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Origin of small-scale anisotropies in Galactic cosmic rays
DOI: 10.1016/j.ppnp.2017.01.004
Bibcode: 2017PrPNP..94..184A
Mertsch, Philipp; Ahlers, Markus
The arrival directions of Galactic cosmic rays are highly isotropic. This is expected from the presence of turbulent magnetic fields in our Galactic environment that repeatedly scatter charged cosmic rays during propagation. However, various cosmic ray observatories have identified weak anisotropies of various angular sizes and with relative inten…
2017
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Progress in Particle and Nuclear Physics
Ulysses
70