht, Rachel Ifanger
Grupo1
2
3
4
5
6 DSA-CPT-INPE-MCTI-GOV-BR
Afiliação1 Deutsches Zentrum für Luft- und Raumfahrt (DLR), Institut für Physik der Atmosphäre, Oberpfaffenhofen, Germany
2 Physics Department, University of Munich, Germany
3 Universidade de São Paulo, Instituto de Astronomia, Geofisica e Ciências Atmosféricas, São Paulo, Brazil
4 NASA Marshall Space Flight Center, Huntsville, USA
5 University of Alabama, Huntsville, USA
6 Instituto Nacional de Pesquisas Espaciais (INPE)
Endereço de e-Mail do Autor1
2
3
4
5
6 rachel.albrecht@gmail.com
Endereço de e-Mailvaldirene.ribeiro@cptec.inpe.br
Nome do EventoCHUVA International Workshop, 1.
Localização do EventoSão Paulo, Brazil
Data2013
Título do LivroAbstracts
Histórico (UTC)2013-06-25 13:37:23 :: valdirene.ribeiro@cptec.inpe.br -> administrator ::
2021-01-03 02:14:21 :: administrator -> marcelo.pazos@inpe.br :: 2013
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-Chavelightning
geostationary satellite systems
CHUVA field experiment
ResumoFuture geostationary satellite systems will offer a variety of improved observing capabilities which will be extremely useful for many applications like numerical weather forecasting, nowcasting of severe weather, climate research or hydrology. The future payloads will include the optical lightning imagers LI on MTG (Meteosat Third Generation) and GLM (Geostationary Lightning Mapper) on GOES-R (Geostationary Operational Environmental Satellite - R Series). Proper interpretation of these optical data requires a better understanding of what components of a flash are to be seen from space and how these observations relate to ground based radio frequency observations. For assessing the future performances and benefits of a geostationary lightning sensor this study takes advantage of the comprehensive lightning data sets obtained from the recent CHUVA field experiment performed in Brazil (CHUVA - Cloud processes of tHe main precipitation systems in Brazil: A contribUtion to cloud resolVing modeling and to the GPM (GlobAl Precipitation Measurement)). During the rainy season of 2011-2012 a large number of ground based lightning detection systems was set up in the Sao Paulo area as part of the CHUVA-GLM Vale do Paraíba campaign. In the present study we look at the detailed radio frequency (RF) based observation from LINET (Lightning detection network operated by DLR, nowcast and USP) observing strokes in the VLF/LF (very low and low frequency) range, the LMA (Lightning Mapping Array) from NASA observing RF sources in the VHF (very high frequency) range and the TRMM-LIS (Tropical Rainfall Measuring Mission-Lightning Imaging Sensor) optical space borne lightning imager. The LIS is used as a reference instrument for the future geostationary sensors. Thus it is possible to study the relations between the RF and optical signals from lightning in detail and to assess the performance of the future geostationary observations from a set of proxy satellite data generated from the ground based observations. In confirmation of previous studies, it was found that often a direct temporal coincidence of RF signals (LINET strokes) and optical pulses (LIS groups) exists. The short baseline configuration of LINET allowed observing the strokes mapping the flash branches similar to LMA, but by locating the limited number of strong cloud strokes rather than a large number of weak source points from leader steps. An initial breakdown phase of vertically propagating sources can often be found in LINET and LMA data. The higher level LINET and LMA signals have higher probability to be optically detected. Lower level LINET and LMA signals are optically detected from above in case of missing high level precipitation as inferred from radar observations provided by USP.
ÁreaMET
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4. Condições de acesso e uso
URL dos dadoshttp://urlib.net/ibi/8JMKD3MGP7W/3EC2GAH
URL dos dados zipadoshttp://urlib.net/zip/8JMKD3MGP7W/3EC2GAH
Idiomaen
Arquivo Alvoabstract-Hartmut_Holler.pdf
Grupo de Usuáriosadministrator
marcelo.pazos@inpe.br
valdirene.ribeiro@cptec.inpe.br
Grupo de Leitoresadministrator
marcelo.pazos@inpe.br
Visibilidadeshown
Permissão de Leituraallow from all
Permissão de Atualizaçãonão transferida
5. Fontes relacionadas
Repositório Espelhoiconet.com.br/banon/2006/11.26.21.31
Unidades Imediatamente Superiores8JMKD3MGPCW/43SRC6S
Lista de Itens Citandosid.inpe.br/bibdigital/2021/01.03.02.10 2
Acervo Hospedeirosid.inpe.br/mtc-m19@80/2009/08.21.17.02
6. Notas
Campos Vaziosarchivingpolicy archivist callnumber copyholder copyright creatorhistory descriptionlevel dissemination doi edition editor format isbn issn lineage mark nextedition notes numberofvolumes orcid organization pages parameterlist parentrepositories previousedition previouslowerunit progress project publisher publisheraddress resumeid rightsholder schedulinginformation secondarydate secondarykey secondarymark serieseditor session shorttitle sponsor subject tertiarymark tertiarytype type url volume
7. Controle da descrição
e-Mail (login)marcelo.pazos@inpe.br
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