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1. Identificação
Tipo de ReferênciaArtigo em Revista Científica (Journal Article)
Sitemtc-m21d.sid.inpe.br
Código do Detentorisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identificador8JMKD3MGP3W34T/499PKC2
Repositóriosid.inpe.br/mtc-m21d/2023/06.13.13.57
Última Atualização2023:12.20.17.28.54 (UTC) administrator
Repositório de Metadadossid.inpe.br/mtc-m21d/2023/06.13.13.57.20
Última Atualização dos Metadados2024:01.10.08.50.19 (UTC) administrator
DOI10.1029/2023JA031408
ISSN2169-9402
Chave de CitaçãoVadasFBHTHMGB:2023:MoMECo
TítuloTraveling Ionospheric Disturbances Induced by the Secondary Gravity Waves From the Tonga Eruption on 15 January 2022: Modeling With MESORAC-HIAMCM-SAMI3 and Comparison With GPS/TEC and Ionosonde Data
Ano2023
MêsJune
Data de Acesso18 maio 2024
Tipo de Trabalhojournal article
Tipo SecundárioPRE PI
Número de Arquivos1
Tamanho13575 KiB
2. Contextualização
Autor1 Vadas, Sharon L.
2 Figueiredo, Cosme Alexandre Oliveira Barros
3 Becker, Erich
4 Huba, J. D.
5 Themens, David R.
6 Hindley, Neil P.
7 Mrak, Sebastijan
8 Galkin, Ivan
9 Bossert, Katrina
Grupo1
2 DICEP-CGCE-INPE-MCTI-GOV-BR
Afiliação1 Northwest Research Associates
2 Instituto Nacional de Pesquisas Espaciais (INPE)
3 Northwest Research Associates
4 Syntek Technology
5 University Birmingham
6 University Bath
7 University Colorado
8 University Massachusetts Lowell
9 Arizona State University
Endereço de e-Mail do Autor1
2 anagetinga@hotmail.com
RevistaJournal of Geophysical Research: Space Physics
Volume128
Número6
Páginase2023JA031408
Histórico (UTC)2023-06-13 13:57:20 :: simone -> administrator ::
2023-06-13 13:57:21 :: administrator -> simone :: 2023
2023-06-13 13:59:50 :: simone -> administrator :: 2023
2024-01-10 08:50:19 :: administrator -> simone :: 2023
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-Chavetraveling ionospheric disturbances
gravity waves
Tonga eruption
dTEC
ResumoWe simulate the gravity waves (GWs) and traveling ionospheric disturbances (TIDs) created by the Hunga Tonga-Hunga Ha'apai (hereafter "Tonga") volcanic eruption on 15 January 2022 at similar to 04:15 UT. We calculate the primary GWs and forces/heatings generated where they dissipate with MESORAC, the secondary GWs with HIAMCM, and the TIDs with SAMI3. We find that medium and large-scale TIDs (MSTIDs and LSTIDs) are induced by the secondary GWs, with horizontal phase speeds c(H) similar or equal to 100-750 m/s, horizontal wavelengths lambda(H) similar or equal to 600-6,000 km, and ground-based periods tau(r) similar or equal to 30 min to 3 hr. The LSTID amplitudes over New Zealand are similar or equal to 2-3 TECU, but decrease sharply similar or equal to 5,000 km from Tonga. The LSTID amplitudes are extremely small over Australia and South Africa because body forces create highly asymmetric GW fields and the GWs propagate perpendicular to the magnetic field there. We analyze the TIDs from SAMI3 and find that a 30 min detrend window eliminates the fastest far-field LSTIDs. We analyze the GPS/TEC via detrending with 2-3 hr windows, and find that the fastest LSTIDs reach the US and South America at similar to 8:30-9:00 UT with c(H) similar or equal to 680 m/s, lambda(H) similar or equal to 3,400 km, and tau(r) similar or equal to 83 min, in good agreement with model results. We find good agreement between modeled and observed TIDs over New Zealand, Australia, Hawaii, Japan and Norway. The observed F-peak height, hmF2, drops by similar or equal to 110-140 km over the western US with a 2.8 hr periodicity from 8:00 to 13:00 UT. We show that the Lamb waves (LWs) observed by AIRS with lambda(H) = 380 km have amplitudes that are similar or equal to 2.3% that of the primary GWs at z similar or equal to 110 km. We conclude that the observed TIDs can be fully explained by secondary GWs rather than by "leaked" LWs. Plain Language Summary Gravity waves (GWs) are created by various processes, such as volcanic eruptions. A breaking GW imparts momentum and energy to the atmosphere, which creates secondary GWs. Traveling ionospheric disturbances (TIDs) are created by GWs through collisions between neutral and ion molecules. We simulate the GWs and TIDs created by the Tonga eruption on 15 January 2022. We find that medium and large-scale TIDs (MSTIDs and LSTIDs) are induced by the secondary GWs. These TIDs propagate globally, and have speeds of 100-750 m/s and horizontal scales of hundreds to thousands of km. The fastest TIDs reach the United States and South America at similar to 8:30-9:00 UT; these TIDs have large scales and large periods, in agreement with observations. These LSTIDs can only be seen if they are not "detrended out" when processing the ionospheric data. Previous studies eliminated these LSTIDs by restricting their detrend windows, and then incorrectly suggested that Lamb waves were responsible for the TIDs they observed. Using longer detrend windows, we find good agreement between the modeled and observed TIDs. We find that the observed TIDs can be fully explained by secondary GWs, rather than by the leakage of Lamb waves into GWs.
ÁreaCEA
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4. Condições de acesso e uso
URL dos dadoshttp://urlib.net/ibi/8JMKD3MGP3W34T/499PKC2
URL dos dados zipadoshttp://urlib.net/zip/8JMKD3MGP3W34T/499PKC2
Idiomaen
Arquivo AlvoVadasJGRTongaTID (1).pdf
Grupo de Usuáriosself-uploading-INPE-MCTI-GOV-BR
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Visibilidadeshown
Política de Arquivamentodenypublisher6 allowfinaldraft
Permissão de Leituraallow from all
Permissão de Atualizaçãonão transferida
5. Fontes relacionadas
Unidades Imediatamente Superiores8JMKD3MGPCW/46KTFK8
DivulgaçãoWEBSCI; AGU; MGA; COMPENDEX.
Acervo Hospedeirourlib.net/www/2021/06.04.03.40
6. Notas
Campos Vaziosalternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel e-mailaddress format isbn label lineage mark mirrorrepository nextedition notes orcid parameterlist parentrepositories previousedition previouslowerunit progress project readergroup resumeid rightsholder schedulinginformation secondarydate secondarykey secondarymark session shorttitle sponsor subject tertiarymark tertiarytype url
7. Controle da descrição
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