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dc.contributor.authorJandieri, George
dc.contributor.authorIshimaru, Akira
dc.contributor.authorPištora, Jaromír
dc.contributor.authorLesňák, Michal
dc.date.accessioned2019-06-18T07:30:09Z
dc.date.available2019-06-18T07:30:09Z
dc.date.issued2019
dc.identifier.citationAdvanced Electromagnetics. 2019, vol. 8, issue 2, special issue, p. 77-84.cs
dc.identifier.issn2119-0275
dc.identifier.urihttp://hdl.handle.net/10084/135212
dc.description.abstractSecond order statistical moments of scattered electromagnetic waves in the turbulent magnetized plasma slab with electron density fluctuations are calculated applying the modify stochastic smooth perturbation theory and the boundary conditions. The obtained results are valid for arbitrary correlation function of electron density fluctuations. Stokes parameters are analyzed both analytically and numerically. The theory predicts that depolarization effect caused by second Stokes parameter may be important in scintillation effects. Numerical calculations are carried out for new spectral function of electron density fluctuations containing both anisotropic Gaussian and power-law spectral functions using the experimental data. Polarimetric parameters are calculated for different anisotropy factor and inclination angle of elongated small-scale irregularities with respect to the magnetic lines of forces. The relationship between the scintillations and the polarimetric parameters is important.cs
dc.language.isoencs
dc.publisherAdvanced Electromagneticscs
dc.relation.ispartofseriesAdvanced Electromagneticscs
dc.relation.urihttps://www.aemjournal.org/index.php/AEM/article/view/1150/432cs
dc.titlePolarimetric parameters of scattered radiation in the magnetized plasmacs
dc.typearticlecs
dc.identifier.doi10.7716/aem.v8i2.1150
dc.rights.accessopenAccesscs
dc.type.versionpublishedVersioncs
dc.type.statusPeer-reviewedcs
dc.description.sourceWeb of Sciencecs
dc.description.volume8cs
dc.description.issue2cs
dc.description.lastpage84cs
dc.description.firstpage77cs
dc.identifier.wos000468128100001


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