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dc.contributor.authorMcCloughan, John Leslieen
dc.date.accessioned2006-03-27
dc.date.available2006-03-27
dc.date.issued2002-01-01
dc.identifier.urihttp://hdl.handle.net/2123/485
dc.description.abstractThis thesis investigates how magnetographic data may be used to study the longterm behaviour of the magnetic field distribution across the surface of the sun.en
dc.format.extent72765 bytes
dc.format.extent2108791 bytes
dc.format.mimetypeapplication/pdf
dc.format.mimetypeapplication/pdf
dc.languageenen
dc.language.isoen_AU
dc.rightsOtheren
dc.subjectsynoptic maps;synoptic transport equation;solar magnetic fielden
dc.titleEvolving Synoptic Maps of the solar magnetic fielden
dc.typeThesisen
dc.date.valid2002-01-01en
dc.type.thesisDoctor of Philosophyen
dc.rights.otherCopyright McCloughan, John Leslie;http://www.library.usyd.edu.au/copyright.htmlen
dc.rights.otherThe author retains copyright of this thesisen
usyd.facultyFaculty of Science, School of Mathematics and Statisticsen
usyd.degreeDoctor of Philosophy Ph.D.en
usyd.awardinginstThe University of Sydneyen


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