This HTML5 document contains 39 embedded RDF statements represented using HTML+Microdata notation.

The embedded RDF content will be recognized by any processor of HTML5 Microdata.

Namespace Prefixes

PrefixIRI
dctermshttp://purl.org/dc/terms/
n9http://linked.opendata.cz/resource/domain/vavai/projekt/
n11http://linked.opendata.cz/ontology/domain/vavai/
n16http://linked.opendata.cz/resource/domain/vavai/zamer/
shttp://schema.org/
n5http://linked.opendata.cz/ontology/domain/vavai/riv/
skoshttp://www.w3.org/2004/02/skos/core#
n7http://linked.opendata.cz/resource/domain/vavai/vysledek/RIV%2F67985815%3A_____%2F10%3A00355145%21RIV11-AV0-67985815/
n2http://linked.opendata.cz/resource/domain/vavai/vysledek/
rdfhttp://www.w3.org/1999/02/22-rdf-syntax-ns#
n15http://linked.opendata.cz/ontology/domain/vavai/riv/klicoveSlovo/
n13http://linked.opendata.cz/ontology/domain/vavai/riv/duvernostUdaju/
xsdhhttp://www.w3.org/2001/XMLSchema#
n17http://linked.opendata.cz/ontology/domain/vavai/riv/jazykVysledku/
n12http://linked.opendata.cz/ontology/domain/vavai/riv/aktivita/
n8http://linked.opendata.cz/ontology/domain/vavai/riv/obor/
n6http://linked.opendata.cz/ontology/domain/vavai/riv/druhVysledku/
n14http://reference.data.gov.uk/id/gregorian-year/

Statements

Subject Item
n2:RIV%2F67985815%3A_____%2F10%3A00355145%21RIV11-AV0-67985815
rdf:type
skos:Concept n11:Vysledek
dcterms:description
We concentrate here on incompressible plasma flows and 2-D equilibria, which allow us to find analytic solutions of the stationary magnetohydrodynamics equations (SMHD). First we solve the magnetohydrostatic (MHS) equations with the help of a Grad-Shafranov equation and then we transform these static equilibria into a stationary state with plasma flow. We are in particular interested to study SMHD-equilibria with strong plasma flow gradients perpendicular to separatrices. We find that induced thin current sheets occur naturally in such situations. The strength of the induced currents depend on the Alfvén Mach number and its gradient, and on the magnetic field. We concentrate here on incompressible plasma flows and 2-D equilibria, which allow us to find analytic solutions of the stationary magnetohydrodynamics equations (SMHD). First we solve the magnetohydrostatic (MHS) equations with the help of a Grad-Shafranov equation and then we transform these static equilibria into a stationary state with plasma flow. We are in particular interested to study SMHD-equilibria with strong plasma flow gradients perpendicular to separatrices. We find that induced thin current sheets occur naturally in such situations. The strength of the induced currents depend on the Alfvén Mach number and its gradient, and on the magnetic field.
dcterms:title
Thin current sheets caused by plasma flow gradients in space and astrophysical plasma Thin current sheets caused by plasma flow gradients in space and astrophysical plasma
skos:prefLabel
Thin current sheets caused by plasma flow gradients in space and astrophysical plasma Thin current sheets caused by plasma flow gradients in space and astrophysical plasma
skos:notation
RIV/67985815:_____/10:00355145!RIV11-AV0-67985815
n5:aktivita
n12:P n12:Z
n5:aktivity
P(IAA300030804), Z(AV0Z10030501)
n5:cisloPeriodika
8
n5:dodaniDat
n14:2011
n5:domaciTvurceVysledku
Nickeler, Dieter Horst
n5:druhVysledku
n6:J
n5:duvernostUdaju
n13:S
n5:entitaPredkladatele
n7:predkladatel
n5:idSjednocenehoVysledku
292793
n5:idVysledku
RIV/67985815:_____/10:00355145
n5:jazykVysledku
n17:eng
n5:klicovaSlova
magnetospheric physics; space plasma physics
n5:klicoveSlovo
n15:magnetospheric%20physics n15:space%20plasma%20physics
n5:kodStatuVydavatele
DE - Spolková republika Německo
n5:kontrolniKodProRIV
[F5D3938CCE96]
n5:nazevZdroje
Annales Geophysicae
n5:obor
n8:BN
n5:pocetDomacichTvurcuVysledku
1
n5:pocetTvurcuVysledku
2
n5:projekt
n9:IAA300030804
n5:rokUplatneniVysledku
n14:2010
n5:svazekPeriodika
28
n5:tvurceVysledku
Wiegelmann, T. Nickeler, Dieter Horst
n5:wos
000281432700006
n5:zamer
n16:AV0Z10030501
s:issn
0992-7689
s:numberOfPages
10