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1. Identity statement
Reference TypeConference Paper (Conference Proceedings)
Sitemtc-m21b.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34P/3N7RDJ8
Repositorysid.inpe.br/mtc-m21b/2017/01.18.15.10
Last Update2017:01.18.15.11.43 (UTC) simone
Metadata Repositorysid.inpe.br/mtc-m21b/2017/01.18.15.10.09
Metadata Last Update2022:03.18.22.12.09 (UTC) administrator
Secondary KeyINPE--PRE/
Citation KeyAlvesBarbSimõ:2016:PaSiWa
TitleParticle-in-cell Simulations of Waves in a Plasma Described by Kappa Velocity Distribution as Observed in the Saturn´s Magnetosphere
Year2016
Access Date2024, May 16
Secondary TypePRE CI
Number of Files1
Size2365 KiB
2. Context
Author1 Alves, Maria Virginia
2 Barbosa, Marcos Vinicius Grala
3 Simões Júnior, Fernando J. L.
Resume Identifier1 8JMKD3MGP5W/3C9JHRS
Group1 DGE-CEA-INPE-MCTI-GOV-BR
2 GESAST-CEA-SPG-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 mvirginia.alves@inpe.br
2 marcos.barbosa@inpe.br
Conference NameAGU Fall Meeting
Conference LocationSan Francisco
Date12-16 dec.
History (UTC)2017-01-18 15:11:43 :: simone -> administrator :: 2016
2022-03-18 22:12:09 :: administrator -> simone :: 2016
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
AbstractObservations have shown that several regions in space plasmas exhibit non-Maxwellian distributions with high energy superthermal tails. Kappa velocity distribution functions can describe many of these regions and have been used since the 60s. They suit well to represent superthermal tails in solar wind as well as to obtain plasma parameters of plasma within planetary magnetospheres. A set of initial velocities following kappa distribution functions is used in KEMPO1 particle simulation code to analyze the normal modes of wave propagation. Initial conditions are determined using observed characteristics for Saturn´s magnetosphere. Two electron species with different temperatures and densities and ions as a third species are used. Each electron population is described by a different kappa index. Particular attention is given to perpendicular propagation, Bernstein modes, and parallel propagation, Langmuir and electron-acoustic modes. The dispersion relation for the Bernstein modes is strongly influenced by the shape of the velocity distribution and consequently by the value of kappa index. Simulation results are compared with numerical solutions of the dispersion relation obtained in the literature and they are in good agreement.
AreaCEA
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4. Conditions of access and use
data URLhttp://mtc-m21b.sid.inpe.br/ibi/8JMKD3MGP3W34P/3N7RDJ8
zipped data URLhttp://mtc-m21b.sid.inpe.br/zip/8JMKD3MGP3W34P/3N7RDJ8
Languageen
User Groupsimone
Reader Groupadministrator
simone
Visibilityshown
Read Permissionallow from all
Update Permissionnot transferred
5. Allied materials
Linking8JMKD3MGP3W34P/3L4PGKH
Mirror Repositorysid.inpe.br/mtc-m21b/2013/09.26.14.25.22
Next Higher Units8JMKD3MGPCW/3EU29DP
8JMKD3MGPCW/3F2PBEE
Citing Item Listsid.inpe.br/bibdigital/2013/10.12.21.02 2
sid.inpe.br/mtc-m21/2012/07.13.14.55.54 1
Host Collectionsid.inpe.br/mtc-m21b/2013/09.26.14.25.20
6. Notes
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