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1. Identity statement
Reference TypeJournal Article
Sitemtc-m16.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier6qtX3pFwXQZ3r59YDa/KbKnQ
Repositorysid.inpe.br/iris@1916/2006/02.16.12.53   (restricted access)
Last Update2006:02.16.12.53.00 (UTC) administrator
Metadata Repositorysid.inpe.br/iris@1916/2006/02.16.12.53.55
Metadata Last Update2021:07.18.04.01.21 (UTC) administrator
Secondary KeyINPE-13527-PRE/8740
ISSN1364-6826
Citation KeyDenardiniAbdPauSobWra:2005:SeChEq
TitleSeasonal characterization of the equatorial electrojet height rise over Brazil as observed by the RESCO 50MHz back-scatter radar
Year2005
MonthDec.
Access Date2024, Apr. 27
Secondary TypePRE PI
Number of Files1
Size1476 KiB
2. Context
Author1 Denardini, Clezio Marcos
2 Abdu, Mangalathyil Ali
3 Paula, Eurico Rodrigues
4 Sobral, José Humberto de
5 Wrasse, C. M.
Group1 DAE-INPE-MCT-BR
Affiliation1 Instituto Nacional de Pesquisas Espaciais, Divisão de Aeronomia (INPE, DAE)
JournalJournal of Atmospheric and Solar-Terrestrial Physics
Volume67
Number17-18
Pages1665-1673
History (UTC)2006-02-20 11:36:44 :: marciana -> administrator ::
2021-07-18 04:01:21 :: administrator -> marciana :: 2005
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
KeywordsE-region
Back-scatter radar
Equatorial electrojet
Plasma irregularities height rise
AbstractIn this paper, we present the seasonal characteristics of the post-noon rise of the equatorial electrojet 3-m irregularities scattering region observed over Sa o Luý´ s, Brazil (2:3S, 44:2W, dip:0:5). The study is based on a 1 year data set collected by the 50MHz coherent back-scatter radar (also known by the acronym RESCO), that started operation in 1998. Using a method to estimate the moments from each individual back-scattered power profiles that constitute the standard rangetimeintensity (RTI) maps we were able to determine the following representative parameters of the electrojet: the total power back-scattered by the electrojet irregularities (EJP), the thickness of the electrojet back-scattered power profile (EJT), the height of the center of the back-scatter region, that is, the power profile, (EJC), and the noise level corresponding to each power profile (EJN). The parameterization was applied to all selected daily RTI maps from 2002. The analysis was carried out by grouping the data according to the radar beam angle (tilted 30 westward or eastward), the magnetic disturbance indices Kp and the season, which enables us to quantify the differences in the parameters on these bases. The results are presented and discussed here focusing on the post-noon ascent of the EJC. We will also present results on the eastwest asymmetry in the radar back-scattered echo power confirming our previous results, and on the appearance of a scattering region after sunset during magnetically quiet conditions around the southern summer solstice. r 2005 Elsevier Ltd. All rights reserved.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAE > Seasonal characterization of...
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4. Conditions of access and use
Target Filewrasse.pdf
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Visibilityshown
Copy HolderSID/SCD
Archiving Policydenypublisher denyfinaldraft24
Read Permissiondeny from all and allow from 150.163
5. Allied materials
Next Higher Units8JMKD3MGPCW/3ETL868
DisseminationWEBSCI; PORTALCAPES; AGU; MGA; COMPENDEX.
Host Collectionsid.inpe.br/banon/2003/08.15.17.40
6. Notes
NotesSelected papers from 7th Latin American Conference, Sao Paulo, Brazil
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