Anisotropies and clustering of extragalactic cosmic rays

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dc.creatorKachelriess, M.
dc.date2006-10-29
dc.date.accessioned2026-07-07T11:00:02Z
dc.date.available2026-07-07T11:00:02Z
dc.descriptionDeviations from isotropy have been a key tool to identify the sources and the primary type of cosmic rays (CRs) at low energies. We argue that anisotropies due to blind regions induced by the Galactic magnetic field, the cosmological Compton-Getting effect, medium-scale anisotropies reflecting the large-scale distribution of CR sources and the small-scale clustering of the CR arrival directions at the highest energies may play the same role for extragalactic CRs.
dc.description9 pages, 3 figures, talk at CRIS, Catania 2006
dc.identifierhttps://arxiv.org/abs/astro-ph/0610862
dc.identifierhttp://arxiv.org/abs/astro-ph/0610862
dc.identifierNucl.Phys.Proc.Suppl.165:272-279,2007
dc.identifierdoi:10.1016/j.nuclphysbps.2006.11.039
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/187606
dc.subjectAstrophysics
dc.titleAnisotropies and clustering of extragalactic cosmic rays
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