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1. Identity statement
Reference TypeConference Paper (Conference Proceedings)
Siteplutao.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W/43NH55Q
Repositorysid.inpe.br/plutao/2020/12.07.14.30.40
Last Update2020:12.08.18.28.16 (UTC) lattes
Metadata Repositorysid.inpe.br/plutao/2020/12.07.14.30.41
Metadata Last Update2022:01.04.01.31.21 (UTC) administrator
DOI10.1109/ICMCECS47690.2020.247003
ISBN9781728131269
Labellattes: 1272123236892781 8 NwankwoDAAFCRCE:2020:SiAtDr
Citation KeyNwankwoDAAFCRCE:2020:SiAtDr
TitleSimulation of atmospheric drag effect on low Earth orbit satellites during intervals of perturbed and quiet geomagnetic conditions in the magnetosphere-ionosphere system
FormatDVD
Year2020
Access Date2024, May 15
Secondary TypePRE CI
Number of Files1
Size618 KiB
2. Context
Author1 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.
Resume Identifier1
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8 8JMKD3MGP5W/3C9JH2C
Group1
2
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8 DIDAS-CGCEA-INPE-MCTIC-GOV-BR
Affiliation1 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
Author e-Mail Address1 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
Conference NameInternational Conference in Mathematics, Computer Engineering and Computer Science (ICMCECS)
Conference LocationAyobo, Nova Yorque
Date18-21 mar.
PublisherIEEE
Pages1-7
Book TitleProceedings
Tertiary TypeArtigo
History (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. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Keywordsatmospheric drag
satellite
ionosphere
AbstractIn 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.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAS > Simulation of atmospheric...
doc Directory Contentaccess
source Directory Contentthere are no files
agreement Directory Contentthere are no files
4. Conditions of access and use
data URLhttp://urlib.net/ibi/8JMKD3MGP3W/43NH55Q
zipped data URLhttp://urlib.net/zip/8JMKD3MGP3W/43NH55Q
Languagept
Target Filenwankwo.pdf
User Grouplattes
Reader Groupadministrator
lattes
Visibilityshown
Update Permissionnot transferred
5. Allied materials
Next Higher Units8JMKD3MGPCW/3ETR8EH
Host Collectiondpi.inpe.br/plutao@80/2008/08.19.15.01
6. Notes
Empty Fieldsarchivingpolicy 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. Description control
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