A magnetoacoustic autowave pulse in acoustically unstable regions of solar atmosphere

dc.contributor.authorMolevich, N.E.
dc.contributor.authorZavershinskiy, D.I.
dc.contributor.authorZavershinskiy, I.P.
dc.date.accessioned2015-08-25T10:22:58Z
dc.date.available2015-08-25T10:22:58Z
dc.date.issued2015
dc.description.abstractPaper presented to the 3rd Southern African Solar Energy Conference, South Africa, 11-13 May, 2015.en_ZA
dc.description.abstractTaking into account the most recent net radiation function model and five different kinds of heating scenarios for the upper solar atmosphere, we have defined some regions where the magnetoacoustical amplification may take place. The nonlinear equation describing the evolution of fast and slow magnetoacoustic waves in a heat-releasing completely ionized plasma has been obtained. The shape and parameters of the magnetoacoustic pulse that is an automodel solution of this equation under conditions of magnetoacoustic instability have been determineden_ZA
dc.description.librariandc2015en_ZA
dc.format.extent4 pagesen_ZA
dc.format.mediumPDFen_ZA
dc.identifier.citationMolevich, N.E., Zavershinskiy, D.I. & Zavershinskiy, I.P. 2015, 'A magnetoacoustic autowave pulse in acoustically unstable regions of solar atmosphere', Paper presented to the 3rd Southern African Solar Energy Conference, South Africa, 11-13 May, 2015.en_ZA
dc.identifier.urihttp://hdl.handle.net/2263/49571
dc.language.isoenen_ZA
dc.publisher3rd Southern African Solar Energy Conference, South Africa, 11-13 May, 2015.en_ZA
dc.rights© 2015 University of Pretoriaen_ZA
dc.subjectNet radiation function modelen_ZA
dc.subjectRadiation functionen_ZA
dc.subjectHeatingen_ZA
dc.subjectSolar atmosphereen_ZA
dc.subjectMagnetoacoustical amplificationen_ZA
dc.titleA magnetoacoustic autowave pulse in acoustically unstable regions of solar atmosphereen_ZA
dc.typePresentationen_ZA

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