Article ID Journal Published Year Pages File Type
8133041 Astroparticle Physics 2013 15 Pages PDF
Abstract
► Understanding of cosmic ray acceleration has progressed remarkably in recent years. ► Magnetic field amplification is necessary for acceleration to 1 PeV. ► There are differences between parallel, oblique and perpendicular shocks. ► High efficiency probably requires non-linear self-regulation. ► There is still much we do not know.
Related Topics
Physical Sciences and Engineering Physics and Astronomy Astronomy and Astrophysics
Authors
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