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1. Identity statement
Reference TypeJournal Article
Sitemarte3.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier6qtX3pFwXQZ3r59YCT/GUhvq
Repositorysid.inpe.br/iris@1905/2005/07.29.01.25.28   (restricted access)
Last Update2013:04.03.12.49.57 (UTC) jefferson
Metadata Repositorysid.inpe.br/iris@1905/2005/07.29.01.25.42
Metadata Last Update2018:06.06.04.02.55 (UTC) administrator
Secondary KeyINPE-5762-PRE/1923
ISSN0273-1177
Label7156
Citation KeyBalanBaiSubAbdRao:1996:MoCoEq
TitleModel comparisons of equatorial plasma fountain and equatorial anomaly at three locations
Year1996
Secondary Date19960320
Access Date2024, May 05
Secondary TypePRE PI
Number of Files1
Size740 KiB
2. Context
Author1 Balan, N.
2 Bailey, G. J.
3 Subbarao, K. S. V.
4 Abdu, Mangalathayil Ali
5 Rao, P. B
Group1 DAE-INPE-MCT-BR
2
3
4 DAE-INPE-MCT-BR
JournalAdvances in Space Research
Volume18
Number6
Pages69-78
History (UTC)2013-03-17 03:46:37 :: administrator -> jefferson :: 1996
2013-04-03 12:49:57 :: jefferson -> administrator :: 1996
2018-06-06 04:02:55 :: administrator -> marciana :: 1996
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
KeywordsAERONOMIA
FORTALEZA (ESTADO)JICAMARCA
IONOSPHERIC PLASMA FOUNTAIN
IONOSPHERIC EQUATORIAL ANOMALY
AbstractThe equatorial plasma fountain and equatorial anomaly in the ionospheres over Jicamarca (77 degrees W), Trivandrum (77 degrees E), and Fortaleza (38 degree W) are compared under magnetically quiet (Ap=4) equinoctial conditions (day 264) at high solar activity (F10.7 = 178). The comparison, carried out using the Sheffield University Plasmaphere-Ionosphere Model with the same perpendicular ExB drift velocity at all locations, is aimed to investigate the modulating effect of neutral wind. The neutral wind is found to produce north-south asymmetries in the plasma fountain and anomaly, with larger plasma flow and stronger anomaly crests occurring in opposite hemispheres at all locations. The north-south asymmetry in the plasma fountain is stronger at locations of larger displacement between the geomagnetic and geographic equators than at locations of larger magnetic declination angle. The vertical ExB drift velocities at the magnetic equators of Trivandrum and Fortaleza are also derived by matching the measured and model values of the peak height hmax. The derived velocities (which correspond to the ionospheric peak) are compared with that measured at Jicamarca using the incoherent scatter radar.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAE > Model comparisons of...
doc Directory Contentaccess
source Directory Contentthere are no files
agreement Directory Contentthere are no files
4. Conditions of access and use
Languageen
Target File1-s2.0-0273117795009027-main.pdf
User Groupadministrator
jefferson
Visibilityshown
Archiving Policydenypublisher denyfinaldraft24
Read Permissiondeny from all and allow from 150.163
Update Permissionnot transferred
5. Allied materials
Next Higher Units8JMKD3MGPCW/3ETL868
DisseminationWEBSCI; PORTALCAPES; MGA; COMPENDEX.
Host Collectionsid.inpe.br/banon/2001/04.03.15.36
6. Notes
Empty Fieldsaffiliation alternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel doi e-mailaddress electronicmailaddress format isbn lineage mark mirrorrepository month nextedition notes orcid parameterlist parentrepositories previousedition previouslowerunit progress project readergroup resumeid rightsholder schedulinginformation secondarymark session shorttitle sponsor subject tertiarymark tertiarytype typeofwork url
7. Description control
e-Mail (login)marciana
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