Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/6178
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dc.contributor.authorVigeesh, G-
dc.contributor.authorHasan, S. S-
dc.date.accessioned2013-07-09T09:49:58Z-
dc.date.available2013-07-09T09:49:58Z-
dc.date.issued2013-
dc.identifier.citationJournal of Physics: Conference Series, Vol. 440, 012045en
dc.identifier.issn1742-6588-
dc.identifier.urihttp://hdl.handle.net/2248/6178-
dc.descriptionOpen Accessen
dc.descriptionContent from this work may be used under the terms of the Creative Commons Attribution 3.0 licence. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI.-
dc.description.abstractWe present the results of three-dimensional numerical simulations to investigate the excitation of waves in the magnetic network of the Sun due to foot point motions of a magnetic flux tube. We consider motions that typically mimic granular buffeting and vortex flows and implement them as driving motions at the base of the flux tube. The driving motions generates various MHD modes within the flux tube and acoustic waves in the ambient medium. The response of the upper atmosphere to the underlying photospheric motion and the role of the flux tube in channeling the waves is investigated. We compute the acoustic energy flux in the various wave modes across different boundary layers defined by the plasma and magnetic field parameters and examine the observational implications for chromospheric and coronal heating.en
dc.language.isoenen
dc.publisherIOP Publishingen
dc.relation.urihttp://dx.doi.org/10.1088/1742-6596/440/1/012045en
dc.relation.urihttp://arxiv.org/abs/1304.5193en
dc.rights© IOP Publishingen
dc.subjectPlasma physicsen
dc.subjectAstrophysics and astroparticlesen
dc.titleAcoustic Emission From Magnetic Flux Tubes in the Solar Networken
dc.typeArticleen
Appears in Collections:IIAP Publications

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