Solution to the cosmic ray anisotropy problem

In the standard diffusive picture for transport of cosmic rays (CRs), a gradient in the CR density induces a typically small, dipolar anisotropy in their arrival directions. This is being widely advertised as a tool for finding nearby sources. However, the predicted dipole amplitude at TeV and PeV e...

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Veröffentlicht in:	Physical review letters 2015-01, Vol.114 (2), p.021101-021101, Article 021101
Hauptverfasser:	Mertsch, Philipp, Funk, Stefan
Format:	Artikel
Sprache:	eng
Schlagworte:	Amplitudes Anisotropy Cosmic rays Density Deviation Dipoles Magnetic fields Searching
Online-Zugang:	Volltext
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