Anisotropies and the power requirements for galactic cosmic rays

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dc.contributor.authorClay, R.
dc.contributor.authorMcDonough, M.
dc.contributor.authorSmith, A.
dc.contributor.authorDawson, B.
dc.date.issued1998
dc.description.abstractMeasurements of cosmic ray directional properties at about tex2html_wrap_inline137eV in both northern and southern hemispheres confirm that those particles have a unidirectional anisotropy and are flowing along the direction of our spiral arm from the inner galactic regions. On the basis of diffusive cosmic ray flow along the galactic arms, the power required for the galaxy to maintain this flow is below tex2html_wrap_inline139watts.
dc.identifier.citationPublications of the Astronomical Society of Australia, 1998; 15(2):208-210
dc.identifier.doi10.1071/AS98208
dc.identifier.issn1323-3580
dc.identifier.issn1448-6083
dc.identifier.orcidClay, R. [0000-0002-9040-9648]
dc.identifier.orcidDawson, B. [0000-0002-4271-3055]
dc.identifier.urihttp://hdl.handle.net/2440/12816
dc.language.isoen
dc.publisherC S I R O PUBLICATIONS
dc.source.urihttp://www.atnf.csiro.au/pasa/15_2/clay/paper/
dc.subjectISM
dc.subjectcosmic rays
dc.titleAnisotropies and the power requirements for galactic cosmic rays
dc.typeJournal article
pubs.publication-statusPublished

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