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1. Identificação
Tipo de ReferênciaArtigo em Evento (Conference Proceedings)
Siteplutao.sid.inpe.br
Código do Detentorisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identificador8JMKD3MGP3W/43NH55Q
Repositóriosid.inpe.br/plutao/2020/12.07.14.30.40
Última Atualização2020:12.08.18.28.16 (UTC) lattes
Repositório de Metadadossid.inpe.br/plutao/2020/12.07.14.30.41
Última Atualização dos Metadados2022:01.04.01.31.21 (UTC) administrator
DOI10.1109/ICMCECS47690.2020.247003
ISBN9781728131269
Rótulolattes: 1272123236892781 8 NwankwoDAAFCRCE:2020:SiAtDr
Chave de CitaçãoNwankwoDAAFCRCE:2020:SiAtDr
TítuloSimulation of atmospheric drag effect on low Earth orbit satellites during intervals of perturbed and quiet geomagnetic conditions in the magnetosphere-ionosphere system
FormatoDVD
Ano2020
Data de Acesso09 maio 2024
Tipo SecundárioPRE CI
Número de Arquivos1
Tamanho618 KiB
2. Contextualização
Autor1 Nwankwo, Victor Uchenna. J.
2 Denig, William
3 Ajakaiye, Muyiwa P.
4 Akanni, Wahabbi
5 Fatokun, Johnson
6 Chakrabarti, Sandip K.
7 Raulin, Jean-Pierre
8 Correia, Emília
9 Enoh, John E.
Identificador de Curriculo1
2
3
4
5
6
7
8 8JMKD3MGP5W/3C9JH2C
Grupo1
2
3
4
5
6
7
8 DIDAS-CGCEA-INPE-MCTIC-GOV-BR
Afiliação1 Anchor University
2 St. Joseph College of Maine
3 Anchor University
4 Anchor University
5 Anchor University
6 Indian Centre for Space Physics
7 Universidade Presbiteriana Mackenzie
8 Instituto Nacional de Pesquisas Espaciais (INPE)
9 Interorbital systems
Endereço de e-Mail do Autor1 vnwankwo@aul.edu.ng
2 wdenig@sjcme.edu.net
3 majakaiye@aul.edu.ng
4 wakanni@aul.edu.ng
5 jfatokun@aul.edu.ng
6 sandipchakrabarti9@gmail.com
7 raulin@craam.mackenzie.br
8 ecorreia@craam.mackenzie.br
9 enojoneno@gmail.com
Nome do EventoInternational Conference in Mathematics, Computer Engineering and Computer Science (ICMCECS)
Localização do EventoAyobo, Nova Yorque
Data18-21 mar.
Editora (Publisher)IEEE
Páginas1-7
Título do LivroProceedings
Tipo TerciárioArtigo
Histórico (UTC)2020-12-08 18:28:17 :: lattes -> administrator :: 2020
2020-12-09 09:17:28 :: administrator -> lattes :: 2020
2020-12-14 13:51:08 :: lattes -> administrator :: 2020
2022-01-04 01:31:21 :: administrator -> simone :: 2020
3. Conteúdo e estrutura
É a matriz ou uma cópia?é a matriz
Estágio do Conteúdoconcluido
Transferível1
Tipo do ConteúdoExternal Contribution
Palavras-Chaveatmospheric drag
satellite
ionosphere
ResumoIn this work, we simulate the effect of atmospheric drag on two model low Earth orbit (LEO) satellites with different ballistic coefficient during 1-month intervals of geomagnetically disturbed and relatively quiet conditions, to understand how solar and geomagnetic activity modulates satellites trajectory in Earths orbit. Our results showed that geomagnetic disturbances on the upper atmosphere associated with high solar activity caused a total decay of 2.77 km and 3.09 km for SAT-A and Sat-B, respectively during the 1-month period, but only about 0.52 km and 0.65 km, respectively during the interval of relatively quiet geomagnetic condition. The mean orbit decay rates (ODR) of the two satellites are ~90 m/day and ~100 m/day, respectively during the perturbed regime, while the respective values for the relatively quiet regime are ~17 m/day and 21 m/day. Within the two regimes, further analysis and simulation of the satellites responses during 12-day intervals of elevated solar and geomagnetic activity and exceptionally quiet activity showed that SAT-A and Sat-B decayed by about 1.13 km and 1.27 km, respectively during the former regime, while the respective decay for the latter regime are 0.16 km and 0.20 km. The respective mean ODR are 101.38 m/day and 113.22 m/day (for elevated activity), and 14.72 m/day and 18.52 m/day (exceptionally quiet). Sat-B has larger values of height decay (h) and ODR in both regimes, and therefore affected by atmospheric drag force more than Sat-A, because its ballistic coefficient is higher. The results of our simulation confirm (i) the dependence of atmospheric drag force on satellites ballistic coefficient, and (ii) geomagnetic storms being the leading driver of large-scale disturbances in the coupled magnetosphere-ionosphere-thermosphere systems, and consequently the leading perturber of satellites motion in low Earth orbit. Our model can be useful for situational awareness and mitigation of the potential threat posed by solar activity in modulating satellites trajectories.
ÁreaCEA
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4. Condições de acesso e uso
URL dos dadoshttp://urlib.net/ibi/8JMKD3MGP3W/43NH55Q
URL dos dados zipadoshttp://urlib.net/zip/8JMKD3MGP3W/43NH55Q
Idiomapt
Arquivo Alvonwankwo.pdf
Grupo de Usuárioslattes
Grupo de Leitoresadministrator
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Visibilidadeshown
Permissão de Atualizaçãonão transferida
5. Fontes relacionadas
Unidades Imediatamente Superiores8JMKD3MGPCW/3ETR8EH
Acervo Hospedeirodpi.inpe.br/plutao@80/2008/08.19.15.01
6. Notas
Campos Vaziosarchivingpolicy archivist callnumber copyholder copyright creatorhistory descriptionlevel dissemination e-mailaddress edition editor issn lineage mark mirrorrepository nextedition notes numberofvolumes orcid organization parameterlist parentrepositories previousedition previouslowerunit progress project publisheraddress readpermission rightsholder schedulinginformation secondarydate secondarykey secondarymark serieseditor session shorttitle sponsor subject tertiarymark type url versiontype volume
7. Controle da descrição
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