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1. Identity statement
Reference TypeConference Paper (Conference Proceedings)
Sitemtc-m16.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Repositorysid.inpe.br/marciana/2004/01.13.13.33
Last Update2004:03.29.03.00.00 (UTC) administrator
Metadata Repositorysid.inpe.br/marciana/2004/01.13.13.33.24
Metadata Last Update2018:06.05.01.20.44 (UTC) administrator
Secondary KeyINPE-10405-PRE/5904
Citation KeySimõesJrGaelAlve:2003:PrElWa
TitlePropagation of electromagnetic waves in the source region of the auroral kilometric radiation in a cold plasma approximation
FormatOn-line
Year2003
Access Date2024, May 16
Secondary TypePRE CI
Number of Files1
Size1068 KiB
2. Context
Author1 Simões Jr., Fernando J. R.
2 Gaelzer, Rudi
3 Alves, Maria Virgínia
Resume Identifier1
2
3 8JMKD3MGP5W/3C9JHRS
Group1 LAP-INPE-MCT-BR
Affiliation1 Laboratório Associado de Plasma - INPE - S. J. dos Campos, SP, Brazil
2 Instituto de Física e Matemática - UFPel - Pelotas, RS, Brazil
Conference NameLatin American Workshop on Plasma Physics, 10; Brazilian Meeting on Plasma Physics, 7.
Conference LocationSão Pedro, 2003
Date2003
Book TitleProceedings
Tertiary TypePosters
History (UTC)2018-06-05 01:20:44 :: administrator -> marciana :: 2003
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Keywordsfísica básica de plasma
basic plasma physics
AbstractIn this work we use the magnetoionic theory to describe the propagation of electromagnetic waves inside a plasma cavity that is immersed in a weakly inhomogeneous, stationary magnetic field BÅ. From the usual expressions for the dielectric tensor and dispersion relation, we derive a set of canonical equations that describe, within the geometrical optics approximation, the time evolution of the wave vector and the ray position inside the plasma cavity. The ray tracing equations thus derived are employed to study the wave propagation and amplification inside the source region of the Auroral Kilometric Radiation (AKR). To this end, we use a specific physical model, derived elsewhere (Gaelzer et al., 1992; Gaelzer et al., 1994), that models a two-dimensional cavity in the auroral region of the magnetosphere, inside of which the AKR is generated by the electron maser mechanism. With this information, we developed a computational code that describes the evolution of an electromagnetic wave spreading inside the source region of the AKR. A comparison with other works found in the literature is presented.
AreaFISPLASMA
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > LABAP > Propagation of electromagnetic...
doc Directory Contentaccess
source Directory Contentthere are no files
agreement Directory Contentthere are no files
4. Conditions of access and use
data URLhttp://urlib.net/ibi/sid.inpe.br/marciana/2004/01.13.13.33
zipped data URLhttp://urlib.net/zip/sid.inpe.br/marciana/2004/01.13.13.33
Languageen
Target Filepropagation.pdf
User Groupadministrator
Visibilityshown
Copy HolderSID/SCD
5. Allied materials
Next Higher Units8JMKD3MGPCW/3ET2RFS
Citing Item Listsid.inpe.br/bibdigital/2013/09.25.21.49 1
sid.inpe.br/mtc-m21/2012/07.13.14.55.54 1
Host Collectionsid.inpe.br/banon/2003/08.15.17.40
6. Notes
Empty Fieldsarchivingpolicy archivist callnumber copyright creatorhistory descriptionlevel dissemination documentstage doi e-mailaddress edition editor electronicmailaddress identifier isbn issn label lineage mark mirrorrepository nextedition notes numberofvolumes orcid organization pages parameterlist parentrepositories previousedition previouslowerunit progress project publisher publisheraddress readergroup readpermission rightsholder schedulinginformation secondarydate secondarymark serieseditor session shorttitle sponsor subject tertiarymark type url versiontype volume
7. Description control
e-Mail (login)marciana
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