Nonlinear structures in solar system plasmas

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dc.contributor.author Verheest, F.
dc.contributor.author Lakhina, G.S.
dc.date.accessioned 2015-09-22T07:13:42Z
dc.date.accessioned 2021-02-12T09:30:18Z
dc.date.available 2015-09-22T07:13:42Z
dc.date.available 2021-02-12T09:30:18Z
dc.date.issued 2002
dc.identifier.citation Physica Scripta, v.T98, p.38-42, 2002, doi: 10.1238/Physica.Topical.098a00038 en_US
dc.identifier.uri http://localhost:8080/xmlui/handle/123456789/457
dc.description.abstract The 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.iso en en_US
dc.subject Solar system plasmas en_US
dc.subject Nonlinear structures en_US
dc.subject Magnetosphere en_US
dc.subject Plasma wave en_US
dc.subject Nonlinear waves en_US
dc.title Nonlinear structures in solar system plasmas en_US
dc.type Article en_US
dcterms.source doi: 10.1238/Physica.Topical.098a00038
dc.identifier.accession 090963


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