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dc.contributor.authorBingham, R.
dc.contributor.authorShukla, P. K.
dc.contributor.authorEliasson, B.
dc.contributor.authorCairns, A.
dc.contributor.authorCairns, R Alan
dc.date.accessioned2016-04-08T14:00:06Z
dc.date.available2016-04-08T14:00:06Z
dc.date.issued2015-09-15
dc.identifier.citationBingham , R , Shukla , P K , Eliasson , B , Cairns , A & Cairns , R A 2015 , ' Solar coronal electron heating by short-wavelength dispersive shear Alfvén waves ' , Physica Scripta , vol. 90 , no. 10 , 108004 , pp. 1-4 . https://doi.org/10.1088/0031-8949/90/10/108004en
dc.identifier.issn0031-8949
dc.identifier.otherPURE: 230685464
dc.identifier.otherPURE UUID: a82cec18-67e4-4858-8a1c-6bd5d606d4fb
dc.identifier.otherWOS: 000362529800014
dc.identifier.otherScopus: 84944810019
dc.identifier.otherWOS: 000362529800014
dc.identifier.urihttp://hdl.handle.net/10023/8581
dc.descriptionThis work was partially supported by the STFC through the Centre for Fundamental Physics (CfFP) at Rutherford Appleton Laboratory, Chilton, Didcot, UK. BE acknowledges support by the Engineering and Physical Sciences Research Council (EPSRC), UK, Grant no EP/M009386/1.en
dc.description.abstractThe electron heating of the solar coronal plasma has remained one of the most important problems in solar physics. An explanation of the electron heating rests on the identification of the energy source and appropriate physical mechanisms via which the energy can be channelled to the electrons. Our objective here is to present an estimate for the electron heating rate in the presence of finite amplitude short-wavelength (in comparison with the ion gyroradius) dispersive shear Alfven (SWDSA) waves that propagate obliquely to the ambient magnetic field direction in the solar corona. Specifically, it is demonstrated that SWDSA waves can significantly contribute to the solar coronal electron heating via collisionless heating involving SWDSA wave-electron interactions.
dc.format.extent4
dc.language.isoeng
dc.relation.ispartofPhysica Scriptaen
dc.rightsThis is an Open Access article. Content 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.en
dc.subjectSolar coronal heatingen
dc.subjectDispersive shear Alfvén wavesen
dc.subjectElectron heatingen
dc.subjectQC Physicsen
dc.subjectQA Mathematicsen
dc.subjectT-NDASen
dc.subject.lccQCen
dc.subject.lccQAen
dc.titleSolar coronal electron heating by short-wavelength dispersive shear Alfvén wavesen
dc.typeJournal articleen
dc.description.versionPublisher PDFen
dc.contributor.institutionUniversity of St Andrews.Applied Mathematicsen
dc.identifier.doihttps://doi.org/10.1088/0031-8949/90/10/108004
dc.description.statusPeer revieweden


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