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1. Identificação
Tipo de ReferênciaArtigo em Evento (Conference Proceedings)
Sitemtc-m16b.sid.inpe.br
Código do Detentorisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Repositóriosid.inpe.br/mtc-m17@80/2007/12.17.14.03
Repositório de Metadadossid.inpe.br/mtc-m17@80/2007/12.17.14.03.30
Última Atualização dos Metadados2018:06.05.03.36.36 (UTC) administrator
Chave SecundáriaINPE--PRE/
Chave de CitaçãoSimõesJúniorAlve:2007:OnDiEl
TítuloOne Dimensional Electromagnetic simulation of multiple electron beams propagation in the Earth's Bow Shock
Ano2007
Data de Acesso21 maio 2024
Tipo SecundárioPRE CN
2. Contextualização
Autor1 Simões Júnior, Fernando
2 Alves, Maria Virgínia
Grupo1 LAP-INPE-MCT-BR
2 LAP-INPE-MCT-BR
Afiliação1 Instituto Nacional de Pesquisas Espaciais (INPE)
2 Instituto Nacional de Pesquisas Espaciais (INPE)
Nome do EventoEncontro Brasileiro de Física dos Plasmas, 9.
Localização do EventoSão Pedro, SP
Data25-28 Nov.
Tipo TerciárioPoster
Histórico (UTC)2007-12-17 14:03:30 :: simone -> administrator ::
2012-10-24 00:13:38 :: administrator -> simone ::
2013-02-20 15:20:14 :: simone -> administrator :: 2007
2018-06-05 03:36:36 :: administrator -> marciana :: 2007
3. Conteúdo e estrutura
É a matriz ou uma cópia?é a matriz
Estágio do Conteúdoconcluido
Transferível1
Tipo do ConteúdoExternal Contribution
ResumoIt is by now well known that electron beams play an important role in generating radio emissions such as commonly observed by spacecraft in the upstream of the Earth's bow shock and those known as type II and III solar radio bursts. Electron beams streaming back from Earth's bow shock into the solar wind have been proposed as a possible source for the electron plasma waves observed by spacecraft in the electron foreshock. Recent researches suggest that multiple electron beams could be injected over a period of time, they tend to lose their individual identity to form just a single beam. In this work we use an electromagnetic PIC code (KEMPO 1D, modi¯ed) to simulate two beams which are injected into a plasma at di®erent times. The ¯rst beam disturbs the background plasma and generates Langmuir waves by electron beam-plasma interaction. Subsequently, another beam is inserted in the system and interacts with the ¯rst one and with the Langmuir waves to produce electromagnetic radiation. The initial conditions for the background plasma and the electron beams are based on the solar wind and electron foreshock observations. In our model we consider that the ¯rst and the second beams (for simple and multiples injections) are, at t = 0, fully injected into the system, i.e., the beam occupies all the system; this is necessary to avoid grid e®ects at the boundaries and gives the possibility of using a more simple model. The preliminary results of our simulation show that the ¯rst beam can produce electrostatic harmonics of plasma frequency while the second beam intensi¯es the emission at the harmonics that are produced for the ¯rst one. The second beam interacts very fast with the Langmuir waves due to the strong electric ¯eld and the phase coupling with the ¯rst beam. An increasing of electromagnetic and kinetic energies is also observed.
ÁreaFISPLASMA
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4. Condições de acesso e uso
Idiomapt
Grupo de Usuáriosadministrator
simone
administrator
Visibilidadeshown
5. Fontes relacionadas
Unidades Imediatamente Superiores8JMKD3MGPCW/3ET2RFS
Acervo Hospedeirolcp.inpe.br/ignes/2004/02.12.18.39
cptec.inpe.br/walmeida/2003/04.25.17.12
6. Notas
Campos Vaziosarchivingpolicy archivist booktitle callnumber copyholder copyright creatorhistory descriptionlevel dissemination documentstage doi e-mailaddress edition editor electronicmailaddress format identifier isbn issn keywords label lineage mark mirrorrepository nextedition notes numberoffiles numberofvolumes orcid organization pages parameterlist parentrepositories previousedition previouslowerunit progress project publisher publisheraddress readergroup readpermission resumeid rightsholder schedulinginformation secondarydate secondarymark serieseditor session shorttitle size sponsor subject targetfile tertiarymark type url versiontype volume
7. Controle da descrição
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