Similarity of jupiter and RRATs

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dc.contributor.authorGezer I.
dc.contributor.authorPekünl¨ E.R.
dc.date.accessioned2019-10-26T22:32:04Z
dc.date.available2019-10-26T22:32:04Z
dc.date.issued2010
dc.departmentEge Üniversitesien_US
dc.description.abstractIn the present investigation, radial diffusion of equatorially trapped electrons in the magnetospheres of Jupiter and Rotating Radio Transients (RRATs) are examined and compared. It is assumed that electrons lose energy through synchrotron radiation and the wave-particle interaction. The phase space density of the electrons, which go through gradB drift in Jupiter's and RRATs magnetospheres and thus resonate with the plasma waves, changes and this change predicted by the model seems to be consistent with the Pioneer 10 and Pioneer 11 data for Jupiter's case and a similar result obtained for RRATs. © 2011 International Astronomical Union.en_US
dc.identifier.doi10.1017/S1743921311006624
dc.identifier.endpage88en_US
dc.identifier.isbn9780521197410
dc.identifier.issn1743-9213
dc.identifier.issn1743-9213en_US
dc.identifier.issueS274en_US
dc.identifier.scopusqualityQ4en_US
dc.identifier.startpage85en_US
dc.identifier.urihttps://doi.org/10.1017/S1743921311006624
dc.identifier.urihttps://hdl.handle.net/11454/19744
dc.identifier.volume6en_US
dc.indekslendigikaynakScopusen_US
dc.language.isoenen_US
dc.relation.ispartofProceedings of the International Astronomical Unionen_US
dc.relation.publicationcategoryKonferans Öğesi - Uluslararası - Kurum Öğretim Elemanıen_US
dc.rightsinfo:eu-repo/semantics/openAccessen_US
dc.subjectJupiteren_US
dc.subjectradio burstsen_US
dc.subjectRRATsen_US
dc.subjectwave-particle interactionen_US
dc.titleSimilarity of jupiter and RRATsen_US
dc.typeConference Objecten_US

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