MHD modes of solar wind flow tubes

dc.contributor.authorChandra, Suresh
dc.date.accessioned2012-03-05T07:06:57Z
dc.date.available2012-03-05T07:06:57Z
dc.date.issued2008-02
dc.description.abstractNakariakov & Roberts (1995) and Nakariakov et al. (1996) investigated the linear mag- netosonic waves trapped within solar wind ow tubes by accounting for a slab having boundaries at x = d and extended up to in nity in y and z directions. They obtained dispersion relations for sausage and kink surface waves in incompressible plasma. Following the approach of Nakariakov & Roberts (1995), we have obtained dispersion relations for sausage and kink surface waves in a compressible plasma. Values of the parameter a !=kCAo are found to vary in the ranges 0.755 0.849 and 1.080 1.356 for the sausage waves and in the ranges 0.850 0.882 and 1.358 1.538 for the kink waves in the compressible plasma. It shows an interesting feature that the sausage and kink surface waves are exclusive from each other.en_US
dc.identifier.urihttp://hdl.handle.net/11007/368
dc.language.isoenen_US
dc.relation.ispartofseriesIUCAA Preprint;06/09
dc.subjectMHDen_US
dc.subjectSolar wind flowen_US
dc.titleMHD modes of solar wind flow tubesen_US
dc.typeArticleen_US

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