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• W2401984795 abstract "Recent measurements of the dipole anisotropy in the arrival directions of Galactic cosmic rays (CRs) indicate a strong energy dependence of the dipole amplitude and phase in the TeV-PeV range. We argue here that these observations can be well understood within standard diffusion theory as a combined effect of (i) one or more local sources at Galactic longitude 120deg < l < 300deg dominating the CR gradient below 0.1-0.3 PeV, (ii) the presence of a strong ordered magnetic field in our local environment, (iii) the relative motion of the solar system, and (iv) the limited reconstruction capabilities of ground-based observatories. We show that an excellent candidate of the local CR source responsible for the dipole anisotropy at 1-100 TeV is the Vela supernova remnant." @default.
• W2401984795 created "2016-06-24" @default.
• W2401984795 creator A5085798900 @default.
• W2401984795 date "2016-10-07" @default.
• W2401984795 modified "2023-10-15" @default.
• W2401984795 title "Deciphering the Dipole Anisotropy of Galactic Cosmic Rays" @default.
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• W2401984795 doi "https://doi.org/10.1103/physrevlett.117.151103" @default.
• W2401984795 hasPubMedId "https://pubmed.ncbi.nlm.nih.gov/27768328" @default.
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