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1. Identity statement
Reference TypeJournal Article
Sitemtc-m21d.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34T/45P6G82
Repositorysid.inpe.br/mtc-m21d/2021/11.08.11.51
Last Update2021:11.08.11.51.29 (UTC) simone
Metadata Repositorysid.inpe.br/mtc-m21d/2021/11.08.11.51.29
Metadata Last Update2022:04.03.19.24.06 (UTC) administrator
DOI10.3390/atmos12111409
ISSN2073-4433
Citation KeyEssienFTWBKLAGB:2021:LoStMe
TitleLong-term study on medium-scale traveling ionospheric disturbances observed over the south american equatorial region
Year2021
MonthNov.
Access Date2024, May 05
Type of Workjournal article
Secondary TypePRE PI
Number of Files1
Size2889 KiB
2. Context
Author 1 Essien, Patrick
 2 Figueiredo, Cosme Alexandre Oliveira Barros
 3 Takahashi, Hisao
 4 Wrasse, Cristiano Max
 5 Barros, Diego
 6 Klutse, N. A. B.
 7 Lomotey, Solomon Otoo
 8 Ayorinde, Toyese Tunde
 9 Gobbi, Delano
10 Bilibio, Anderson Vestena
Resume Identifier 1
 2
 3 8JMKD3MGP5W/3C9JHCM
 4
 5
 6
 7
 8
 9 8JMKD3MGP5W/3C9JGTE
ORCID 1 0000-0002-7258-9307
 2 0000-0003-4423-5111
Group 1 GESATM-CEA-DIPGR-INPE-MCTI-GOV-BR
 2 DICEP-CGCE-INPE-MCTI-GOV-BR
 3 DICEP-CGCE-INPE-MCTI-GOV-BR
 4 DICEP-CGCE-INPE-MCTI-GOV-BR
 5 GESATM-CEA-DIPGR-INPE-MCTI-GOV-BR
 6
 7 GESATM-CEA-DIPGR-INPE-MCTI-GOV-BR
 8 GESATM-CEA-DIPGR-INPE-MCTI-GOV-BR
 9 DICEP-CGCE-INPE-MCTI-GOV-BR
10 GESATM-CEA-DIPGR-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 Instituto Nacional de Pesquisas Espaciais (INPE)
 5 Instituto Nacional de Pesquisas Espaciais (INPE)
 6 African Institute for Mathematical Sciences (AIMS)
 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 pessien@aims.edu.gh
 2 cosme.figueiredo@inpe.br
 3 hisao.takahashi@inpe.br
 4 cristiano.Wrasse@inpe.br
 5 diego.barros@inpe.br
 6 nklutse@ug.edu.gh
 7 solomon.lomotey@inpe.br
 8 tndayorinde@gmail.com
 9 delano.gobbi@inpe.br
10 anderson.bilibio@inpe.br
JournalAtmosphere
Volume12
Number11
Pagese1409
Secondary MarkB3_ENGENHARIAS_III B3_ENGENHARIAS_I B3_CIÊNCIAS_AMBIENTAIS B4_ENGENHARIAS_II B5_GEOCIÊNCIAS
History (UTC)2021-11-08 11:51:29 :: simone -> administrator ::
2021-11-08 11:51:31 :: administrator -> simone :: 2021
2021-11-08 11:52:31 :: simone -> administrator :: 2021
2022-04-03 19:24:06 :: administrator -> simone :: 2021
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
KeywordsDetrended TEC
Equatorial
Medium-scale traveling ionospheric disturbances
AbstractUsing data collected by the GNSS dual-frequency receivers network, de-trended TEC maps were generated to identify and characterize the medium-scale traveling ionospheric disturbances (MSTIDs) over the South American equatorial region (latitude: 0◦ to 15◦ S and longitude: 30◦ to 55◦ W) during solar cycle 24 (from January 2014 to December 2019). A total of 712 MSTIDs were observed during quiet geomagnetic conditions. The Frequency of occurrence of MSTID is high during the solar maximum and low in the minimum phase. This might be due to the solar cycle dependence of gravity wave activity in the lower atmosphere and gravity wave propagation conditions in the thermosphere. The predominant daytime MSTIDs, representing 80% of the total observations, occurred in winter (June-August season in the southern hemisphere) with the secondary peak in the equinox; while the evening time MSTIDs, representing 18% of the entire events, occurred in summer (December to February season) and equinox (March to May and September to November), and the remaining 2% of the MSTIDs were observed during nighttime. The seasonal variation of the MSTID events was attributed to the source mechanisms generating them, the wind filtering and dissipation effects, and the local time dependency. The horizontal wavelengths of the MSTIDs were mostly concentrated between 500 and 800 km, with the mean value of 667 ± 131 km. The observed periods ranged from 30 to 45 min with the mean value of 36 ± 7 min. The observed horizontal phase speeds were distributed around 200 to 400 m/s, with the corresponding mean of 301 ± 75 m/s. The MSTIDs in the winter solstice and equinoctial months preferentially propagated northeastward and northwestward. Meanwhile, during the summer solstice, they propagated in all directions. The anisotropy of the propagation direction might be due to several reasons: the wind and dissipative filtering effects, ion drag effects, the primary source region, and the presence of the secondary or tertiary gravity waves in the thermosphere. Atmospheric gravity waves from strong convective sources might be the primary precursor for the observed equatorial MSTIDs. In all seasons, we noted that the MSTIDs propagating southeastward were probably excited by the likely gravity waves generated by the intertropical convergence zone (ITCZ).
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4. Conditions of access and use
data URLhttp://urlib.net/ibi/8JMKD3MGP3W34T/45P6G82
zipped data URLhttp://urlib.net/zip/8JMKD3MGP3W34T/45P6G82
Languageen
Target Fileessien_atmosphere.pdf
User Groupsimone
Reader Groupadministrator
simone
Visibilityshown
Archiving Policyallowpublisher allowfinaldraft
Update Permissionnot transferred
5. Allied materials
Next Higher Units8JMKD3MGPCW/3F2PBEE
8JMKD3MGPCW/46KTFK8
Citing Item Listsid.inpe.br/mtc-m21/2012/07.13.14.44.27 1
DisseminationWEBSCI; PORTALCAPES; SCOPUS.
Host Collectionurlib.net/www/2021/06.04.03.40
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