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dc.contributor.authorReznikova, V. E.
dc.contributor.authorAntolin, P.
dc.contributor.authorVan Doorsselaere, T.
dc.date.accessioned2017-02-13T16:30:13Z
dc.date.available2017-02-13T16:30:13Z
dc.date.issued2014-03-28
dc.identifier248970011
dc.identifier6376cf1e-1fae-4317-a4a8-778260b29438
dc.identifier84898005050
dc.identifier.citationReznikova , V E , Antolin , P & Van Doorsselaere , T 2014 , ' Forward modeling of gyrosynchrotron intensity perturbations by sausage modes ' , Astrophysical Journal , vol. 785 , no. 2 , 86 . https://doi.org/10.1088/0004-637X/785/2/86en
dc.identifier.issn0004-637X
dc.identifier.otherBibCode: 2014ApJ...785...86R
dc.identifier.urihttps://hdl.handle.net/10023/10280
dc.description.abstractTo determine the observable radio signatures of the fast sausagestanding wave, we examine gyrosynchrotron (GS) emission modulation usinga linear three-dimensional magnetohydrodynamic model of a plasmacylinder. Effects of the line-of-sight angle and instrumental resolutionon perturbations of the GS intensity are analyzed for two models: a basemodel with strong Razin suppression and a low-density model in which theRazin effect was unimportant. Our finding contradicts previouspredictions made with simpler models: an in-phase variation of intensitybetween low (f <fpeak) and high (f > fpeak) frequencies is found for the low-density model and ananti-phase variation for the base model in the case of a viewing angleof 45°. The spatially inhomogeneous character of the oscillatingemission source and the spatial resolution of the model are found tohave a significant effect on the resulting intensity.
dc.format.extent11
dc.format.extent2035739
dc.language.isoeng
dc.relation.ispartofAstrophysical Journalen
dc.subjectSun: flaresen
dc.subjectSun: oscillationsen
dc.subjectSun: radio radiationen
dc.subjectWavesen
dc.subjectQB Astronomyen
dc.subjectQC Physicsen
dc.subject.lccQBen
dc.subject.lccQCen
dc.titleForward modeling of gyrosynchrotron intensity perturbations by sausage modesen
dc.typeJournal articleen
dc.contributor.institutionUniversity of St Andrews. Applied Mathematicsen
dc.identifier.doi10.1088/0004-637X/785/2/86
dc.description.statusPeer revieweden
dc.identifier.urlhttp://adsabs.harvard.edu/abs/2014ApJ...785...86Ren


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