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1. Identity statement
Reference TypeJournal Article
Sitemtc-m16d.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP7W/3A77RCL
Repositorysid.inpe.br/mtc-m19/2011/08.01.17.27   (restricted access)
Last Update2011:12.21.12.44.22 (UTC) administrator
Metadata Repositorysid.inpe.br/mtc-m19/2011/08.01.17.27.24
Metadata Last Update2018:06.05.04.24.39 (UTC) administrator
Secondary KeyINPE--PRE/
DOI10.1029/2010JA016056
ISSN0926-9851
Citation KeyLiNiAbYuLiWaHu:2011:OcPoEq
TitleOn the occurrence of postmidnight equatorial F region irregularities during the June solstice
Year2011
MonthAPR
Access Date2024, May 04
Secondary TypePRE PI
Number of Files1
Size6366 KiB
2. Context
Author1 Li, Guozhu
2 Ning, Baiqi
3 Abdu, Mangalthayil Ali
4 Yue, Xinan
5 Liu, Libo
6 Wan, Weixing
7 Hu, Lianhuan
Group1
2
3 DAE-CEA-INPE-MCT-BR
Affiliation1 Chinese Acad Sci, Inst Geol & Geophys, Beijing Natl Observ Space Environm, Beijing 100029, Peoples R China
2 Chinese Acad Sci, Inst Geol & Geophys, Beijing Natl Observ Space Environm, Beijing 100029, Peoples R China
3 Instituto Nacional de Pesquisas Espaciais (INPE)
4 Univ Corp Atmospher Res, Boulder, CO 80307 USA
5 Chinese Acad Sci, Inst Geol & Geophys, Beijing Natl Observ Space Environm, Beijing 100029, Peoples R China v
6 Chinese Acad Sci, Inst Geol & Geophys, Beijing Natl Observ Space Environm, Beijing 100029, Peoples R China
7 Chinese Acad Sci, Inst Geol & Geophys, Beijing Natl Observ Space Environm, Beijing 100029, Peoples R China
e-Mail Addresssecretaria.cpa@dir.inpe.br
JournalJournal of Applied Geophysics
Volume116
PagesAO4318
History (UTC)2011-08-04 12:58:05 :: secretaria.cpa@dir.inpe.br -> administrator :: 2011
2011-08-15 04:59:12 :: administrator -> secretaria.cpa@dir.inpe.br :: 2011
2011-11-01 11:45:46 :: secretaria.cpa@dir.inpe.br -> banon :: 2011
2011-11-18 18:44:20 :: banon -> tereza@sid.inpe.br :: 2011
2011-12-21 12:44:32 :: tereza@sid.inpe.br -> administrator :: 2011
2012-07-15 02:59:04 :: administrator -> banon :: 2011
2012-09-26 15:28:23 :: banon -> administrator :: 2011
2018-06-05 04:24:39 :: administrator -> tereza@sid.inpe.br :: 2011
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
KeywordsIONOSPHERE-THERMOSPHERE SYSTEM
MERIDIONAL WIND CONTROL
SPREAD-F
ELECTRIC-FIELD
DRIFT VELOCITIES
PLASMA BUBBLES
RADAR
MODEL
ELECTRODYNAMICS
INSTABILITY
AbstractPostmidnight equatorial F region irregularities (EFIs) are known to develop mainly during the solstitial months. However, it is not well understood whether they occur at all longitudes and what process causes their occurrence at different longitude sectors. In this study, we use the GPS total electron content (TEC) fluctuations obtained from a global GPS network and spread F in ionograms from Jicamarca (283 degrees E, 12 degrees S, Dip 1 degrees N) in the American longitude sector and Kwajalein (167 degrees E, 9 degrees N, Dip 4 degrees N), Bac Lieu (106 degrees E, 9 degrees N, Dip 2 degrees N), and Chumphon (99 degrees E, 11 degrees N, Dip 3 degrees N) in the Pacific and Asian longitude sectors during 2000-2009, to investigate the EFI characteristics during June solstice. Results from global TEC fluctuations show that at solar maximum, the occurrence rate of postmidnight EFIs is high in African and Pacific regions, moderate in the Southeast Asian region, and low in the Peruvian region and that most postmidnight EFIs are the continuation of postsunset EFIs. During solar minimum the postmidnight EFIs were rarely observed in TEC but were very frequent in ionograms. The latter had more frequent postmidnight onsets over Peru, whereas they were initiated during late postsunset hours in Pacific and Southeast Asian longitudes. In both longitudes the postsunset layer rise occurred with some delay. The layer rise was more prominent on spread F nights over Jicamarca and less so over Pacific longitudes. The results showing different degrees of association at the different longitudes between the postsunset/postmidnight EFIs and F layer heights highlight the influence of other factors in the late-night EFI development. Perturbation seeds and plasma drifts/neutral winds, in particular, are discussed as strong candidates for causing these irregularities in the June solstitial months of solar minimum years.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAE > On the occurrence...
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4. Conditions of access and use
Languageen
User Groupadministrator
banon
secretaria.cpa@dir.inpe.br
tereza@sid.inpe.br
Visibilityshown
Archiving Policydenypublisher denyfinaldraft24
Read Permissiondeny from all and allow from 150.163
Update Permissionnot transferred
5. Allied materials
Mirror Repositorysid.inpe.br/mtc-m19@80/2009/08.21.17.02.53
Next Higher Units8JMKD3MGPCW/3ETL868
DisseminationWEBSCI; AGU; MGA; COMPENDEX.
Host Collectionsid.inpe.br/mtc-m19@80/2009/08.21.17.02
6. Notes
Empty Fieldsalternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel electronicmailaddress format isbn label lineage mark nextedition notes number orcid parameterlist parentrepositories previousedition previouslowerunit progress project readergroup resumeid rightsholder schedulinginformation secondarydate secondarymark session shorttitle sponsor subject targetfile tertiarymark tertiarytype typeofwork url
7. Description control
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