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dc.contributor.authorHussain, G.A.J.
dc.contributor.authorJardine, M.
dc.contributor.authorCollier Cameron, A.
dc.contributor.authorBarnes, J.R.
dc.contributor.authorDonati, J-F.
dc.date.accessioned2008-01-30T10:44:40Z
dc.date.available2008-01-30T10:44:40Z
dc.date.issued2000
dc.identifier.citationHussain , G A J , Jardine , M , Collier Cameron , A , Barnes , J R & Donati , J-F 2000 , Can the magnetic topology of AB Doradus be explained by a potential field distribution . in In: Stellar Clusters and Associations: Convection, Rotation, and Dynamos - ASP Conf Series 198 . Astronomical Society of the Pacific , pp. 463-466 .
dc.identifier.isbn1-58381-025-0
dc.identifier.otherPURE: 163592
dc.identifier.otherPURE UUID: 565145a9-5062-4396-b191-99230b8f5bf8
dc.identifier.otherdspace: 2299/1480
dc.identifier.urihttp://hdl.handle.net/2299/1480
dc.descriptionOriginal paper can be found at: http://www.astrosociety.org/pubs/cs/195-221.html--Copyright Astronomical Society of the Pacific
dc.description.abstractWe present potential magnetic field maps of the surface of the active KO dwarf, AB Dor. Maps of the surface magnetic flux distributions of rapid rotators can be produced using the technique of Zeeman Doppler imaging (ZDI). Magnetic flux maps of active cool stars produced using ZDI show many features that have no solar counterpart. Currently, ZDI codes map only the simplest possible magnetic field distributions that will fit the observed data. It remains unclear how physically realistic these maps really are and this is what we are concerned with here.en
dc.language.isoeng
dc.publisherAstronomical Society of the Pacific
dc.relation.ispartofIn: Stellar Clusters and Associations: Convection, Rotation, and Dynamos - ASP Conf Series 198
dc.rightsOpen
dc.titleCan the magnetic topology of AB Doradus be explained by a potential field distributionen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.relation.schoolSchool of Physics, Astronomy and Mathematics
dcterms.dateAccepted2000
rioxxterms.typeOther
herts.preservation.rarelyaccessedtrue
herts.rights.accesstypeOpen


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