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1. Identity statement
Reference TypeConference Abstract (Conference Proceedings)
Sitemtc-m21b.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34P/3LR5K48
Repositorysid.inpe.br/mtc-m21b/2016/06.06.16.31
Last Update2016:06.06.16.31.59 (UTC) simone
Metadata Repositorysid.inpe.br/mtc-m21b/2016/06.06.16.31.29
Metadata Last Update2021:09.16.02.59.19 (UTC) administrator
Secondary KeyINPE--PRE/
Citation KeyBarbosaAlveSimõ:2016:PISiTh
TitlePIC simulations of a three component plasma described by Kappa distribution functions as observed in Saturn’s magnetosphere
Year2016
Access Date2024, May 17
Secondary TypePRE CI
Number of Files1
Size34 KiB
2. Context
Author1 Barbosa, Marcos Vinicius Grala
2 Alves, Maria Virginia
3 Simões Júnior, Fernando
Resume Identifier1
2 8JMKD3MGP5W/3C9JHRS
Group1 GES-CEA-SPG-INPE-MCTI-GOV-BR
2 DGE-CEA-INPE-MCTI-GOV-BR
Affiliation1 Instituto Nacional de Pesquisas Espaciais (INPE)
2 Instituto Nacional de Pesquisas Espaciais (INPE)
3 Universidade Federal de Pelotas (UFPel)
Author e-Mail Address1 marcos.barbosa@inpe.br
2 mvirginia.alves@inpe.br
Conference NameEuropean Geophysical Society General Assembly
Conference LocationVienna, Austria
Date17-22 Apr.
Book TitleAbstracts
History (UTC)2016-06-06 16:31:59 :: simone -> administrator :: 2016
2016-07-04 12:30:02 :: administrator -> simone :: 2016
2017-01-18 15:02:37 :: simone -> administrator :: 2016
2021-09-16 02:59:19 :: administrator -> simone :: 2016
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Version Typepublisher
AbstractIn plasmas out of thermodynamic equilibrium the particle velocity distribution can be described by the so called Kappa distribution. These velocity distribution functions are a generalization of the Maxwellian distribution. Since 1960, Kappa velocity distributions were observed in several regions of interplanetary space and astrophysical plasmas. Using KEMPO1 particle simulation code, modified to introduce Kappa distribution functions as initial conditions for particle velocities, the normal modes of propagation were analyzed in a plasma containing two species of electrons with different temperatures and densities and ions as a third specie.This type of plasma is usually found in magnetospheres such as in Saturn. Numerical solutions for the dispersion relation for such a plasma predict the presence of an electron-acoustic mode, besides the Langmuir and ion-acoustic modes. In the presence of an ambient magnetic field, the perpendicular propagation (Bernstein mode) also changes, as compared to a Maxwellian plasma, due to the Kappa distribution function. Here results for simulations with and without external magnetic field are presented. The parameters for the initial conditions in the simulations were obtained from the Cassini spacecraft data. Simulation results are compared with numerical solutions of the dispersion relation obtained in the literature and they are in good agreement.
AreaCEA
Arrangement 1urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDGE > PIC simulations of...
Arrangement 2urlib.net > BDMCI > Fonds > Produção pgr ATUAIS > GES > PIC simulations of...
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4. Conditions of access and use
data URLhttp://mtc-m21b.sid.inpe.br/ibi/8JMKD3MGP3W34P/3LR5K48
zipped data URLhttp://mtc-m21b.sid.inpe.br/zip/8JMKD3MGP3W34P/3LR5K48
Languageen
Target Filebarbosa_pic.pdf
User Groupsimone
Reader Groupadministrator
simone
Visibilityshown
Update Permissionnot transferred
5. Allied materials
Linking8JMKD3MGP3W34P/3L4PGKH
Mirror Repositoryurlib.net/www/2011/03.29.20.55
Next Higher Units8JMKD3MGPCW/3EU29DP
8JMKD3MGPCW/3F2PBEE
Citing Item Listsid.inpe.br/mtc-m21/2012/07.13.14.55.54 4
sid.inpe.br/mtc-m21b/2013/09.26.14.25.22 2
Host Collectionsid.inpe.br/mtc-m21b/2013/09.26.14.25.20
6. Notes
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