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dc.contributor.authorVerheest, F.
dc.contributor.authorLakhina, G.S.
dc.date.accessioned2015-09-22T07:13:42Z
dc.date.accessioned2021-02-12T09:30:18Z
dc.date.available2015-09-22T07:13:42Z
dc.date.available2021-02-12T09:30:18Z
dc.date.issued2002
dc.identifier.citationPhysica Scripta, v.T98, p.38-42, 2002, doi: 10.1238/Physica.Topical.098a00038en_US
dc.identifier.urihttp://localhost:8080/xmlui/handle/123456789/457
dc.description.abstractThe magnetosphere and the heliosphere constitute a magnificent laboratory for plasma wave phenomena, some of which have been studied in situ by ingenious spacecraft instrumentation, on board satellites probing interplanetary space as well as planetary and cometary environments. In several of these missions nonlinear structures have been observed. On the theoretical side, there are well known paradigms for nonlinear waves and solitons, like the different versions of the Korteweg-de Vries or nonlinear Schrödinger equations in multi-ion plasmas. We give a brief overview of how some of the more recent observations can be connected to the archetypical mathematical descriptions, in particular for magnetospheric boundary layer waves, nonlinear Alfvén waves in interplanetary space and solitary waves in cometary plasmas.en_US
dc.language.isoenen_US
dc.subjectSolar system plasmasen_US
dc.subjectNonlinear structuresen_US
dc.subjectMagnetosphereen_US
dc.subjectPlasma waveen_US
dc.subjectNonlinear wavesen_US
dc.titleNonlinear structures in solar system plasmasen_US
dc.typeArticleen_US
dcterms.sourcedoi: 10.1238/Physica.Topical.098a00038
dc.identifier.accession090963
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