Nonlinear electromagnetic waves and spherical arc-polarized waves in space plasmas

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dc.contributor.author Tsurutani, B.T.
dc.contributor.author Ho, Christian M.
dc.contributor.author Arballo, John K.
dc.contributor.author Lakhina, G.S.
dc.contributor.author Glassmeier, Karl-Heinz
dc.contributor.author Neubauer, Fritz M.
dc.date.accessioned 2015-09-28T06:58:18Z
dc.date.accessioned 2021-02-12T09:31:37Z
dc.date.available 2015-09-28T06:58:18Z
dc.date.available 2021-02-12T09:31:37Z
dc.date.issued 1997
dc.identifier.citation Plasma Physics and Controlled Fusion, v.39, p.A237-A250, 1997, doi: 10.1088/0741-3335/39/5A/022 en_US
dc.identifier.uri http://localhost:8080/xmlui/handle/123456789/489
dc.description.abstract We review observations of nonlinear plasma waves detected by interplanetary spacecraft. For this paper we will focus primarily on the phase-steepened properties of such waves. Plasma waves at comet Giacobini - Zinner measured by the international cometary explorer (ICE), at comets Halley and Grigg - Skjellerup measured by Giotto, and interplanetary Alfvén waves measured by Ulysses, will be discussed and intercompared. Owing to the page limitations of this paper we will keep the cometary wave discussion brief (but references for the interested reader will be provided), and we will focus more on the recent Ulysses observations of phase-steepened Alfvén waves. For the latter, classical `interplanetary rotational discontinuities' are explained as phase-steepened edges of Alfvén waves. Both the Alfvén waves and their phase-steepened edges will be shown to be arc-polarized. A method of determination of the direction of propagation of these waves will be discussed. en_US
dc.language.iso en en_US
dc.subject Nonlinear electromagnetic waves en_US
dc.subject Spherical arc-polarized waves en_US
dc.subject Space plasma en_US
dc.subject Nonlinear plasma waves en_US
dc.subject Alfvén waves en_US
dc.title Nonlinear electromagnetic waves and spherical arc-polarized waves in space plasmas en_US
dc.type Article en_US
dcterms.source doi: 10.1088/0741-3335/39/5A/022
dc.identifier.accession 090998


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