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The solar activity cycle

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dc.contributor.author Thomas, William Mark
dc.date.accessioned 2011-08-25T21:16:30Z
dc.date.accessioned 2022-10-30T18:58:14Z
dc.date.available 2011-08-25T21:16:30Z
dc.date.available 2022-10-30T18:58:14Z
dc.date.copyright 1977
dc.date.issued 1977
dc.identifier.uri https://ir.wgtn.ac.nz/handle/123456789/25929
dc.description.abstract This thesis reviews the currently accepted theories of solar activity along with a new conflicting theory. The current theory due to Babcock and Leighton is outlined along with the supporting evidence and then the new theory due to Wolff. The new theory is claimed to be well supported by solar activity data so the data is reviewed and analysed to determine how well founded the claimed support actually is. It is found that the basis of support for the new theory, the relative sunspot numbers ,do not in fact provide the support claimed. It is also shown that the new theory at present, is not able to explain many of the observed phenomena of the activity cycle. en_NZ
dc.format pdf en_NZ
dc.language en_NZ
dc.language.iso en_NZ
dc.publisher Te Herenga Waka—Victoria University of Wellington en_NZ
dc.title The solar activity cycle en_NZ
dc.type Text en_NZ
vuwschema.type.vuw Awarded Research Masters Thesis en_NZ
thesis.degree.discipline Physics en_NZ
thesis.degree.grantor Te Herenga Waka—Victoria University of Wellington en_NZ
thesis.degree.level Masters en_NZ
thesis.degree.name Master of Science en_NZ


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