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1. Identity statement
Reference TypeJournal Article
Siteplutao.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W/44SJKSH
Repositorysid.inpe.br/plutao/2021/06.16.15.16   (restricted access)
Last Update2021:06.17.12.26.10 (UTC) lattes
Metadata Repositorysid.inpe.br/plutao/2021/06.16.15.16.03
Metadata Last Update2022:04.03.22.39.33 (UTC) administrator
DOI10.1029/2020JD034527
ISSN2169-897X
Labellattes: 8485072131969726 10 NyassorWGPVNTBFB:2021:CaStCo
Citation KeyNyassorWGPVNTBFB:2021:CaStCo
TitleCase Studies on Concentric Gravity Waves Source using Lightning Flash Rate, Brightness Temperature and Backward Ray Tracing at São Martinho da Serra (29.44°S, 53.82°W)
Year2021
Access Date2025, May 31
Type of Workjournal article
Secondary TypePRE PI
Number of Files1
Size4739 KiB
2. Context
Author 1 Nyassor, Prosper Kwamla
 2 Wrasse, Cristiano Max
 3 Gobbi, Delano
 4 Paulino, Igo
 5 Vadas, S. L.
 6 Naccarato, Kleber Pinheiro
 7 Takahashi, Hisao
 8 Bageston, José Valentin
 9 Figueiredo, Cosme Alexandre Oliveira Barros
10 Barros, Diego
Resume Identifier 1
 2
 3 8JMKD3MGP5W/3C9JGTE
 4
 5
 6
 7 8JMKD3MGP5W/3C9JHCM
ORCID 1 0000-0001-8484-6334
 2 0000-0001-8026-3625
 3 0000-0002-8260-1007
 4 0000-0001-9560-1842
 5 0000-0002-6459-005X
 6 0000-0001-9184-4935
 7 0000-0002-8844-8920
 8 0000-0003-2931-8488
 9 0000-0003-4423-5111
10 0000-0003-0144-6584
Group 1 DICEP-CGCE-INPE-MCTI-GOV-BR
 2 DICEP-CGCE-INPE-MCTI-GOV-BR
 3 DICEP-CGCE-INPE-MCTI-GOV-BR
 4
 5
 6 DIIAV-CGCT-INPE-MCTI-GOV-BR
 7 DICEP-CGCE-INPE-MCTI-GOV-BR
 8 COESU-CGGO-INPE-MCTI-GOV-BR
 9 DICEP-CGCE-INPE-MCTI-GOV-BR
10 YYY-CGCE-INPE-MCTI-GOV-BR
Affiliation 1 Instituto Nacional de Pesquisas Espaciais (INPE)
 2 Instituto Nacional de Pesquisas Espaciais (INPE)
 3 Instituto Nacional de Pesquisas Espaciais (INPE)
 4 Universidade Federal de Campina Grande (UFCG)
 5 NorthWest Research Associates
 6 Instituto Nacional de Pesquisas Espaciais (INPE)
 7 Instituto Nacional de Pesquisas Espaciais (INPE)
 8 Instituto Nacional de Pesquisas Espaciais (INPE)
 9 Instituto Nacional de Pesquisas Espaciais (INPE)
10 Instituto Nacional de Pesquisas Espaciais (INPE)
Author e-Mail Address 1 pnyassor@gmail.com
 2 cristiano.wrasse@inpe.br
 3 delano.gobbi@inpe.br
 4
 5
 6 kleber.naccarato@inpe.br
 7
 8 jose.bageston@inpe.br
 9 anagetinga@hotmail.com
JournalJournal of Geophysical Research: Atmospheres
Volume126
Pages1-22
History (UTC)2021-06-17 12:26:12 :: lattes -> administrator :: 2021
2022-04-03 22:39:33 :: administrator -> simone :: 2021
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
AbstractWe relate the spatial and temporal distribution of lightning flash rates and cloud top brightness temperature (CTBT) to concentric atmospheric gravity wave (CGW) events observed at the Southern Space Observatory (SSO) in São Martinho da Serra (29.44°S, 53.82°W, 488.7m) in southern Brazil. The selected identified cases from 2017 to 2018 were observed by a hydroxyl (OH) all-sky imager. Backward ray tracing shows that the time of gravity wave excitation agrees with the highest values of lightning flash rates (indicating lightning jump) as well as the coldest brightness temperatures that indicate the time of convective overshoot. Radiosonde measurements show high convective available potential energy (CAPE), associated with a maximum updraft velocity just prior to the wave events. We find that these possible source locations correspond to the positions and times that convective plumes overshot the tropopause (seen in GOES-16 CTBT images). We also show that higher spatial lightning density (i.e., number of lightning flashes at a given longitude and latitude) agree with the overshoot locations from the GOES satellite. We also find that the overshoot times from the GOES-16 satellite agree with the times lightning jumps were observed in the lightning flash rate. Finally, we find that the periodicities in the lightning flash rate agree with the periods of the observed CGWs, which further strengthens the result that the CGWs were excited by the deep convective systems determined from backward ray tracing.
AreaCEA
Arrangement 1urlib.net > BDMCI > Fonds > Produção a partir de 2021 > CGCE > Case Studies on...
Arrangement 2urlib.net > BDMCI > Fonds > Produção a partir de 2021 > CGCT > Case Studies on...
Arrangement 3urlib.net > BDMCI > Fonds > Produção a partir de 2021 > CGGO > Case Studies on...
doc Directory Contentaccess
source Directory Contentthere are no files
agreement Directory Contentthere are no files
4. Conditions of access and use
Languageen
Target Filenyassor_case.pdf
User Grouplattes
Reader Groupadministrator
lattes
Visibilityshown
Read Permissiondeny from all and allow from 150.163
Update Permissionnot transferred
5. Allied materials
Next Higher Units8JMKD3MGPCW/46KTFK8
8JMKD3MGPCW/46KUATE
8JMKD3MGPCW/46KUBT5
Citing Item Listsid.inpe.br/bibdigital/2022/04.03.22.35 27
sid.inpe.br/mtc-m21/2012/07.13.14.49.58 11
sid.inpe.br/bibdigital/2022/04.03.17.52 6
DisseminationWEBSCI
Host Collectiondpi.inpe.br/plutao@80/2008/08.19.15.01
6. Notes
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