Close

1. Identity statement
Reference TypeReport
Sitemarte3.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier6qtX3pFwXQZ3r59YCT/GSj4f
Repositorysid.inpe.br/iris@1905/2005/07.25.15.53.24   (restricted access)
Last Update2015:07.13.16.14.37 (UTC) marciana
Metadata Repositorysid.inpe.br/iris@1905/2005/07.25.15.53.26
Metadata Last Update2019:10.08.15.14.33 (UTC) marciana
Report NumberINPE-76/LAFE
Label1473
Citation KeyTeracine:1968:SaObLo
TitleSatellite observations of the low latitudes ionosphere (PART I AND II)
Year1968
Secondary Date19940125
Access Date2024, May 05
TypeRPQ
Number of Pages120
Number of Files1
Size2425 KiB
2. Context
AuthorTeracine, Edson Baptista
GroupCNAE-BR
InstitutionCNAE
CitySao Jose dos Campos
History (UTC)2006-11-15 21:53:13 :: administrator -> jefferson ::
2012-10-05 17:25:48 :: jefferson -> administrator :: 1968
2014-09-29 15:30:50 :: administrator -> marciana :: 1968
2015-12-22 13:15:44 :: marciana -> administrator :: 1968
2018-06-06 04:38:58 :: administrator -> marciana :: 1968
2019-10-08 15:14:33 :: marciana -> sergio :: 1968
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Keywordsneutral atmosphere
atmosfera neutra
AbstractAbstract A brief review on the behavior of the neutral atmosphere when acted on by solar radiation and the consequent formation of the ionosphere is made. A mathematical model is chosen to be representative of the ionospheric electron density profile. Using data on the total absorption suffered by radio waves which traverse the ionosphere, the electron temperature is calculated. The results thus obtained are applied to the assumed distribution and important ionospheric parameters are determined. Resumo Uma breve revisão sobre o comportamento da atmosfera neutra quando actuado por radiação solar e a consequente formação da ionosfera é feita. Um modelo matemático é escolhido para ser representativo do perfil de densidade de electrões ionosférico. Usando dados sobre a total absorção sofrida por ondas de rádio que atravessam a ionosfera, a temperatura eletrônica é calculado. Os resultados assim obtidos são aplicados para a distribuição assumida e parâmetros importantes são determinados ionosféricas.
AreaCEA
doc Directory Contentaccess
source Directory Content
publicacao.pdf 22/12/2015 11:15 502.2 KiB 
agreement Directory Contentthere are no files
4. Conditions of access and use
Languageen
User Groupadministrator
jefferson
marciana
sergio
Visibilityshown
Rightsholderoriginalauthor yes locatedauthor no
Read Permissiondeny from all and allow from 150.163
Update Permissiontransferred to sergio
5. Allied materials
Host Collectionsid.inpe.br/banon/2001/04.03.15.36
6. Notes
Empty Fieldsaffiliation archivingpolicy archivist callnumber contenttype copyholder copyright creatorhistory date descriptionlevel dissemination doi e-mailaddress edition electronicmailaddress format isbn issn lineage mark mirrorrepository nextedition nexthigherunit notes orcid parameterlist parentrepositories previousedition previouslowerunit progress project readergroup recipient resumeid schedulinginformation secondarykey secondarymark secondarytype session shorttitle sponsor subject targetfile tertiarymark tertiarytype translator url versiontype
7. Description control
e-Mail (login)sergio
update 


Close