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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.rights© 2014. The American Astronomical Society. All rights reserved. Printed in the U.S.A. This work is made available online in accordance with the publisher’s policies. This is the final published version of the work, which was originally published at: https://dx.doi.org/10.1088/0004-637X/785/2/86en
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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