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Please use this identifier to cite or link to this item: https://hdl.handle.net/2440/18139
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dc.contributor.authorClay, R.-
dc.date.issued2003-
dc.identifier.citationProgress of Theoretical Physics Supplement, 2003; 151(151):74-84-
dc.identifier.issn0375-9687-
dc.identifier.urihttp://hdl.handle.net/2440/18139-
dc.descriptionThe original publication is available at http://ptp.ipap.jp (or http://ptp.ipap.jp/link?PTPS/151/74) Copyright © 2003 Progress of Theoretical Physics. All rights reserved.-
dc.description.abstractCosmic rays with energies above 1 EeV are currently of considerable interest in astrophysics and are to be further studied in a number of projects which are either currently under construction or the subject of well-developed proposals. This paper aims to discuss some of the physics of such particles in terms of current knowledge and information from particle astrophysics at other energies. Included is an argument that the role of galactic sources at these ultra high energies should not be ignored. Also, the key role of the unknown structure and magnitude of the intergalactic magnetic field is emphasised.-
dc.description.statementofresponsibilityRoger Clay-
dc.language.isoen-
dc.publisherProgress Theoretical Physics Publication Office-
dc.source.urihttp://ptp.ipap.jp/link?PTPS/151/74/-
dc.titleUltra high energy cosmic rays-
dc.typeJournal article-
dc.identifier.doi10.1143/PTPS.151.74-
pubs.publication-statusPublished-
dc.identifier.orcidClay, R. [0000-0002-9040-9648]-
Appears in Collections:Aurora harvest 2
Physics publications

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