Puzzles of the cosmic ray anisotropy. (arXiv:1901.00160v1 [astro-ph.HE])
<a href="http://arxiv.org/find/astro-ph/1/au:+Erlykin_A/0/1/0/all/0/1">Anatoly Erlykin</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Machavariani_S/0/1/0/all/0/1">Svetlana Machavariani</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Wolfendale_A/0/1/0/all/0/1">Arnold Wolfendale</a>
We discuss three of the known puzzles of the cosmic ray anisotropy in the PeV
and sub-PeV energy region. They are: (1) the so called inverse anisotropy, (2)
the irregularity in the energy dependence of the amplitude and phase of the
first harmonic and (3) the contribution of the single source.
We discuss three of the known puzzles of the cosmic ray anisotropy in the PeV
and sub-PeV energy region. They are: (1) the so called inverse anisotropy, (2)
the irregularity in the energy dependence of the amplitude and phase of the
first harmonic and (3) the contribution of the single source.
http://arxiv.org/icons/sfx.gif
