Cosmic ray propagation through turbulent magnetic fields.

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DC Field	Value	Language
dc.contributor.author	Switalska, Eliza	en
dc.date.issued	2006	en
dc.identifier.uri	http://hdl.handle.net/2440/69438	-
dc.description.abstract	This thesis is a study of cosmic ray propagation within turbulent magnetic fields. Turbulent scale-lengths were altered and the behaviour of cosmic rays was observed within both large and small-scale magnetic fields, thereby giving an indication of the actual paths they may follow in space, and consequently providing some clues as to their origins.	en
dc.subject	cosmic rays; cosmic magnetic fields; cosmic physics	en
dc.title	Cosmic ray propagation through turbulent magnetic fields.	en
dc.type	Thesis	en
dc.contributor.school	School of Chemistry and Physics	en
dc.provenance	This electronic version is made publicly available by the University of Adelaide in accordance with its open access policy for student theses. Copyright in this thesis remains with the author. This thesis may incorporate third party material which has been used by the author pursuant to Fair Dealing exception. If you are the author of this thesis and do not wish it to be made publicly available or If you are the owner of any included third party copyright material you wish to be removed from this electronic version, please complete the take down form located at: http://www.adelaide.edu.au/legals	-
dc.description.dissertation	Thesis (M.Sc.) -- University of Adelaide, School of Chemistry and Physics, 2006	en
Appears in Collections:	Research Theses

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